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Invertible disformal transformations with higher derivatives

Kazufumi Takahashi Center for Gravitational Physics, Yukawa Institute for Theoretical Physics, Kyoto University, Kyoto 606-8502, Japan    Hayato Motohashi Division of Liberal Arts, Kogakuin University, 2665-1 Nakano-machi, Hachioji, Tokyo 192-0015, Japan    Masato Minamitsuji Centro de Astrofísica e Gravitação - CENTRA, Departamento de Física, Instituto Superior Técnico - IST, Universidade de Lisboa - UL, Av. Rovisco Pais 1, 1049-001 Lisboa, Portugal
Abstract

We consider a higher-derivative generalization of disformal transformations in DD-dimensional spacetime and clarify the conditions under which they form a group with respect to the matrix product and the functional composition. These conditions allow us to systematically construct the inverse transformation in a fully covariant manner. Applying the invertible generalized disformal transformation to known ghost-free scalar-tensor theories, we obtain a novel class of ghost-free scalar-tensor theories, whose action contains the third- or higher-order derivatives of the scalar field as well as nontrivial higher-order derivative couplings to the curvature tensor.

preprint: YITP-21-137

I Introduction

Scalar-tensor theories have been studied extensively as a model of inflation/dark energy, and there has been a growing interest in incorporating higher-derivative interactions of the scalar field into the action without introducing Ostrogradsky ghost Woodard (2015); Motohashi and Suyama (2020). It was shown that the ghost can be eliminated if the higher-derivative terms are degenerate Motohashi and Suyama (2015); Langlois and Noui (2016); Motohashi et al. (2016); Klein and Roest (2016); Motohashi et al. (2018a, b). With the knowledge of the degeneracy conditions, one can systematically construct ghost-free scalar-tensor theories, which are known as degenerate higher-order scalar-tensor (DHOST) theories Langlois and Noui (2016); Crisostomi et al. (2016); Ben Achour et al. (2016); Takahashi and Kobayashi (2017); Langlois et al. (2019).*1*1*1Relaxing the degeneracy conditions so that the higher-derivative terms are degenerate only in the unitary gauge, we obtain a broader class of scalar-tensor theories Gao (2014); De Felice et al. (2018); Gao and Yao (2019); Motohashi and Hu (2020); De Felice et al. (2021). In that case, there is an apparent extra DOF in a generic gauge, but it satisfies an elliptic differential equation and hence is an instantaneous (or “shadowy”) mode De Felice et al. (2018, 2021). The DHOST theory includes the Horndeski Horndeski (1974); Deffayet et al. (2011); Kobayashi et al. (2011) and the Gleyzes-Langlois-Piazza-Vernizzi theories Gleyzes et al. (2015) as special cases, and hence form a general class of healthy scalar-tensor theories (see Langlois (2019); Kobayashi (2019) for reviews).

To pursue more general frameworks of scalar-tensor theories, a redefinition of the metric or an invertible transformation has been playing an important role. This is because, in general, an invertible transformation maps a ghost-free theory to another ghost-free theory as it does not change the number of dynamical degrees of freedom (DOFs) Domènech et al. (2015); Takahashi et al. (2017). Let us consider a transformation between gμνg_{\mu\nu} and g¯μν\bar{g}_{\mu\nu}. For a given action of scalar-tensor theories S¯[g¯μν,ϕ]\bar{S}[\bar{g}_{\mu\nu},\phi], we substitute the transformation law to obtain a new action S[gμν,ϕ]S[g_{\mu\nu},\phi]. Hence, g¯μν\bar{g}_{\mu\nu} and gμνg_{\mu\nu} are respectively referred to as the original- and new-frame metrics. So long as the transformation is invertible, the two actions are mathematically equivalent up to the redefinition of variables and boundary terms. However, when matter fields are taken into account, one has to define the metric to which the matter fields are minimally coupled. As an aside, even if the gravity sector is degenerate, introducing a matter sector could revive the Ostrogradsky ghost, and hence one needs a careful analysis Deffayet and Garcia-Saenz (2020). Therefore, the resultant action S[gμν,ϕ]S[g_{\mu\nu},\phi] can be regarded as a new theory, rather than a mere redefinition of the original action S¯[g¯μν,ϕ]\bar{S}[\bar{g}_{\mu\nu},\phi].

A well-established example of such metric transformations is the disformal transformation Bekenstein (1993); Bruneton and Esposito-Farèse (2007); Bettoni and Liberati (2013), which is of the form,

g¯μν=F0(ϕ,X)gμν+F1(ϕ,X)μϕνϕ,Xgμνμϕνϕ,\bar{g}_{\mu\nu}=F_{0}(\phi,X)g_{\mu\nu}+F_{1}(\phi,X)\nabla_{\mu}\phi\nabla_{\nu}\phi,\qquad X\coloneqq g^{\mu\nu}\nabla_{\mu}\phi\nabla_{\nu}\phi, (1)

where Greek indices μ,ν,\mu,\nu,\cdots represent spacetime indices and μ\nabla_{\mu} denotes the covariant derivative with respect to the metric gμνg_{\mu\nu}, with the scalar field ϕ\phi unchanged. Note that in the present paper, for simplicity, a “disformal transformation” denotes a transformation of the form (1) with F01F_{0}\neq 1 and F10F_{1}\neq 0 in general (and also its generalization discussed below), which also contains the purely conformal transformation with F1=0F_{1}=0 as a special case. As we shall see in detail in §II.1, the transformation (1) is invertible (i.e., the new-frame metric gμνg_{\mu\nu} can be uniquely expressed in terms of ϕ\phi and g¯μν\bar{g}_{\mu\nu} without referring to any particular configuration) if and only if F0(F0+XF1)(F0XF0XX2F1X)0F_{0}(F_{0}+XF_{1})(F_{0}-XF_{0X}-X^{2}F_{1X})\neq 0, where FiXFi/XF_{iX}\coloneqq\partial F_{i}/\partial X (i=0,1i=0,1). Interestingly, it was shown in Zumalacárregui and García-Bellido (2014) that the disformal transformation (1) in general maps the Horndeski class to its exterior, which is now known as the quadratic/cubic DHOST class Langlois and Noui (2016); Crisostomi et al. (2016); Ben Achour et al. (2016).*2*2*2However, in two spacetime dimensions, the Horndeski class is closed under the disformal transformation of the form (1Takahashi and Kobayashi (2019). Also, the quadratic/cubic DHOST class itself is closed under the disformal transformation Ben Achour et al. (2016). Applications of the disformal transformation have been extensively explored in various contexts; inflation Kaloper (2004); van de Bruck et al. (2016, 2017); Karwan and Channuie (2017); Bordin et al. (2017); Sato and Maeda (2018); Qiu et al. (2020); Gialamas et al. (2020, 2021), cosmic microwave background van de Bruck et al. (2013); Brax et al. (2013); Burrage et al. (2016), dark matter and dark energy Zumalacárregui et al. (2010); Koivisto et al. (2012); Neveu et al. (2014); Sakstein (2015); van de Bruck and Morrice (2015); Hagala et al. (2016); Brax et al. (2015); Emond and Saffin (2016); Karwan and Sapa (2017); Sapa et al. (2018); Llinares et al. (2020); Teixeira et al. (2020); Trojanowski et al. (2020); Dusoye et al. (2021); Brax et al. (2021a); Gómez et al. (2021), cosmological perturbations Minamitsuji (2014); Tsujikawa (2015a); Motohashi and White (2016); Tsujikawa (2015b); Fujita et al. (2016); Chiba et al. (2020); Alinea and Kubota (2021); Minamitsuji (2021a), solar system tests and screening mechanisms Brax and Burrage (2014); Sakstein (2014, 2015); Ip et al. (2015); Brax and Davis (2018); Davis and Melville (2020); Brax et al. (2021b), relativistic stars Minamitsuji and Silva (2016); Brax et al. (2019); Silva and Minamitsuji (2019); Ramazanoğlu and Ünlütürk (2019); Minamitsuji (2021b); Ikeda et al. (2021), and black holes Koivisto and Nyrhinen (2017); Takahashi et al. (2019); Ben Achour et al. (2020a); Anson et al. (2021); Ben Achour et al. (2020b); Long et al. (2020); Minamitsuji (2020); Chen et al. (2021); Erices et al. (2021); Takahashi and Motohashi (2021); Ben Achour et al. (2021); Faraoni and Leblanc (2021); Zhou et al. (2021); Chatzifotis et al. (2021); Bakopoulos et al. (2021).

A natural question is whether there exists a more general class of invertible transformations, which would bring us new fruitful insights on scalar-tensor theories. The transformation (1) is the most general up to the first derivative of the scalar field. Recently, a higher-derivative generalization of the disformal transformation was studied in the context of cosmological perturbations Alinea and Kubota (2021); Minamitsuji (2021a). However, the invertibility of such generalized disformal transformations remains unclear. The aim of the present paper is to address this issue. The authors of Alinea and Kubota (2021) studied the generalized disformal transformation in the context of inflationary cosmology and showed that the transformation can be regarded as invertible if higher-derivative terms are suppressed by the slow-roll parameter and can be neglected. On the other hand, the authors of Babichev et al. (2019, 2021) studied a general derivative-dependent field transformation by applying the method of characteristics, and formulated a set of necessary and sufficient conditions for the local invertibility as the degeneracy condition to remove additional DOFs after the transformation. In particular, they applied the criteria to a disformal transformation of the form

g¯μν=F0(ϕ,X)gμν+F1(ϕ,X)μϕνϕ+F2(ϕ,X)μνϕ,\bar{g}_{\mu\nu}=F_{0}(\phi,X)g_{\mu\nu}+F_{1}(\phi,X)\nabla_{\mu}\phi\nabla_{\nu}\phi+F_{2}(\phi,X)\nabla_{\mu}\nabla_{\nu}\phi, (2)

on a homogeneous and isotropic cosmological background and showed that the transformation is noninvertible unless F2=0F_{2}=0, for which the transformation (2) reduces to (1). The point is that, in order to prove the noninvertibility of a transformation, it is sufficient to show it on a particular background. In contrast, the invertibility of a transformation on a particular background does not guarantee the invertibility on generic backgrounds. In principle, the invertibility conditions obtained in Babichev et al. (2019, 2021) would apply to the construction of invertible generalized disformal transformations without referring to a particular background. Nevertheless, in practice, the application would not be so straightforward, and so far there is no known explicit example of invertible disformal transformations with higher-order field derivatives.

In the present paper, we will construct a general class of invertible disformal transformations with higher-order field derivatives in DD-dimensional spacetime. We first clarify that the invertibility of the conventional disformal transformation (1) originates from its closedness under the matrix product and the functional composition. We then consider a higher-derivative generalization of the disformal transformation with these properties and construct the inverse transformation in a fully covariant manner. We also clarify how known DHOST theories are transformed under the generalized disformal transformations. As a result, we obtain a novel class of healthy degenerate theories, which possesses at most three propagating DOFs. Interestingly, the resultant action contains the third- or higher-order derivatives of the scalar field as well as a novel type of higher-order derivative couplings to the curvature tensor.

The rest of this paper is organized as follows. In §II, we discuss under which conditions the generalized disformal transformations can be invertible and explicitly construct the inverse transformation. Our construction also applies to the vector disformal transformation Kimura et al. (2017), which we shall discuss in the Appendix. In §III, we provide several specific examples of invertible disformal transformations with the second or third derivatives of the scalar field. Then, in §IV, we study the generalized disformal transformation of known DHOST theories. Finally, we draw our conclusions in §V.

II Invertibility of disformal transformations

II.1 Transformations up to the first derivative

We first review the case of the conventional disformal transformation that contains up to the first derivative of the scalar field to clarify the reason why it is possible to construct the inverse transformation in this case. Let us consider a class of metric transformations of the form (1), which we recapitulate here for convenience:

g¯μν=F0(ϕ,X)gμν+F1(ϕ,X)ϕμϕν,\bar{g}_{\mu\nu}=F_{0}(\phi,X)g_{\mu\nu}+F_{1}(\phi,X)\phi_{\mu}\phi_{\nu}, (3)

where we have introduced ϕμμϕ\phi_{\mu}\coloneqq\partial_{\mu}\phi and then XϕμϕμX\coloneqq\phi_{\mu}\phi^{\mu}. Note that the following results hold in general DD-dimensional spacetime.

A remarkable feature of this class of transformations is that it is equipped with two binary operations and hence forms a group under each of the two operations. One of the two operations is the matrix product of two disformal metrics, while the other is the functional composition of two sequential disformal transformations. In what follows, we demonstrate that the class of conventional disformal transformations is indeed closed under the two operations mentioned above.

  1. [A]

    Closedness under the matrix product. We consider two independent transformations of the form (3),

    g¯μν=F0(ϕ,X)gμν+F1(ϕ,X)ϕμϕν,g~μν=f0(ϕ,X)gμν+f1(ϕ,X)ϕμϕν.\bar{g}_{\mu\nu}=F_{0}(\phi,X)g_{\mu\nu}+F_{1}(\phi,X)\phi_{\mu}\phi_{\nu},\qquad\tilde{g}_{\mu\nu}=f_{0}(\phi,X)g_{\mu\nu}+f_{1}(\phi,X)\phi_{\mu}\phi_{\nu}. (4)

    By contracting g¯μν\bar{g}_{\mu\nu} and g~μν\tilde{g}_{\mu\nu} with the unbarred metric, one can construct another disformal metric, which we call the matrix product of two disformal metrics. Written explicitly, the matrix product is computed as

    gαβg¯μαg~βν=F0f0gμν+[(F0+XF1)f1+F1f0]ϕμϕν,g^{\alpha\beta}\bar{g}_{\mu\alpha}\tilde{g}_{\beta\nu}=F_{0}f_{0}g_{\mu\nu}+\left[(F_{0}+XF_{1})f_{1}+F_{1}f_{0}\right]\phi_{\mu}\phi_{\nu}, (5)

    which is again of the form (3).

This property allows us to construct the inverse metric for g¯μν\bar{g}_{\mu\nu} as the inverse element in the group under the matrix product. Indeed, by choosing

f0=1F0,f1=F1F0(F0+XF1),f_{0}=\frac{1}{F_{0}},\qquad f_{1}=-\frac{F_{1}}{F_{0}(F_{0}+XF_{1})}, (6)

we can make gαβg¯μαg~βν=gμνg^{\alpha\beta}\bar{g}_{\mu\alpha}\tilde{g}_{\beta\nu}=g_{\mu\nu}, which means that the inverse metric g¯μν\bar{g}^{\mu\nu} is given by

g¯μν=gμαgνβg~αβ=1F0(gμνF1F0+XF1ϕμϕν).\bar{g}^{\mu\nu}=g^{\mu\alpha}g^{\nu\beta}\tilde{g}_{\alpha\beta}=\frac{1}{F_{0}}\left(g^{\mu\nu}-\frac{F_{1}}{F_{0}+XF_{1}}\phi^{\mu}\phi^{\nu}\right). (7)

Here, we have assumed F00F_{0}\neq 0 and F0+XF10F_{0}+XF_{1}\neq 0.

  1. [B]

    Closedness under the functional composition. We consider two sequential transformations of the form (3),

    g¯μν=F0(ϕ,X)gμν+F1(ϕ,X)ϕμϕν,g^μν=F¯0(ϕ,X¯)g¯μν+F¯1(ϕ,X¯)ϕμϕν.\bar{g}_{\mu\nu}=F_{0}(\phi,X)g_{\mu\nu}+F_{1}(\phi,X)\phi_{\mu}\phi_{\nu},\qquad\hat{g}_{\mu\nu}=\bar{F}_{0}(\phi,\bar{X})\bar{g}_{\mu\nu}+\bar{F}_{1}(\phi,\bar{X})\phi_{\mu}\phi_{\nu}. (8)

    Here, X¯\bar{X} denotes the kinetic term of the scalar field contracted by g¯μν\bar{g}^{\mu\nu}, which is computed by use of (7) as

    X¯g¯μνϕμϕν=XF0+XF1.\bar{X}\coloneqq\bar{g}^{\mu\nu}\phi_{\mu}\phi_{\nu}=\frac{X}{F_{0}+XF_{1}}. (9)

    Then, the composition of the two transformations is given by

    g^μν=F0(ϕ,X)F¯0(ϕ,X¯(ϕ,X))gμν+[F¯1(ϕ,X¯(ϕ,X))+F1(ϕ,X)F¯0(ϕ,X¯(ϕ,X))]ϕμϕν,\hat{g}_{\mu\nu}=F_{0}(\phi,X)\bar{F}_{0}(\phi,\bar{X}(\phi,X))g_{\mu\nu}+\left[\bar{F}_{1}(\phi,\bar{X}(\phi,X))+F_{1}(\phi,X)\bar{F}_{0}(\phi,\bar{X}(\phi,X))\right]\phi_{\mu}\phi_{\nu}, (10)

    which is again of the form (3).

The inverse for the map g¯μν=g¯μν[gαβ,ϕ]\bar{g}_{\mu\nu}=\bar{g}_{\mu\nu}[g_{\alpha\beta},\phi] is nothing but the inverse element of g¯μν\bar{g}_{\mu\nu} in the group under the functional composition and hence is given by requiring g^μν=gμν\hat{g}_{\mu\nu}=g_{\mu\nu}, i.e.,

F¯0(ϕ,X¯)=1F0(ϕ,X(ϕ,X¯)),F¯1(ϕ,X¯)=F1(ϕ,X(ϕ,X¯))F0(ϕ,X(ϕ,X¯)),\bar{F}_{0}(\phi,\bar{X})=\frac{1}{F_{0}(\phi,X(\phi,\bar{X}))},\qquad\bar{F}_{1}(\phi,\bar{X})=-\frac{F_{1}(\phi,X(\phi,\bar{X}))}{F_{0}(\phi,X(\phi,\bar{X}))}, (11)

where XX in the right-hand sides is regarded as a function of (ϕ,X¯)(\phi,\bar{X}) by use of (9). Note that we need

X¯XX¯X=F0XF0XX2F1X(F0+XF1)20,\bar{X}_{X}\coloneqq\frac{\partial\bar{X}}{\partial X}=\frac{F_{0}-XF_{0X}-X^{2}F_{1X}}{(F_{0}+XF_{1})^{2}}\neq 0, (12)

to locally express XX in terms of X¯\bar{X}. Hence, the explicit form of the inverse transformation is given by

gμν=1F0(ϕ,X(ϕ,X¯))[g¯μνF1(ϕ,X(ϕ,X¯))ϕμϕν],g_{\mu\nu}=\frac{1}{F_{0}(\phi,X(\phi,\bar{X}))}\left[\bar{g}_{\mu\nu}-F_{1}(\phi,X(\phi,\bar{X}))\phi_{\mu}\phi_{\nu}\right], (13)

and a set of necessary and sufficient conditions for the disformal transformation (3) to be invertible is summarized as

F00,F0+XF10,F0XF0XX2F1X0.F_{0}\neq 0,\qquad F_{0}+XF_{1}\neq 0,\qquad F_{0}-XF_{0X}-X^{2}F_{1X}\neq 0. (14)

Although not directly related to the invertibility of the transformation, F0>0F_{0}>0 and F0+XF1>0F_{0}+XF_{1}>0 are necessary to preserve the metric signature Bruneton and Esposito-Farèse (2007).

The above analysis demonstrates that the two properties [A] and [B] play an essential role in the systematic construction of the inverse metric and the inverse transformation. Note that for the existence of the inverse transformation, the existence of the inverse metric is necessary. As we saw above, when computing the functional composition of the two disformal transformations in (8), one needs to express X¯\bar{X} in terms of the unbarred quantities, in which the inverse metric g¯μν\bar{g}^{\mu\nu} shows up. In the next subsection, we study a generalized disformal transformation with higher derivatives satisfying the above two properties and explicitly construct its inverse transformation.

II.2 Transformations with higher derivatives

Having clarified the reason why the conventional disformal transformation (3) is invertible, we now consider transformations with higher derivatives. The main difficulty here is that the higher covariant derivatives depend on the Christoffel symbol, i.e., the derivative of the metric. This generically spoils the property [B] since a functional composition of two transformations generically yields unwanted extra terms with higher derivatives that are not contained in the original transformation law. In order to make a transformation invertible, one has to tune it so that such extra terms do not show up. As a general example of transformations for which this tuning is possible, let us consider a metric transformation in DD-dimensional spacetime defined by

g¯μν=F0gμν+F1ϕμϕν+2F2ϕ(μXν)+F3XμXν.\bar{g}_{\mu\nu}=F_{0}g_{\mu\nu}+F_{1}\phi_{\mu}\phi_{\nu}+2F_{2}\phi_{(\mu}X_{\nu)}+F_{3}X_{\mu}X_{\nu}. (15)

Here, XμμX=2ϕαϕμαX_{\mu}\coloneqq\partial_{\mu}X=2\phi_{\alpha}\phi^{\alpha}_{\mu} with ϕμνμνϕ\phi_{\mu\nu}\coloneqq\nabla_{\mu}\nabla_{\nu}\phi and T(μν)(Tμν+Tνμ)/2T_{({\mu\nu})}\coloneqq(T_{\mu\nu}+T_{\nu\mu})/2. Also, FiF_{i}’s (i=0,1,2,3i=0,1,2,3) are functions of (ϕ,X,Y,Z)(\phi,X,Y,Z), where YY and ZZ are defined as follows:

YϕμXμ,ZXμXμ.Y\coloneqq\phi_{\mu}X^{\mu},\qquad Z\coloneqq X_{\mu}X^{\mu}. (16)

Note that the conventional disformal transformation (3) is included as a special case with F0=F0(ϕ,X)F_{0}=F_{0}(\phi,X), F1=F1(ϕ,X)F_{1}=F_{1}(\phi,X), and F2=F3=0F_{2}=F_{3}=0. In what follows, we explicitly construct the inverse transformation for (15) with a particular focus on the properties [A] and [B].

We first examine the property [A], i.e., the closedness under the matrix product. To this end, we consider two independent transformations of the form (15),

g¯μν=F0gμν+F1ϕμϕν+2F2ϕ(μXν)+F3XμXν,g~μν=f0gμν+f1ϕμϕν+2f2ϕ(μXν)+f3XμXν.\begin{split}\bar{g}_{\mu\nu}&=F_{0}g_{\mu\nu}+F_{1}\phi_{\mu}\phi_{\nu}+2F_{2}\phi_{(\mu}X_{\nu)}+F_{3}X_{\mu}X_{\nu},\\ \tilde{g}_{\mu\nu}&=f_{0}g_{\mu\nu}+f_{1}\phi_{\mu}\phi_{\nu}+2f_{2}\phi_{(\mu}X_{\nu)}+f_{3}X_{\mu}X_{\nu}.\end{split} (17)

The matrix product of g¯μν\bar{g}_{\mu\nu} and g~μν\tilde{g}_{\mu\nu} is calculated as follows:

gαβg¯μαg~βν=\displaystyle g^{\alpha\beta}\bar{g}_{\mu\alpha}\tilde{g}_{\beta\nu}=\; F0f0gμν+[F0f1+F1(f0+Xf1+Yf2)+F2(Yf1+Zf2)]ϕμϕν\displaystyle F_{0}f_{0}g_{\mu\nu}+\left[F_{0}f_{1}+F_{1}\left(f_{0}+Xf_{1}+Yf_{2}\right)+F_{2}\left(Yf_{1}+Zf_{2}\right)\right]\phi_{\mu}\phi_{\nu}
+[F0f2+F1(Xf2+Yf3)+F2(f0+Yf2+Zf3)]ϕμXν\displaystyle+\left[F_{0}f_{2}+F_{1}\left(Xf_{2}+Yf_{3}\right)+F_{2}\left(f_{0}+Yf_{2}+Zf_{3}\right)\right]\phi_{\mu}X_{\nu}
+[F0f2+F2(f0+Xf1+Yf2)+F3(Yf1+Zf2)]Xμϕν\displaystyle+\left[F_{0}f_{2}+F_{2}\left(f_{0}+Xf_{1}+Yf_{2}\right)+F_{3}\left(Yf_{1}+Zf_{2}\right)\right]X_{\mu}\phi_{\nu}
+[F0f3+F2(Xf2+Yf3)+F3(f0+Yf2+Zf3)]XμXν,\displaystyle+\left[F_{0}f_{3}+F_{2}\left(Xf_{2}+Yf_{3}\right)+F_{3}\left(f_{0}+Yf_{2}+Zf_{3}\right)\right]X_{\mu}X_{\nu}, (18)

which is again of the form (15), and hence the property [A] is satisfied.*3*3*3Precisely speaking, the right-hand side of (18) is not of the form (15) as it is not symmetric in μ\mu and ν\nu in general. Therefore, for the closedness under the matrix product, the underlying set of transformations should be enlarged to include such asymmetric terms. Nevertheless, as mentioned in the main text, the inverse element of (15) can be found in the symmetric subset. This is reminiscent of the fact that a product of two symmetric matrices is not necessarily symmetric, while the inverse of a symmetric matrix is symmetric. The inverse matrix for g¯μν\bar{g}_{\mu\nu} is obtained by putting gαβg¯μαg~βν=gμνg^{\alpha\beta}\bar{g}_{\mu\alpha}\tilde{g}_{\beta\nu}=g_{\mu\nu} in (18). While this requirement apparently yields five equations for four unknown functions f0,f1,f2,f3f_{0},f_{1},f_{2},f_{3}, only four of them are independent, and hence the system is not overdetermined. Thus, the coefficient functions in g~μν\tilde{g}_{\mu\nu} are fixed as

f0=1F0,f1=F0F1Z(F22F1F3)F0,f2=F0F2+Y(F22F1F3)F0,f3=F0F3X(F22F1F3)F0.\begin{split}&f_{0}=\frac{1}{F_{0}},\qquad f_{1}=-\frac{F_{0}F_{1}-Z(F_{2}^{2}-F_{1}F_{3})}{F_{0}\mathcal{F}},\\ &f_{2}=-\frac{F_{0}F_{2}+Y(F_{2}^{2}-F_{1}F_{3})}{F_{0}\mathcal{F}},\qquad f_{3}=-\frac{F_{0}F_{3}-X(F_{2}^{2}-F_{1}F_{3})}{F_{0}\mathcal{F}}.\end{split} (19)

Here, we assumed F00F_{0}\neq 0 and defined the following quantity:

F02+F0(XF1+2YF2+ZF3)+(F22F1F3)(Y2XZ),\mathcal{F}\coloneqq F_{0}^{2}+F_{0}(XF_{1}+2YF_{2}+ZF_{3})+(F_{2}^{2}-F_{1}F_{3})(Y^{2}-XZ), (20)

which was also assumed to be nonvanishing. As a result, the inverse metric g¯μν\bar{g}^{\mu\nu} is given by

g¯μν=1F0[gμνF0F1Z(F22F1F3)ϕμϕν2F0F2+Y(F22F1F3)ϕ(μXν)F0F3X(F22F1F3)XμXν].\bar{g}^{\mu\nu}=\frac{1}{F_{0}}\bigg{[}g^{\mu\nu}-\frac{F_{0}F_{1}-Z(F_{2}^{2}-F_{1}F_{3})}{\mathcal{F}}\phi^{\mu}\phi^{\nu}-2\frac{F_{0}F_{2}+Y(F_{2}^{2}-F_{1}F_{3})}{\mathcal{F}}\phi^{(\mu}X^{\nu)}-\frac{F_{0}F_{3}-X(F_{2}^{2}-F_{1}F_{3})}{\mathcal{F}}X^{\mu}X^{\nu}\bigg{]}. (21)

Next, let us study under which conditions the transformation (15) can satisfy the property [B], i.e., the closedness under the functional composition. We consider sequential transformations with

g¯μν=F0gμν+F1ϕμϕν+2F2ϕ(μXν)+F3XμXν,g^μν=F¯0g¯μν+F¯1ϕμϕν+2F¯2ϕ(μX¯ν)+F¯3X¯μX¯ν,\begin{split}\bar{g}_{\mu\nu}&=F_{0}g_{\mu\nu}+F_{1}\phi_{\mu}\phi_{\nu}+2F_{2}\phi_{(\mu}X_{\nu)}+F_{3}X_{\mu}X_{\nu},\\ \hat{g}_{\mu\nu}&=\bar{F}_{0}\bar{g}_{\mu\nu}+\bar{F}_{1}\phi_{\mu}\phi_{\nu}+2\bar{F}_{2}\phi_{(\mu}\bar{X}_{\nu)}+\bar{F}_{3}\bar{X}_{\mu}\bar{X}_{\nu},\end{split} (22)

with F¯i\bar{F}_{i}’s (i=0,1,2,3i=0,1,2,3) being functions of (ϕ,X¯,Y¯,Z¯)(\phi,\bar{X},\bar{Y},\bar{Z}). In the case of the first-order disformal transformations studied in §II.1, the invertibility is guaranteed if XX can be locally expressed in terms of X¯\bar{X}. In the present case with higher derivatives, we have

X¯=g¯μνϕμϕν=XF0F3(Y2XZ),\bar{X}=\bar{g}^{\mu\nu}\phi_{\mu}\phi_{\nu}=\frac{XF_{0}-F_{3}(Y^{2}-XZ)}{\mathcal{F}}, (23)

which is a function of (ϕ,X,Y,Z)(\phi,X,Y,Z) in general. Let us consider to express g^μν\hat{g}_{\mu\nu} as a functional of ϕ\phi and gμνg_{\mu\nu}. If X¯\bar{X} depends on YY or ZZ in a nontrivial manner, then the derivatives of X¯\bar{X} in g^μν\hat{g}_{\mu\nu} yield derivatives of YY or ZZ, which do not appear in the transformation law (15). On the other hand, so long as X¯\bar{X} has no dependence on either YY or ZZ, then the composition of the two transformations is again of the form (15), meaning that the property [B] is satisfied. Therefore, we require

X¯Y=X¯Z=0,\bar{X}_{Y}=\bar{X}_{Z}=0, (24)

where X¯YX¯/Y{\bar{X}}_{Y}\coloneqq\partial{\bar{X}}/\partial Y and X¯ZX¯/Z{\bar{X}}_{Z}\coloneqq\partial{\bar{X}}/\partial Z, so that X¯=X¯(ϕ,X)\bar{X}=\bar{X}(\phi,X). We also assume X¯X0\bar{X}_{X}\neq 0 so that we can solve the relation X¯=X¯(ϕ,X)\bar{X}=\bar{X}(\phi,X) for XX to have X=X(ϕ,X¯)X=X(\phi,\bar{X}). Then, we have X¯μ=X¯XXμ+X¯ϕϕμ\bar{X}_{\mu}=\bar{X}_{X}X_{\mu}+\bar{X}_{\phi}\phi_{\mu} with X¯ϕX¯/ϕ{\bar{X}}_{\phi}\coloneqq\partial{\bar{X}}/\partial\phi, and hence

Y¯=g¯μνϕμX¯ν=X¯XYF0+F2(Y2XZ)+X¯ϕX¯,Z¯=g¯μνX¯μX¯ν=X¯X2ZF0F1(Y2XZ)+2X¯ϕY¯X¯ϕ2X¯.\begin{split}\bar{Y}&=\bar{g}^{\mu\nu}\phi_{\mu}\bar{X}_{\nu}=\bar{X}_{X}\frac{YF_{0}+F_{2}(Y^{2}-XZ)}{\mathcal{F}}+\bar{X}_{\phi}\bar{X},\\ \bar{Z}&=\bar{g}^{\mu\nu}\bar{X}_{\mu}\bar{X}_{\nu}=\bar{X}_{X}^{2}\frac{ZF_{0}-F_{1}(Y^{2}-XZ)}{\mathcal{F}}+2\bar{X}_{\phi}\bar{Y}-\bar{X}_{\phi}^{2}\bar{X}.\end{split} (25)

Here, we require that these two equations can be solved for YY and ZZ to obtain Y=Y(ϕ,X¯,Y¯,Z¯)Y=Y(\phi,\bar{X},\bar{Y},\bar{Z}) and Z=Z(ϕ,X¯,Y¯,Z¯)Z=Z(\phi,\bar{X},\bar{Y},\bar{Z}), which is guaranteed if the Jacobian determinant |(Y¯,Z¯)/(Y,Z)||\partial(\bar{Y},\bar{Z})/\partial(Y,Z)| is nonvanishing.

We are now ready to write down the expression for the inverse transformation for g¯μν=g¯μν[gαβ,ϕ]\bar{g}_{\mu\nu}=\bar{g}_{\mu\nu}[g_{\alpha\beta},\phi]. With the requirement X¯=X¯(ϕ,X)\bar{X}=\bar{X}(\phi,X), we can express g^μν\hat{g}_{\mu\nu} in terms of the unbarred quantities as

g^μν=F0F¯0gμν+(F¯1+F1F¯0+2X¯ϕF¯2+X¯ϕ2F¯3)ϕμϕν+2(X¯XF¯2+F2F¯0+X¯ϕX¯XF¯3)ϕ(μXν)+(X¯X2F¯3+F3F¯0)XμXν,\hat{g}_{\mu\nu}=F_{0}\bar{F}_{0}g_{\mu\nu}+(\bar{F}_{1}+F_{1}\bar{F}_{0}+2\bar{X}_{\phi}\bar{F}_{2}+\bar{X}_{\phi}^{2}\bar{F}_{3})\phi_{\mu}\phi_{\nu}+2(\bar{X}_{X}\bar{F}_{2}+F_{2}\bar{F}_{0}+\bar{X}_{\phi}\bar{X}_{X}\bar{F}_{3})\phi_{(\mu}X_{\nu)}+(\bar{X}_{X}^{2}\bar{F}_{3}+F_{3}\bar{F}_{0})X_{\mu}X_{\nu}, (26)

where the functions of (ϕ,X¯,Y¯,Z¯)(\phi,\bar{X},\bar{Y},\bar{Z}) in the right-hand side are regarded as functions of (ϕ,X,Y,Z)(\phi,X,Y,Z) by (23) and (25). The inverse transformation can be obtained by putting g^μν=gμν\hat{g}_{\mu\nu}=g_{\mu\nu}, which fixes the coefficient functions in g^μν\hat{g}_{\mu\nu} as

F¯0=1F0,F¯1=X¯X2F12X¯ϕX¯XF2+X¯ϕ2F3X¯X2F0,F¯2=X¯XF2X¯ϕF3X¯X2F0,F¯3=F3X¯X2F0.\bar{F}_{0}=\frac{1}{F_{0}},\qquad\bar{F}_{1}=-\frac{\bar{X}_{X}^{2}F_{1}-2\bar{X}_{\phi}\bar{X}_{X}F_{2}+\bar{X}_{\phi}^{2}F_{3}}{\bar{X}_{X}^{2}F_{0}},\qquad\bar{F}_{2}=-\frac{\bar{X}_{X}F_{2}-\bar{X}_{\phi}F_{3}}{\bar{X}_{X}^{2}F_{0}},\qquad\bar{F}_{3}=-\frac{F_{3}}{\bar{X}_{X}^{2}F_{0}}. (27)

Thus, we have obtained the inverse transformation in the following form:

gμν=1F0(g¯μνX¯X2F12X¯ϕX¯XF2+X¯ϕ2F3X¯X2ϕμϕν2X¯XF2X¯ϕF3X¯X2ϕ(μX¯ν)F3X¯X2X¯μX¯ν),g_{\mu\nu}=\frac{1}{F_{0}}\left(\bar{g}_{\mu\nu}-\frac{\bar{X}_{X}^{2}F_{1}-2\bar{X}_{\phi}\bar{X}_{X}F_{2}+\bar{X}_{\phi}^{2}F_{3}}{\bar{X}_{X}^{2}}\phi_{\mu}\phi_{\nu}-2\frac{\bar{X}_{X}F_{2}-\bar{X}_{\phi}F_{3}}{\bar{X}_{X}^{2}}\phi_{(\mu}\bar{X}_{\nu)}-\frac{F_{3}}{\bar{X}_{X}^{2}}\bar{X}_{\mu}\bar{X}_{\nu}\right), (28)

where the functions of (ϕ,X,Y,Z)(\phi,X,Y,Z) in the right-hand side can be translated back into functions of (ϕ,X¯,Y¯,Z¯)(\phi,\bar{X},\bar{Y},\bar{Z}) by use of (23) and (25).*4*4*4The above analysis shows that the transformation D¯:(g¯μν,ϕ)(gμν,ϕ)\bar{D}\colon(\bar{g}_{\mu\nu},\phi)\mapsto(g_{\mu\nu},\phi) defined by (28) is the left inverse of the transformation D:(gμν,ϕ)(g¯μν,ϕ)D\colon(g_{\mu\nu},\phi)\mapsto(\bar{g}_{\mu\nu},\phi) defined by (15), i.e., D¯D(gμν,ϕ)=(gμν,ϕ)\bar{D}\circ D(g_{\mu\nu},\phi)=(g_{\mu\nu},\phi). Since the left inverse of a group element is also its right inverse, it follows that DD¯(g¯μν,ϕ)=(g¯μν,ϕ)D\circ\bar{D}(\bar{g}_{\mu\nu},\phi)=(\bar{g}_{\mu\nu},\phi).

To summarize, we have obtained a set of sufficient conditions for the generalized disformal transformation (15) to be invertible. The conditions are summarized as

F00,0,X¯X0,X¯Y=X¯Z=0,|(Y¯,Z¯)(Y,Z)|0.F_{0}\neq 0,\qquad\mathcal{F}\neq 0,\qquad\bar{X}_{X}\neq 0,\qquad\bar{X}_{Y}=\bar{X}_{Z}=0,\qquad\left|\frac{\partial(\bar{Y},\bar{Z})}{\partial(Y,Z)}\right|\neq 0. (29)

This set of conditions can be used not only as a simple criterion for the invertibility of a given transformation of the form (15) but also as a useful tool to construct invertible generalized disformal transformations as we shall see below. In order for the condition X¯Y=X¯Z=0\bar{X}_{Y}=\bar{X}_{Z}=0 and X¯X0\bar{X}_{X}\neq 0 to be satisfied, let us take X¯=X¯0(ϕ,X)\bar{X}=\bar{X}_{0}(\phi,X) as an input, with X¯0\bar{X}_{0} being an arbitrary function of (ϕ,X)(\phi,X) such that X¯0X0\bar{X}_{0X}\neq 0. Then, by use of (23), e.g., the function F3F_{3} is written in terms of X¯0\bar{X}_{0}, F0F_{0}, F1F_{1}, and F2F_{2} as

F3=XF0X¯0(ϕ,X)[F0(F0+XF1+2YF2)+F22(Y2XZ)]Y2XZ+X¯0(ϕ,X)[ZF0F1(Y2XZ)].F_{3}=\frac{XF_{0}-\bar{X}_{0}(\phi,X)\left[F_{0}(F_{0}+XF_{1}+2YF_{2})+F_{2}^{2}(Y^{2}-XZ)\right]}{Y^{2}-XZ+\bar{X}_{0}(\phi,X)\left[ZF_{0}-F_{1}(Y^{2}-XZ)\right]}. (30)

Therefore, we obtain invertible transformations by choosing the functions X¯0\bar{X}_{0}, F0F_{0}, F1F_{1}, and F2F_{2} so that they satisfy the remaining conditions in (29), i.e., F00F_{0}\neq 0, 0\mathcal{F}\neq 0, and |(Y¯,Z¯)/(Y,Z)|0|\partial(\bar{Y},\bar{Z})/\partial(Y,Z)|\neq 0. In particular, for the above F3F_{3}, the condition 0\mathcal{F}\neq 0 yields

[YF0+F2(Y2XZ)]20.\mathcal{F}\propto\left[YF_{0}+F_{2}(Y^{2}-XZ)\right]^{2}\neq 0. (31)

We shall use this strategy to construct a nontrivial example of invertible transformations of the form (15) in §III.1.

A caveat here is that the transformation law could be ill defined for some particular configuration of (gμν,ϕ)(g_{\mu\nu},\phi). Nevertheless, it is still possible to perform the invertible disformal transformation g¯μν=g¯μν[gαβ,ϕ]\bar{g}_{\mu\nu}=\bar{g}_{\mu\nu}[g_{\alpha\beta},\phi] on some seed action of scalar-tensor theories S¯[g¯μν,ϕ]\bar{S}[\bar{g}_{\mu\nu},\phi] to generate a new action S[gμν,ϕ]S[g_{\mu\nu},\phi]. For instance, provided that X¯0\bar{X}_{0}, F0F_{0}, and F1F_{1} are regular functions, the denominator of (30) vanishes for configurations with Y=Z=0Y=Z=0, which happens when X=constX={\rm const}. This means that, even if the new action S[gμν,ϕ]S[g_{\mu\nu},\phi] admits a solution with X=constX={\rm const}, one cannot map the solution via the disformal transformation to generate a solution in the original frame. On the other hand, so long as we consider configurations for which the transformation law is well defined, there is one-to-one correspondence between the configuration space in the new frame and the one in the original frame.

One may think that arbitrary tensors of the form Φμνnϕμα1ϕα1α2ϕαn1ν\Phi_{\mu\nu}^{n}\coloneqq\phi_{\mu}^{\alpha_{1}}\phi_{\alpha_{1}}^{\alpha_{2}}\cdots\phi_{\alpha_{n-1}\nu} (e.g., Φμν1=ϕμν\Phi_{\mu\nu}^{1}=\phi_{\mu\nu} and Φμν2=ϕμαϕαν\Phi_{\mu\nu}^{2}=\phi_{\mu}^{\alpha}\phi_{\alpha\nu}) and/or scalar quantities constructed from gμνg_{\mu\nu}, ϕμ\phi_{\mu}, and Φμνn\Phi_{\mu\nu}^{n} (e.g., ϕ\Box\phi and ϕαβϕβα\phi_{\alpha}^{\beta}\phi_{\beta}^{\alpha}) can be included in the transformation law (15). For instance, one could consider transformations of the form (2), in which a term with ϕμν\phi_{\mu\nu} is present. In this case, one can make use of the Cayley-Hamilton theorem, which allows us to write any Φμνn\Phi_{\mu\nu}^{n} with nDn\geq D in terms of gμν,ϕμν,Φμν2,,ΦμνD1g_{\mu\nu},\phi_{\mu\nu},\Phi_{\mu\nu}^{2},\cdots,\Phi_{\mu\nu}^{D-1}. Therefore, considering a transformation composed of gμν,ϕμν,Φμν2,,ΦμνD1g_{\mu\nu},\phi_{\mu\nu},\Phi_{\mu\nu}^{2},\cdots,\Phi_{\mu\nu}^{D-1}, the property [A] may be satisfied, which allows us to systematically construct the inverse metric. However, as mentioned earlier, a composition of such transformations generates various terms with the third-order derivative of the scalar field as well as the second-order derivative of the metric through the Christoffel symbol [see (51) and (54)], which are not contained in the original transformation law. Hence, it is practically difficult to remove all such terms, implying that the property [B] cannot be satisfied in general. This explains why transformations of the form (2) are noninvertible, as shown in Babichev et al. (2021). The reason why we could obtain a concise invertibility condition for the transformation (15) is that there is only a single function X¯(ϕ,X,Y,Z)\bar{X}(\phi,X,Y,Z) that controls whether or not the class of transformations is closed under the functional composition. The point is that, so long as the conditions in (29) are satisfied, the Christoffel symbols are encapsulated in two sets of scalar quantities (Y,Z)(Y,Z) and (Y¯,Z¯)(\bar{Y},\bar{Z}), between which the invertibility is manifest.

As a final remark, the above discussion can be extended to more general transformations containing the third derivative of ϕ\phi,

g¯μν=\displaystyle\bar{g}_{\mu\nu}=\; F0gμν+F1ϕμϕν+2F2ϕ(μXν)+F3XμXν+2F4ϕ(μYν)+2F5ϕ(μZν)+2F6X(μYν)+2F7X(μZν)\displaystyle F_{0}g_{\mu\nu}+F_{1}\phi_{\mu}\phi_{\nu}+2F_{2}\phi_{(\mu}X_{\nu)}+F_{3}X_{\mu}X_{\nu}+2F_{4}\phi_{(\mu}Y_{\nu)}+2F_{5}\phi_{(\mu}Z_{\nu)}+2F_{6}X_{(\mu}Y_{\nu)}+2F_{7}X_{(\mu}Z_{\nu)}
+F8YμYν+2F9Y(μZν)+F10ZμZν,\displaystyle+F_{8}Y_{\mu}Y_{\nu}+2F_{9}Y_{(\mu}Z_{\nu)}+F_{10}Z_{\mu}Z_{\nu}, (32)

where YμμYY_{\mu}\coloneqq\partial_{\mu}Y, ZμμZZ_{\mu}\coloneqq\partial_{\mu}Z, and here

Fi=Fi(ϕ,X,Y,Z,ϕμYμ,ϕμZμ,XμYμ,XμZμ,YμYμ,YμZμ,ZμZμ).F_{i}=F_{i}(\phi,X,Y,Z,\phi_{\mu}Y^{\mu},\phi_{\mu}Z^{\mu},X_{\mu}Y^{\mu},X_{\mu}Z^{\mu},Y_{\mu}Y^{\mu},Y_{\mu}Z^{\mu},Z_{\mu}Z^{\mu}). (33)

Likewise, it is straightforward to include arbitrarily higher-order derivatives of ϕ\phi in the transformation. Rather than presenting a general discussion, we shall provide an example of invertible disformal transformations with the third derivative of ϕ\phi in §III.2.

III Examples

III.1 Example with the second derivative of the scalar field

As an example of invertible disformal transformations of the form (15), let us consider the case with F0=1F_{0}=1, F1=F2=0F_{1}=F_{2}=0, and F3=F3(ϕ,X,Y,Z)0F_{3}=F_{3}(\phi,X,Y,Z)\neq 0, i.e.,

g¯μν=gμν+F3(ϕ,X,Y,Z)XμXν.\bar{g}_{\mu\nu}=g_{\mu\nu}+F_{3}(\phi,X,Y,Z)X_{\mu}X_{\nu}. (34)

In this case, we have

X¯(ϕ,X,Y,Z)=XF3(Y2XZ)1+ZF3,\bar{X}(\phi,X,Y,Z)=\frac{X-F_{3}(Y^{2}-XZ)}{1+ZF_{3}}, (35)

which we require to be a function only of (ϕ,X)(\phi,X). Assuming that X¯=X+P(ϕ,X)\bar{X}=X+P(\phi,X) with P0P\neq 0 and PX1P_{X}\neq-1, from (30) we have

F3=P(ϕ,X)Y2+ZP(ϕ,X),F_{3}=-\frac{P(\phi,X)}{Y^{2}+ZP(\phi,X)}, (36)

for which the transformation law of the metric is explicitly written as

g¯μν=gμνP(ϕ,X)Y2+ZP(ϕ,X)XμXν.\bar{g}_{\mu\nu}=g_{\mu\nu}-\frac{P(\phi,X)}{Y^{2}+ZP(\phi,X)}X_{\mu}X_{\nu}. (37)

Then, the inverse metric is given by

g¯μν=gμν+P(ϕ,X)Y2XμXν.\bar{g}^{\mu\nu}=g^{\mu\nu}+\frac{P(\phi,X)}{Y^{2}}X^{\mu}X^{\nu}. (38)

We also have

Y¯=(1+PX)(Y+ZPY)+Pϕ(X+P),Z¯=(1+PX)(Y+ZPY)[ZY(1+PX)+2Pϕ]+Pϕ2(X+P),\begin{split}\bar{Y}&=(1+P_{X})\left(Y+\frac{ZP}{Y}\right)+P_{\phi}(X+P),\\ \bar{Z}&=(1+P_{X})\left(Y+\frac{ZP}{Y}\right)\left[\frac{Z}{Y}(1+P_{X})+2P_{\phi}\right]+P_{\phi}^{2}(X+P),\end{split} (39)

which can be inverted as

Y=Y¯2Z¯PPϕ(X¯P)(2Y¯X¯Pϕ)(1+PX)(Y¯X¯Pϕ),Z=Z¯Pϕ(2Y¯X¯Pϕ)(1+PX)(Y¯X¯Pϕ)Y.\begin{split}Y&=\frac{\bar{Y}^{2}-\bar{Z}P-P_{\phi}(\bar{X}-P)(2\bar{Y}-\bar{X}P_{\phi})}{(1+P_{X})(\bar{Y}-\bar{X}P_{\phi})},\\ Z&=\frac{\bar{Z}-P_{\phi}(2\bar{Y}-\bar{X}P_{\phi})}{(1+P_{X})(\bar{Y}-\bar{X}P_{\phi})}Y.\end{split} (40)

The inverse disformal transformation takes the form,

gμν=g¯μν+PY¯2Z¯PPϕ(X¯P)(2Y¯X¯Pϕ)(Pϕ2ϕμϕν2Pϕϕ(μX¯ν)+X¯μX¯ν),g_{\mu\nu}=\bar{g}_{\mu\nu}+\frac{P}{\bar{Y}^{2}-\bar{Z}P-P_{\phi}(\bar{X}-P)(2\bar{Y}-\bar{X}P_{\phi})}\left(P^{2}_{\phi}\phi_{\mu}\phi_{\nu}-2P_{\phi}\phi_{(\mu}\bar{X}_{\nu)}+\bar{X}_{\mu}\bar{X}_{\nu}\right), (41)

where XX in the arguments of PP and PϕP_{\phi} is regarded as a function of (ϕ,X¯)(\phi,\bar{X}) by solving X¯=X+P(ϕ,X)\bar{X}=X+P(\phi,X) for XX. Note that, while the transformation (37) does not contain either ϕμϕν\phi_{\mu}\phi_{\nu} or ϕ(μXν)\phi_{(\mu}X_{\nu)}, in general these terms show up in the inverse transformation (41). If P=P(X)P=P(X), such terms vanish in (41). The simplest case would be P(ϕ,X)=c0P(\phi,X)=c_{0} with c0c_{0} being a nonvanishing constant, for which the disformal transformation (37) and its inverse (41) are explicitly written as

g¯μν=gμνc0Y2+c0ZXμXν,gμν=g¯μν+c0Y¯2c0Z¯X¯μX¯ν.\bar{g}_{\mu\nu}=g_{\mu\nu}-\frac{c_{0}}{Y^{2}+c_{0}Z}X_{\mu}X_{\nu},\qquad g_{\mu\nu}=\bar{g}_{\mu\nu}+\frac{c_{0}}{\bar{Y}^{2}-c_{0}\bar{Z}}\bar{X}_{\mu}\bar{X}_{\nu}. (42)

III.2 Example with the third derivative of the scalar field

Let us now consider another example of invertible transformations of the following form:

g¯μν=V2XU2ZV2(X+c1)U2Z[gμν+c1ZV2XU2Z+c1(V2WZ)ZμZν],\bar{g}_{\mu\nu}=\frac{V^{2}X-U^{2}Z}{V^{2}(X+c_{1})-U^{2}Z}\left[g_{\mu\nu}+\frac{c_{1}Z}{V^{2}X-U^{2}Z+c_{1}(V^{2}-WZ)}Z_{\mu}Z_{\nu}\right], (43)

where c1c_{1} is a nonvanishing constant and we have defined

UϕμZμ,VXμZμ,WZμZμ.U\coloneqq\phi_{\mu}Z^{\mu},\qquad V\coloneqq X_{\mu}Z^{\mu},\qquad W\coloneqq Z_{\mu}Z^{\mu}. (44)

This transformation is of the form (32) and the third derivative of ϕ\phi appears in Zμ=8ϕαϕβαμ(ϕγϕγβ)Z_{\mu}=8\phi_{\alpha}\phi^{\alpha}_{\beta}\nabla_{\mu}(\phi^{\gamma}\phi^{\beta}_{\gamma}). The inverse metric takes the form

g¯μν=V2(X+c1)U2ZV2XU2Z[gμνc1ZV2(X+c1)U2ZZμZν].\bar{g}^{\mu\nu}=\frac{V^{2}(X+c_{1})-U^{2}Z}{V^{2}X-U^{2}Z}\left[g^{\mu\nu}-\frac{c_{1}Z}{V^{2}(X+c_{1})-U^{2}Z}Z^{\mu}Z^{\nu}\right]. (45)

Then, the relevant scalar quantities transform as follows:

X¯=X+c1,Z¯=Z,U¯U=V¯V=W¯W=1+c1(V2WZ)V2XU2Z.\bar{X}=X+c_{1},\qquad\bar{Z}=Z,\qquad\frac{\bar{U}}{U}=\frac{\bar{V}}{V}=\frac{\bar{W}}{W}=1+\frac{c_{1}(V^{2}-WZ)}{V^{2}X-U^{2}Z}. (46)

Note that the property [B] is guaranteed by Z¯U=Z¯V=Z¯W=0\bar{Z}_{U}=\bar{Z}_{V}=\bar{Z}_{W}=0, which is a natural generalization of the condition X¯Y=X¯Z=0\bar{X}_{Y}=\bar{X}_{Z}=0 in (29).*5*5*5It should also be noted that Y¯\bar{Y} takes the form, Y¯=Y+c1V(VYUZ)V2XU2Z,\bar{Y}=Y+\frac{c_{1}V(VY-UZ)}{V^{2}X-U^{2}Z}, and hence has a nontrivial dependence on UU and VV, but this does not spoil the invertibility as the transformation (43) is independent of YY. On the other hand, if the transformation law had a nontrivial YY dependence, then Y¯\bar{Y} should satisfy Y¯U=Y¯V=Y¯W=0\bar{Y}_{U}=\bar{Y}_{V}=\bar{Y}_{W}=0. The relations in (46) can be solved for the unbarred quantities as

X=X¯c1,Z=Z¯,UU¯=VV¯=WW¯=1c1(V¯2W¯Z¯)V¯2X¯U¯2Z¯.X=\bar{X}-c_{1},\qquad Z=\bar{Z},\qquad\frac{U}{\bar{U}}=\frac{V}{\bar{V}}=\frac{W}{\bar{W}}=1-\frac{c_{1}(\bar{V}^{2}-\bar{W}\bar{Z})}{\bar{V}^{2}\bar{X}-\bar{U}^{2}\bar{Z}}. (47)

Hence, the inverse transformation is obtained as follows:

gμν=V¯2X¯U¯2Z¯V¯2(X¯c1)U¯2Z¯[g¯μνc1Z¯V¯2X¯U¯2Z¯c1(V¯2W¯Z¯)Z¯μZ¯ν].g_{\mu\nu}=\frac{\bar{V}^{2}\bar{X}-\bar{U}^{2}\bar{Z}}{\bar{V}^{2}(\bar{X}-c_{1})-\bar{U}^{2}\bar{Z}}\left[\bar{g}_{\mu\nu}-\frac{c_{1}\bar{Z}}{\bar{V}^{2}\bar{X}-\bar{U}^{2}\bar{Z}-c_{1}(\bar{V}^{2}-\bar{W}\bar{Z})}\bar{Z}_{\mu}\bar{Z}_{\nu}\right]. (48)

IV Generalized disformal transformation of scalar-tensor theories

As mentioned earlier, substituting the transformation law of a disformal transformation g¯μν=g¯μν[gαβ,ϕ]\bar{g}_{\mu\nu}=\bar{g}_{\mu\nu}[g_{\alpha\beta},\phi] into some seed action of scalar-tensor theories S¯[g¯μν,ϕ]\bar{S}[\bar{g}_{\mu\nu},\phi], we obtain a new action SS as a functional of gμνg_{\mu\nu} and ϕ\phi. In this section, we use DHOST theories known so far as a seed and discuss what action is obtained as a result of the generalized disformal transformation.

The known classes of DHOST theories in four dimensions are described by the action of the following form Langlois and Noui (2016); Crisostomi et al. (2016); Ben Achour et al. (2016); Takahashi and Kobayashi (2017); Langlois et al. (2019):

S¯[g¯μν,ϕ]=d4xg¯[a¯0(ϕ,X¯)R¯+a¯1(ϕ,X¯)G¯μν¯μ¯νϕ+¯(g¯μν,ϕ,¯μϕ,¯μ¯νϕ)],\bar{S}[\bar{g}_{\mu\nu},\phi]=\int{\rm d}^{4}x\sqrt{-\bar{g}}\left[\bar{a}_{0}(\phi,\bar{X})\bar{R}+\bar{a}_{1}(\phi,\bar{X})\bar{G}^{\mu\nu}\bar{\nabla}_{\mu}\bar{\nabla}_{\nu}\phi+\bar{\mathcal{L}}(\bar{g}_{\mu\nu},\phi,\bar{\nabla}_{\mu}\phi,\bar{\nabla}_{\mu}\bar{\nabla}_{\nu}\phi)\right], (49)

with R¯\bar{R} and G¯μν\bar{G}_{\mu\nu} being respectively the Ricci scalar and the Einstein tensor in the original frame. Here, ¯\bar{\mathcal{L}} is a scalar quantity constructed from g¯μν\bar{g}_{\mu\nu}, ϕ\phi, ¯μϕ\bar{\nabla}_{\mu}\phi, and ¯μ¯νϕ\bar{\nabla}_{\mu}\bar{\nabla}_{\nu}\phi. We discuss how the action (49) is transformed under the generalized disformal transformation (15). Note that the first covariant derivative of the scalar field remains unchanged (namely, ¯μϕ=ϕμ\bar{\nabla}_{\mu}\phi=\phi_{\mu}) and that the transformation law for X¯\bar{X} is given by (23). Hence, in what follows, we derive the transformation law for the other building blocks of the action (49), i.e., the square root of the metric determinant g¯\sqrt{-\bar{g}}, the Ricci tensor R¯μν\bar{R}_{\mu\nu}, and the second covariant derivative of the scalar field ¯μ¯νϕ\bar{\nabla}_{\mu}\bar{\nabla}_{\nu}\phi.

By repeated use of the matrix determinant lemma, we obtain*6*6*6In DD-dimensional spacetime, we have g¯/g=F0(D2)/21/2\sqrt{-\bar{g}}/\sqrt{-g}=F_{0}^{(D-2)/2}\mathcal{F}^{1/2}.

g¯g=F01/2,\frac{\sqrt{-\bar{g}}}{\sqrt{-g}}=F_{0}\mathcal{F}^{1/2}, (50)

with \mathcal{F} defined in (20). Here, we have assumed F0>0F_{0}>0 and >0\mathcal{F}>0, which are necessary to preserve the metric signature. The change of the Christoffel symbol is a tensor, which is written as follows:

CλμνΓ¯μνλΓμνλ=g¯λα((μg¯ν)α12αg¯μν).C^{\lambda}{}_{\mu\nu}\coloneqq\bar{\Gamma}^{\lambda}_{\mu\nu}-\Gamma^{\lambda}_{\mu\nu}=\bar{g}^{\lambda\alpha}\left(\nabla_{(\mu}\bar{g}_{\nu)\alpha}-\frac{1}{2}\nabla_{\alpha}\bar{g}_{\mu\nu}\right). (51)

In terms of this CλμνC^{\lambda}{}_{\mu\nu}, the Ricci tensor in the original frame can be expressed as

R¯μν\displaystyle\bar{R}_{{\mu\nu}} =Rμν+2[αCα+ν]μ2CαCββ[αν]μ\displaystyle=R_{{\mu\nu}}+2\nabla_{[\alpha}C^{\alpha}{}_{\nu]\mu}+2C^{\alpha}{}_{\beta[\alpha}C^{\beta}{}_{\nu]\mu}
=Rμν+2¯[αCαν]μ2CαCββ[α,ν]μ\displaystyle=R_{{\mu\nu}}+2\bar{\nabla}_{[\alpha}C^{\alpha}{}_{\nu]\mu}-2C^{\alpha}{}_{\beta[\alpha}C^{\beta}{}_{\nu]\mu}, (52)

where T[μν](TμνTνμ)/2T_{[{\mu\nu}]}\coloneqq(T_{\mu\nu}-T_{\nu\mu})/2. The Ricci scalar in the original frame can be written in the form,

R¯=g¯μνR¯μν=g¯μν(Rμν2CαCββ[α)ν]μ+2¯α(g¯μ[νCα])μν,\bar{R}=\bar{g}^{\mu\nu}\bar{R}_{\mu\nu}=\bar{g}^{\mu\nu}\left(R_{{\mu\nu}}-2C^{\alpha}{}_{\beta[\alpha}C^{\beta}{}_{\nu]\mu}\right)+2\bar{\nabla}_{\alpha}\left(\bar{g}^{\mu[\nu}C^{\alpha]}{}_{\mu\nu}\right), (53)

where the last term is the covariant divergence associated with g¯μν\bar{g}_{\mu\nu}. Also, the tensor CλμνC^{\lambda}{}_{\mu\nu} shows up in the transformation law for the second derivative of ϕ\phi as

¯μ¯νϕ=ϕμνCλϕλμν.\bar{\nabla}_{\mu}\bar{\nabla}_{\nu}\phi=\phi_{\mu\nu}-C^{\lambda}{}_{\mu\nu}\phi_{\lambda}. (54)

The above relations allow us to systematically compute the transformation of the action (49). Since CλμνC^{\lambda}{}_{\mu\nu} contains the derivative of g¯μν\bar{g}_{\mu\nu} in which there are second derivatives of ϕ\phi, the resultant action contains the third or higher derivatives of ϕ\phi in general. It should be noted that so long as the transformation (15) is invertible, the number of DOFs does not change under the transformation Domènech et al. (2015); Takahashi et al. (2017). Hence, the generalized disformal transformation (15) can generate a new class of higher-derivative ghost-free theories, which itself is closed under the same class of transformations. Also, performing the generalized disformal transformation on the known minimally modified gravity theories Lin and Mukohyama (2017); Chagoya and Tasinato (2019); Aoki et al. (2018); Afshordi et al. (2007); Iyonaga et al. (2018, 2020); Gao and Yao (2020) (i.e., those without a propagating scalar DOF) yields a novel class of minimally modified gravity.

Given the above transformation rules for the building blocks, it is straightforward to write down the transformation of the action (49). Since the full expression is quite involved, here we demonstrate the transformation of the following subclass of the action:

S¯0[g¯μν,ϕ]d4xg¯[a¯0(ϕ)R¯+K¯(ϕ,X¯)],\bar{S}_{0}[\bar{g}_{\mu\nu},\phi]\coloneqq\int{\rm d}^{4}x\sqrt{-\bar{g}}\,[\bar{a}_{0}(\phi)\bar{R}+\bar{K}(\phi,\bar{X})], (55)

which reduces to the Einstein-Hilbert action with a canonical scalar field when a¯0=MPl2/2\bar{a}_{0}=M_{\rm Pl}^{2}/2 and K¯=X¯/2\bar{K}=-\bar{X}/2 with MPl2M_{\rm Pl}^{2} being the reduced Planck mass. Note that, if a¯0\bar{a}_{0} has a nontrivial dependence on X¯\bar{X}, this action itself does not yield a degenerate theory. When a¯0X¯0\bar{a}_{0\bar{X}}\neq 0, one has to take into account quadratic terms of ¯μ¯νϕ\bar{\nabla}_{\mu}\bar{\nabla}_{\nu}\phi to render the theory degenerate. Applying the above transformation rules, we obtain

S¯0[gμν,ϕ]=d4xgF01/2[a¯0g¯μν(Rμν2CαCββ[α)ν]μ2a¯0αg¯μ[νCα]+μνK¯(ϕ,X¯)],\bar{S}_{0}[g_{\mu\nu},\phi]=\int{\rm d}^{4}x\sqrt{-g}\,F_{0}\mathcal{F}^{1/2}\left[\bar{a}_{0}\bar{g}^{\mu\nu}\left(R_{{\mu\nu}}-2C^{\alpha}{}_{\beta[\alpha}C^{\beta}{}_{\nu]\mu}\right)-2\bar{a}_{0\alpha}\bar{g}^{\mu[\nu}C^{\alpha]}{}_{{\mu\nu}}+\bar{K}(\phi,\bar{X})\right], (56)

with a¯0μμa¯0=a¯0ϕϕμ\bar{a}_{0\mu}\coloneqq\partial_{\mu}\bar{a}_{0}=\bar{a}_{0\phi}\phi_{\mu}. In particular, for transformations of the form (37), we have

S¯0=d4xg1/2{\displaystyle\bar{S}_{0}=\int{\rm d}^{4}x\sqrt{-g}\,\mathcal{F}^{1/2}\bigg{\{} a¯0(gαβF3XαXβ)(RαβF322XγγXαβ+F342Zαβ)\displaystyle\bar{a}_{0}\left(g^{\alpha\beta}-\frac{F_{3}}{\mathcal{F}}X^{\alpha}X^{\beta}\right)\left(R_{\alpha\beta}-\frac{F_{3}}{2\mathcal{F}^{2}}X^{\gamma}\mathcal{F}_{\gamma}X_{\alpha\beta}+\frac{F_{3}}{4\mathcal{F}^{2}}Z_{\alpha}\mathcal{F}_{\beta}\right)
1a¯0α[Xαβ(XβF3)ZF3α12ZαF3]+K¯(ϕ,X+P(ϕ,X))},\displaystyle-\frac{1}{\mathcal{F}}\bar{a}_{0\alpha}\left[X^{\alpha}\nabla_{\beta}(X^{\beta}F_{3})-ZF_{3}^{\alpha}-\frac{1}{2}Z^{\alpha}F_{3}\right]+\bar{K}(\phi,X+P(\phi,X))\bigg{\}}, (57)

with F3μ=F3ϕϕμ+F3XXμ+F3YYμ+F3ZZμF_{3\mu}=F_{3\phi}\phi_{\mu}+F_{3X}X_{\mu}+F_{3Y}Y_{\mu}+F_{3Z}Z_{\mu} and

F3=P(ϕ,X)Y2+ZP(ϕ,X),=1+ZF3=Y2Y2+ZP(ϕ,X).F_{3}=-\frac{P(\phi,X)}{Y^{2}+ZP(\phi,X)},\qquad\mathcal{F}=1+ZF_{3}=\frac{Y^{2}}{Y^{2}+ZP(\phi,X)}. (58)

Thus, as mentioned earlier, the resultant action contains the third derivative of ϕ\phi. Moreover, there is a new type of higher-order derivative coupling to the curvature tensor of the form XαXβRαβX^{\alpha}X^{\beta}R_{\alpha\beta}. Clearly, one would obtain even higher-order derivatives of ϕ\phi and other new types of coupling such as ϕαXβRαβ\phi^{\alpha}X^{\beta}R_{\alpha\beta} or ZαZβRαβZ^{\alpha}Z^{\beta}R_{\alpha\beta} if one considers the more general transformation (32). Nevertheless, since it is generated from the ghost-free action via the invertible transformation, this higher-derivative action describes a healthy degenerate theory, i.e., there are at most three propagating DOFs without the Ostrogradsky ghosts.

V Conclusions

In the present paper, we studied a higher-derivative generalization of the disformal transformation, with a special focus on transformations of the form (15), which we recapitulate here:

g¯μν=F0gμν+F1μϕνϕ+2F2(μϕν)X+F3μXνX,\bar{g}_{\mu\nu}=F_{0}g_{\mu\nu}+F_{1}\nabla_{\mu}\phi\nabla_{\nu}\phi+2F_{2}\nabla_{(\mu}\phi\nabla_{\nu)}X+F_{3}\nabla_{\mu}X\nabla_{\nu}X, (59)

with FiF_{i}’s (i=0,1,2,3i=0,1,2,3) being functions of ϕ\phi, X=μϕμϕX=\nabla_{\mu}\phi\nabla^{\mu}\phi, Y=μϕμXY=\nabla_{\mu}\phi\nabla^{\mu}X, and Z=μXμXZ=\nabla_{\mu}X\nabla^{\mu}X. For this type of transformation, we derived the invertibility conditions (29) focusing on the group structure and explicitly constructed its inverse transformation (28). Our construction of the inverse transformation is based on the following two properties: [A] the closedness under the matrix product and [B] the closedness under the functional composition. With these two properties, the generalized disformal transformations form a group with respect to the matrix product and the functional composition, which allows us to systematically construct the inverse metric and the inverse transformation in a fully covariant manner. This strategy can be straightforwardly extended to even more general disformal transformations, e.g., of the form (32). Our results hold in general DD-dimensional spacetime. Moreover, it also applies to the vector disformal transformation Kimura et al. (2017) and the multidisformal transformation Watanabe et al. (2015); Firouzjahi et al. (2018), the former of which is discussed in the Appendix. We also investigated the generalized disformal transformation of known DHOST theories which contain up to the second derivative of the scalar field. As a consequence, we obtained a new class of ghost-free theories containing the third or higher derivatives of the scalar field as well as novel derivative couplings to the curvature tensor, e.g., RαβαXβXR_{\alpha\beta}\nabla^{\alpha}X\nabla^{\beta}X.

There are several interesting directions for further studies. One of them is to study cosmology in the novel class of theories obtained via the generalized disformal transformation. In particular, it would be important to study which subclass accommodates models where the speed of gravitational waves coincides with that of light, in accordance with the almost simultaneous detection of the gravitational waves GW170817 and the γ\gamma-ray burst 170817A emitted from a binary neutron star merger Abbott et al. (2017a, b, c). Applied to the early universe, especially cosmological inflation, it would be important to clarify the frame invariance of cosmological perturbations by extending the analysis in Alinea and Kubota (2021); Minamitsuji (2021a). Investigating how the generalized disformal coupling affects the screening mechanism would also be intriguing. Another direction of interest is to see how the known solutions in scalar-tensor theories are transformed under (15), following the works Anson et al. (2021); Ben Achour et al. (2020b). Note that the new terms in the transformation law (15) depend on the derivative of the scalar kinetic term XX, meaning that they become trivial for solutions with XX being constant Babichev and Charmousis (2014); Kobayashi and Tanahashi (2014); Babichev and Esposito-Farèse (2017); Babichev et al. (2017, 2018); Ben Achour and Liu (2019); Motohashi and Minamitsuji (2019); Minamitsuji and Edholm (2019); Khoury et al. (2020); Babichev et al. (2017); Charmousis et al. (2019); Takahashi and Motohashi (2020), while there would be a nontrivial contribution for solutions with a nonconstant XX Babichev et al. (2017); Minamitsuji and Edholm (2020); Ben Achour et al. (2020a). We leave these issues for future work.

Acknowledgements.
K.T. was supported by JSPS (Japan Society for the Promotion of Science) KAKENHI Grant No. JP21J00695. H.M. was supported by JSPS KAKENHI Grant No. JP18K13565. M.M. was supported by the Portuguese national fund through the Fundação para a Ciência e a Tecnologia in the scope of the framework of the Decree-Law 57/2016 of August 29, changed by Law 57/2017 of July 19, and the Centro de Astrofísica e Gravitação through the Project No. UIDB/00099/2020. M.M. also would like to thank Yukawa Institute for Theoretical Physics for the hospitality under the Visitors Program of FY2021. *

Appendix A Vector disformal transformations with derivatives

In the main text, we constructed an invertible disformal transformation with higher derivatives (15) as a generalization of the conventional disformal transformation (1) in the context of scalar-tensor theories. A similar transformation was also studied in the context of vector-tensor theories Kimura et al. (2017), which is explicitly written as

g¯μν=F0gμν+F1AμAν,\bar{g}_{\mu\nu}=F_{0}g_{\mu\nu}+F_{1}A_{\mu}A_{\nu}, (60)

with the vector field AμA_{\mu} unchanged. Here, F0F_{0} and F1F_{1} are functions of XAμAμX\coloneqq A_{\mu}A^{\mu}. In this appendix, we construct invertible disformal transformations with the derivative of AμA_{\mu}. Note that the following results reduce to those in §II under the replacement AμϕμA_{\mu}\to\phi_{\mu}, while the dependence on ϕ\phi without derivative is not reproduced. We shall adopt a notation similar to the one used in the main text to make the correspondence clear. Namely, X,Y,Z,Fi,X,Y,Z,F_{i},\mathcal{F} in this appendix are the vector counterparts corresponding to the ones defined for the case of scalar field.

Let us consider a metric transformation in DD dimensions defined by

g¯μν=F0gμν+F1AμAν+2F2A(μXν)+F3XμXν,\bar{g}_{\mu\nu}=F_{0}g_{\mu\nu}+F_{1}A_{\mu}A_{\nu}+2F_{2}A_{(\mu}X_{\nu)}+F_{3}X_{\mu}X_{\nu}, (61)

where XμμX=2AαμAαX_{\mu}\coloneqq\partial_{\mu}X=2A^{\alpha}\nabla_{\mu}A_{\alpha}. Here, FiF_{i}’s (i=0,1,2,3i=0,1,2,3) are functions of (X,Y,Z)(X,Y,Z), in which YY and ZZ are defined as follows:

YAμXμ,ZXμXμ.Y\coloneqq A_{\mu}X^{\mu},\qquad Z\coloneqq X_{\mu}X^{\mu}. (62)

It is straightforward to verify that the transformation (61) satisfies the property [A], i.e., the closedness under the matrix product. Therefore, one can systematically construct the inverse metric g¯μν\bar{g}^{\mu\nu}, and the result is given by

g¯μν=1F0[gμνF0F1Z(F22F1F3)AμAν2F0F2+Y(F22F1F3)A(μXν)F0F3X(F22F1F3)XμXν],\bar{g}^{\mu\nu}=\frac{1}{F_{0}}\bigg{[}g^{\mu\nu}-\frac{F_{0}F_{1}-Z(F_{2}^{2}-F_{1}F_{3})}{\mathcal{F}}A^{\mu}A^{\nu}-2\frac{F_{0}F_{2}+Y(F_{2}^{2}-F_{1}F_{3})}{\mathcal{F}}A^{(\mu}X^{\nu)}-\frac{F_{0}F_{3}-X(F_{2}^{2}-F_{1}F_{3})}{\mathcal{F}}X^{\mu}X^{\nu}\bigg{]}, (63)

with \mathcal{F} defined by

F02+F0(XF1+2YF2+ZF3)+(F22F1F3)(Y2XZ).\mathcal{F}\coloneqq F_{0}^{2}+F_{0}(XF_{1}+2YF_{2}+ZF_{3})+(F_{2}^{2}-F_{1}F_{3})(Y^{2}-XZ). (64)

Hence, we have

X¯=g¯μνAμAν=XF0F3(Y2XZ),\bar{X}=\bar{g}^{\mu\nu}A_{\mu}A_{\nu}=\frac{XF_{0}-F_{3}(Y^{2}-XZ)}{\mathcal{F}}, (65)

which is a function of (X,Y,Z)(X,Y,Z) in general. As we did in §II, we require X¯Y=X¯Z=0\bar{X}_{Y}=\bar{X}_{Z}=0 [i.e., X¯=X¯(X)\bar{X}=\bar{X}(X)] so that the transformation satisfies the property [B], i.e., the closedness under the functional composition. We also assume X¯X0\bar{X}_{X}\neq 0 so that we can solve the relation X¯=X¯(X)\bar{X}=\bar{X}(X) for XX to have X=X(X¯)X=X(\bar{X}). Then, we have

Y¯=g¯μνAμX¯ν=X¯XYF0+F2(Y2XZ),Z¯=g¯μνX¯μX¯ν=X¯X2ZF0F1(Y2XZ).\begin{split}\bar{Y}&=\bar{g}^{\mu\nu}A_{\mu}\bar{X}_{\nu}=\bar{X}_{X}\frac{YF_{0}+F_{2}(Y^{2}-XZ)}{\mathcal{F}},\\ \bar{Z}&=\bar{g}^{\mu\nu}\bar{X}_{\mu}\bar{X}_{\nu}=\bar{X}_{X}^{2}\frac{ZF_{0}-F_{1}(Y^{2}-XZ)}{\mathcal{F}}.\end{split} (66)

Here, we require that these two equations can be solved for YY and ZZ to obtain Y=Y(X¯,Y¯,Z¯)Y=Y(\bar{X},\bar{Y},\bar{Z}) and Z=Z(X¯,Y¯,Z¯)Z=Z(\bar{X},\bar{Y},\bar{Z}). The inverse transformation is written as

gμν=1F0(g¯μνF1AμAν2F2X¯XA(μX¯ν)F3X¯X2X¯μX¯ν),g_{\mu\nu}=\frac{1}{F_{0}}\left(\bar{g}_{\mu\nu}-F_{1}A_{\mu}A_{\nu}-2\frac{F_{2}}{\bar{X}_{X}}A_{(\mu}\bar{X}_{\nu)}-\frac{F_{3}}{\bar{X}_{X}^{2}}\bar{X}_{\mu}\bar{X}_{\nu}\right), (67)

where the functions of (X,Y,Z)(X,Y,Z) in the right-hand side can be translated into functions of (X¯,Y¯,Z¯)(\bar{X},\bar{Y},\bar{Z}) by use of (65) and (66).

For vector-tensor theories, further generalization including the field strength tensor Fμν2[μAν]F_{\mu\nu}\coloneqq 2\partial_{[\mu}A_{\nu]} would also be possible. Note that FμνF_{\mu\nu} vanishes in the scalar limit AμϕμA_{\mu}\to\phi_{\mu}, and hence such an extension is peculiar to the vector disformal transformation. The disformal transformation with FμνF_{\mu\nu} in four dimensions was first studied in Gümrükçüoğlu and Namba (2019), which has the form

g¯μν=Ω(F2,F4)gμν+Γ(F2,F4)Fμν2,\bar{g}_{\mu\nu}=\Omega(\langle F^{2}\rangle,\langle F^{4}\rangle)g_{\mu\nu}+\Gamma(\langle F^{2}\rangle,\langle F^{4}\rangle)F^{2}_{\mu\nu}, (68)

with FμνnFμFα1α1α2Fαn1νF^{n}_{\mu\nu}\coloneqq F_{\mu}{}^{\alpha_{1}}F_{\alpha_{1}}{}^{\alpha_{2}}\cdots F_{\alpha_{n-1}\nu} and FngμνFμνn\langle F^{n}\rangle\coloneqq g^{\mu\nu}F^{n}_{\mu\nu} (n=2,4,6,n=2,4,6,\cdots). For instance, we have Fμν2=FμFαναF^{2}_{\mu\nu}=F_{\mu}{}^{\alpha}F_{\alpha\nu} and F2=FαFββα\langle F^{2}\rangle=F_{\alpha}{}^{\beta}F_{\beta}{}^{\alpha}. Interestingly, this was shown to be the most general metric transformation in four dimensions that consists of FμνF_{\mu\nu} and its dual De Felice and Naruko (2020). Note that the transformation (68) does not contain the derivative of the metric, and hence the invertibility condition can be obtained by simply requiring that the Jacobian determinant is nonvanishing Gümrükçüoğlu and Namba (2019). It should be noted that the Cayley-Hamilton theorem yields

Fμν4=12F2Fμν2+(14F418F22)gμν,F^{4}_{\mu\nu}=\frac{1}{2}\langle F^{2}\rangle F^{2}_{\mu\nu}+\left(\frac{1}{4}\langle F^{4}\rangle-\frac{1}{8}\langle F^{2}\rangle^{2}\right)g_{\mu\nu}, (69)

in four dimensions, which allows us to express any FμνnF_{\mu\nu}^{n} with n4n\geq 4 as a linear combination of gμνg_{\mu\nu} and Fμν2F_{\mu\nu}^{2}. Thanks to this relation, the transformation (68) can satisfy both the properties [A] and [B]. Likewise, it could in principle be possible to incorporate FμνF_{\mu\nu} into the transformation law (61) to obtain a more nontrivial class of invertible vector disformal transformations. However, it should be noted that the matrix identity following from the Cayley-Hamilton theorem is dimension dependent, and hence a dimension-independent expression for the inverse transformation would no longer be available in this case.

References