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On multivariate contribution measures of systemic risk with applications in cryptocurrency market

Limin Wena, Junxue Lia, Tong Pub, Yiying Zhangb
a. Research Center of Management Science and Engineering, Jiangxi Normal University, Nanchang, 330022, China.
b. Department of Mathematics, Southern University of Science and Technology, Shenzhen, 518055, China.
Corresponding author. E-mail: zhangyy3@sustech.edu.cn.
(September 13, 2025)
Abstract

Conditional risk measures and their associated risk contribution measures are commonly employed in finance and actuarial science for evaluating systemic risk and quantifying the effects of risk interactions. This paper introduces various types of contribution ratio measures based on the MCoVaR, MCoES, and MMME studied in Ortega-Jiménez et al. (2021) and Das & Fasen-Hartmann (2018) to assess the relative effects of a single risk when other risks in a group are in distress. The properties of these contribution risk measures are examined, and sufficient conditions for comparing these measures between two sets of random vectors are established using univariate and multivariate stochastic orders and statistically dependent notions. Numerical examples are presented to validate these conditions. Finally, a real dataset from the cryptocurrency market is used to analyze the spillover effects through our proposed contribution measures.


Keywords: Systemic risk; Conditional risk measures; Spillover effects; Cryptocurrency market; Stochastic orders
MSC 2010 Classification: Primary 90B25; Secondary 60E15, 60K10.
JEL Classification: G20, G21, G22, G31, C3.

1 Introduction

In actuarial science and finance, risks are often not isolated events but are highly correlated and capable of spreading. When financial institutions face adverse conditions, such risks can quickly propagate through complex market interconnections, creating a domino effect that escalates losses from a single institution to the entire market, potentially triggering widespread systemic risk. Systemic risk is a core concept in these fields, as it leads to market failures, large-scale financial crises, and profound, long-lasting impacts on the real economy. Typical examples of systemic risk include financial crises, market crashes, bank runs, and contagion effects spreading across multiple industries (Dičpinigaitienė & Novickytė, 2018; Zhang et al., 2023).

In this paper, we focus on the “capital” type of systemic risk model, which is a method to assess systemic risk losses and their probability of occurrence, and can be characterized by a risk measure111Systemic risk models can be categorized into the following five types: (i) early warning systems (EWS); (ii) capital; (iii) liquidity; (iv) contagion; and (v) network. For further details, the reader can refer to Silva et al. (2017) and Ellis et al. (2022).. Among widely recognized risk measures, Value-at-Risk (VaR) and Expected Shortfall (ES) have been extensively discussed in the literature (Duffie & Pan, 1997; Delbaen & Biagini, 2000; Acerbi & Tasche, 2002). However, they fail to effectively quantify systemic risk as they only consider isolated individual economic entities. Hence, there is a need for novel conditional risk (co-risk) measures to quantify and evaluate systemic risk in financial systems. The Conditional Value-at-Risk (CoVaR), introduced by Adrian & Brunnermeier (2016), measures the VaR of a particular asset under a certain level of systemic stress. Mainik & Schaanning (2014) proposed Conditional Expected Shortfall (CoES), which measures the ES of a specific asset or portfolio under a certain level of systemic stress and is defined by the average tail integral of CoVaR. Acharya et al. (2017) introduced the concept of Marginal Expected Shortfall (MES) and empirically validated its effectiveness in predicting emerging risks during the 2007-2009 financial crisis. The theoretical properties of these co-risk measures and their applications in finance and insurance can be found in Kritzman et al. (2011); Asimit & Gerrard (2016); Feinstein et al. (2017); Asimit & Li (2018); Lin et al. (2018); Duarte & Eisenbach (2021); Liu & Yang (2021); Waltz et al. (2022); Yang et al. (2024). However, these co-risk measures can only assess the interaction effect from one entity to another entity, but cannot characterize the absolute or relative spillover effects, which lays the foundation for relevant research on proposing various risk contribution measures.

The class of risk contribution measures can be divided into two types: difference-based and ratio-based contribution measures. The former is usually defined as the difference between conditional and unconditional risk measures, while the latter is defined as the ratio between the difference-based contribution measure and the benchmark unconditional risk measure. For example, Adrian & Brunnermeier (2016) introduced the well-known difference-based and ratio-based contribution measures in terms of CoVaR when the conditional systemic event is taken as VaR at some fixed level. Girardi & Ergün (2013) also defined the difference-based contribution measures (denoted as Δ\DeltaCoVaR and Δ\DeltaCoES) based on CoVaR and CoES with different types of conditional events. From the perspective of stochastic orders and dependence structures, Sordo et al. (2018) provided sufficient conditions to rank CoVaR, CoES, and their risk contribution measures ΔCoVaR\Delta{\rm CoVaR} and ΔCoES\Delta{\rm CoES}. Dhaene et al. (2022) introduced conditional distortion (CoD) risk measures and the difference-based distortion risk contribution measures (ΔCoD\Delta{\rm CoD}), discussing sufficient conditions to rank different bivariate vectors with respect to these measures. Recently, Zhang (2024) introduced several types of ratio-based distortion risk contribution measures (ΔRCoD\Delta^{\rm R}{\rm CoD}) and examined sufficient conditions for comparing these measures in terms of a new characterization of the convex transform order.

Most of the above-mentioned works only consider a single risk as the systemic risk event, which runs counter to the reality in the financial market that there might be multiple risks collapsing simultaneously. This scenario hinders the usage of the aforementioned systemic risk measures, which calls for the definitions of multivariate systemic risk measures. In fact, multivariate risks are attracting increasing attention from many researchers such as Lee & Prékopa (2013), Sun et al. (2018), and Ling (2019). Let 𝑿=(X1,,Xn){\bm{X}}=(X_{1},\cdots,X_{n}) represent a portfolio of risks. Here, we assume X2,,XnX_{2},\cdots,X_{n} represent systemic risk, capturing the volatility and uncertainty of the entire system or market, rather than just the impact of any individual asset or event. The definition of multivariate marginal mean excess (in short, MMME) is initially introduced by Das & Fasen-Hartmann (2018) and the asymptotic behavior is studied under suitable conditions within the framework of multivariate regular variation, hidden regular variation and asymptotic tail independence. The multivariate CoVaR (in short, MCoVaR) and multivariate CoES (in short, MCoES) are firstly formally defined in Ortega-Jiménez et al. (2021) to quantify the risk of X2,,XnX_{2},\cdots,X_{n} spilled over to X1X_{1}. Besides, the difference-based contribution risk measures are also introduced. Utilizing MCoVaR, MCoES and MMME, and their associated difference-based contribution measures (with unconditional risk measure as the benchmark), Ortega-Jiménez et al. (2021) investigated sufficient conditions for implementing comparisons between two different sets of multivariate risk vectors.

In this paper, we introduce two types of multivariate risk contribution ratios to reassess the concepts of MCoVaR, MCoES, and MMME. Our research motivation stems from the fact that when we are more concerned with relative contributions rather than absolute contributions of systemic risks, the effectiveness of those contribution measures studied in Ortega-Jiménez et al. (2021) is limited. Therefore, this paper introduces the multivariate risk contribution ratio measures to address this issue, where the first type of benchmark measure uses unconditional risk values such as VaR or ES, which are univariate risk measures, and the second type of benchmark measure uses a multivariate joint risk measure based on the median of systemic events, a method commonly used in financial markets. Based on the newly proposed contribution measures, we theoretically analyze sufficient conditions for comparing two distinct multivariate risk portfolios. In particular, for two risk vectors (X1,,Xn)(X_{1},\dots,X_{n}) and (Y1,,Yn)(Y_{1},\dots,Y_{n}), the consistency of co-risk measures is examined under different stochastic orders and dependence assumptions. Further, we compute the values of these new risk measures using real-world dataset in the cryptocurrency market, comparing with existing related risk measures, and analyzing the market interactions.

The remaining sections of this paper are structured as follows. Section 2 reviews some basic concepts, including univariate and multivariate stochastic orders, copula functions, and some well-known (conditional) risk measures. Section 3 introduces several new definitions of multivariate systemic risk contribution ratio measures based on MCoVaR, MCoES and MMME, and establishes sufficient conditions to compare two different risk portfolios under these new measures. Section 4 analyzes the risk co-movement effect in the cryptocurrency market by computing and comparing these proposed contribution risk measures. Section 5 concludes the paper. All proofs and supplementary definitions are provided in the appendix.

2 Preliminaries

Throughout this paper, let 𝑿=(X1,,Xn)\bm{X}=(X_{1},\dots,X_{n}) and 𝒀=(Y1,,Yn)\bm{Y}=(Y_{1},\dots,Y_{n}) represent two nn-dimensional random vectors with joint distribution functions (d.f.) denoted by FF and GG, and joint density functions f(𝒙)f({\bm{x}}) and g(𝒙)g({\bm{x}}), respectively, which will be abbreviated to “𝑿F\bm{X}\sim F” and “𝒀G\bm{Y}\sim G”. Their marginal distributions are denoted by F1,,FnF_{1},\dots,F_{n} and G1,,GnG_{1},\dots,G_{n}, which are continuous and have finite expectations. Additionally, their joint survival functions are denoted by F¯\overline{F} and G¯\overline{G}, that is, F¯(𝒙)\overline{F}({\bm{x}})=(𝑿>𝒙)=\mathbb{P}({\bm{X}}>{\bm{x}}) and G¯(𝒙)=(𝒀>𝒙)\overline{G}({\bm{x}})=\mathbb{P}({\bm{Y}}>{\bm{x}}) for 𝒙n{\bm{x}}\in\mathbb{R}^{n}. Let 𝒙=(x1,,xn){\bm{x}}=(x_{1},\dots,x_{n}) and 𝒚=(y1,,yn){\bm{y}}=(y_{1},\dots,y_{n}) be two real-valued vectors in n\mathbb{R}^{n}, we denote 𝒙𝒚=(min{x1,y1},,min{xn,yn}){\bm{x}}\vee{\bm{y}}=\left({\rm min}\{x_{1},y_{1}\},\dots,{\rm min}\{x_{n},y_{n}\}\right) and 𝒙𝒚=(max{x1,y1},,max{xn,yn}){\bm{x}}\wedge{\bm{y}}=\left({\rm max}\{x_{1},y_{1}\},\dots,{\rm max}\{x_{n},y_{n}\}\right).

2.1 Stochastic orders

The quantile function for a random variable XX with distribution function FXF_{X} is defined as:

VaRp(X):=FX1(p)=inf{x|FX(x)p},p(0,1).\mathrm{VaR}_{p}(X):={F_{X}^{-1}}(p)=\inf\{x\in{\mathbb{R}}|F_{X}(x)\geq p\},~~p\in(0,1).

Now, we present several pertinent definitions of univariate stochastic orders that will be utilized in subsequent discussions.

Definition 2.1.

Let XX and YY be two random variables with distribution functions FXF_{X} and FYF_{Y}, density functions fXf_{X} and fYf_{Y}, and survival functions F¯X\overline{F}_{X} and F¯Y\overline{F}_{Y}, respectively. Then XX is said to be smaller than YY in the:

  1. (i)

    usual stochastic order (denoted by XstYX\leq_{\rm st}Y) if F¯X(t)F¯Y(t){\overline{F}}_{X}(t)\leq{\overline{F}}_{Y}(t) for all tt\in{\mathbb{R}};

  2. (ii)

    excess wealth order (denoted by XewYX\leq_{\rm ew}Y) if 𝔼[(XFX1(p))+]𝔼[(YFY1(p))+]\mathbb{E}\left[\left(X-F_{X}^{-1}(p)\right)_{+}\right]\leq\mathbb{E}\left[\left(Y-F_{Y}^{-1}(p)\right)_{+}\right] for all 0<p<10<p<1, where x+=max(0,x)x_{+}={\rm max}(0,x);

  3. (iii)

    star order (denoted by XYX\leq_{\star}Y) if FY1(p)/FX1(p)F_{Y}^{-1}(p)/F_{X}^{-1}(p) is increasing in p(0,1)p\in(0,1), when the two random variables are non-negative;

  4. (iv)

    expected proportional shortfall order (denoted by XpsYX\leq_{\rm ps}Y) if EPSp(X)EPSp(Y){\rm EPS}_{p}(X)\leq{\rm EPS}_{p}(Y) for all pDXDYp\in D_{X}\cap D_{Y}, when the two random variables are non-negative, where DX={p(0,1):FX1(p)>0}D_{X}=\{p\in(0,1):F_{X}^{-1}(p)>0\}, DY={p(0,1):FY1(p)>0}D_{Y}=\{p\in(0,1):F_{Y}^{-1}(p)>0\}. Here,

    EPSp(X)=𝔼[(XVaRp(X)VaRp(X))+] and EPSp(Y)=𝔼[(YVaRp(Y)VaRp(Y))+].\mathrm{EPS}_{p}(X)=\mathbb{E}\left[\left(\frac{X-\mathrm{VaR}_{p}(X)}{\mathrm{VaR}_{p}(X)}\right)_{+}\right]~\text{ and }~\mathrm{EPS}_{p}(Y)=\mathbb{E}\left[\left(\frac{Y-\mathrm{VaR}_{p}(Y)}{\mathrm{VaR}_{p}(Y)}\right)_{+}\right].

In Definition 2.1, (i)–(iii) are referenced in Shaked & Shanthikumar (2007), and (iv) can be found in Belzunce et al. (2012). It is also known that both of the star order and the expected proportional shortfall order are scaled invariant and the former implies the latter. Interested readers can refer to the monographs Shaked & Shanthikumar (2007) and Belzunce et al. (2015) for more detailed discussions.

Next, for the random vector 𝑿=(X1,,Xn)\bm{X}=(X_{1},\dots,X_{n}), we introduce some multivariate stochastic orders and dependence notions, indicating that in some stochastic sense, larger values of one random vector are associated with larger or smaller values of another random vector.

Definition 2.2.

(Shaked & Shanthikumar, 2007) Let 𝐗=(X1,,Xn)\bm{X}=(X_{1},\dots,X_{n}) and 𝐘=(Y1,,Yn)\bm{Y}=(Y_{1},\dots,Y_{n}) be two random vectors with joint distribution functions FF and GG, respectively. Then

  1. (i)

    the random variable {Xi,iAc}\{X_{i},i\in A^{c}\}, is said to be right-tail increasing (decreasing) in {Xj,jA}\{X_{j},j\in A\}, (denoted by {Xi,iAc}RTI[RTD]{Xj,jA}\{X_{i},i\in A^{c}\}\uparrow_{\rm RTI[RTD]}\{X_{j},j\in A\}) if (Xi>xi,iAc|Xj>xj,jA)\mathbb{P}(X_{i}>x_{i},i\in A^{c}|X_{j}>x_{j},j\in A) increases (decreases) in xjx_{j}, where AA is a subset of {1,,n}\{1,\dots,n\} with at least one element, and AcA^{c} denotes the complement of AA;

  2. (ii)

    the random vector 𝑿\bm{X} is said to be smaller than 𝒀\bm{Y} in the multivariate hazard rate order (denoted by 𝑿hr𝒀\bm{X}\leq_{\rm hr}\bm{Y}) if F¯(𝒙)G¯(𝒚)F¯(𝒙𝒚)G¯(𝒙𝒚)\overline{F}({\bm{x}})\overline{G}({\bm{y}})\leq\overline{F}({\bm{x}}\wedge{\bm{y}})\overline{G}({\bm{x}}\vee{\bm{y}}) for all 𝒙,𝒚n{\bm{x}},{\bm{y}}\in{\mathbb{R}}^{n};

  3. (iii)

    the random vector 𝑿\bm{X} is said to be smaller than 𝒀\bm{Y} in the weak multivariate hazard rate order (denoted by 𝑿whr𝒀\bm{X}\leq_{\rm whr}\bm{Y}) if G¯(𝒙)/F¯(𝒙)\overline{G}(\bm{x})/\overline{F}(\bm{x}) is increasing in 𝒙{𝒙:G¯(𝒙)>0}\bm{x}\in\left\{\bm{x}:\overline{G}({\bm{x}})>0\right\};

  4. (iv)

    the random vector 𝑿\bm{X} is said to be smaller than 𝒀\bm{Y} in the usual stochastic order (denoted by 𝑿st𝒀\bm{X}\leq_{\rm st}\bm{Y}) if 𝔼[h(𝑿)]𝔼[h(𝒀)]\mathbb{E}[h(\bm{X})]\leq\mathbb{E}[h(\bm{Y})] for all bounded increasing h:nh:\mathbb{R}^{n}\rightarrow\mathbb{R};

  5. (v)

    the random vector 𝑿\bm{X} is said to be multivariate totally positive of order 2 (denoted by MTP2{\rm MTP}_{2}) if f(𝒙)f(𝒚)f(𝒙𝒚)f(𝒙𝒚)f(\bm{x})f(\bm{y})\leq f(\bm{x}\wedge\bm{y})f(\bm{x}\vee\bm{y}) holds for all 𝒙,𝒚n\bm{x},\bm{y}\in{\mathbb{R}}^{n};

  6. (vi)

    the random vector 𝑿\bm{X} is said to be smaller than 𝒀\bm{Y} in the multivariate likelihood ratio order (denoted by 𝑿lr𝒀\bm{X}\leq_{\rm lr}\bm{Y}) if f(𝒙)g(𝒚)f(𝒙𝒚)g(𝒙𝒚)f({\bm{x}})g({\bm{y}})\leq f({\bm{x}}\wedge{\bm{y}})g({\bm{x}}\vee{\bm{y}}) for all 𝒙,𝒚n{\bm{x}},{\bm{y}}\in{\mathbb{R}}^{n};

  7. (vii)

    the random vector 𝑿^i=(X1,,Xi1,Xi+1,,Xn)\hat{\bm{X}}_{i}=(X_{1},\dots,X_{i-1},X_{i+1},\dots,X_{n}) is said to be stochastically increasing in XiX_{i} (denoted by 𝑿^iSIXi\hat{\bm{X}}_{i}\uparrow_{\rm SI}X_{i}) if the conditional distribution {(X1,,Xi1,Xi+1,,Xn|Xi=xi)}\left\{(X_{1},\dots,X_{i-1},X_{i+1},\dots,X_{n}|X_{i}=x_{i})\right\} is stochatically increasing as xix_{i} increases;

  8. (viii)

    the random vector 𝑿\bm{X} is said to be positive dependent through the stochastic order (or PDS) if 𝑿^iSIXi\hat{\bm{X}}_{i}\uparrow_{\rm SI}X_{i} for i{1,,n}i\in\{1,\dots,n\}.

According to Hu et al. (2003), the following relationships hold:

𝑿lr𝒀𝑿hr𝒀𝑿whr𝒀and𝑿lr𝒀𝑿st𝒀.\bm{X}\leq_{\rm lr}\bm{Y}\Longrightarrow\bm{X}\leq_{\rm hr}\bm{Y}\Longrightarrow\bm{X}\leq_{\rm whr}\bm{Y}~~\text{and}~~\bm{X}\leq_{\rm lr}\bm{Y}\Longrightarrow\bm{X}\leq_{\rm st}\bm{Y}.

2.2 Copula

Let FF be the joint distribution function of the random vector 𝑿\bm{X} with continuous marginal distribution functions F1,,FnF_{1},\dots,F_{n}. Then, there exists an nn-dimensional copula function C(p1,,pn)C(p_{1},\dots,p_{n}) defined on [0,1]n[0,1]^{n} such that

F(x1,,xn)=C(F1(x1),,Fn(xn)),x1,,xn.F(x_{1},\dots,x_{n})=C(F_{1}(x_{1}),\dots,F_{n}(x_{n})),\quad\forall~x_{1},\dots,x_{n}\in\mathbb{R}.

Here, the copula function CC captures the dependence structure of the random vector (X1,,Xn)(X_{1},\dots,X_{n}). Let Ui=Fi(Xi)U_{i}=F_{i}(X_{i}), which follows a uniform distribution U[0,1]U[0,1]. Then the copula function CC can be re-expressed as:

C(p1,,pn)=(U1p1,,Unpn),C(p_{1},\dots,p_{n})=\mathbb{P}(U_{1}\leq p_{1},\dots,U_{n}\leq p_{n}),

where pi=Fi(xi)p_{i}=F_{i}(x_{i}) for i=1,,ni=1,\dots,n. Clearly, it is deduced that

C(p1,,pn)=F(F11(p1),,Fn1(pn)).C(p_{1},\dots,p_{n})=F\left(F_{1}^{-1}(p_{1}),\dots,F_{n}^{-1}(p_{n})\right).

The joint tail function, denoted as C¯\overline{C}, is expressed as

C¯(p1,,pn)=(X1>F11(p1),,Xn>Fn1(pn)).\overline{C}(p_{1},\dots,p_{n})=\mathbb{P}(X_{1}>F_{1}^{-1}(p_{1}),\dots,X_{n}>F_{n}^{-1}(p_{n})).

For an nn-dimensional uniform random vector, the joint tail function C¯\overline{C} can be represented in terms of the copula CC as follows (see Theorem 4.7 in Cherubini et al. (2004)):

C¯(p1,,pn)=i=0n[(1)i𝒘(𝒑)Z(ni,n,1)C(𝒘(𝒑))],\overline{C}(p_{1},\dots,p_{n})=\sum_{i=0}^{n}\left[(-1)^{i}\sum_{{\bm{w}}(\bm{p})\in Z(n-i,n,1)}C({\bm{w}(\bm{p})})\right],

where Z(ni,n,i)Z(n-i,n,i) is the set of the (ni)\binom{n}{i} possible vectors with nin-i components equal to 1, ii components equal to pip_{i}.

The Archimedean copula, a prevalent category within the family of copulas, is characterized by a generating function known as the Archimedean generator. The expression for an nn-dimensional Archimedean copula is given by:

Cψ(u1,u2,,un)=ψ1(ψ(u1)+ψ(u2)++ψ(un)),C_{\psi}(u_{1},u_{2},\ldots,u_{n})=\psi^{-1}\left(\psi(u_{1})+\psi(u_{2})+\cdots+\psi(u_{n})\right),

where ψ\psi is a strictly decreasing function called the generating function, with its inverse denoted as ψ1\psi^{-1}. Prominent examples of Archimedean copulas include the Clayton, Gumbel, and Frank copulas, each employing distinct generating functions to model the dependencies among random variables. For these specific forms of Archimedean copulas, please refer to Appendix B.2.

Next, the definition of concordance order is provided describing one copula is more positively dependent than the other.

Definition 2.3.

(Nelsen, 2006) Given two nn-dimensional copulas CC and CC^{\prime}, CC is smaller than CC^{\prime} in the concordance order (denote by CcCC\leq_{\rm c}C^{\prime}) if C(𝐩)C(𝐩)C(\bm{p})\leq C^{\prime}(\bm{p}), for all 𝐩[0,1]n\bm{p}\in[0,1]^{n}.

For copula functions CC and CC^{\prime}, there also exists a stronger ranking relationship in terms of the weak multivariate hazard rate order (Hu et al., 2003), which is defined as follows.

Definition 2.4.

Given two nn-dimensional copulas CC and CC^{\prime}, CC is said to be smaller than CC^{\prime} in the weak multivariate hazard rate order (denote by CwhrCC\leq_{\rm whr}C^{\prime}) if C¯(𝐩)/C¯(𝐩)\overline{C}^{\prime}(\bm{p})/\overline{C}(\bm{p}) is increasing in 𝐩{𝐩[0,1]n:C¯(𝐩)>0}\bm{p}\in\left\{\bm{p}\in[0,1]^{n}:\overline{C}(\bm{p})>0\right\}.

2.3 Multivariate co-risk measures

For an individual risk XX with distribution function FXF_{X}, the Expected Shortfall (ES) of XX at a given probability level p(0,1)p\in(0,1) is defined as

ESp[X]=11pp1VaRt[X]𝑑t.{\rm ES}_{p}[X]=\frac{1}{1-p}\int_{p}^{1}{{\rm VaR}_{t}}[X]dt.

Essentially, VaR represents the one-sided critical value of asset value loss over a certain holding period at a given confidence level, practically manifesting as an amount serving as the threshold. Compared to VaR, ES considers the magnitude of losses beyond the VaR threshold, making it a more comprehensive measure of risk. ES is particularly suitable when tail risk is of concern or when a more comprehensive risk assessment is needed. Besides, according to the Basel IV accords, the internal/advanced model approach is revised by replacing the VaR measure with the ES measure, which further highlights the importance of ES in solvency regulation; see Kou et al. (2013) and Zaevski & Nedeltchev (2023).

In finance, the interconnections among entities’ (e.g. banks or financial institutions) risks can lead to varying levels of systemic risk. To investigate the risk spillover of other individuals on one concerned entity, Ortega-Jiménez et al. (2021) introduced a multivariate co-risk measure called MCoVaR as follows:

MCoVaR𝒑[X1|X2,,Xn]=VaRp1[X1|j=2n{Xj>VaRpj[Xj]}],\mathrm{MCoVaR}_{\bm{p}}[X_{1}|X_{2},\ldots,X_{n}]={\rm VaR}_{p_{1}}\left[X_{1}\bigg{|}\bigcap\limits_{j=2}^{n}\left\{{X_{j}}>{\rm VaR}_{p_{j}}[X_{j}]\right\}\right],

where 𝒑=(p1,,pn)(0,1)n\bm{p}=(p_{1},\dots,p_{n})\in(0,1)^{n}. Clearly, MCoVaR is the VaR of the conditional distribution of X1X_{1} at level p1p_{1}, given the joint systemic risk event {X2>VaRp2[X2],,Xn>VaRpn[Xn]}\{X_{2}>{\rm VaR}_{p_{2}}[X_{2}],...,X_{n}>{\rm VaR}_{p_{n}}[X_{n}]\}. As a direct generalization, the MCoES is further introduced in Ortega-Jiménez et al. (2021) as follows:

MCoES𝒑[X1|X2,,Xn]=11p1p11MCoVaRt,p2,,pn[X1|X2,,Xn]𝑑t.\mathrm{MCoES}_{\bm{p}}[X_{1}|X_{2},\dots,X_{n}]=\frac{1}{1-p_{1}}\int_{p_{1}}^{1}{\rm MCoVaR}_{t,p_{2},\dots,p_{n}}[X_{1}|X_{2},\dots,X_{n}]dt.

Following Das & Fasen-Hartmann (2018), the MMME is delineated as:

MMME𝒑[1][X1|X2,,Xn]=𝔼[(X1AX,p[1])+|j=2n{Xj>VaRpj[Xj]}],\mathrm{MMME}_{\bm{p}_{[-1]}}[X_{1}|X_{2},\dots,X_{n}]=\mathbb{E}\left[\left(X_{1}-A_{X,p_{[-1]}}\right)_{+}\bigg{|}\bigcap\limits_{j=2}^{n}\left\{{X_{j}}>{\rm VaR}_{p_{j}}[X_{j}]\right\}\right],

where 𝒑[1]=(p2,,pn)(0,1)n1{\bm{p}}_{[-1]}=(p_{2},\dots,p_{n})\in(0,1)^{n-1}, AX,p[1]=i=2naiVaRpi[Xi]A_{X,p_{[-1]}}=\sum_{i=2}^{n}a_{i}{\rm VaR}_{p_{i}}[X_{i}] and ai[0,1]a_{i}\in[0,1] satisfies i=2nai=1\sum_{i=2}^{n}a_{i}=1. The MMME𝒑[1][X1|X2,,Xn]\mathrm{MMME}_{\bm{p}_{[-1]}}[X_{1}|X_{2},\dots,X_{n}] represents the expected excess of X1X_{1} over a threshold AX,p[1]A_{X,p_{[-1]}}, conditional on the event that each XjX_{j} exceeds its VaR at level pjp_{j}, for j=2,,nj=2,\ldots,n. The threshold AX,p[1]A_{X,p_{[-1]}} is a weighted sum of the VaRs of X2X_{2} to XnX_{n}. This measure captures the expected amount by which X1X_{1} exceeds the threshold, reflecting the marginal mean excess risk under the given joint conditions.

3 Multivariate conditional risk contribution ratio measures and comparison results

Ortega-Jiménez et al. (2021) introduced two definitions of difference-based multivariate risk contribution measures corresponding to MCoVaR and MCoES, where the benchmark risk measure does not involve systemic risk. However, when regulators in financial markets focus on the relative spillover effects of systemic risk, the effectiveness of these measures becomes limited. To assess relative risk, the relative spillover effect of risk can be measured by dividing the multivariate risk contribution of an entity by its benchmark. One way to evaluate the risk contribution ratio of X2,,XnX_{2},\ldots,X_{n} to X1X_{1} is to compare the conditional risk measure of X1X_{1} (MCoVaR) with its unconditional risk value (VaR). Another method is to replace the unconditional risk value VaR\mathrm{VaR} with the conditional VaR of X1X_{1} when X2,,XnX_{2},\ldots,X_{n} are under benchmark conditions, where the benchmark state is typically defined by the median (Sordo et al., 2018).

We introduce the definition of a risk contribution ratio measure leveraging MCoVaR as follows.

Definition 3.1.

For 𝐩=(p1,,pn)(0,1)n\bm{p}=(p_{1},\dots,p_{n})\in(0,1)^{n}, the ratio-based contribution MCoVaR\rm MCoVaR with unconditional VaR\rm VaR as benchmark measure is defined by222To avoid misleading, we sometimes use MCoVaRp1,p2,,pn[X1|X2,,Xn]{\rm MCoVaR}_{p_{1},p_{2},\dots,p_{n}}[X_{1}|X_{2},\dots,X_{n}] to represent MCoVaR𝐩[X1|X2,,Xn]{\rm MCoVaR}_{\bm{p}}[X_{1}|X_{2},\dots,X_{n}].

ΔRMCoVaR𝒑[X1|X2,,Xn]=MCoVaR𝒑[X1|X2,,Xn]VaRp1[X1]VaRp1[X1],\Delta^{\rm R}{\rm MCoVaR}_{\bm{p}}[X_{1}|X_{2},\dots,X_{n}]=\frac{{\rm MCoVaR}_{\bm{p}}[X_{1}|X_{2},\dots,X_{n}]-{\rm VaR}_{p_{1}}[X_{1}]}{{\rm VaR}_{p_{1}}[X_{1}]}, (1)

provided that VaRp1[X1]0{\rm VaR}_{p_{1}}[X_{1}]\neq 0. For p1(0,1)p_{1}\in(0,1), the ratio-based contribution MCoVaR\rm MCoVaR with median-type MCoVaR\rm MCoVaR as the benchmark measure is defined by

ΔRmedMCoVaR𝒑[X1|X2,,Xn]=MCoVaRp1,𝒑[1][X1|X2,,Xn]MCoVaRp1,𝟏𝟐[X1|X2,,Xn]MCoVaRp1,𝟏𝟐[X1|X2,,Xn],\Delta^{\rm R-med}{\rm MCoVaR}_{\bm{p}}[X_{1}|X_{2},\dots,X_{n}]=\frac{{\rm MCoVaR}_{p_{1},\bm{p}_{[-1]}}[X_{1}|X_{2},\dots,X_{n}]-{\rm MCoVaR}_{p_{1},\frac{\bm{1}}{\bm{2}}}[X_{1}|X_{2},\dots,X_{n}]}{{\rm MCoVaR}_{p_{1},\frac{\bm{1}}{\bm{2}}}[X_{1}|X_{2},\dots,X_{n}]}, (2)

provided that MCoVaRp1,𝟏𝟐[X1|X2,,Xn]0{\rm MCoVaR}_{p_{1},\frac{\bm{1}}{\bm{2}}}[X_{1}|X_{2},\dots,X_{n}]\neq 0, where 𝐩[1]=(p2,,pn)(1/2,1)n1\bm{p}_{[-1]}=(p_{2},\dots,p_{n})\in(1/2,1)^{n-1} and 𝟏𝟐=(12,,12)n1\frac{\bm{1}}{\bm{2}}=\left(\frac{1}{2},\dots,\frac{1}{2}\right)\in\mathbb{R}^{n-1}.

Similarly, the multivariate risk contribution measures for MCoES are defined as follow.

Definition 3.2.

For 𝐩=(p1,,pn)(0,1)n\bm{p}=(p_{1},\dots,p_{n})\in(0,1)^{n}, the ratio-based contribution MCoES\rm MCoES with unconditional ES\rm ES as benchmark measure is defined by

ΔRMCoES𝒑[X1|X2,,Xn]=MCoES𝒑[X1|X2,,Xn]ESp1[X1]ESp1[X1],\Delta^{\rm R}{\rm MCoES}_{\bm{p}}[X_{1}|X_{2},\dots,X_{n}]=\frac{{\rm MCoES}_{\bm{p}}[X_{1}|X_{2},\dots,X_{n}]-{\rm ES}_{p_{1}}[X_{1}]}{{\rm ES}_{p_{1}}[X_{1}]}, (3)

provided that ESp1[X1]0{\rm ES}_{p_{1}}[X_{1}]\neq 0. For p1(0,1)p_{1}\in(0,1), the ratio-based contribution MCoES\rm MCoES with median-type MCoES\rm MCoES as the benchmark measure is defined by

ΔRmedMCoES𝒑[X1|X2,,Xn]=MCoESp1,𝒑[1][X1|X2,,Xn]MCoESp1,𝟏𝟐[X1|X2,,Xn]MCoESp1,𝟏𝟐[X1|X2,,Xn],\Delta^{\rm R-med}{\rm MCoES}_{\bm{p}}[X_{1}|X_{2},\dots,X_{n}]=\frac{{\rm MCoES}_{p_{1},\bm{p}_{[-1]}}[X_{1}|X_{2},\dots,X_{n}]-{\rm MCoES}_{p_{1},\frac{\bm{1}}{\bm{2}}}[X_{1}|X_{2},\dots,X_{n}]}{{\rm MCoES}_{p_{1},\frac{\bm{1}}{\bm{2}}}[X_{1}|X_{2},\dots,X_{n}]}, (4)

provided that MCoESp1,𝟏𝟐[X1|X2,,Xn]0{\rm MCoES}_{p_{1},\frac{\bm{1}}{\bm{2}}}[X_{1}|X_{2},\dots,X_{n}]\neq 0, where 𝐩[1]=(p2,,pn)(1/2,1)n1\bm{p}_{[-1]}=(p_{2},\dots,p_{n})\in(1/2,1)^{n-1} and 𝟏𝟐=(12,,12)n1\frac{\bm{1}}{\bm{2}}=\left(\frac{1}{2},\dots,\frac{1}{2}\right)\in\mathbb{R}^{n-1}.

Correspondingly, the ratio-based contribution MMME\rm MMME with unconditional mean excess as the benchmark measure is defined as follows.

Definition 3.3.

For 𝐩[1]=(p2,,pn)(0,1)n1{\bm{p}}_{[-1]}=(p_{2},\dots,p_{n})\in(0,1)^{n-1}, the risk contribution ratio measure of MMME\rm MMME is defined by

ΔRMMME𝒑[1][X1|X2,,Xn]=𝔼[(X1AX,p[1])+|j=2n{Xj>VaRpj[Xj]}]𝔼[(X1AX,p[1])+]𝔼[(X1AX,p[1])+],\Delta^{\rm R}\mathrm{MMME}_{\bm{p}_{[-1]}}[X_{1}|X_{2},\dots,X_{n}]=\frac{\mathbb{E}\left[\left(X_{1}-A_{X,p_{[-1]}}\right)_{+}\bigg{|}\bigcap\limits_{j=2}^{n}\left\{{X_{j}}>{\rm VaR}_{p_{j}}[X_{j}]\right\}\right]-\mathbb{E}\left[\left(X_{1}-A_{X,p_{[-1]}}\right)_{+}\right]}{\mathbb{E}[(X_{1}-A_{X,p_{[-1]}})_{+}]}, (5)

provided that 𝔼[(X1AX,p[1])+]0\mathbb{E}[(X_{1}-A_{X,p_{[-1]}})_{+}]\neq 0.

These multivariate risk contribution ratio measures are new compared with the ones introduced in Ortega-Jiménez et al. (2021). Next, we shall establish sufficient conditions for comparing these newly proposed measures for multivariate risk vectors. For two nn-dimensional portfolio of risks 𝑿\bm{X} and 𝒀\bm{Y}, this section established sufficient conditions for comparing the ratio-based risk contribution measures in terms of MCoVaR, MCoES, and MMME. The next result compares ΔRMCoVaR𝒑[X1|X2,,Xn]\Delta^{\rm R}{\rm MCoVaR}_{\bm{p}}[X_{1}|X_{2},\dots,X_{n}] and ΔRMCoVaR𝒑[Y1|Y2,,Yn]\Delta^{\rm R}{\rm MCoVaR}_{\bm{p}}[Y_{1}|Y_{2},\dots,Y_{n}] under some appropriate conditions imposed on marginal risks X1X_{1} and Y1Y_{1} and the dependence structure.

Theorem 3.4.

Let 𝐗=(X1,,Xn)\bm{X}=(X_{1},\dots,X_{n}) and 𝐘=(Y1,,Yn)\bm{Y}=(Y_{1},\dots,Y_{n}) be two nonnegative random vectors with the distribution functions FF and GG, marginal distributions F1,,FnF_{1},\dots,F_{n} and G1,,GnG_{1},\dots,G_{n}, and copulas CC and CC^{\prime}, respectively. Suppose that CwhrCC\leq_{\rm whr}C^{\prime}, and either (X2,,Xn)SIX1(X_{2},\dots,X_{n})\uparrow_{\rm SI}X_{1} or (Y2,,Yn)SIY1(Y_{2},\dots,Y_{n})\uparrow_{\rm SI}Y_{1} holds. Then, for 𝐩=(p1,,pn)(0,1)n\bm{p}=(p_{1},\dots,p_{n})\in(0,1)^{n}, X1Y1X_{1}\leq_{\star}Y_{1} implies that

ΔRMCoVaR𝒑[X1|X2,,Xn]ΔRMCoVaR𝒑[Y1|Y2,,Yn].\Delta^{\rm R}{\rm MCoVaR}_{\bm{p}}[X_{1}|X_{2},\dots,X_{n}]\leq\Delta^{\rm R}{\rm MCoVaR}_{\bm{p}}[Y_{1}|Y_{2},\dots,Y_{n}]. (6)

Recall that an increasing function h:[0,1][0,1]h:[0,1]\rightarrow[0,1] is said to be a distortion function if it satisfies h(0)=0h(0)=0 and h(1)=1h(1)=1. The following lemma is needed for proving the comparison results under other types of ratio-based contribution measures.

Lemma 3.5.

(Belzunce et al., 2012). Let XX and YY be two nonnegative random variables with distribution functions FXF_{X} and FYF_{Y}, respectively. Then,

  1. (i)

    XYX\leq_{\star}Y if and only if IA,B(X)IA,B(Y)I_{A,B}(X)\leq I_{A,B}(Y) for all distortion function A(t)A(t), B(t)B(t) and convex function AB1(t)A\circ B^{-1}(t), where

    IA,B(X)=01FX1(t)𝑑A(t)01FX1(t)𝑑B(t).I_{A,B}(X)=\frac{\int_{0}^{1}F_{X}^{-1}(t)dA(t)}{\int_{0}^{1}F_{X}^{-1}(t)dB(t)}. (7)
  2. (ii)

    XpsYX\leq_{\rm ps}Y if and only if IA,B(X)IA,B(Y)I_{A,B}(X)\leq I_{A,B}(Y) for all distortion function A(t)A(t), convex distortion function B(t)B(t) and convex function AB1(t)A\circ B^{-1}(t).

In the following theorem, sufficient conditions for comparison between ΔRMCoES𝒑[X1|X2,,Xn]\Delta^{\rm R}{\rm MCoES}_{\bm{p}}[X_{1}|X_{2},\dots,X_{n}] and ΔRMCoES𝒑[Y1|Y2,,Yn]\Delta^{\rm R}{\rm MCoES}_{\bm{p}}[Y_{1}|Y_{2},\dots,Y_{n}] are provided in terms of the expected proportional shortfall order.

Theorem 3.6.

Let 𝐗=(X1,,Xn)\bm{X}=(X_{1},\dots,X_{n}) and 𝐘=(Y1,,Yn)\bm{Y}=(Y_{1},\dots,Y_{n}) be two nonnegative random vectors with distribution functions FF and GG, marginal distributions F1,,FnF_{1},\dots,F_{n} and G1,,GnG_{1},\dots,G_{n}, and copulas CC and CC^{\prime}, respectively. Suppose that CwhrCC\leq_{\rm whr}C^{\prime}, and either (X2,,Xn)SIX1(X_{2},\dots,X_{n})\uparrow_{\rm SI}X_{1} or (Y2,,Yn)SIY1(Y_{2},\dots,Y_{n})\uparrow_{\rm SI}Y_{1} holds. Then, for 𝐩=(p1,,pn)(0,1)n\bm{p}=(p_{1},\dots,p_{n})\in(0,1)^{n}, X1psY1X_{1}\leq_{\rm ps}Y_{1} implies that

ΔRMCoES𝒑[X1|X2,,Xn]ΔRMCoES𝒑[Y1|Y2,,Yn].\Delta^{\rm R}{\rm MCoES}_{\bm{p}}[X_{1}|X_{2},\dots,X_{n}]\leq\Delta^{\rm R}{\rm MCoES}_{\bm{p}}[Y_{1}|Y_{2},\dots,Y_{n}]. (8)

Next, we provide an example to illustrate the findings in Theorems 3.4 and 3.6. It is known that if a random vector 𝑿\bm{X} satisfies MTP2{\rm MTP}_{2}, it then implies that 𝑿^iSIXi\hat{\bm{X}}_{i}\uparrow_{\rm SI}X_{i} holds for all i{1,,n}i\in\{1,\dots,n\}. An example of a copula satisfying MTP2{\rm MTP}_{2} is provided below. As per Müller & Scarsini (2005), the Archimedean copula CψC_{\psi} is MTP2{\rm MTP}_{2} if and only if (1)nψ(n)(-1)^{n}\psi^{(n)} is log-convex, where ψ(n)\psi^{(n)} denotes the nn-th derivative. Let Ψ(n):=ln((1)nψ(n))\Psi^{(n)}:={\rm ln}\left((-1)^{n}\psi^{(n)}\right). For the Gumbel copula, ψ(u)=(lnu)θ\psi(u)=(-{\rm ln}~u)^{\theta}, with n=3n=3, we have

Cθ(u1,u2,u3)=exp{[(lnu1)θ+(lnu2)θ+(lnu3)θ]1θ}.C_{\theta}(u_{1},u_{2},u_{3})={\rm exp}\left\{-\left[(-\rm ln~u_{1})^{\theta}+(-\rm ln~u_{2})^{\theta}+(-\rm ln~u_{3})^{\theta}\right]^{\frac{1}{\theta}}\right\}.

Fixing θ=2\theta=2, it follows that

Ψ(3)(u)=ln(64lnuu3).\Psi^{(3)}(u)={\rm ln}\left(\frac{6-4\cdot{\rm ln}~u}{u^{3}}\right).

Furthermore, taking the second derivative with respect to uu yields that

d2Ψ(3)(u)du2=12(lnu)240lnu+29u2(2lnu3)2>0,u(0,1),\frac{d^{2}\Psi^{(3)}(u)}{du^{2}}=\frac{12({\rm ln}~u)^{2}-40\cdot{\rm ln}~u+29}{u^{2}(2\cdot{\rm ln}~u-3)^{2}}>0,~u\in(0,1),

which implies that C2(u1,u2,u3)C_{2}(u_{1},u_{2},u_{3}) is MTP2{\rm MTP}_{2}. Based on this observation, the following two examples can be established.

Example 3.7.

Let 𝐗=(X1,X2,X3)\bm{X}=(X_{1},X_{2},X_{3}) and 𝐘=(Y1,Y2,Y3)\bm{Y}=(Y_{1},Y_{2},Y_{3}) are two random vectors with Gumbel copula CC and CC^{\prime}, respectively. By taking θ=2\theta=2, it satisfies (X2,X3)SIX1(X_{2},X_{3})\uparrow_{\rm SI}X_{1}. We denote by ZW(α,β)Z\sim W(\alpha,\beta) to state that ZZ has a Weibull distribution with scale parameter α>0\alpha>0 and shape parameter β>0\beta>0. Suppose X1W(1,5)X_{1}\sim W(1,5) and Y1W(1,4)Y_{1}\sim W(1,4), indicating X1Y1X_{1}\leq_{\star}Y_{1} (see Table 2.1 on p.102 of Belzunce et al. (2015)). As plotted in Figure 1, the result of Theorem 3.4 is illustrated.

Refer to caption
Figure 1: Plots of ΔRMCoVaR𝒑[X1|X2,X3]\Delta^{\rm R}{\rm MCoVaR}_{\bm{p}}[X_{1}|X_{2},X_{3}] and ΔRMCoVaR𝒑[Y1|Y2,Y3]\Delta^{\rm R}{\rm MCoVaR}_{\bm{p}}[Y_{1}|Y_{2},Y_{3}].
Example 3.8.

Let 𝐗=(X1,X2,X3)\bm{X}=(X_{1},X_{2},X_{3}) and 𝐘=(Y1,Y2,Y3)\bm{Y}=(Y_{1},Y_{2},Y_{3}) are two random vectors with Gumbel copula CC and CC^{\prime}, respectively. By taking θ=2\theta=2, it satisfies (X2,X3)SIX1(X_{2},X_{3})\uparrow_{\rm SI}X_{1}. We denote ZG(α,β)Z\sim G(\alpha,\beta) to represent that the random variable ZZ follows the Gamma distribution with shape parameter α>0\alpha>0 and scale parameter β>0\beta>0. Suppose X1G(3,1)X_{1}\sim G(3,1) and Y1G(1,1)Y_{1}\sim G(1,1), indicating X1Y1X_{1}\leq_{\star}Y_{1} (see Table 2.1 on p.102 of Belzunce et al. (2015)). As plotted in Figure 2, the result of Theorem 3.6 is illustrated.

Refer to caption
Figure 2: Plots of ΔRMCoES𝒑[X1|X2,X3]\Delta^{\rm R}{\rm MCoES}_{\bm{p}}[X_{1}|X_{2},X_{3}] and ΔRMCoES𝒑[Y1|Y2,Y3]\Delta^{\rm R}{\rm MCoES}_{\bm{p}}[Y_{1}|Y_{2},Y_{3}].

The next result compares ΔRMMME𝒑[1][X1|X2,,Xn]\Delta^{\rm R}\mathrm{MMME}_{\bm{p}_{[-1]}}[X_{1}|X_{2},\dots,X_{n}] and ΔRMMME𝒑[1][Y1|Y2,,Yn]\Delta^{\rm R}\mathrm{MMME}_{\bm{p}_{[-1]}}[Y_{1}|Y_{2},\dots,Y_{n}] under some appropriate conditions imposed on the dependence structure when 𝑿\bm{X} and 𝒀\bm{Y} have the same marginals.

Theorem 3.9.

Let 𝐗=(X1,,Xn)\bm{X}=(X_{1},\dots,X_{n}) and 𝐘=(Y1,,Yn)\bm{Y}=(Y_{1},\dots,Y_{n}) be two random vectors with the distribution functions FF and GG and same marginal distributions. If CwhrCC\leq_{\rm whr}C^{\prime}, then for all 𝐩[1]=(p2,,pn)(0,1)n1\bm{p}_{[-1]}=(p_{2},\dots,p_{n})\in(0,1)^{n-1}, we have

ΔRMMME𝒑[1][X1|X2,,Xn]ΔRMMME𝒑[1][Y1|Y2,,Yn].\Delta^{\rm R}\mathrm{MMME}_{\bm{p}_{[-1]}}[X_{1}|X_{2},\dots,X_{n}]\leq\Delta^{\rm R}\mathrm{MMME}_{\bm{p}_{[-1]}}[Y_{1}|Y_{2},\dots,Y_{n}]. (9)

In Theorem 3.9, we assumed that both vectors have the same marginal distributions. Under this assumption, the comparison of ΔRMMME\Delta^{\rm R}{\rm MMME} can be equivalent to the comparison of MMME, with conditions similar to Corollary 2 in Ortega-Jiménez et al. (2021). Therefore, the two measures exhibit consistent ordering under the copula structure, a property we refer to as dependence consistency.

The following example is provided to show the validity of Theorem 3.9.

Example 3.10.

Let 𝐗\bm{X} be an nn-dimensional random vector following the multivariate Gumbel Exponential distribution with its joint survival function given by

F¯𝝀(x1,,xn)=exp{IλIiIxi},xi0,i=1,,n,\overline{F}_{\bm{\lambda}}(x_{1},\dots,x_{n})={\rm exp}\left\{-\sum_{I}\lambda_{I}\prod_{i\in I}x_{i}\right\},~x_{i}\geq 0,~i=1,\dots,n,

where 𝛌={λI:I{1,,n},λI0,I}\bm{\lambda}=\{\lambda_{I}:I\subseteq\{1,\dots,n\},\lambda_{I}\geq 0,I\neq\emptyset\}. Let 𝐘\bm{Y} be another nn-dimensional random vector with a multivariate Gumbel Exponential survival distribution G¯𝛌\overline{G}_{{\bm{\lambda}}^{*}}. For n=3n=3, let λi=λi=10\lambda^{*}_{i}=\lambda_{i}=10, which implies Xi=stYiX_{i}\stackrel{{\scriptstyle\rm st}}{{=}}Y_{i} for i=1,2,3i=1,2,3. Additionally, set λ12=λ13=λ23=λ123=10\lambda^{*}_{12}=\lambda^{*}_{13}=\lambda^{*}_{23}=\lambda^{*}_{123}=10 and λ12=λ13=λ23=λ123=100\lambda_{12}=\lambda_{13}=\lambda_{23}=\lambda_{123}=100. Since 𝛌𝛌\bm{\lambda}\geq\bm{\lambda}^{*}, according to Khaledi & Kochar (2005), this implies 𝐗whr𝐘\bm{X}\leq_{\rm whr}\bm{Y} (or CwhrCC\leq_{\rm whr}C^{\prime}). The plots of ΔRMMME𝐩[1][X1|X2,X3]\Delta^{\rm R}{\rm MMME}_{\bm{p}_{[-1]}}[X_{1}|X_{2},X_{3}] and ΔRMMME𝐩[1][Y1|Y2,Y3]\Delta^{\rm R}{\rm MMME}_{\bm{p}_{[-1]}}[Y_{1}|Y_{2},Y_{3}] are displayed in Figure 3, which is consistent with the result of Theorem 3.9.

Refer to caption
Figure 3: Plots of ΔRMMME𝒑[1][X1|X2,X3]\Delta^{\rm R}{\rm MMME}_{\bm{p}_{[-1]}}[X_{1}|X_{2},X_{3}] and ΔRMMME𝒑[1][Y1|Y2,Y3]\Delta^{\rm R}{\rm MMME}_{\bm{p}_{[-1]}}[Y_{1}|Y_{2},Y_{3}].

Under an unconditional risk measure as benchmark, different copulas can be used to measure the risk contributions of two multivariate risk vectors, as the benchmark is unaffected by the copula. This is the reason why we can consider different copulas in the comparison results developed in Theorems 3.4, 3.6 and 3.9. However, when a median-type co-risk measure as the benchmark, which is also affected by the copula, using different copulas can make the comparison of risk contribution measures challenging. Therefore, to ensure the comparability of median-type risk contribution measures, the same copula will be adopted in the following discussions.

The next result establishes sufficient conditions for comparison between ΔRmedMCoVaR𝒑[X1|X2,,Xn]\Delta^{\rm R-med}{\rm MCoVaR}_{\bm{p}}[X_{1}|X_{2},\dots,X_{n}] and ΔRmedMCoVaR𝒑[Y1|Y2,,Yn]\Delta^{\rm R-med}{\rm MCoVaR}_{\bm{p}}[Y_{1}|Y_{2},\dots,Y_{n}] when X1X_{1} and Y1Y_{1} are ranked by the star order.

Theorem 3.11.

Let 𝐗=(X1,,Xn)\bm{X}=(X_{1},\dots,X_{n}) and 𝐘=(Y1,,Yn)\bm{Y}=(Y_{1},\dots,Y_{n}) be two nonnegative random vectors with distribution functions FF and GG, and marginal distributions are F1,,FnF_{1},\dots,F_{n} and G1,,GnG_{1},\dots,G_{n}, respectively. Suppose that 𝐗\bm{X} and 𝐘\bm{Y} have the same copula CC such that X1RTI(X2,,Xn)X_{1}\uparrow_{\rm RTI}(X_{2},\dots,X_{n}). For p1(0,1)p_{1}\in(0,1) and (p2,,pn)(1/2,1)n1(p_{2},\dots,p_{n})\in(1/2,1)^{n-1}, X1Y1X_{1}\leq_{\star}Y_{1} implies that

ΔRmedMCoVaR𝒑[X1|X2,,Xn]ΔRmedMCoVaR𝒑[Y1|Y2,,Yn].\Delta^{\rm R-med}{\rm MCoVaR}_{\bm{p}}[X_{1}|X_{2},\dots,X_{n}]\leq\Delta^{\rm R-med}{\rm MCoVaR}_{\bm{p}}[Y_{1}|Y_{2},\dots,Y_{n}]. (10)

It is worth addressing that the condition X1RTI(X2,,Xn)X_{1}\uparrow_{\rm RTI}(X_{2},\dots,X_{n}) indicates that the conditional probability (X1>x1X2>x2,,Xn>xn)\mathbb{P}(X_{1}>x_{1}\mid X_{2}>x_{2},\dots,X_{n}>x_{n}) increases with xjx_{j}, focusing on how X1X_{1} behaves given (X2,,Xn)(X_{2},\dots,X_{n}). Such condition can be implied from X1SI(X2,,Xn)X_{1}\uparrow_{\rm SI}(X_{2},\dots,X_{n}), which is very different from (X2,,Xn)SIX1(X_{2},\dots,X_{n})\uparrow_{\rm SI}X_{1}. In fact, the later condition (X2,,Xn)SIX1(X_{2},\dots,X_{n})\uparrow_{\rm SI}X_{1} means that the conditional distribution of (X2,,Xn|X1=x1)(X_{2},\dots,X_{n}|X_{1}=x_{1}) is stochastically increasing in x1x_{1}, showing how the random vector (X2,,Xn)(X_{2},\dots,X_{n}) shifts as X1X_{1} changes. These conditions describe different stochastic relationships and do not imply any interdeducible relationship.

In the following theorem, we establish sufficient conditions for comparing ΔRmedMCoES𝒑[X1|X2,,Xn]\Delta^{\rm R-med}{\rm MCoES}_{\bm{p}}[X_{1}|X_{2},\dots,X_{n}] and ΔRmedMCoES𝒑[Y1|Y2,,Yn]\Delta^{\rm R-med}{\rm MCoES}_{\bm{p}}[Y_{1}|Y_{2},\dots,Y_{n}] when X1X_{1} and Y1Y_{1} are ranked by the expected proportional shortfall order.

Theorem 3.12.

Let 𝐗=(X1,,Xn)\bm{X}=(X_{1},\dots,X_{n}) and 𝐘=(Y1,,Yn)\bm{Y}=(Y_{1},\dots,Y_{n}) be two nonnegative random vectors with distribution functions FF and GG, and marginal distributions are F1,,FnF_{1},\dots,F_{n} and G1,,GnG_{1},\dots,G_{n}, respectively. Suppose that 𝐗\bm{X} and 𝐘\bm{Y} have the same copula CC such that CC is MTP2{\rm MTP}_{2}. For p1(0,1)p_{1}\in(0,1) and (p2,,pn)(1/2,1)n1(p_{2},\dots,p_{n})\in(1/2,1)^{n-1}, X1psY1X_{1}\leq_{\rm ps}Y_{1} implies that

ΔRmedMCoES𝒑[X1|X2,,Xn]ΔRmedMCoES𝒑[Y1|Y2,,Yn].\Delta^{\rm R-med}{\rm MCoES}_{\bm{p}}[X_{1}|X_{2},\dots,X_{n}]\leq\Delta^{\rm R-med}{\rm MCoES}_{\bm{p}}[Y_{1}|Y_{2},\dots,Y_{n}]. (11)
Refer to caption
Figure 4: Subfigure A: plots of ΔRmedMCoVaR𝒑[X1|X2,X3]\Delta^{\rm R-med}{\rm MCoVaR}_{\bm{p}}[X_{1}|X_{2},X_{3}] and ΔRmedMCoVaR𝒑[Y1|Y2,Y3]\Delta^{\rm R-med}{\rm MCoVaR}_{\bm{p}}[Y_{1}|Y_{2},Y_{3}]. Subfigure B: plots of ΔRmedMCoES𝒑[X1|X2,X3]\Delta^{\rm R-med}{\rm MCoES}_{\bm{p}}[X_{1}|X_{2},X_{3}] and ΔRmedMCoES𝒑[Y1|Y2,Y3]\Delta^{\rm R-med}{\rm MCoES}_{\bm{p}}[Y_{1}|Y_{2},Y_{3}].

The following example illustrates the results of Theorems 3.11 and 3.12.

Example 3.13.

Let 𝐗=(X1,X2,X3)\bm{X}=(X_{1},X_{2},X_{3}) and 𝐘=(Y1,Y2,Y3)\bm{Y}=(Y_{1},Y_{2},Y_{3}) be two random vectors with the same Gumbel copula CC with θ=2\theta=2. Thus, CC is MTP2{\rm MTP}_{2} and X1RTI(X2,X3)X_{1}\uparrow_{\rm RTI}(X_{2},X_{3}). Suppose X1G(3,1)X_{1}\sim G(3,1) and Y1G(1,1)Y_{1}\sim G(1,1), which implies X1[ps]Y1X_{1}\leq_{\star{\rm[ps]}}Y_{1} (see Table 2.2 on p.102 of Belzunce et al. (2015)). The plots of ΔRmedMCoVaR\Delta^{\rm R-med}{\rm MCoVaR} and ΔRmedMCoES\Delta^{\rm R-med}{\rm MCoES} are shown in Figure 4, which agree with both of the results in Theorem 3.11 and Theorem 3.12.

4 An application in the cryptocurrency market

In this section, risk measures proposed in Section 3 are applied for cryptocurrency market dataset to quantify the relative spillover effects. We employ a static methodology to quantify the relative risk contributions of cryptocurrencies using the multivariate risk measures discussed in this paper. The static approach offers several distinct advantages that align with the goals of this study. Firstly, it delivers clear and interpretable results, allowing for a straightforward comparison of risk contributions among different assets. This clarity is essential for both theoretical validation and practical application, as it provides actionable insights for investors and regulators. Secondly, the static method is computationally efficient, enabling the analysis of large datasets and the application of complex risk measures without excessive resource demands. This efficiency is particularly valuable in the context of cryptocurrencies, where data volumes are substantial and market dynamics are intricate. Lastly, the static approach provides a stable framework for initial exploration and validation of new risk measurement tools, ensuring that the core properties of these tools can be assessed reliably before extending to more complex dynamic analyses.

The analysis utilizes three cryptocurrencies (CCs): Bitcoin (BTC), Ethereum (ETH), and Monero (XMR). The data contains daily closing prices in USD stemming from the Community Network Data provided by CoinMetrics.333See https://coinmetrics.io/. The sample includes N=3226N=3226 observations from 01/09/2015 to 30/06/2024 as CCs are traded every day, including weekends. For ease of our subsequent analysis, the prices are transformed in log-losses, that is,

Xi,t=100ln(pi,t/pi,t1),X_{i,t}=-100\cdot\ln\left(p_{i,t}/p_{i,t-1}\right),

where Xi,tX_{i,t} represents the percentage-based log-losses444Differing from the majority of economics and finance literature, this paper focuses on risk measurement based on the probability distributions of losses. Since we denote LtL_{t} as the stock index’s declining changing pattern, the right tail of the distribution of LtL_{t} represents extreme risk. on day tt with i{1,2,3}i\in\{1,2,3\} for BTC, ETH, and XRP and pi,tp_{i,t} denotes the closing price for cryptocurrency ii on day tt. For each cryptocurrency ii, NN observations (xi,1,,xi,N)(x_{i,1},\dots,x_{i,N}) are obtained. A statistical summary for these percentage-based log-loss samples is shown in Table 1, and their Spearman and Kendall correlation matrices are provided in Table 2. From Table 1, it can be observed that both BTC and XMR have relatively low mean losses, with BTC showing the smallest standard deviation, indicating a more stable performance. The elevated standard deviations observed for Ethereum and Monero relative to Bitcoin may reflect heightened exposure to volatility inherent in the cryptocurrency market, particularly during discrete events or periods of acute market stress. Ethereum, for instance, has demonstrated sensitivity to regulatory scrutiny and protocol upgrades (e.g., transitions to Ethereum 2.0), while Monero’s volatility has been amplified by debates over privacy regulations and network congestion. These idiosyncratic factors, coupled with broader market uncertainty, likely contribute to the pronounced fluctuations seen in both assets compared to Bitcoin. The results from Table 2 indicate that all the three cryptocurrencies enjoy positive dependence structure in losses, and the correlation between BTC and ETH is relatively stronger compared with the correlation between ETH and XMR.

Table 1: Statistical summary for log-losses of the cryptocurrencies
Cryptocurrency Mean Median Max Min Standard Deviation
BTC -0.174 -0.171 47.056 -22.405 3.705
ETH -0.243 -0.054 56.561 -30.062 5.527
XMR -0.183 -0.203 49.224 -59.634 5.625
Table 2: Correlation matrix for log-losses of cryptocurrencies
Panel A: Spearman correlation matrix
BTC ETH XMR
BTC 1.000 0.630 0.575
ETH 0.630 1.000 0.565
XMR 0.575 0.565 1.000
Panel B: Kendall correlation matrix
BTC ETH XMR
BTC 1.000 0.486 0.424
ETH 0.486 1.000 0.418
XMR 0.424 0.418 1.000

We use the method of inference function for margins (IFM) proposed in Joe (2005), which has been also widely applied by many research papers such as Shi & Yang (2018) and Zhu et al. (2023). Interested readers can refer to Joe (2005) for more efficiency properties of IFM. To calculate the co-risk measures introduced both in Sections 2 and 3, the following empirical procedure is adopted:

  • Step 1: Estimate the respective marginal model for each group of samples separately.

  • Step 2: Estimate the copula based on the pseudo-sample observations obtained from the parametric probability integral transformation on the samples.

  • Step 3: Calculate the respective risk measures.

4.1 Parameter estimation of the marginal distributions

The Generalized Pareto Distribution (GPD) is widely applied in the insurance and finance sectors as a probability distribution for modeling extreme values (Embrechts et al., 2013; Castillo & Hadi, 1997). Its distribution function is defined as follows:

F(x;ξ,β)={1(1+ξβx)1ξ,ξ01exp(xβ),ξ=0,F(x;\xi,\beta)=\left\{\begin{array}[]{l}1-\left(1+\frac{\xi}{\beta}x\right)^{-\frac{1}{\xi}},~~\xi\neq 0\\ 1-{\rm exp}\left(-\frac{x}{\beta}\right),~~~~~\xi=0\end{array}\right., (12)

where ξ\xi is the shape parameter and β\beta is the scale parameter. For each individual risk XiX_{i} with distribution function FiF_{i} and a confidential level α\alpha, the GPD serves as a suitable approximation for the excess distribution function (Xiαx|Xi>α)\mathbb{P}(X_{i}-\alpha\leq x|X_{i}>\alpha). Consequently, the following approximation can be utilized:

Fi(x)\displaystyle F_{i}(x) =\displaystyle= Fi(α)+(Xiαxα|Xi>α)(1Fi(α))\displaystyle F_{i}(\alpha)+\mathbb{P}(X_{i}-\alpha\leq x-\alpha|X_{i}>\alpha)\left(1-F_{i}(\alpha)\right)
\displaystyle\approx Fi(α)+F(xα;ξi,βi)(1Fi(α)),xα.\displaystyle F_{i}(\alpha)+F(x-\alpha;\xi_{i},\beta_{i})\left(1-F_{i}(\alpha)\right),~x\geq\alpha.

For t=1,,Tt=1,\dots,T, let xi,(1)xi,(T)x_{i,(1)}\leq\dots\leq x_{i,(T)} denote the order statistics of {xi,t}1tT\{x_{i,t}\}_{1\leq t\leq T}, i=1,2,3i=1,2,3. Setting threshold α\alpha, we apply the empirical distribution to fit the samples that are less than the α\alpha-quantile and utilize the GPD to fit the samples that are greater than the α\alpha-quantile. Using the Maximum Likelihood Estimation (MLE) method to estimate parameters ξi\xi_{i} and βi\beta_{i}, denote as ξ^i\hat{\xi}_{i} and β^i\hat{\beta}_{i}, the estimated marginal distribution FiF_{i} is as follows:

F^i(x)={t=1T𝐈(xi,tx)T,xxi,(αT)1(1α)exp(xxi,(αT)β^i),x>xi,(αT)\hat{F}_{i}(x)=\left\{\begin{array}[]{l}\frac{\sum_{t=1}^{T}{\rm{\bm{I}}}(x_{i,t}\leq x)}{T},~~~~~~~~~~~~~~~~~~~~~~~~x\leq x_{i,(\left\lceil\alpha T\right\rceil)}\\ 1-(1-\alpha)\exp\left(-\frac{x-x_{i,(\left\lceil\alpha T\right\rceil)}}{\hat{\beta}_{i}}\right),~~x>x_{i,(\left\lceil\alpha T\right\rceil)}\end{array}\right. (13)

when ξ^i=0\hat{\xi}_{i}=0,555k\left\lceil k\right\rceil denotes the ceiling of kk, i.e., rounding kk up to the nearest integer. and

F^i(x)={t=1T𝐈(xi,tx)T,xxi,(αT)1(1α)(1+ξ^iβ^i(xxi,(αT))),x>xi,(αT)\hat{F}_{i}(x)=\left\{\begin{array}[]{l}\frac{\sum_{t=1}^{T}{\rm{\bm{I}}}(x_{i,t}\leq x)}{T},~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~x\leq x_{i,(\left\lceil\alpha T\right\rceil)}\\ 1-(1-\alpha)\left(1+\frac{\hat{\xi}_{i}}{\hat{\beta}_{i}}(x-x_{i,(\left\lceil\alpha T\right\rceil)})\right),~~x>x_{i,(\left\lceil\alpha T\right\rceil)}\end{array}\right. (14)

when ξ^i0\hat{\xi}_{i}\neq 0.

We set the threshold α=90%\alpha=90\% (cf. Koliai, 2016), and then use MLE to estimate parameters ξi\xi_{i} and βi\beta_{i}, i=1,2,3i=1,2,3 of GPDs. MLE estimations ξi^\hat{\xi_{i}} and βi^\hat{\beta_{i}} of ξi\xi_{i} and βi\beta_{i} for three cryptocurrencies are shown in Table 3. The QQ plots based on the GPD and the normal distribution for all three cryptocurrencies are provided in Figure 5, which illustrates that the GPD provides significantly better fits for the tails of the data than the normal distribution.

Table 3: MLE results for the three cryptocurrencies
CC Parameter Estimation Std. Error
BTC ξ1\xi_{1} 0.083 0.051
β1\beta_{1} 2.841 0.214
ETH ξ2\xi_{2} 0.171 0.067
β2\beta_{2} 3.757 0.325
XMR ξ3\xi_{3} 0.136 0.056
β3\beta_{3} 3.612 0.283
Refer to caption
(a) QQ plot for BTC based on GPD.
Refer to caption
(b) QQ plot for ETH based on GPD.
Refer to caption
(c) QQ plot for XMR based on GPD.
Refer to caption
(d) QQ plot for BTC based on normal distribution.
Refer to caption
(e) QQ plot for ETH based on normal distribution.
Refer to caption
(f) QQ plot for XMR based on normal distribution.
Figure 5: QQ plots for all three cryptocurrencies.

It must be pointed out that GPD degenerates to Exponential distribution when ξ=0\xi=0, according to (12). Hence, the expressions of estimated marginal distributions depend on whether the values of ξi\xi_{i} are nonzero or not, for i=1,2,3i=1,2,3. Based on the method developed in Tsay (2014), we carry on testing ξi\xi_{i}\neq 0 by applying the principle that 0 is not in the 95% confidence interval [ξi^1.96×\hat{\xi_{i}}-1.96\times SE(ξi^\hat{\xi_{i}}), ξi^+1.96×\hat{\xi_{i}}+1.96\timesSE(ξi^\hat{\xi_{i}})] of the estimation ξi\xi_{i}, where SE(ξi^\hat{\xi_{i}}) denotes the standard error of ξi^\hat{\xi_{i}}.666The test can be also implemented for the case ξ1=0\xi_{1}=0. The results, which can be provided upon request, show that the computed values of various risk measures are very close, and thus we do not show them repeatedly here. As shown in Table 3, we find out that with a significant level 5%, the parameters ξ1\xi_{1} of BTC is not significantly nonzero. In the remainder of this section, we will use the parameters in Table 3 to carry out parameter estimations and the calculation of risk measures.

By employing the marginal distributions F^i\hat{F}_{i}’s given in (13) and (14), for each i=1,,ni=1,\ldots,n, we can convert observations {xi,k}1kN\left\{x_{i,k}\right\}_{1\leq k\leq N} into pseudo-samples {U^i,k}1kN\left\{\hat{U}_{i,k}\right\}_{1\leq k\leq N}, where

U^i,k=F^i(xi,k),1kN.\hat{U}_{i,k}=\hat{F}_{i}\left(x_{i,k}\right),\quad 1\leq k\leq N. (15)

Figure 6 shows the scatter plot of pseudo-samples for different pairs of cryptocurrencies.

Refer to caption
Refer to caption
Refer to caption
Figure 6: Scatter plots of LtL_{t} for three paired cryptocurrencies.

4.2 Parameter estimation of the mixed copula

As per Table 2, it can be noted that the correlation coefficients between cryptocurrencies pairs are different, indicating that the interdependence among cryptocurrencies is significantly asymmetric. Hence, the dependence structure between these cryptocurrencies cannot be characterized by symmetric copulas. Besides, Figure 6 shows that any pair of these three cryptocurrencies have a strong positive dependence at extreme values (for both of the left and right tails). Take these observations into consideration, we ought to use an asymmetric copula with non-zero left and right tail dependence coefficients to model the dependence structure between these cryptocurrencies. As a result, we employ a mixed copula model to characterize the dependence structure. The mixed copula model is widely used in the existing literature, like Cai & Wang (2014) and Zhu et al. (2023).

We use the mixed Copula model

CM(𝒖)=a1CGau(𝒖)+a2CGum(𝒖)+(1a1a2)CCla(𝒖),0a1,a21,a1+a21,𝒖[0,1]3\small C^{M}(\bm{u})=a_{1}C^{Gau}(\bm{u})+a_{2}C^{Gum}(\bm{u})+(1-a_{1}-a_{2})C^{Cla}(\bm{u}),\quad 0\leq a_{1},a_{2}\leq 1,\quad a_{1}+a_{2}\leq 1,\quad\bm{u}\in[0,1]^{3} (16)

as the dependency model, where the Gaussian copula is used to capture the correlation between variables, the Gumbel copula models upper tail dependence, and the Clayton copula models lower tail dependence. We estimate these parameters using command “fitCopula” in R package “copula”. There are seven parameters (ρ12M,ρ13M,ρ23M,θGM,θCM,a1,a2)\left(\rho_{12}^{M},\rho_{13}^{M},\rho_{23}^{M},\theta_{G}^{M},\theta_{C}^{M},a_{1},a_{2}\right) to be estimated, where ρ12M,ρ13M,ρ23M\rho_{12}^{M},\rho_{13}^{M},\rho_{23}^{M} are the correlation coefficients in the Gaussian copula CGauC^{Gau}, θGM\theta_{G}^{M} is the parameter in the Gumbel copula CGumC^{Gum}, θCM\theta_{C}^{M} is the parameter in the Clayton copula CClaC^{Cla}, and a1,a2a_{1},a_{2} and 1a1a21-a_{1}-a_{2}are the weights of the Gaussian copula, Gumbel copula, and Clayton copula, respectively. We performed maximum likelihood estimation on the pseudo-samples derived in (15) using seven different mixed Copula models and selected the most suitable model based on the Akaike Information Criterion (AIC) and Bayesian Information Criterion (BIC). The seven mixed Copula models are as follows:

  • Model 1: Gaussian copula CGauC^{Gau};

  • Model 2: Gumbel copula CGumC^{Gum};

  • Model 3: Clayton copula CClaC^{Cla} ;

  • Model 4: Gaussian-Gumbel mixed copula, formulated by setting 1a1a2=01-a_{1}-a_{2}=0 in (16);

  • Model 5: Gaussian-Clayton mixed copula, formulated by setting a2=0a_{2}=0 in (16);

  • Model 6: Gumbel-Clayton mixed copula, formulated by setting a1=0a_{1}=0 in (16);

  • Model 7: Gaussian-Gumbel-Clayton mixed copula, formulated as in (16).

The mixed copula model with the smallest AIC and BIC values is selected as the most suitable model. The estimated parameters of the seven mixed copula models are shown in Table 4. The results in Tabel 4 show that the mixed copula model with the smallest AIC and BIC values is Model 7, which is the Gaussian-Gumbel-Clayton mixed copula. Then, we use the estimated parameters of Model 7 to calculate the risk measures in the following analysis.

Table 4: Performance of various mixed copula models
Estimated Parameters AIC BIC
Model 1 ρ^12M=0.630\hat{\rho}_{12}^{M}=0.630, ρ^13M=0.560\hat{\rho}_{13}^{M}=0.560, ρ^23M=0.567\hat{\rho}_{23}^{M}=0.567 -3349.372 -3331.136
Model 2 θ^GM=1.727\hat{\theta}_{G}^{M}=1.727 -3911.606 -3905.527
Model 3 θ^CM=0.806\hat{\theta}_{C}^{M}=0.806 -2202.380 -2196.302
Model 4 ρ^12M=0.140\hat{\rho}_{12}^{M}=0.140, ρ^13M=0.095\hat{\rho}_{13}^{M}=0.095, ρ^23M=0.076\hat{\rho}_{23}^{M}=0.076, -4603.278 -4566.805
θ^GM=2.650\hat{\theta}_{G}^{M}=2.650, a1=0.314a_{1}=0.314, a2=0.686a_{2}=0.686
Model 5 ρ^12M=0.5675\hat{\rho}_{12}^{M}=0.5675, ρ^13M=0.5288\hat{\rho}_{13}^{M}=0.5288, ρ^23M=0.4962\hat{\rho}_{23}^{M}=0.4962 -3608.101 -3571.629
θ^GM=7.7034\hat{\theta}_{G}^{M}=7.7034, a1=0.8287a_{1}=0.8287, a2=0a_{2}=0
Model 6 θ^GM=2.559\hat{\theta}_{G}^{M}=2.559, θ^CM=0.005\hat{\theta}_{C}^{M}=0.005 -4595.905 -4571.591
a1=0a_{1}=0, a2=0.2770a_{2}=0.2770
Model 7 ρ^12M=0.104\hat{\rho}_{12}^{M}=0.104, ρ^13M=0.061\hat{\rho}_{13}^{M}=0.061, ρ^23M=0.048\hat{\rho}_{23}^{M}=0.048, -4619.705 -4571.076
θ^GM=2.583\hat{\theta}_{G}^{M}=2.583, θ^CM=9.465\hat{\theta}_{C}^{M}=9.465, a1=0.299a_{1}=0.299, a2=0.670a_{2}=0.670

4.3 Empirical results

Based on the respective marginal distributions and the selected copula, a range of risk measures are provided in Table 5, where we take the confidence levels p1=p2=p3=0.95p_{1}=p_{2}=p_{3}=0.95777The market capitalization ratio among BTC, ETH, and XMR is approximately 9:3:1, considering the fluctuations in total market capitalization over time. We use this ratio as the reference weight for the calculations of MMME. Taking the MMME value of BTC as an example, the weight vector is set as a=(0,0.75,0.25)a=(0,0.75,0.25).. More collected values under the settings of p1=p2=p3=0.975p_{1}=p_{2}=p_{3}=0.975 and p1=p2=p3=0.99p_{1}=p_{2}=p_{3}=0.99 can be found in Appendix B.4. The following observations can be noted888The specific definition s of ΔMCoVaR\Delta\mathrm{MCoVaR} and ΔmedMCoVaR\Delta^{\mathrm{med}}\mathrm{MCoVaR} can be found in the appendix B.1.:

Table 5: Values of some systemic risk measures of the three cryptocurrencies (p1=p2=p3=0.95p_{1}=p_{2}=p_{3}=0.95).
VaR-based BTC ETH XMR
VaR 5.727 7.892 8.084
MCoVaR 17.151 26.614 24.552
ΔMCoVaR\Delta\mathrm{MCoVaR} 11.424 18.722 16.468
ΔRMCoVaR\Delta^{\mathrm{R}}\mathrm{MCoVaR} 1.995 2.372 2.037
ΔmedMCoVaR\Delta^{\mathrm{med}}\mathrm{MCoVaR} 8.951 15.140 13.202
ΔRmedMCoVaR\Delta^{\mathrm{R-med}}\mathrm{MCoVaR} 1.092 1.320 1.163
ES-based BTC ETH XMR
ES 8.973 12.915 12.617
MCoES 21.427 35.450 31.652
ΔMCoES\Delta\mathrm{MCoES} 12.454 22.535 19.035
ΔRMCoES\Delta^{\mathrm{R}}\mathrm{MCoES} 1.388 1.745 1.509
ΔmedMCoES\Delta^{\mathrm{med}}\mathrm{MCoES} 9.740 18.194 15.242
ΔRmedMCoES\Delta^{\mathrm{R-med}}\mathrm{MCoES} 0.833 1.054 0.929
MMME-based BTC ETH XMR
MMME 2.166 7.539 6.798
ΔMMME\Delta\mathrm{MMME} 2.082 7.166 6.457
ΔRMMME\Delta^{\mathrm{R}}\mathrm{MMME} 24.678 19.240 18.940
  1. (i)

    Conditional risk measures, such as MCoVaR, MCoES and MMME, consistently surpass their unconditional counterparts, namely VaR and ES. This discrepancy underscores the heightened potential risk of individual assets when systemic risk is taken into account. These systemic risk measures capture the essence of how the performance of interconnected assets during periods of market extremity can amplify the risk profile of individual assets, thereby highlighting the risk co-movement effect. The implications are profound: there exists a pronounced risk interaction in the currency market, characterized by robust correlations among various currencies. Relying on unconditional risk measures in isolation may lead to an underestimation of the true risk exposure.

  2. (ii)

    Under majority risk measures, ETH emerges with the highest risk profile, while BTC exhibits a comparatively lower risk level, with XMR occupying an intermediate position. This indicates that within the cryptocurrency market, ETH is more susceptible to systemic risk impacts, marked by notably higher price volatility and risk exposure in comparison to the other two digital assets. Conversely, BTC displays relative stability, with a lower risk exposure and spill-over effects, underscoring its status as the cryptocurrency with the largest market share and its perceived stability.

  3. (iii)

    Across a spectrum of risk measures, the risk ranking among the three currencies exhibits a noticeable consistency. This uniformity in risk perception across different cryptocurrencies indicates a stable market assessment of risk. It implies that within the currency market, relative measures such as ratio-based risk contribution measures (ΔR\Delta^{\rm R} and ΔRmed\Delta^{\rm R-med}) can effectively capture the systemic risk’s relative change. These measures offer a nuanced approach beyond the reliance on absolute risk metrics like MCoVaR, MCoES and MMME.

  4. (iv)

    For the difference-based risk contribution measures (Δ\Delta and Δmed\Delta^{\mathrm{med}}), the indicators derived from ES surpass those predicated on VaR. Conversely, for the ratio-based risk contribution measures (ΔR\Delta^{\mathrm{R}} and ΔRmed\Delta^{\mathrm{R-med}}), the scenario inverts, with VaR-based measures taking precedence. This suggests that ES-based measures confer a higher significance to individual assets’ role in the distribution of systemic risk, while VaR-based measures accentuate the individual assets’ proportional contribution to systemic risk as a whole. The disparity underscores the imperative to strike a balance in the selection of risk metrics, contingent upon the goals of risk management and the prevailing market conditions.

  5. (v)

    The ratio-based risk contribution measures (ΔR\Delta^{\rm R} and ΔRmed\Delta^{\rm R-med}) offer a advantage over other risk metrics by virtue of their capacity to articulate the systemic risk’s relative co-movement effect on individual assets via relative ratios. This methodology provides clarity on the comparative risk contributions of various assets within systemic risk frameworks. It affords a perspective that not only uncovers potential market extreme losses but also equips investors with a deeper comprehension and management of relative risk exposures across diverse market conditions. This is in contrast to the sole assessment of an asset’s absolute risk level.

5 Conclusion

Systemic risk plays a significant role in financial markets and portfolio management. This article delves into new tools for quantifying and analyzing systemic risk, with a specific emphasis on the absolute and relative spillover effects induced by systemic risk. Some comparison results are conducted based on these proposed measures for two different sets of multivariate vectors with the same or different copulas. The theoretical findings have been validated through numerical examples, demonstrating the applicability and effectiveness of the proposed measures. Furthermore, we implement these measures as well as some known ones to quantify the interaction effect in cryptocurrency market by considering three typical cryptocurrencies.

Acknowledgements

The authors are very grateful for the helpful comments and suggestions from two anonymous reviewers, which have improved the presentation of this manuscript. Limin Wen thanks the financial support from the National Natural Science Foundation of China (No.72263019). Junxue Li thanks the Graduate Innovation Fund Project of Jiangxi Provincial Department of Education (No. YC2024-B089). Yiying Zhang acknowledges the financial support from the GuangDong Basic and Applied Basic Research Foundation (No. 2023A1515011806), and Shenzhen Science and Technology Program (No. JCYJ20230807093312026).

Disclosure statements

No potential competing interest was reported by the authors.

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Appendix A Proof of the main results

For a random variable XX with distribution function FXF_{X}, if hh is continuous, then h(F¯X(x))=hF¯X(x)h\left(\overline{F}_{X}(x)\right)=h\circ\overline{F}_{X}(x) applied to the tail function F¯X(x)=1FX(x)\overline{F}_{X}(x)=1-F_{X}(x) results in a new tail function. This new tail function corresponds to a random variable XhX_{h}, which is derived from XX by applying the distortion function hh. The following lemma derives the distorted function of X1X_{1} given that the remaining entities are in distress, as discussed in Sordo et al. (2015) and Ortega-Jiménez et al. (2021).

Lemma A.1.

Let 𝐗=(X1,,Xn)\bm{X}=(X_{1},\dots,X_{n}) be an nn-dimensional random vector with copula CC, joint distribution function FF and marginal distributions F1,,FnF_{1},\dots,F_{n}. Assume that (X2,,Xn)SIX1(X_{2},\dots,X_{n})\uparrow_{\rm SI}X_{1}. Then, for (p2,,pn)(0,1)n1(p_{2},\dots,p_{n})\in(0,1)^{n-1}, the conditional random variable [X1|j=2n{Xj>VaRpj[Xj]}]\left[X_{1}\bigg{|}\bigcap\limits_{j=2}^{n}\left\{{X_{j}}>{\rm VaR}_{p_{j}}[X_{j}]\right\}\right] is a distorted random variable induced from X1X_{1} by the concave distortion function

h𝒑(t)=C¯(1t,p2,,pn)C¯(0,p2,,pn),t[0,1].h_{\bm{p}}(t)=\frac{\overline{C}(1-t,p_{2},\dots,p_{n})}{\overline{C}(0,p_{2},\dots,p_{n})},~~t\in[0,1]. (17)

A.1 Proof of Theorem 3.4

Proof.

Let Xh,𝒑X_{h,\bm{p}} be defined as the conditional random variable [X1|j=2n{Xj>VaRpj[Xj]}]\left[X_{1}\bigg{|}\bigcap\limits_{j=2}^{n}\left\{{X_{j}}>{\rm VaR}_{p_{j}}[X_{j}]\right\}\right] for 𝒑=(p1,,pn)(0,1)n\bm{p}=(p_{1},...,p_{n})\in(0,1)^{n}. Assuming Xh,𝒑FXh,𝒑X_{h,\bm{p}}\sim F_{X_{h,\bm{p}}}, it follows that

MCoVaR𝒑[X1|X2,,Xn]=FXh,𝒑1(p1).{\rm MCoVaR}_{\bm{p}}[X_{1}|X_{2},...,X_{n}]=F_{X_{h,\bm{p}}}^{-1}(p_{1}).

By applying Lemma A.1, we find that FXh,𝒑(x)=1h𝒑(F¯1(x))F_{X_{h,{\bm{p}}}}(x)=1-h_{\bm{p}}\left(\overline{F}_{1}(x)\right), where h𝒑(t)h_{\bm{p}}(t) is given by

h𝒑(t)=C¯(1t,p2,,pn)C¯(0,p2,,pn).h_{\bm{p}}(t)=\frac{\overline{C}(1-t,p_{2},...,p_{n})}{\overline{C}(0,p_{2},...,p_{n})}.

Setting FXh,𝒑(x)=1h𝒑(F¯1(x))=p1F_{X_{h,{\bm{p}}}}(x)=1-h_{\bm{p}}(\overline{F}_{1}(x))=p_{1}, we obtain FXh,𝒑1(p1)=F11(1h𝒑1(1p1))F_{X_{h,{\bm{p}}}}^{-1}(p_{1})=F_{1}^{-1}\left(1-h_{\bm{p}}^{-1}(1-p_{1})\right). Hence, we have

ΔRMCoVaR𝒑[X1|X2,,Xn]=F11(1h𝒑1(1p1))F11(p1)1.\Delta^{\rm R}{\rm MCoVaR}_{\bm{p}}[X_{1}|X_{2},\dots,X_{n}]=\frac{F_{1}^{-1}\left(1-h_{\bm{p}}^{-1}(1-p_{1})\right)}{F_{1}^{-1}(p_{1})}-1.

Similarly,

ΔRMCoVaR𝒑[Y1|Y2,,Yn]=G11(1h𝒑1(1p1))G11(p1)1,\Delta^{\rm R}{\rm MCoVaR}_{\bm{p}}[Y_{1}|Y_{2},\dots,Y_{n}]=\frac{G_{1}^{-1}\left(1-{h^{\prime}}_{\bm{p}}^{-1}(1-p_{1})\right)}{G_{1}^{-1}(p_{1})}-1,

where h𝒑(t)=C¯(1t,p2,,pn)C¯(0,p2,,pn)h^{\prime}_{\bm{p}}(t)=\frac{\overline{C}^{\prime}(1-t,p_{2},\dots,p_{n})}{\overline{C}^{\prime}(0,p_{2},\dots,p_{n})}. Without loss of generality, we assume that (X2,..,Xn)SIX1(X_{2},..,X_{n})\uparrow_{\rm SI}X_{1}. The proof for the other case is similar. Lemma A.1 indicates that h𝒑h_{\bm{p}} is a concave distortion function, satisfying h𝒑(t)th_{\bm{p}}(t)\geq t, which leads to t1h𝒑1(1t)t\leq 1-h_{\bm{p}}^{-1}(1-t). By applying X1Y1X_{1}\leq_{\star}Y_{1}, it follows that

F11(1h𝒑1(1p1))F11(p1)G11(1h𝒑1(1p1))G11(p1).\frac{F_{1}^{-1}\left(1-h_{\bm{p}}^{-1}(1-p_{1})\right)}{F_{1}^{-1}(p_{1})}\leq\frac{G_{1}^{-1}\left(1-h_{\bm{p}}^{-1}(1-p_{1})\right)}{G_{1}^{-1}(p_{1})}.

Utilizing the definition of CwhrCC\leq_{\rm whr}C^{\prime}, we directly obtain that

C¯(0,p2,,pn)C¯(0,p2,,pn)C¯(1t,p2,,pn)C¯(1t,p2,,pn),\frac{\overline{C}^{\prime}(0,p_{2},\dots,p_{n})}{\overline{C}(0,p_{2},\dots,p_{n})}\leq\frac{\overline{C}^{\prime}(1-t,p_{2},\dots,p_{n})}{\overline{C}(1-t,p_{2},\dots,p_{n})},

which leads to h𝒑(t)h𝒑(t)h_{\bm{p}}(t)\leq h^{\prime}_{\bm{p}}(t) for all t(0,1)t\in(0,1). Hence, G11(1h𝒑1(1p1))G11(1h𝒑1(1p1))G_{1}^{-1}\left(1-h_{\bm{p}}^{-1}(1-p_{1})\right)\leq G_{1}^{-1}\left(1-{h^{\prime}}_{\bm{p}}^{-1}(1-p_{1})\right), confirming that (6) is valid. This completes the proof.  

A.2 Proof of Theorem 3.6

Proof.

Given Definition 3.2 and the proof of Theorem 3.4, the MCoES can be reformulated as:

MCoES𝒑[X1|X2,,Xn]=11p1p11F11(1h𝒑1(1t))𝑑t=01F11(s)𝑑A𝒑(s),{\rm MCoES}_{\bm{p}}[X_{1}|X_{2},...,X_{n}]=\frac{1}{1-p_{1}}{\int_{p_{1}}^{1}F_{1}^{-1}\left(1-h_{\bm{p}}^{-1}(1-t)\right)dt}=\int_{0}^{1}F_{1}^{-1}(s)dA_{\bm{p}}(s),

where A𝒑(s)A_{\bm{p}}(s) is specified as

A𝒑(s)={0,s1h𝒑1(1p1),111p1C¯(s,p2,,pn)C¯(0,p2,,pn),s>1h𝒑1(1p1),A_{\bm{p}}(s)=\begin{cases}0,&s\leq 1-h_{\bm{p}}^{-1}(1-p_{1}),\\ 1-\frac{1}{1-p_{1}}\cdot\frac{\overline{C}(s,p_{2},...,p_{n})}{\overline{C}(0,p_{2},...,p_{n})},&s>1-h_{\bm{p}}^{-1}(1-p_{1}),\end{cases}

for 𝒑(0,1)n\bm{p}\in(0,1)^{n}. Hence, it follows that

ΔRMCoES𝒑[X1|X2,,Xn]=01F11(s)𝑑A𝒑(s)01F11(s)𝑑B(s)1,\Delta^{\rm R}{\rm MCoES}_{\bm{p}}[X_{1}|X_{2},\dots,X_{n}]=\frac{\int_{0}^{1}F_{1}^{-1}(s)dA_{\bm{p}}(s)}{\int_{0}^{1}F_{1}^{-1}(s)dB(s)}-1,

where

A𝒑(s)={0,s1h𝒑1(1p1),111p1C¯(s,p2,,pn)C¯(0,p2,,pn),s>1h𝒑1(1p1),A_{\bm{p}}(s)=\begin{cases}0,&s\leq 1-h_{\bm{p}}^{-1}(1-p_{1}),\\ 1-\frac{1}{1-p_{1}}\cdot\frac{\overline{C}(s,p_{2},\dots,p_{n})}{\overline{C}(0,p_{2},\dots,p_{n})},&s>1-h_{\bm{p}}^{-1}(1-p_{1}),\end{cases}

for 𝒑(0,1)n\bm{p}\in(0,1)^{n}, with h𝒑(t)=C¯(1t,p2,,pn)C¯(0,p2,,pn)h_{\bm{p}}(t)=\frac{\overline{C}(1-t,p_{2},\dots,p_{n})}{\overline{C}(0,p_{2},\dots,p_{n})} and B(s)=max{0,sp11p1}B(s)={\rm max}\left\{0,\frac{s-p_{1}}{1-p_{1}}\right\}. Similarly,

ΔRMCoES𝒑[Y1|Y2,,Yn]=01G11(s)𝑑A𝒑(s)01G11(s)𝑑B(s)1,\Delta^{\rm R}{\rm MCoES}_{\bm{p}}[Y_{1}|Y_{2},\dots,Y_{n}]=\frac{\int_{0}^{1}G_{1}^{-1}(s)dA^{\prime}_{\bm{p}}(s)}{\int_{0}^{1}G_{1}^{-1}(s)dB(s)}-1,

where

A𝒑(s)={0,s1h𝒑1(1p1),111p1C¯(s,p2,,pn)C¯(0,p2,,pn),s>1h𝒑1(1p1),A^{\prime}_{\bm{p}}(s)=\begin{cases}0,&s\leq 1-{h}_{\bm{p}}^{\prime-1}(1-p_{1}),\\ 1-\frac{1}{1-p_{1}}\cdot\frac{\overline{C}^{\prime}(s,p_{2},\dots,p_{n})}{\overline{C}^{\prime}(0,p_{2},\dots,p_{n})},&s>1-{h}_{\bm{p}}^{\prime-1}(1-p_{1}),\end{cases}

for 𝒑(0,1)n\bm{p}\in(0,1)^{n}, with h𝒑(t)=C¯(1t,p2,,pn)C¯(0,p2,,pn)h^{\prime}_{\bm{p}}(t)=\frac{\overline{C}^{\prime}(1-t,p_{2},\dots,p_{n})}{\overline{C}^{\prime}(0,p_{2},\dots,p_{n})}. Since (X2,,Xn)SIX1(X_{2},\dots,X_{n})\uparrow_{\rm SI}X_{1}, it can be inferred from Lemma A.1 that A𝒑(s)A_{\bm{p}}(s) is convex, and thus A𝒑(B1(s))A_{\bm{p}}\left(B^{-1}(s)\right) is also convex in ss. By Lemma 3.5, it follows that

01F11(s)𝑑A𝒑(s)01F11(s)𝑑B(s)101G11(s)𝑑A𝒑(s)01G11(s)𝑑B(s)1.\frac{\int_{0}^{1}F_{1}^{-1}(s)dA_{\bm{p}}(s)}{\int_{0}^{1}F_{1}^{-1}(s)dB(s)}-1\leq\frac{\int_{0}^{1}G_{1}^{-1}(s)dA_{\bm{p}}(s)}{\int_{0}^{1}G_{1}^{-1}(s)dB(s)}-1.

Besides, the condition CwhrCC\leq_{\rm whr}C^{\prime} ensures that h𝒑(t)h𝒑(t)h_{\bm{p}}(t)\leq h^{\prime}_{\bm{p}}(t), which further implies A𝒑(s)A𝒑(s)A_{\bm{p}}(s)\geq A^{\prime}_{\bm{p}}(s). Using integration by parts, we obtain

01G11(s)𝑑A𝒑(s)01G11(s)𝑑A𝒑(s)=01(A𝒑(s)A𝒑(s))𝑑G11(s)0.\int_{0}^{1}G_{1}^{-1}(s)dA_{\bm{p}}(s)-\int_{0}^{1}G_{1}^{-1}(s)dA^{\prime}_{\bm{p}}(s)=\int_{0}^{1}\left(A_{\bm{p}}(s)-A^{\prime}_{\bm{p}}(s)\right)dG_{1}^{-1}(s)\leq 0.

which establishes (8) and completes the proof.  

A.3 Proof of Theorem 3.9

Proof.

Define Ui=Fi(Xi)U_{i}=F_{i}(X_{i}) for i=1,,ni=1,...,n. The MMME is then expressed as

MMME𝒑[1][X1|X2,,Xn]=𝔼[(X1AX,𝒑[1])+|j=2n{Xj>VaRpj[Xj]}]\displaystyle{\rm MMME}_{\bm{p}_{[-1]}}[X_{1}|X_{2},...,X_{n}]=\mathbb{E}\left[(X_{1}-A_{X,\bm{p}_{[-1]}})_{+}\bigg{|}\bigcap\limits_{j=2}^{n}\left\{{X_{j}}>{\rm VaR}_{p_{j}}[X_{j}]\right\}\right]
=\displaystyle= AX,𝒑[1](1FU1|j=2nUj>pj(F1(t)))𝑑t=F1(AX,𝒑[1])1(1FU1|j=2nUj>pj(u))𝑑F11(u)\displaystyle\int_{A_{X,\bm{p}_{[-1]}}}^{\infty}\left(1-F_{U_{1}|\bigcap\limits_{j=2}^{n}U_{j}>p_{j}}(F_{1}(t))\right)dt=\int_{F_{1}\left(A_{X,\bm{p}_{[-1]}}\right)}^{1}\left(1-F_{U_{1}|\bigcap\limits_{j=2}^{n}U_{j}>p_{j}}(u)\right)dF_{1}^{-1}(u)
=\displaystyle= F1(AX,𝒑[1])1(F11(u)AX,𝒑[1])𝑑h¯𝒑(u),\displaystyle\int_{F_{1}\left(A_{X,\bm{p}_{[-1]}}\right)}^{1}\left(F_{1}^{-1}(u)-A_{X,\bm{p}_{[-1]}}\right)d\overline{h}_{\bm{p}}(u),

where h¯𝒑(t)=1h𝒑(1t)\overline{h}_{\bm{p}}(t)=1-h_{\bm{p}}(1-t). We have

ΔRMMME𝒑[1][X1|X2,,Xn]=F1(AX,𝒑[1])1(F11(u)AX,𝒑[1])𝑑h¯𝒑(u)F1(AX,𝒑[1])1(F11(u)AX,𝒑[1])𝑑u1,\Delta^{\rm R}\mathrm{MMME}_{\bm{p}_{[-1]}}[X_{1}|X_{2},\dots,X_{n}]=\frac{\int_{F_{1}\left(A_{X,\bm{p}_{[-1]}}\right)}^{1}\left(F_{1}^{-1}(u)-A_{X,\bm{p}_{[-1]}}\right)d\overline{h}_{\bm{p}}(u)}{\int_{F_{1}\left(A_{X,\bm{p}_{[-1]}}\right)}^{1}\left(F_{1}^{-1}(u)-A_{X,\bm{p}_{[-1]}}\right)du}-1,

where h𝒑(t)=C¯(1t,p2,,pn)C¯(0,p2,,pn)h_{\bm{p}}(t)=\frac{\overline{C}(1-t,p_{2},\dots,p_{n})}{\overline{C}(0,p_{2},\dots,p_{n})} and h¯𝒑(t)=1h𝒑(1t)\overline{h}_{\bm{p}}(t)=1-h_{\bm{p}}(1-t). Similarly,

ΔRMMME𝒑[1][Y1|Y2,,Yn]=G1(AY,𝒑[1])1(G11(u)AY,𝒑[1])𝑑h¯𝒑(u)G1(AY,𝒑[1])1(G11(u)AY,𝒑[1])𝑑u1,\Delta^{\rm R}\mathrm{MMME}_{\bm{p}_{[-1]}}[Y_{1}|Y_{2},\dots,Y_{n}]=\frac{\int_{G_{1}\left(A_{Y,\bm{p}_{[-1]}}\right)}^{1}\left(G_{1}^{-1}(u)-A_{Y,\bm{p}_{[-1]}}\right)d\overline{h}^{\prime}_{\bm{p}}(u)}{\int_{G_{1}\left(A_{Y,\bm{p}_{[-1]}}\right)}^{1}\left(G_{1}^{-1}(u)-A_{Y,\bm{p}_{[-1]}}\right)du}-1,

where h𝒑(t)=C¯(1t,p2,,pn)C¯(0,p2,,pn)h^{\prime}_{\bm{p}}(t)=\frac{\overline{C}^{\prime}(1-t,p_{2},\dots,p_{n})}{\overline{C}^{\prime}(0,p_{2},\dots,p_{n})} and h¯𝒑(t)=1h𝒑(1t)\overline{h}^{\prime}_{\bm{p}}(t)=1-h^{\prime}_{\bm{p}}(1-t). Given that Xi=stYiX_{i}=_{\rm st}Y_{i}, it suffices to demonstrate that

F1(AX,𝒑[1])1(F11(u)AX,𝒑[1])𝑑h¯𝒑(u)F1(AX,𝒑[1])1(F11(u)AX,𝒑[1])𝑑h¯𝒑(u),\int_{F_{1}\left(A_{X,\bm{p}_{[-1]}}\right)}^{1}\left(F_{1}^{-1}(u)-A_{X,\bm{p}_{[-1]}}\right)d\overline{h}_{\bm{p}}(u)\leq\int_{F_{1}\left(A_{X,\bm{p}_{[-1]}}\right)}^{1}\left(F_{1}^{-1}(u)-A_{X,\bm{p}_{[-1]}}\right)d\overline{h}^{\prime}_{\bm{p}}(u),

which follows from CwhrCC\leq_{\rm whr}C^{\prime}. This completes the proof.  

A.4 Proof of Theorem 3.11

Proof.

By the proof of Theorem 3.4, it follows that

ΔRmedMCoVaR𝒑(X1|X2,,Xn)=F11(1h𝒑[1]1(1p1))F11(1h𝟏𝟐1(1p1))1,\Delta^{\rm R-med}{\rm MCoVaR}_{\bm{p}}(X_{1}|X_{2},\dots,X_{n})=\frac{F_{1}^{-1}\left(1-h_{\bm{p}_{[-1]}}^{-1}(1-p_{1})\right)}{F_{1}^{-1}\left(1-h_{\frac{\bm{1}}{\bm{2}}}^{-1}(1-p_{1})\right)}-1,

where h𝒑^(t)=C¯(1t,p2,,pn)C¯(0,p2,,pn)h_{\hat{\bm{p}}}(t)=\frac{\overline{C}(1-t,p_{2},\dots,p_{n})}{\overline{C}(0,p_{2},\dots,p_{n})} with 𝒑^={𝒑[1],𝟏𝟐}\hat{\bm{p}}=\left\{\bm{p}_{[-1]},\frac{\bm{1}}{\bm{2}}\right\}, 𝒑[1]=(p2,,pn)(1/2,1)n1\bm{p}_{[-1]}=(p_{2},\dots,p_{n})\in(1/2,1)^{n-1} and 𝟏𝟐=(12,,12)n1\frac{\bm{1}}{\bm{2}}=\left(\frac{1}{2},\dots,\frac{1}{2}\right)\in\mathbb{R}^{n-1}. Similarly,

ΔRmedMCoVaR𝒑[Y1|Y2,,Yn]=G11(1h𝒑[1]1(1p1))G11(1h𝟏𝟐1(1p1))1.\Delta^{\rm R-med}{\rm MCoVaR}_{\bm{p}}[Y_{1}|Y_{2},\dots,Y_{n}]=\frac{G_{1}^{-1}\left(1-h_{\bm{p}_{[-1]}}^{-1}(1-p_{1})\right)}{G_{1}^{-1}\left(1-h_{\frac{\bm{1}}{\bm{2}}}^{-1}(1-p_{1})\right)}-1.

Given that X1RTI(X2,,Xn)X_{1}\uparrow_{\rm RTI}(X_{2},\dots,X_{n}), it follows that h𝒑[1](t)h𝟏𝟐(t)h_{\bm{p}_{[-1]}}(t)\geq h_{\frac{\bm{1}}{\bm{2}}}(t), which implies 1h𝟏𝟐1(1p1)1h𝒑[1]1(1p1)1-h_{\frac{\bm{1}}{\bm{2}}}^{-1}(1-p_{1})\leq 1-h_{\bm{p}_{[-1]}}^{-1}(1-p_{1}). Hence, X1Y1X_{1}\leq_{\star}Y_{1} implies that

G11(1h𝟏𝟐1(1p1))F11(1h𝟏𝟐1(1p1))G11(1h𝒑[1]1(1p1))F11(1h𝒑[1]1(1p1)),\frac{G_{1}^{-1}\left(1-h_{\frac{\bm{1}}{\bm{2}}}^{-1}(1-p_{1})\right)}{F_{1}^{-1}\left(1-h_{\frac{\bm{1}}{\bm{2}}}^{-1}(1-p_{1})\right)}\leq\frac{G_{1}^{-1}\left(1-h_{\bm{p}_{[-1]}}^{-1}(1-p_{1})\right)}{F_{1}^{-1}\left(1-h_{\bm{p}_{[-1]}}^{-1}(1-p_{1})\right)},

which confirms that (10) is satisfied. This completes the proof.  

A.5 Proof of Theorem 3.12

Proof.

By the proof of Theorem 3.6, we obtain

ΔRmedMCoES𝒑[X1|X2,,Xn]=01F11(s)𝑑A𝒑[1](s)01F11(s)𝑑A𝟏𝟐(s)1\Delta^{\rm R-med}{\rm MCoES}_{\bm{p}}[X_{1}|X_{2},\dots,X_{n}]=\frac{\int_{0}^{1}F_{1}^{-1}(s)dA_{\bm{p}_{[-1]}}(s)}{\int_{0}^{1}F_{1}^{-1}(s)dA_{\frac{\bm{1}}{\bm{2}}}(s)}-1

and

ΔRmedMCoES𝒑[Y1|Y2,,Yn]=01G11(s)𝑑A𝒑[1](s)01G11(s)𝑑A𝟏𝟐(s)1,\Delta^{\rm R-med}{\rm MCoES}_{\bm{p}}[Y_{1}|Y_{2},\dots,Y_{n}]=\frac{\int_{0}^{1}G_{1}^{-1}(s)dA_{\bm{p}_{[-1]}}(s)}{\int_{0}^{1}G_{1}^{-1}(s)dA_{\frac{\bm{1}}{\bm{2}}}(s)}-1,

where

A𝒑^(s)={0,s1h𝒑^1(1p1),111p1C¯(s,p2,,pn)C¯(0,p2,,pn),s>1h𝒑^1(1p1),A_{\hat{\bm{p}}}(s)=\begin{cases}0,&s\leq 1-h_{\hat{\bm{p}}}^{-1}(1-p_{1}),\\ 1-\frac{1}{1-p_{1}}\cdot\frac{\overline{C}(s,p_{2},\dots,p_{n})}{\overline{C}(0,p_{2},\dots,p_{n})},&s>1-h_{\hat{\bm{p}}}^{-1}(1-p_{1}),\end{cases}

for p1(0,1)p_{1}\in(0,1) and 𝒑^{𝒑[1],𝟏𝟐}\hat{\bm{p}}\in\left\{\bm{p}_{[-1]},\frac{\bm{1}}{\bm{2}}\right\}, with 𝒑[1]=(p2,,pn)(1/2,1)n1\bm{p}_{[-1]}=(p_{2},\dots,p_{n})\in(1/2,1)^{n-1} and 𝟏𝟐=(12,,12)n1\frac{\bm{1}}{\bm{2}}=\left(\frac{1}{2},\dots,\frac{1}{2}\right)\in\mathbb{R}^{n-1}.
Given that CC is MTP2{\rm MTP}_{2}, and (X2,,Xn)SIX1(X_{2},\dots,X_{n})\uparrow_{\rm SI}X_{1}, Lemma A.1 implies that h𝒑^h_{\hat{\bm{p}}} is a concave distortion function, making A𝒑^(s)A_{\hat{\bm{p}}}(s) a convex distortion function. To apply Lemma 3.5, we demonstrate that A𝒑[1](A𝟏𝟐1(s))A_{\bm{p}_{[-1]}}\left(A_{\frac{\bm{1}}{\bm{2}}}^{-1}(s)\right) is convex, equivalent to showing that (A𝒑[1](s))/(A𝟏𝟐(s))\left(A_{\bm{p}_{[-1]}}(s)\right)^{\prime}/\left(A_{\frac{\bm{1}}{\bm{2}}}(s)\right)^{\prime} is increasing in ss, where

(A𝒑^(s))=A𝒑^(s)s=11p1(U2>p2,,Un>pn|U1=s)C¯(0,p2,,pn),\left(A_{\hat{\bm{p}}}(s)\right)^{\prime}=\frac{\partial A_{\hat{\bm{p}}}(s)}{\partial s}=\frac{1}{1-p_{1}}\cdot\frac{\mathbb{P}(U_{2}>p_{2},\dots,U_{n}>p_{n}|U_{1}=s)}{\overline{C}(0,p_{2},\dots,p_{n})},

with Ui=Fi(Xi)U_{i}=F_{i}(X_{i}). Using CC being MTP2{\rm MTP}_{2}, we have

(U2,,Un|U1=u1)whr(U2,,Un|U1=u1),u1u1,(U_{2},\dots,U_{n}|U_{1}=u_{1})\leq_{\rm whr}(U_{2},\dots,U_{n}|U_{1}=u_{1}^{\prime}),\quad\forall u_{1}\leq u_{1}^{\prime},

which implies that

(A𝒑[1](s))(A𝟏𝟐(s))=C¯(0,1/2,,1/2)C¯(0,p2,,pn)(U2>p2,,Un>pn|U1=s)(U2>1/2,,Un>1/2|U1=s)\frac{\left(A_{\bm{p}_{[-1]}}(s)\right)^{\prime}}{\left(A_{\frac{\bm{1}}{\bm{2}}}(s)\right)^{\prime}}=\frac{\overline{C}(0,1/2,\dots,1/2)}{\overline{C}(0,p_{2},\dots,p_{n})}\cdot\frac{\mathbb{P}(U_{2}>p_{2},\dots,U_{n}>p_{n}|U_{1}=s)}{\mathbb{P}(U_{2}>1/2,\dots,U_{n}>1/2|U_{1}=s)}

is increasing in ss. It has been shown that A𝒑[1](s)A_{\bm{p}_{[-1]}}(s), A𝟏𝟐(s)A_{\frac{\bm{1}}{\bm{2}}}(s), and A𝒑[1](A𝟏𝟐1(s))A_{\bm{p}_{[-1]}}\left(A^{-1}_{\frac{\bm{1}}{\bm{2}}}(s)\right) are convex functions. Therefore, applying Lemma 3.5 and X1psY1X_{1}\leq_{\rm ps}Y_{1}, we deduce that (11) holds. This completes the proof.  

Appendix B Supplementary materials

B.1 Risk measures

The contribution measures employed in Tables 5 are presented, as detailed in Sordo et al. (2018) and Ortega-Jiménez et al. (2021).

Definition B.1.

For any p1(0,1)p_{1}\in(0,1), the difference-based contribution MCoVaR\rm MCoVaR with systemic risk event is defined by

ΔMCoVaR𝒑[X1|X2,,Xn]=MCoVaRp1,𝒑[1][X1|X2,,Xn]VaRp1[X1],\Delta{\rm MCoVaR}_{\bm{p}}[X_{1}|X_{2},\dots,X_{n}]={\rm MCoVaR}_{p_{1},\bm{p}_{[-1]}}[X_{1}|X_{2},\dots,X_{n}]-{\rm VaR}_{p_{1}}[X_{1}], (18)

and

ΔmedMCoVaR𝒑[X1|X2,,Xn]=MCoVaRp1,𝒑[1][X1|X2,,Xn]MCoVaRp1,𝟏𝟐[X1|X2,,Xn],\Delta^{\rm med}{\rm MCoVaR}_{\bm{p}}[X_{1}|X_{2},\dots,X_{n}]={\rm MCoVaR}_{p_{1},\bm{p}_{[-1]}}[X_{1}|X_{2},\dots,X_{n}]-{\rm MCoVaR}_{p_{1},\frac{\bm{1}}{\bm{2}}}[X_{1}|X_{2},\dots,X_{n}], (19)

where 𝐩[1]=(p2,,pn)(1/2,1)n1\bm{p}_{[-1]}=(p_{2},\dots,p_{n})\in(1/2,1)^{n-1} and 𝟏𝟐=(12,,12)n1\frac{\bm{1}}{\bm{2}}=\left(\frac{1}{2},\dots,\frac{1}{2}\right)\in\mathbb{R}^{n-1}.

Definition B.2.

For p1(0,1)p_{1}\in(0,1), the difference-based contribution MCoES\rm MCoES with systemic risk event is defined by

ΔMCoES𝒑[X1|X2,,Xn]=MCoESp1,𝒑[1][X1|X2,,Xn]ESp1[X1],\Delta{\rm MCoES}_{\bm{p}}[X_{1}|X_{2},\dots,X_{n}]={\rm MCoES}_{p_{1},\bm{p}_{[-1]}}[X_{1}|X_{2},\dots,X_{n}]-{\rm ES}_{p_{1}}[X_{1}], (20)

and

ΔmedMCoES𝒑[X1|X2,,Xn]=MCoESp1,𝒑[1][X1|X2,,Xn]MCoESp1,𝟏𝟐[X1|X2,,Xn],\Delta^{\rm med}{\rm MCoES}_{\bm{p}}[X_{1}|X_{2},\dots,X_{n}]={\rm MCoES}_{p_{1},\bm{p}_{[-1]}}[X_{1}|X_{2},\dots,X_{n}]-{\rm MCoES}_{p_{1},\frac{\bm{1}}{\bm{2}}}[X_{1}|X_{2},\dots,X_{n}], (21)

where 𝐩[1]=(p2,,pn)(1/2,1)n1\bm{p}_{[-1]}=(p_{2},\dots,p_{n})\in(1/2,1)^{n-1} and 𝟏𝟐=(12,,12)n1\frac{\bm{1}}{\bm{2}}=\left(\frac{1}{2},\dots,\frac{1}{2}\right)\in\mathbb{R}^{n-1}.

B.2 Copula

Definition B.3.

Setting the generating function to ψ(u)=(lnu)θ\psi(u)=(-{\rm ln}~u)^{\theta}, thus ψ1(u)=exp(u1θ)\psi^{-1}(u)={\rm exp}\left(-u^{\frac{1}{\theta}}\right). The nn-dimensional Gumbel copula is defined as follows:

Cθ(u1,,un)=exp{[i=1n(lnui)θ]1θ},θ>1,𝒖[0,1]n.C_{\theta}(u_{1},\dots,u_{n})={\rm exp}\left\{-\left[\sum_{i=1}^{n}(-{\rm ln}~u_{i})^{\theta}\right]^{\frac{1}{\theta}}\right\},~\theta>1,~{\bm{u}}\in[0,1]^{n}.

Gumbel copula exhibits different dependency properties in the left and right tails. Typically, it demonstrates positive right-tail dependency, implying that when one variable exhibits an extreme value in the right tail, there is a higher probability for the other variable to also have an extreme value in the right tail.

Definition B.4.

Setting the generating function to ψ(u)=uθ1\psi(u)=u^{-\theta}-1, thus ψ1(u)=(u+1)1θ\psi^{-1}(u)=(u+1)^{\frac{1}{\theta}}. The nn-dimensional Clayton copula is defined as follows:

Cθ(u1,,un)=[i=1nuiθn+1]1θ,θ>0,𝒖[0,1]n.C_{\theta}(u_{1},\dots,u_{n})=\left[\sum_{i=1}^{n}u_{i}^{-\theta}-n+1\right]^{-\frac{1}{\theta}},~\theta>0,~{\bm{u}}\in[0,1]^{n}.

The Clayton copula exhibits significant dependency in the left tail, meaning that when one variable exhibits an extreme value in the left tail, there is a higher probability for the other variable to also have an extreme value in the left tail. Therefore, the combination of the Gumbel copula and the Clayton copula can simulate asymmetric upper and lower tail dependencies.

In addition to Archimedean copulas, there is another class of copula functions called elliptical copulas, such as the Gaussian copula. The Gaussian copula exhibits a certain degree of symmetry in terms of its dependence properties in the left and right tails. which is defined as follows.

Definition B.5.

Let RR be a symmetric, positive definite matrix with diag(R)=(1,,1){\rm diag}(R)=(1,\dots,1)^{\prime} and ΦR\Phi_{R} the standardized multivariate normal distribution with correlation matrix RR. The multivariate Gaussian copula is defined as follows:

CR(u1,,un)=ΦR(Φ1(u1),,Φ1(un)),C_{R}(u_{1},\dots,u_{n})=\Phi_{R}\left(\Phi^{-1}(u_{1}),\dots,\Phi^{-1}(u_{n})\right),

where Φ1\Phi^{-1} is the inverse of the standard univariate normal distribution function Φ\Phi.

B.3 Tail dependence coefficient

The tail dependence coefficient is a measure of the dependence between random variables in the tails of their joint distribution. It is divided into the upper tail dependence coefficient and the lower tail dependence coefficient, which describe the dependence of random variables in the upper and lower tails of their joint distribution, respectively. Based on this concept, the notion of multivariate upper and lower tail dependence coefficients is introduced.

Definition B.6.

For a random vector 𝐗=(X1,,Xn)\bm{X}=(X_{1},\ldots,X_{n}), let SS be a randomly chosen subset of {1,,n}\{1,\ldots,n\} with |S|=k|S|=k, and let S¯={1,,n}S\bar{S}=\{1,\ldots,n\}\setminus S. The multivariate upper tail dependence coefficient is defined as:

λUS|S¯=limu1(iS{Fi(Xi)>u}|jS¯{Fj(Xj)>u}).\lambda_{U}^{S|\bar{S}}=\lim_{u\to 1^{-}}\mathbb{P}\left(\bigcap_{i\in S}\{F_{i}(X_{i})>u\}\bigg{|}\bigcap_{j\in\bar{S}}\{F_{j}(X_{j})>u\}\right).

The multivariate lower tail dependence coefficient is defined as:

λLS|S¯=limu0+(iS{Fi(Xi)u}|jS¯{Fj(Xj)u}).\lambda_{L}^{S|\bar{S}}=\lim_{u\to 0^{+}}\mathbb{P}\left(\bigcap_{i\in S}\{F_{i}(X_{i})\leq u\}\bigg{|}\bigcap_{j\in\bar{S}}\{F_{j}(X_{j})\leq u\}\right).

B.4 Additional tables under different confidence levels

Tables 6 and 7 summarize the computed values of some systemic risk measures of the three cryptocurrencies under p1=p2=p3=0.975p_{1}=p_{2}=p_{3}=0.975 and p1=p2=p3=0.99p_{1}=p_{2}=p_{3}=0.99, respectively. It can be noted that the overall trend of these risk measures in the two additional tables is similar to the one for p1=p2=p3=0.95p_{1}=p_{2}=p_{3}=0.95. Moreover, as pip_{i} (i=1,2,3i=1,2,3) increases, the risk measures generally show an upward trend. This indicates that as the extremity of the conditional events increases, the value of co-risk measures also grows.

Table 6: Values of some systemic risk measures of the three cryptocurrencies (p1=p2=p3=0.975p_{1}=p_{2}=p_{3}=0.975).
VaR-based BTC ETH XMR
VaR 7.874 11.003 10.968
MCoVaR 23.078 38.473 34.230
ΔMCoVaR\Delta\mathrm{MCoVaR} 15.205 27.470 23.262
ΔRMCoVaR\Delta^{\mathrm{R}}\mathrm{MCoVaR} 1.931 2.497 2.121
ΔmedMCoVaR\Delta^{\mathrm{med}}\mathrm{MCoVaR} 12.571 23.417 19.659
ΔRmedMCoVaR\Delta^{\mathrm{R-med}}\mathrm{MCoVaR} 1.196 1.555 1.349
ES-based BTC ETH XMR
ES 11.313 16.657 15.948
MCoES 27.880 49.701 42.822
ΔMCoES\Delta\mathrm{MCoES} 16.567 33.044 26.873
ΔRMCoES\Delta^{\mathrm{R}}\mathrm{MCoES} 1.464 1.984 1.685
ΔmedMCoES\Delta^{\mathrm{med}}\mathrm{MCoES} 13.680 28.139 22.694
ΔRmedMCoES\Delta^{\mathrm{R-med}}\mathrm{MCoES} 0.963 1.305 1.127
MMME-based BTC ETH XMR
MMME 1.943 8.100 7.195
ΔMMME\Delta\mathrm{MMME} 1.907 7.913 7.025
ΔRMMME\Delta^{\mathrm{R}}\mathrm{MMME} 52.467 42.147 41.358
Table 7: Values of some systemic risk measures of the three cryptocurrencies (p1=p2=p3=0.99p_{1}=p_{2}=p_{3}=0.99).
VaR-based BTC ETH XMR
VaR 10.908 15.723 15.222
MCoVaR 31.983 59.056 50.088
ΔMCoVaR\Delta\mathrm{MCoVaR} 21.075 43.333 34.865
ΔRMCoVaR\Delta^{\mathrm{R}}\mathrm{MCoVaR} 1.932 2.756 2.290
ΔmedMCoVaR\Delta^{\mathrm{med}}\mathrm{MCoVaR} 18.217 38.570 30.770
ΔRmedMCoVaR\Delta^{\mathrm{R-med}}\mathrm{MCoVaR} 1.323 1.883 1.593
ES-based BTC ETH XMR
ES 14.618 22.333 20.862
MCoES 37.578 74.451 61.134
ΔMCoES\Delta\mathrm{MCoES} 22.960 52.117 40.272
ΔRMCoES\Delta^{\mathrm{R}}\mathrm{MCoES} 1.571 2.334 1.930
ΔmedMCoES\Delta^{\mathrm{med}}\mathrm{MCoES} 19.829 46.355 35.523
ΔRmedMCoES\Delta^{\mathrm{R-med}}\mathrm{MCoES} 1.117 1.650 1.387
MMME-based BTC ETH XMR
MMME 1.619 10.394 8.464
ΔMMME\Delta\mathrm{MMME} 1.607 10.294 8.385
ΔRMMME\Delta^{\mathrm{R}}\mathrm{MMME} 137.496 103.021 105.524