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Multiple steady states and the form of response functions to antigen in a model for the initiation of T cell activation

Alan D. Rendall
Institut für Mathematik
Johannes Gutenberg-Universität
Staudingerweg 9
D-55099 Mainz
Germany

and

Eduardo D. Sontag
Department of Mathematics and the Center for Quantitative Biology
Rutgers University
Piscataway, NJ 08854
USA
Abstract

The aim of this paper is to study the qualitative behaviour predicted by a mathematical model for the initial stage of T cell activation. The state variables in the model are the concentrations of phosphorylation states of the T cell receptor complex and the phosphatase SHP-1 in the cell. It is shown that these quantities cannot approach zero and that the model possesses more than one positive steady state for certain values of the parameters. It can also exhibit damped oscillations. It is proved that the chemical concentration which represents the degree of activation of the cell, that of the maximally phosphorylated form of the T cell receptor complex, is in general a non-monotone function of the activating signal. In particular there are cases where there is a value of the dissociation constant of the ligand from the receptor which produces an optimal activation of the T cell. In this way the results of certain simulations in the literature have been confirmed rigorously and some important features which had not previously been seen have been discovered.

1 Introduction

In humans and other vertebrates the immune system is of crucial importance for protecting an individual from dangers such as pathogens, toxins and cancer. (For background information on immunology we refer to [12].) The central players in the immune system are the white blood cells (leukocytes) and it is important that these cells be able to distinguish between dangerous substances and host tissues. This is often referred to as the distinction between non-self and self. A failure to combat dangerous substances may lead to infectious diseases becoming life-threatening. On the other hand, if the immune system attacks host tissues this can lead to autoimmune disease. The task of discrimination is complicated. An important element of the process of distinction between self and non-self is the activity of the class of leukocytes called T cells. An individual T cell is supposed to recognize a particular substance (antigen) and take suitable action if that substance is dangerous. Recognition is based on the binding of the antigen to a molecule on the T cell surface, the T cell receptor (TCR). It is believed that the most important aspect of this process is the time the antigen remains bound before being released (the dissociation time), an idea which has been called the ’lifetime dogma’ [4]. When it recognizes its antigen the T cell changes its behaviour and is said to be activated. In what follows we study a mathematical model for what happens in the first few minutes after a T cell recognizes its antigen.

In [1] Altan-Bonnet and Germain introduced a model for the initial stage of T cell activation. Simulations using this model gave results which fitted a number of experimental findings. On the other hand it was too elaborate to be readily accessible to a mathematical analysis of its dynamics. In [5] the authors introduced a radically simplified version of the model of [1]. The new model includes the essential explanatory power of the old one while being much more transparent and tractable for analytical investigation. It also made some new predictions which were confirmed experimentally. In [5] a number of interesting analytical calculations were performed but the mathematical conclusions which can be drawn from these were not worked out in detail.

The aim of the present paper is to obtain results about the qualitative behaviour of solutions of the model of [5] which are as general as possible. In Section 2 the model is defined and some of its basic properties are derived. The model describes a situation where both an agonist (the antigen which should be recognized) and an antagonist (a competing antigen) are present. Section 3 is concerned with the number of steady states and their stability. After some general results have been derived, the discussion turns to more detailed properties of the solutions in the case that the antagonist is absent and treats cases where the number NN of phosphorylation sites included in the model is small. In particular it is shown that when N=3N=3 there are parameters for which three positive steady states exist (Theorem 1). A numerical calculation reveals that for a specific choice of these parameters two of the steady states are stable while the third is a saddle. For N2N\leq 2 there is a unique steady state and in the case N=1N=1 it is proved to be globally asymptotically stable. There are parameter values for which the approach to this steady state is oscillatory.

The qualitative behaviour of the steady state concentration of the maximally phosphorylated state, which expresses the degree of activation of the T cell, as a function of the antigen concentration and the dissociation time, is investigated in the case where only the agonist is present in Section 4. Let us consider the function f(L1,ν1)f(L_{1},\nu_{1}), which expresses the degree of activation in terms of the parameters L1L_{1} (concentration of agonist ligand) and ν1\nu_{1} (reaction rate for the dissociation of the ligand from the receptor, i.e. the reciprocal of the dissociation time). It is shown that the dependence exhibits certain types of non-monotone behaviour in some cases. The results obtained include both rigorous results on general features of the function ff (Theorem 2) and simulations which reveal more detailed features. In particular it is found that are values of the parameters in the model for which the function ff has a maximum as a function of ν1\nu_{1} for fixed L1L_{1}. In other words, there is a value of the dissociation time which is optimal for T cell activation. Thus the model studied here is able to reproduce this fact which has been experimentally observed [10].

The analysis of the response function is extended to cover the effects of the antagonist in Section 5. The last section is devoted to conclusions and an outlook.

2 Definition of the model

In the introduction it was stated that a T cell recognizes an antigen. In more detail the molecule concerned is a peptide (a small protein) which is bound to a host molecule called an MHC molecule. Thus we talk about a pMHC complex as the object to be recognized. In the model of [5] two types of pMHC complexes are considered. The first, called an agonist, represents the case where the antigen comes from a pathogen and should activate the T cell. The second, called an antagonist, represents the case of a self-antigen, which should not activate the T cell. Detection takes place through the binding of a pMHC complex to the T cell receptor. When this happens certain proteins associated to the T cell receptor are phosphorylated, i.e. phosphate groups become attached to them. For simplicity we will describe this by saying that the receptor-pMHC complex is phosphorylated.

The reaction network for the model of [5] is shown in Figure 1.

Refer to caption
Figure 1: The model considered in this paper. The species RR represents the T cell receptor, and L1L_{1} and L2L_{2} are the two ligands, i.e. the agonist and antagonist. The species C0C_{0} represents unphosphorylated complexes of the T cell receptor with the agonist, and the CjC_{j}’s are the jj-phosphorylated complexes. The DjD_{j}’s are the analogous complexes for the antagonist. The phosphatase SHP-1 provides a negative feedback, and is represented by SS. The different reactions represent receptor complex phosphorylation with rate constant ϕ\phi and dephosphorylation with rate constant bb, as well as receptor complex dephosphorylation by SS with rate constant γ\gamma and dissociation rate constants ν1\nu_{1} and ν2\nu_{2}. Antigens bind to RR with rate constant κ\kappa, and SS is activated by the singly phosphorylated complexes with rate constant α\alpha and deactivated with rate constant β\beta.

The state variables will now be listed. The concentration of unphosphorylated complexes of the T cell receptor with the agonist will be denoted by C0C_{0} and the concentration of unphosphorylated complexes of the T cell receptor with the antagonist will be denoted by D0D_{0}. CjC_{j} and DjD_{j} are the corresponding quantities for the case of jj phosphorylations, up to a maximum value NN. The specific value of NN has little influence in what follows but it may be worth to note that a biologically reasonable value of NN could be as large as 20 while in the model of [1] we have N=9N=9. RR, L1L_{1} and L2L_{2} are the total concentrations of receptors and the two ligands, i.e. the agonist and antagonist. Another important element of the system is SHP-1. This substance is a phosphatase which means that when active it can remove phosphate groups from the receptor-pMHC complex. It contributes a negative feedback loop to the system. SS is the concentration of active SHP-1. The receptor complexes are subject to phosphorylation with rate constant ϕ\phi and dephosphorylation with rate constant bb. They are also dephosphorylated by SHP-1 with rate constant γ\gamma and dissociate with rate constants ν1\nu_{1} and ν2\nu_{2}. Antigens bind to the receptor with rate constant κ\kappa. SHP-1 is activated by the singly phosphorylated complexes with rate constant α\alpha and deactivated with rate constant β\beta. All the rate constants are assumed positive. STS_{T} is the total concentration of SHP-1. It is assumed that all reactions exhibit mass action kinetics and this leads to the following system of equations

S˙=α(C1+D1)(STS)βS,\displaystyle\dot{S}=\alpha(C_{1}+D_{1})(S_{T}-S)-\beta S, (1)
C˙0=κ(L1j=0NCj)(Rj=0N(Cj+Dj))+(b+γS)C1(ϕ+ν1)C0,\displaystyle\dot{C}_{0}=\kappa(L_{1}-\sum_{j=0}^{N}C_{j})(R-\sum_{j=0}^{N}(C_{j}+D_{j}))+(b+\gamma S)C_{1}-(\phi+\nu_{1})C_{0}, (2)
C˙j=ϕCj1+(b+γS)Cj+1(ϕ+b+γS+ν1)Cj, 1jN1,\displaystyle\dot{C}_{j}=\phi C_{j-1}+(b+\gamma S)C_{j+1}-(\phi+b+\gamma S+\nu_{1})C_{j},\ \ 1\leq j\leq N-1, (3)
C˙N=ϕCN1(b+γS+ν1)CN,\displaystyle\dot{C}_{N}=\phi C_{N-1}-(b+\gamma S+\nu_{1})C_{N}, (4)
D˙0=κ(L2j=0NDj)(Rj=0N(Cj+Dj))+(b+γS)D1(ϕ+ν2)D0,\displaystyle\dot{D}_{0}=\kappa(L_{2}-\sum_{j=0}^{N}D_{j})(R-\sum_{j=0}^{N}(C_{j}+D_{j}))+(b+\gamma S)D_{1}-(\phi+\nu_{2})D_{0}, (5)
D˙j=ϕDj1+(b+γS)Dj+1(ϕ+b+γS+ν2)Dj, 1jN1,\displaystyle\dot{D}_{j}=\phi D_{j-1}+(b+\gamma S)D_{j+1}-(\phi+b+\gamma S+\nu_{2})D_{j},\ \ 1\leq j\leq N-1, (6)
D˙N=ϕDN1(b+γS+ν2)DN.\displaystyle\dot{D}_{N}=\phi D_{N-1}-(b+\gamma S+\nu_{2})D_{N}. (7)

In a direct formulation of the system as arising from the reaction network it is necessary to include the concentrations of free ligands, free receptors and inactive phosphatase. This extended system has four conservation laws corresponding to the total amounts of ligands, receptors and phosphatase. Using these to eliminate the additional variables leads to the system (1)-(7).

The right hand sides of the equations are Lipschitz and so there is a unique solution corresponding to each choice of initial data. To have a biologically relevant solution the quantities in the extended system should be non-negative. It is a well-known fact for reaction networks of this type that data for which all concentrations are positive give rise to solutions with the same property and that data for which all concentrations are non-negative give rise to non-negative solutions. In terms of (1)-(7) this implies statements about the positivity of the quantities SS, CjC_{j} and DjD_{j} and of the differences STSS_{T}-S, Rj=0N(Cj+Dj)R-\sum_{j=0}^{N}(C_{j}+D_{j}), L1j=0NCjL_{1}-\sum_{j=0}^{N}C_{j} and L2j=0NDjL_{2}-\sum_{j=0}^{N}D_{j}. Let us call the region where all these quantities are strictly positive the biologically feasible region. Note that due to the conservation laws this region is bounded. Let Σ1=j=0NCj\Sigma_{1}=\sum_{j=0}^{N}C_{j} and Σ2=j=0NCj\Sigma_{2}=\sum_{j=0}^{N}C_{j}. Then it follows from (1)-(7) that

Σ˙1=κ(L1Σ1)(RΣ1Σ2)ν1Σ1,\displaystyle\dot{\Sigma}_{1}=\kappa(L_{1}-\Sigma_{1})(R-\Sigma_{1}-\Sigma_{2})-\nu_{1}\Sigma_{1}, (8)
Σ˙2=κ(L2Σ2)(RΣ1Σ2)ν2Σ2.\displaystyle\dot{\Sigma}_{2}=\kappa(L_{2}-\Sigma_{2})(R-\Sigma_{1}-\Sigma_{2})-\nu_{2}\Sigma_{2}. (9)

Lemma 1 Consider a solution (S(t),C0(t),,CN(t),D0(t),,DN(t))(S(t),C_{0}(t),\ldots,C_{N}(t),D_{0}(t),\ldots,D_{N}(t)) in the closure of the biologically feasible region. Then if (S,C0,,CN,D0,,DN)(S^{*},C_{0}^{*},\ldots,C_{N}^{*},D_{0}^{*},\ldots,D_{N}^{*}) is an ω\omega-limit point of this solution it is also in the biologically feasible region. In particular, any steady state is in the biologically feasible region.

Proof If S=STS^{*}=S_{T} we can consider the solution starting at that point at some time t0t_{0}. Since the ω\omega limit set of a given solution is invariant the solution under consideration lies entirely in the ω\omega-limit set of the original solution. In particular, it is contained in the closure of the biologically feasible region. The solution starting at the point with S=STS^{*}=S_{T} satisfies S˙(t0)<0\dot{S}(t_{0})<0 and therefore the inequality S(t)>STS(t)>S_{T} for tt slightly less than t0t_{0}, a contradiction. In a similar way equation (8) implies that j=0NCj\sum_{j=0}^{N}C^{*}_{j} cannot attain the value L1L_{1} and equation (9) implies that j=0NDj\sum_{j=0}^{N}D^{*}_{j} cannot attain the value L2L_{2}. Summing (8) and (9) shows that j=0NCj+j=0NDj\sum_{j=0}^{N}C^{*}_{j}+\sum_{j=0}^{N}D^{*}_{j} cannot attain the value RR.

Note next that C0C_{0} cannot be zero at an ω\omega-limit point. For if it were zero at such a point we could consider the solution passing through that point at a time t0t_{0}. The equation (2) would imply that C˙0(t0)>0\dot{C}_{0}(t_{0})>0 and that C0(t)<0C_{0}(t)<0 for tt slightly less than t0t_{0}, a contradiction. Once the positivity of C0C_{0} has been proved we can use equation (3) with j=1j=1 to show that C1C_{1} cannot be zero at an ω\omega-limit point. This in turn allows us to prove using (1) that SS can never be zero at an ω\omega-limit point. In a similar way it can be concluded successively that C2,,CNC_{2},\ldots,C_{N} and D0,,DND_{0},\ldots,D_{N} are positive at any ω\omega-limit point of a non-negative solution. This concludes the proof of the lemma.

The fact that all ω\omega-limit points of solutions in the closure of the biologically feasible region are in the biologically feasible region together with the fact that the closure of that region is compact implies that the infimum of the distance of a given solution to the boundary in the limit tt\to\infty is strictly positive. When this last property holds the system is said to be persistent [2]. Note in addition that the closure of the biologically feasible region is convex and hence homeomorphic to a closed ball in a Euclidean space. It follows from the Brouwer fixed point theorem that a steady state exists (cf. [7], Chapter I, Theorem 8.2). Since steady states on the boundary have already been excluded we can conclude that there is at least one steady state in the biologically feasible region for any fixed choice of parameters. That this is the case was assumed implicitly in [5].

3 Multiplicity of steady states

A question not addressed in [5] is whether there might exist more than one positive steady state for a fixed choice of parameters. In this section it will be shown that for some values of NN and the reaction constants this is the case. The aim is to find any parameter values with this property while not worrying for the moment how biologically relevant this choice of parameters is. Let f1f_{1} and f2f_{2} denote the right hand sides of equations (8) and (9). Then f1Σ2\frac{\partial f_{1}}{\partial\Sigma_{2}} and f2Σ1\frac{\partial f_{2}}{\partial\Sigma_{1}} are negative and hence the system (8)-(9) is competitive. It follows that every solution of this system converges to a steady state as tt\to\infty [8].

A steady state (Σ1,Σ2)(\Sigma_{1}^{*},\Sigma_{2}^{*}) of (8)-(9) satisfies the equations

κ(L1Σ1)(RΣ1Σ2)ν1Σ1=0,\displaystyle\kappa(L_{1}-\Sigma_{1}^{*})(R-\Sigma_{1}^{*}-\Sigma_{2}^{*})-\nu_{1}\Sigma_{1}^{*}=0, (10)
κ(L2Σ2)(RΣ1Σ2)ν2Σ2=0.\displaystyle\kappa(L_{2}-\Sigma_{2}^{*})(R-\Sigma_{1}^{*}-\Sigma_{2}^{*})-\nu_{2}\Sigma_{2}^{*}=0. (11)

We can solve for Σ1\Sigma_{1}^{*} and Σ2\Sigma_{2}^{*} as functions of Σ1+Σ2\Sigma_{1}^{*}+\Sigma_{2}^{*}.

Σ1=κL1(RΣ1Σ2)κ(RΣ1Σ2)+ν1,\displaystyle\Sigma_{1}^{*}=\frac{\kappa L_{1}(R-\Sigma_{1}^{*}-\Sigma_{2}^{*})}{\kappa(R-\Sigma_{1}^{*}-\Sigma_{2}^{*})+\nu_{1}}, (12)
Σ2=κL2(RΣ1Σ2)κ(RΣ1Σ2)+ν2.\displaystyle\Sigma_{2}^{*}=\frac{\kappa L_{2}(R-\Sigma_{1}^{*}-\Sigma_{2}^{*})}{\kappa(R-\Sigma_{1}^{*}-\Sigma_{2}^{*})+\nu_{2}}. (13)

Hence

κ(L1+L2Σ1Σ2)=κL1ν1κ(RΣ1Σ2)+ν1+κL2ν2κ(RΣ1Σ2)+ν2.\kappa(L_{1}+L_{2}-\Sigma_{1}^{*}-\Sigma_{2}^{*})=\frac{\kappa L_{1}\nu_{1}}{\kappa(R-\Sigma_{1}^{*}-\Sigma_{2}^{*})+\nu_{1}}+\frac{\kappa L_{2}\nu_{2}}{\kappa(R-\Sigma_{1}^{*}-\Sigma_{2}^{*})+\nu_{2}}. (14)

The function of Σ1+Σ2\Sigma_{1}^{*}+\Sigma_{2}^{*} on the left hand side of this equation is decreasing on the interval [0,L1+L2][0,L_{1}+L_{2}]. The function on the right hand side is increasing on the interval [0,R][0,R]. Their graphs can intersect in at most one point. We already know that they must intersect since a positive steady state of the full system exists. That they intersect can also be seen directly. For in all cases the left hand side is greater than the right hand side for Σ1+Σ2=0\Sigma_{1}^{*}+\Sigma_{2}^{*}=0 and the opposite inequality holds for Σ1+Σ2=min{L1+L2,R}\Sigma_{1}^{*}+\Sigma_{2}^{*}=\min\{L_{1}+L_{2},R\}. Thus the equation has a unique solution for Σ1+Σ2\Sigma_{1}^{*}+\Sigma_{2}^{*} in the interval [0,min{L1+L2,R}][0,\min\{L_{1}+L_{2},R\}] From this it is possible to compute values of Σ1\Sigma_{1}^{*} and Σ2\Sigma_{2}^{*} which solve (10) and (11) and lie in the intervals [0,min{L1,R}][0,\min\{L_{1},R\}] and [0,min{L2,R}][0,\min\{L_{2},R\}], respectively. The quantities Σ1\Sigma_{1}^{*} and Σ2\Sigma_{2}^{*} are functions of the parameters RR, L1L_{1}, L2L_{2}, κ\kappa, ν1\nu_{1} and ν2\nu_{2}.

It can be concluded that the solution passing through an ω\omega-limit point of a solution of the original system satisfies a simplified system containing Σ1\Sigma_{1}^{*} and Σ2\Sigma_{2}^{*} as parameters. C0C_{0} and D0D_{0} can be eliminated from this system in favour of the other CjC_{j} and DjD_{j}. The result is

S˙=α(C1+D1)(STS)βS,\displaystyle\dot{S}=\alpha(C_{1}+D_{1})(S_{T}-S)-\beta S, (15)
C˙1=ϕΣ1+(b+γSϕ)C2(2ϕ+b+γS+ν1)C1ϕj=3NCj\displaystyle\dot{C}_{1}=\phi\Sigma_{1}^{*}+(b+\gamma S-\phi)C_{2}-(2\phi+b+\gamma S+\nu_{1})C_{1}-\phi\sum_{j=3}^{N}C_{j} (16)
C˙j=ϕCj1+(b+γS)Cj+1(ϕ+b+γS+ν1)Cj, 2jN1,\displaystyle\dot{C}_{j}=\phi C_{j-1}+(b+\gamma S)C_{j+1}-(\phi+b+\gamma S+\nu_{1})C_{j},\ \ 2\leq j\leq N-1, (17)
C˙N=ϕCN1(b+γS+ν1)CN,\displaystyle\dot{C}_{N}=\phi C_{N-1}-(b+\gamma S+\nu_{1})C_{N}, (18)
D˙1=ϕΣ2+(b+γSϕ)D2(2ϕ+b+γS+ν2)D1ϕj=3NDj,\displaystyle\dot{D}_{1}=\phi\Sigma_{2}^{*}+(b+\gamma S-\phi)D_{2}-(2\phi+b+\gamma S+\nu_{2})D_{1}-\phi\sum_{j=3}^{N}D_{j}, (19)
D˙j=ϕDj1+(b+γS)Dj+1(ϕ+b+γS+ν2)Dj, 2jN1,\displaystyle\dot{D}_{j}=\phi D_{j-1}+(b+\gamma S)D_{j+1}-(\phi+b+\gamma S+\nu_{2})D_{j},\ \ 2\leq j\leq N-1, (20)
D˙N=ϕDN1(b+γS+ν2)DN.\displaystyle\dot{D}_{N}=\phi D_{N-1}-(b+\gamma S+\nu_{2})D_{N}. (21)

This form of the equations is valid for N3N\geq 3. In the case N=2N=2 it is still correct if it is taken into account that the condition 2jN12\leq j\leq N-1 is never satisfied so that the equations containing that condition are absent. The sum from j=3j=3 to NN is zero in that case. The case N=1N=1 is exceptional from the point of the notation.

In order to get more information we will restrict in the remainder of this section to what we call the agonist-only case. This is obtained from the system (1)-(7) by setting L2L_{2} and the DiD_{i} to zero. There is a corresponding limiting system, which is obtained from (15)-(21) by setting Σ2\Sigma_{2}^{*} and the DiD_{i} to zero. In this case we write Σ\Sigma^{*} instead of Σ1\Sigma_{1}^{*} for brevity. Consider the limiting system in the agonist-only case with N=1N=1. This is

S˙=αC1(STS)βS,\displaystyle\dot{S}=\alpha C_{1}(S_{T}-S)-\beta S, (22)
C˙1=ϕΣ(ϕ+b+γS+ν1)C1.\displaystyle\dot{C}_{1}=\phi\Sigma^{*}-(\phi+b+\gamma S+\nu_{1})C_{1}. (23)

Solving the equation S˙=0\dot{S}=0 for C1C_{1} and substituting the result into the equation C˙1=0\dot{C}_{1}=0 gives the quadratic equation

βγS2+[β(ϕ+b+ν1)+αϕΣ]SαϕΣST=0.\beta\gamma S^{2}+[\beta(\phi+b+\nu_{1})+\alpha\phi\Sigma^{*}]S-\alpha\phi\Sigma^{*}S_{T}=0. (24)

Since the quadratic polynomial has positive leading term and is negative for S=0S=0 it is clear that it has a unique positive root. It follows from (24) that this root is less than STS_{T}. Equation (23) implies that C1<ΣC_{1}<\Sigma^{*} at a steady state and so these quantities can be completed to a steady state of the original system by defining C0=ΣC1C_{0}=\Sigma^{*}-C_{1}. The steady state is unique in this case.

In the case N=2N=2 the equations are

S˙=αC1(STS)βS,\displaystyle\dot{S}=\alpha C_{1}(S_{T}-S)-\beta S, (25)
C˙1=ϕΣ(2ϕ+b+γS+ν1)C1+(ϕ+b+γS)C2,\displaystyle\dot{C}_{1}=\phi\Sigma^{*}-(2\phi+b+\gamma S+\nu_{1})C_{1}+(-\phi+b+\gamma S)C_{2}, (26)
C˙2=ϕC1(b+γS+ν1)C2.\displaystyle\dot{C}_{2}=\phi C_{1}-(b+\gamma S+\nu_{1})C_{2}. (27)

Proceeding in a manner analogous to what we did in the case N=1N=1 it is possible to get a cubic equation for SS in the case N=2N=2, which we can write schematically in the form p(S)=k=0NakSkp(S)=\sum_{k=0}^{N}a_{k}S^{k}. We have

a0=αST(b+ν1)ϕΣ,\displaystyle a_{0}=-\alpha S_{T}(b+\nu_{1})\phi\Sigma^{*},
a1=β[b(ϕ+b+ν1)+ν1(2ϕ+b+ν1)+ϕ2]+α(b+ν1)ϕΣαγSTϕΣ,\displaystyle a_{1}=\beta[b(\phi+b+\nu_{1})+\nu_{1}(2\phi+b+\nu_{1})+\phi^{2}]+\alpha(b+\nu_{1})\phi\Sigma^{*}-\alpha\gamma S_{T}\phi\Sigma^{*},
a2=βγ(ϕ+2b+2ν1)+αγϕΣ,\displaystyle a_{2}=\beta\gamma(\phi+2b+2\nu_{1})+\alpha\gamma\phi\Sigma^{*},
a3=βγ2.\displaystyle a_{3}=\beta\gamma^{2}.

The sequence of signs of the coefficients aia_{i} is either (,,+,+)(-,-,+,+) or (,+,+,+)(-,+,+,+). There is precisely one change of sign and thus by Descartes’ rule of signs the polynomial has precisely one positive root. Once a value of SS is given the values of C1C_{1} and C2C_{2} at the steady state can be determined successively. Following the arguments in the case N=1N=1 we see that S<STS<S_{T}, C1+C2<ΣC_{1}+C_{2}<\Sigma^{*} and that the steady state is unique.

In the case N=3N=3 the system is

S˙=αC1(STS)βS,\displaystyle\dot{S}=\alpha C_{1}(S_{T}-S)-\beta S, (28)
C˙1=ϕΣ(2ϕ+b+γS+ν1)C1+(ϕ+b+γS)C2ϕC3,\displaystyle\dot{C}_{1}=\phi\Sigma^{*}-(2\phi+b+\gamma S+\nu_{1})C_{1}+(-\phi+b+\gamma S)C_{2}-\phi C_{3}, (29)
C˙2=ϕC1(ϕ+b+γS+ν1)C2+(b+γS)C3,\displaystyle\dot{C}_{2}=\phi C_{1}-(\phi+b+\gamma S+\nu_{1})C_{2}+(b+\gamma S)C_{3}, (30)
C˙3=ϕC2(b+γS+ν1)C3.\displaystyle\dot{C}_{3}=\phi C_{2}-(b+\gamma S+\nu_{1})C_{3}. (31)

A calculation for N=3N=3 analogous to those already done gives a quartic polynomial. Its coefficients are

a0=[(b+ν1)2+ϕν1]αϕΣST,\displaystyle a_{0}=-[(b+\nu_{1})^{2}+\phi\nu_{1}]\alpha\phi\Sigma^{*}S_{T},
a1=βγ{(ϕ+b+ν1)[(b(b+ν1)+ν1(ϕ+b+ν1)]+ν1(ϕ+b+ν1)\displaystyle a_{1}=\beta\gamma\{(\phi+b+\nu_{1})[(b(b+\nu_{1})+\nu_{1}(\phi+b+\nu_{1})]+\nu_{1}(\phi+b+\nu_{1})
+ϕ2(b+ν1)+ϕ3}+[(b+ν1)2+ν1ϕ]αϕΣ2(b+ν1)αγϕΣST,\displaystyle+\phi^{2}(b+\nu_{1})+\phi^{3}\}+[(b+\nu_{1})^{2}+\nu_{1}\phi]\alpha\phi\Sigma^{*}-2(b+\nu_{1})\alpha\gamma\phi\Sigma^{*}S_{T},
a2=βγ{b(b+ν1)+ν1(ϕ+b+ν1)+2(ϕ+b+ν1)(b+ν1)+ϕν1+ϕ2}\displaystyle a_{2}=\beta\gamma\{b(b+\nu_{1})+\nu_{1}(\phi+b+\nu_{1})+2(\phi+b+\nu_{1})(b+\nu_{1})+\phi\nu_{1}+\phi^{2}\}
+2(b+ν1)αγϕΣγ2αϕΣST,\displaystyle+2(b+\nu_{1})\alpha\gamma\phi\Sigma^{*}-\gamma^{2}\alpha\phi\Sigma^{*}S_{T},
a3=β{2γ(b+ν1)+γ2(ϕ+b+ν1)}+γ2αϕΣ,\displaystyle a_{3}=\beta\{2\gamma(b+\nu_{1})+\gamma^{2}(\phi+b+\nu_{1})\}+\gamma^{2}\alpha\phi\Sigma^{*},
a4=βγ3.\displaystyle a_{4}=\beta\gamma^{3}.

The coefficient a0a_{0} is negative while a3a_{3} and a4a_{4} are positive. Unless a1>0a_{1}>0 and a2<0a_{2}<0 Descartes’ rule of signs implies that the polynomial only has one positive root. Otherwise the rule implies that it has one or three positive roots (counting multiplicity) but does not decide between these two cases.

It will now be shown that in the case N=3N=3 there are values of the coefficients for which the polynomial p(S)p(S) has three positive roots. To do this we vary the coefficients STS_{T} and ν1\nu_{1} in the system (28)-(31) and keep all others fixed. Note that these coefficients come from the parameters in the agonist-only case of (1)-(4). To obtain the desired variation of the coefficients we fix all parameters in (1)-(4) except STS_{T}, ν1\nu_{1} and κ\kappa and vary κ\kappa in such a way that ν1κ\frac{\nu_{1}}{\kappa} does not change. This ensures that Σ\Sigma^{*} does not change. In fact we may simplify the calculations by setting b=0b=0 since if three positive roots can be obtained in that case the same thing can be obtained for bb small and positive by continuity. Suppose that STS_{T} and ν1\nu_{1} depend on a parameter ϵ\epsilon with both of them being positive for ϵ>0\epsilon>0. Suppose in addition that in the limit ϵ0\epsilon\to 0 we have the asymptotic relations ST=S¯Tϵ1+o(ϵ1)S_{T}=\bar{S}_{T}\epsilon^{-1}+o(\epsilon^{-1}) and ν1=ν¯1ϵ4+o(ϵ4)\nu_{1}=\bar{\nu}_{1}\epsilon^{4}+o(\epsilon^{4}) for constants S¯T\bar{S}_{T} and ν¯1\bar{\nu}_{1}. Then we obtain asymptotic expansions a4=A4a_{4}=A_{4}, a3=A3+o(1)a_{3}=A_{3}+o(1), a1=A1+o(1)a_{1}=A_{1}+o(1) for positive constants A4A_{4}, A3A_{3} and A1A_{1}, a0=A0ϵ3+o(ϵ3)a_{0}=A_{0}\epsilon^{3}+o(\epsilon^{3}) for a constant A0<0A_{0}<0 and a2=A2ϵ1+o(ϵ1)a_{2}=A_{2}\epsilon^{-1}+o(\epsilon^{-1}) for a constant A2<0A_{2}<0. Let q(S)=ϵp(S)q(S)=\epsilon p(S). Then q(1)q(1) converges to A2A_{2} for ϵ0\epsilon\to 0 and is thus negative for ϵ\epsilon small enough. The same is true for p(1)p(1). On the other hand

p(ϵ2)=A0ϵ3+A1ϵ2+A2ϵ3+A3ϵ6+A4ϵ8+o(ϵ2)=A1ϵ2+o(ϵ2).p(\epsilon^{2})=A_{0}\epsilon^{3}+A_{1}\epsilon^{2}+A_{2}\epsilon^{3}+A_{3}\epsilon^{6}+A_{4}\epsilon^{8}+o(\epsilon^{2})=A_{1}\epsilon^{2}+o(\epsilon^{2}). (32)

Hence for ϵ\epsilon sufficiently small p(ϵ2)>0p(\epsilon^{2})>0. Putting these facts together shows that pp has three positive roots when ϵ\epsilon is small. For each of these roots the values of C1C_{1}, C2C_{2} and C3C_{3} at the steady state can be determined successively. S<STS<S_{T}, C1+C2+C3<ΣC_{1}+C_{2}+C_{3}<\Sigma^{*} and defining C0=Σ(C1+C2+C3)C_{0}=\Sigma^{*}-(C_{1}+C_{2}+C_{3}) gives a steady state of the original system.

It has already been noted that pp cannot have more than three positive roots. There are parameter values for which the positive steady state is unique. To see this it is enough to assume that STS_{T} is small while keeping the other parameters fixed. Then ai>0a_{i}>0 for all i>0i>0 and the polynomial can have no more that one positive root since its derivative has no positive root. These results can be summed up as follows:

Theorem 1 The agonist-only case of the system (1)-(7) has exactly one positive steady state for N=1N=1 and N=2N=2. In the case N=3N=3 there are parameters for which it has three positive steady states and it can never have more than three.

A concrete example of parameters for which there are three positive steady states is obtained by setting α\alpha, β\beta, γ\gamma, ϕ\phi, L1L_{1} and RR equal to one and choosing ST=10S_{T}=10, κ=2×104\kappa=2\times 10^{-4}, ν1=104\nu_{1}=10^{-4}. A computer calculation shows that the coordinates (S,C0,C1,C2,C3)(S^{*},C_{0}^{*},C_{1}^{*},C_{2}^{*},C_{3}^{*}) of the steady states are approximately

(1.1769,0.1570,0.1334,0.1133,0.0963),\displaystyle(1.1769,0.1570,0.1334,0.1133,0.0963), (33)
(0.0005,0.0001,0.0001,0.0003,0.4996),\displaystyle(0.0005,0.0001,0.0001,0.0003,0.4996), (34)
(0.2860,0.0085,0.0294,0.1028,0.3593).\displaystyle(0.2860,0.0085,0.0294,0.1028,0.3593). (35)

It shows in addition that while the first and second of these steady states are asymptotically stable the third is a saddle with a one-dimensional unstable manifold. A plot of the steady states as a function of the parameter L1L_{1}, see Figure 2, suggests that there is a fold bifurcation.

Refer to caption   Refer to caption

Figure 2: Multistability of steady states as a function of L1L_{1}. Shown is the coordinate C3C_{3}, but other coordinates behave similarly. Stable branches are shown in green colour and unstable in red. Left: linear scale, right: log-log scale. Parameters are α=1\alpha=1, ST=10S_{T}=10, β=1\beta=1, κ=2×104\kappa=2\times 10^{-4}, R=1R=1, b=0b=0, γ=1\gamma=1, ϕ=1\phi=1, ν1=1\nu_{1}=1.

For higher values of NN it is possible to derive a polynomial equation of degree N+1N+1 for SS. There is no obvious reason why this polynomial should not have an arbitrarily large number of positive roots for NN arbitrarily large. A simple upper bound is that the polynomial can have no more than NN positive roots for NN odd and no more than N+1N+1 for NN even.

In general it is difficult to obtain information about the stability of the steady states by analytic methods. In the case N=1N=1 the vector field defining the dynamical system has negative divergence and so by Dulac’s criterion und Poincaré-Bendixson theory all solutions converge to the steady state as tt\to\infty. The system can exhibit damped oscillations as will now be shown. To do this we choose parameters so that

αC1+β=ϕ+b+γS+ν1.\alpha C_{1}+\beta=\phi+b+\gamma S+\nu_{1}. (36)

For fixed values of the quantities RR and STS_{T} the quantities C1C_{1} and SS are bounded uniformly in the quantities appearing in (36). Thus if we make α\alpha and β\beta small while fixing the other parameters we can arrange that the left hand side is smaller than the right hand side. If starting from there we make β\beta large while fixing the other parameters we can arrange that the left hand side of (36) is greater than the right hand side. It follows that parameter values exist for which (36) holds. The reason why this is interesting is that the discriminant of the characteristic equation of the linearization is the sum of a term which vanishes when (36) holds and the expression 4αγ(STS)C1-4\alpha\gamma(S_{T}-S)C_{1}. Thus when (36) holds the linearization has eigenvalues with negative real part and non-zero imaginary part and there are damped oscillations.

An interesting limiting case of the agonist-only system is obtained by assuming that α=0\alpha=0 and S=0S=0. We refer to this as the kinetic proofreading system since it is closely related to McKeithan’s kinetic proofreading model [11]. In fact McKeithan only considered the case b=0b=0 but this makes no essential difference for the analysis which follows. It was observed by Sontag [13] that the deficiency zero theorem of chemical reaction network theory can be applied to McKeithan’s system to conclude that there is a unique steady state in each stoichiometric compatibility class and that this solution is asymptotically stable in its class. Strictly speaking chemical reaction network theory is applied to the extended system which includes free receptors and free ligand as variables. To show that the steady state is globally asymptotically stable it suffices to show that there are no ω\omega-limit points on the boundary. That this is the case can be proved just as we did for the full system above. The steady state is hyperbolic as follows from Appendix C of [3].

Consider now the full agonist-only system. Setting α=0\alpha=0 gives a system where the kinetic proofreading system is coupled to a system describing the decay of SS. The steady state of the kinetic proofreading system gives rise to a steady state of the agonist-only system with α=0\alpha=0 which is on the boundary of the biologically feasible region and is a hyperbolic sink. Denote its coordinates by (0,Cj)(0,C_{j}^{*}). For α\alpha small and positive there exists a hyperbolic sink which is a small perturbation of that for α=0\alpha=0. It must be in the biologically feasible region since C1>0C_{1}>0 there and equation (1) would imply that S˙>0\dot{S}>0 there if SS were negative. Thus for sufficiently small values of α\alpha there exists a positive steady state which is a hyperbolic sink (S(α),Cj(α))(S^{*}(\alpha),C_{j}^{*}(\alpha)) close to (0,Cj)(0,C_{j}^{*}). There exists a positive number rr such that for α\alpha sufficiently small, say αα0\alpha\leq\alpha_{0}, (S(α),Cj(α))(S^{*}(\alpha),C_{j}^{*}(\alpha)) is the only ω\omega-limit point of any solution in the open ball of radius rr about that steady state.

Let h(Cj)h(C_{j}) be the Lyapunov function in the proof of the deficiency zero theorem. It is known from general arguments that h˙0\dot{h}\leq 0 with equality only for Cj=CjC_{j}=C_{j}^{*}. It follows that on the complement of the ball of radius rr about the steady state the function h˙\dot{h} has a strictly negative maximum. We can consider the behaviour of the function hh for solutions of the system for positive α\alpha. For small α\alpha it is still a Lyapunov function on the complement of a small ball about the steady state while there are no ω\omega-limit points except the steady state itself within that ball. Hence for α\alpha sufficiently small a solution can have no ω\omega-limit points other than the steady state. It follows that for α\alpha small the steady state is globally asymptotically stable. Of course this means that the limiting system obtained from the agonist-only system by passing to a solution through an ω\omega-limit point also has a unique steady state which is globally asymptotically stable for α\alpha sufficiently small. A similar argument applies in the case of the full system (1)-(7) since in that case the system obtained by setting α\alpha and SS to zero is just the product of two copies of the corresponding system in the agonist-only case.

4 The response function

This section is concerned with the agonist-only system. From a biological point of view the essential input parameters to the system are the ligand concentration L1L_{1} and the binding time of the ligand to the receptor, which in the model corresponds to ν11\nu_{1}^{-1}. The latter is a measure of the signal strength. The essential output is the value of CNC_{N} which is a measure of the activation of the T cell. Given values of L1L_{1}, ν1\nu_{1} and the other parameters we can consider the value of CNC_{N} in a steady state. In fact it is more convenient to use the quantities logCN\log C_{N} and logL1\log L_{1}. This leads to a response function logCN=F(logL1,ν1)\log C^{*}_{N}=F(\log L_{1},\nu_{1}). If there is more than one steady state for a given choice of the parameters this has to be thought of as a multi-valued function. It might naively be thought that FF should be an increasing function of L1L_{1} and a decreasing function of ν1\nu_{1}: more antigen leads to more activation of the T cell and a longer binding time leads to more activation. This turns out not to be the case and the function FF is not a monotone function of its arguments. This was observed in the case of the dependence on L1L_{1} in the simulations of [5]. It is possible to understand intuitively how this situation can arise. An increase in the stimulation of the T cell leads to activation of SHP-1 and that in turn has a negative effect on the activation of the T cell. Many of the calculations in this section are guided by those in [5].

The behaviour of the response function will be estimated in various parameter ranges. In order to do this it is useful to parametrize the solutions in a certain manner which will now be described. In the case of a steady state the equation (3) is a linear difference equation for the CjC_{j} with constant coefficients. This suggests looking for power-law solutions, an idea which motivates the following result.

Lemma 2 Steady state solutions of equations (2)-(4) in the agonist-only case can be parametrized in the form

Cj=a+r+j+arjC_{j}=a_{+}r_{+}^{j}+a_{-}r_{-}^{j} (37)

where the coefficients r±r_{\pm} and a±a_{\pm} are positive and depend on SS. The quantities r+r_{+} and rr_{-} are given by

r±=ϕ+b+γS+ν1±(ϕ+b+γS+ν1)24ϕ(b+γS)2(b+γS)r_{\pm}=\frac{\phi+b+\gamma S+\nu_{1}\pm\sqrt{(\phi+b+\gamma S+\nu_{1})^{2}-4\phi(b+\gamma S)}}{2(b+\gamma S)} (38)

and satisfy r<1<r+r_{-}<1<r_{+}.

Proof Note first that the quantities r±r_{\pm} in (38) are the roots of the characteristic equation

ϕ+(b+γS)r2(ϕ+b+γS+ν1)r=0\phi+(b+\gamma S)r^{2}-(\phi+b+\gamma S+\nu_{1})r=0 (39)

associated to the difference equation already mentioned and it is obvious that they are positive. The fact that they satisfy the characteristic equation is equivalent to the condition that the CjC_{j} defined by (37) satisfy the steady state form of equation (3). That r<1<r+r_{-}<1<r_{+} can be seen by noting that the function on the left hand side of (39) is negative at r=1r=1. The condition that the quantities CjC_{j} satisfy the equations (2)-(4) with C˙j=0\dot{C}_{j}=0 is equivalent to the conditions that they satisfy (37) with r±r_{\pm} as in (38) and certain coefficients aa_{-} and a+a_{+} together with the equations obtained by substituting (37) into the equations C˙0=0\dot{C}_{0}=0 and C˙N=0\dot{C}_{N}=0. The explicit form of these last equations is

[(b+γS)r(ϕ+ν1)]a+[(b+γS)r+(ϕ+ν1)]a+=ν1j=0NCj\displaystyle[(b+\gamma S)r_{-}-(\phi+\nu_{1})]a_{-}+[(b+\gamma S)r_{+}-(\phi+\nu_{1})]a_{+}=-\nu_{1}\sum_{j=0}^{N}C_{j} (40)
rN1[ϕ(b+γS+ν1)r]a+r+N1[ϕ(b+γS+ν1)r+]a+=0.\displaystyle r_{-}^{N-1}[\phi-(b+\gamma S+\nu_{1})r_{-}]a_{-}+r_{+}^{N-1}[\phi-(b+\gamma S+\nu_{1})r_{+}]a_{+}=0. (41)

It follows from the discussion in Section 3 that j=0NCj\sum_{j=0}^{N}C_{j}, which was denoted there by Σ1\Sigma_{1}^{*}, is uniquely determined for fixed values of the parameters in (2)(4)(\ref{phen2})-(\ref{phen4}) and fixed SS. Thus for fixed values of these parameters and SS all quantities in (40) and (41) except aa_{-} and a+a_{+} are known. It will now be shown that these equations have a unique solution for aa_{-} and a+a_{+}. Note that

[ϕ(b+γS+ν1)r][ϕ(b+γS+ν1)r+]=ϕ2ν1b+γS,[\phi-(b+\gamma S+\nu_{1})r_{-}][\phi-(b+\gamma S+\nu_{1})r_{+}]=-\frac{\phi^{2}\nu_{1}}{b+\gamma S}, (42)

as can most easily be seen by multiplying out the left hand side of this equation and substituting for r+rr_{+}r_{-} and r++rr_{+}+r_{-}, which are the sum and product of the roots of the characteristic equation (39). Thus equation (41) gives a positive expression for a+/aa_{+}/a_{-}. Note also that (42) implies that the factors in the product on the left hand side of that equation have opposite signs. Since r<r+r_{-}<r_{+} the first factor is positive and the second negative. Substituting the expression for a+/aa_{+}/a_{-} into (40) gives an equation of the form

a[AB(r/r+)N1]=ν1Σ1[ϕ(b+γS+ν1)r+]a_{-}[A-B(r_{-}/r_{+})^{N-1}]=-\nu_{1}\Sigma_{1}^{*}[\phi-(b+\gamma S+\nu_{1})r_{+}] (43)

whose right hand side is positive. Here

A=[(b+γS)r(ϕ+ν1)][ϕ(b+γS+ν1)r+]\displaystyle A=[(b+\gamma S)r_{-}-(\phi+\nu_{1})][\phi-(b+\gamma S+\nu_{1})r_{+}] (44)
B=[(b+γS)r+(ϕ+ν1)][ϕ(b+γS+ν1)r]\displaystyle B=[(b+\gamma S)r_{+}-(\phi+\nu_{1})][\phi-(b+\gamma S+\nu_{1})r_{-}] (45)

It follows from the fact that the first factor on the left hand side of (42) is positive that the first factor in the expression for AA is negative and hence that AA itself is positive. In addition, a straightforward computation shows that A>BA>B. If BB were not positive then the quantity in square brackets on the left hand side of (43) would be positive. If BB is positive then the fact that r<r+r_{-}<r_{+} implies that the quantity in square brackets is again positive. Hence in any case (43) can be solved to give a unique positive value of aa_{-}. Then a+a_{+} can be determined in such a way that (40) and (41) hold. This completes the proof of Lemma 2.

Lemma 2 shows that for fixed parameters in (2)-(4) and a fixed value of SS the steady state values of all the CjC_{j} are determined but this does not yet give expressions for the CjC_{j} which can be directly applied to study the properties of the response function. For the purposes of what follows it is convenient to rewrite (8) in the form

κ(L1j=0NCj)(Rj=0NCj)ν1j=0NCj=0.\kappa(L_{1}-\sum_{j=0}^{N}C_{j})(R-\sum_{j=0}^{N}C_{j})-\nu_{1}\sum_{j=0}^{N}C_{j}=0. (46)

The equation for SS can be solved to give the relation S=STC1C1+CS=S_{T}\frac{C_{1}}{C_{1}+C_{*}} with C=βαC_{*}=\frac{\beta}{\alpha}. Summing the expression for CjC_{j} given in Lemma 2 over jj gives

j=0NCj=a+r+N+11r+1+arN+11r1.\sum_{j=0}^{N}C_{j}=a_{+}\frac{r_{+}^{N+1}-1}{r_{+}-1}+a_{-}\frac{r_{-}^{N+1}-1}{r_{-}-1}. (47)

The following equation relating aa_{-} and a+a_{+} is equation (21) of [5].

a+=a(rr+)N+1r+1r1.a_{+}=-a_{-}\left(\frac{r_{-}}{r_{+}}\right)^{N+1}\frac{r_{+}-1}{r_{-}-1}. (48)

Combining the last two equations gives

j=0NCj=a1r[1(rr+)N+1].\sum_{j=0}^{N}C_{j}=\frac{a_{-}}{1-r_{-}}\left[1-\left(\frac{r_{-}}{r_{+}}\right)^{N+1}\right]. (49)

Having completed the necessary preliminaries we now proceed to study the qualitative behaviour of the reponse function in different regimes. When L1L_{1} is small it is to be expected that the concentration of the phosphatase is small and that the response function resembles that of the kinetic proofreading model. It will now be shown that when L1L_{1} is small the leading term in the function FF depends linearly on logL1\log L_{1} with slope one and the additive constant in this linear function will be determined. The equation (46) can be written in the form

j=0NCj=κRL1κR+ν1[1+L1R((j=0NCj/L1)2(j=0NCj/L1))].\sum_{j=0}^{N}C_{j}=\frac{\kappa RL_{1}}{\kappa R+\nu_{1}}\left[1+\frac{L_{1}}{R}\left((\sum_{j=0}^{N}C_{j}/L_{1})^{2}-(\sum_{j=0}^{N}C_{j}/L_{1})\right)\right]. (50)

Note that j=0NCjL1\sum_{j=0}^{N}C_{j}\leq L_{1} so that this equation implies that

j=0NCj=κRL1κR+ν1(1+qL1/R).\sum_{j=0}^{N}C_{j}=\frac{\kappa RL_{1}}{\kappa R+\nu_{1}}(1+qL_{1}/R). (51)

where 14<q<0-\frac{1}{4}<q<0. Using (48) it is possible to write down an explicit expression for CNC_{N}, namely

CN=arN(r+r)r+(1r).C_{N}=\frac{a_{-}r_{-}^{N}(r_{+}-r_{-})}{r_{+}(1-r_{-})}. (52)

It follows from (49) that

CN=rN1rr+1(rr+)N+1j=0NCj.C_{N}=r_{-}^{N}\frac{1-\frac{r_{-}}{r_{+}}}{1-(\frac{r_{-}}{r_{+}})^{N+1}}\sum_{j=0}^{N}C_{j}. (53)

Combining these equations gives

CN={rN1rr+1(rr+)N+1κRκR+ν1}L1(1+qL1/R).C_{N}=\left\{r_{-}^{N}\frac{1-\frac{r_{-}}{r_{+}}}{1-(\frac{r_{-}}{r_{+}})^{N+1}}\frac{\kappa R}{\kappa R+\nu_{1}}\right\}L_{1}(1+qL_{1}/R). (54)

The function of rr_{-} and r+r_{+} in this equation defines a function of SS. This function of SS tends to a positive limiting value as S0S\to 0. Now C1j=0NCi=O(L1)C_{1}\leq\sum_{j=0}^{N}C_{i}=O(L_{1}) and S=O(C1)S=O(C_{1}). Hence for RR fixed we can replace the function of r+r_{+} and rr_{-} in the above expression by its limiting value for S0S\to 0. If the resulting relation is plotted logarithmically it gives a straight line of slope one as the leading order approximation in the limit logL1\log L_{1}\to-\infty.

Next we look at an intermediate regime where the amount of activated SHP-1 is well away from both zero and STS_{T}. As a first step, we obtain an estimate for rr_{-} which is sharper than that in Lemma 2. To do this we compute the left hand side of the characteristic equation (39) for r=ϕϕ+ν1r=\frac{\phi}{\phi+\nu_{1}}. The result is ϕν1(b+γS)(ϕ+ν1)2<0-\frac{\phi\nu_{1}(b+\gamma S)}{(\phi+\nu_{1})^{2}}<0. It follows that r<ϕϕ+ν1r_{-}<\frac{\phi}{\phi+\nu_{1}}. Hence 1r>ν1ϕ+ν11-r_{-}>\frac{\nu_{1}}{\phi+\nu_{1}}. Substituting this into (49) gives a>ν1ϕ+ν1(j=0NCj)a_{-}>\frac{\nu_{1}}{\phi+\nu_{1}}\left(\sum_{j=0}^{N}C_{j}\right). Note that SSTmin{C12C,12}\frac{S}{S_{T}}\geq\min\left\{\frac{C_{1}}{2C_{*}},\frac{1}{2}\right\}. Hence a positive lower bound for C1C_{1} implies a positive lower bound for SST\frac{S}{S_{T}}.

Next we will derive a lower bound for γS\gamma S in the case that STS_{T} is large. This will be proved by contradiction. Suppose that γSρ\gamma S\leq\rho for some ρ>0\rho>0. Then it follows from the characteristic equation that rϕϕ+ρ+ν1r_{-}\geq\frac{\phi}{\phi+\rho+\nu_{1}}. Using this in the equation for C1C_{1} gives C1ϕν1(ϕ+ν1)(ϕ+ρ+ν1)(j=0NCj)C_{1}\geq\frac{\phi\nu_{1}}{(\phi+\nu_{1})(\phi+\rho+\nu_{1})}\left(\sum_{j=0}^{N}C_{j}\right). It follows that

SSTmin{ϕν12C(ϕ+ν1)(ϕ+ρ+ν1)(j=0NCj),12}S\geq S_{T}\min\left\{\frac{\phi\nu_{1}}{2C_{*}(\phi+\nu_{1})(\phi+\rho+\nu_{1})}\left(\sum_{j=0}^{N}C_{j}\right),\frac{1}{2}\right\} (55)

It is then clear that for a given value of ρ\rho and fixed values of the parameters other than STS_{T} this leads to a contradiction if STS_{T} is sufficiently large. In other words, given any ρ>0\rho>0 there is a lower bound for STS_{T} which implies that γSρ\gamma S\geq\rho. It is convenient to make the restrictions that κR1\kappa R\geq 1 and L1/R1L_{1}/R\leq 1 since then it is possible to replace j=0NCj\sum_{j=0}^{N}C_{j} in (55) by 3L14(1+ν1)\frac{3L_{1}}{4(1+\nu_{1})} by using (51).

From (38) it can be concluded that

r=ϕb+γS(1+O(η)),\displaystyle r_{-}=\frac{\phi}{b+\gamma S}(1+O(\eta)), (56)
r+=1+O(η).\displaystyle r_{+}=1+O(\eta). (57)

where η=ϕ+ν1b+γS\eta=\frac{\phi+\nu_{1}}{b+\gamma S}. This gives approximate expressions for the roots of the characteristic equation if ϕ+ν1b+γS\frac{\phi+\nu_{1}}{b+\gamma S} is small. As a consequence of these equations

rr+=ϕb+γS(1+O(η)).\frac{r_{-}}{r_{+}}=\frac{\phi}{b+\gamma S}(1+O(\eta)). (58)

Taking the expression for C1C_{1} supplied by Lemma 2 and using (48), (49) and (51) gives

C1=rκRL1κR+ν1(1+O(η)).C_{1}=r_{-}\frac{\kappa RL_{1}}{\kappa R+\nu_{1}}(1+O(\eta)). (59)

This implies that C1=O(η)C_{1}=O(\eta) and the expression relating SS and C1C_{1} then shows that SST=O(η)\frac{S}{S_{T}}=O(\eta). In fact

C1=CSST(1+O(η))C_{1}=\frac{C_{*}S}{S_{T}}(1+O(\eta)) (60)

These relations indicate that in leading order rr_{-} is proportional to SS. However it is also the case that

r=1Sϕγ11+b/(γS)(1+O(η))r_{-}=\frac{1}{S}\frac{\phi}{\gamma}\frac{1}{1+b/(\gamma S)}(1+O(\eta)) (61)

which indicates that in leading order rr_{-} is proportional to S1S^{-1}. Hence

r=C(κR+ν1)κRL1STS(1+O(η))r_{-}=\frac{C_{*}(\kappa R+\nu_{1})}{\kappa RL_{1}S_{T}}S(1+O(\eta)) (62)

and

r=1Sϕγ(1+O(η)).r_{-}=\frac{1}{S}\frac{\phi}{\gamma}(1+O(\eta^{\prime})). (63)

where η=max{η,b/(γS)}\eta^{\prime}=\max\{\eta,b/(\gamma S)\}. Combining these two relations gives

S=ϕκRSTL1Cγ(κR+ν1)(1+O(η)).S=\sqrt{\frac{\phi\kappa RS_{T}L_{1}}{C_{*}\gamma(\kappa R+\nu_{1})}}(1+O(\eta^{\prime})). (64)

Substituting this back into the equation for rr_{-} gives

r=ϕC(κR+ν1)γSTL1κR(1+O(η)).r_{-}=\sqrt{\frac{\phi C_{*}(\kappa R+\nu_{1})}{\gamma S_{T}L_{1}\kappa R}}(1+O(\eta^{\prime})). (65)

This means that

CN=(j=0NCj)rN(1+O(η′′))\displaystyle C_{N}=(\sum_{j=0}^{N}C_{j})r_{-}^{N}(1+O(\eta^{\prime\prime}))
=(κR+ν1κRL1)N/21(ϕCγST)N/2(1+O(η′′))\displaystyle=\left(\frac{\kappa R+\nu_{1}}{\kappa RL_{1}}\right)^{N/2-1}\left(\frac{\phi C_{*}}{\gamma S_{T}}\right)^{N/2}(1+O(\eta^{\prime\prime}))
=(ϕβαγST)N/2(κR+ν1κR)N/21(L1)1N/2(1+O(η′′))\displaystyle=\left(\frac{\phi\beta}{\alpha\gamma S_{T}}\right)^{N/2}\left(\frac{\kappa R+\nu_{1}}{\kappa R}\right)^{N/2-1}(L_{1})^{1-N/2}(1+O(\eta^{\prime\prime})) (66)

where η′′=max{η,L1/R}\eta^{\prime\prime}=\max\{\eta^{\prime},L_{1}/R\}. Choosing L1L_{1} small enough makes L1/RL_{1}/R small. With L1L_{1} fixed, making STS_{T} large enough makes η\eta small. Thus η′′\eta^{\prime\prime} can be made as small as desired by choosing L1L_{1} sufficiently small and STS_{T} sufficiently large.

Theorem 2 Consider the response function logCN=F(logL1,ν1)\log C_{N}=F(\log L_{1},\nu_{1}) for the steady states of the system (1)-(4) with L2=0L_{2}=0 and Dj=0D_{j}=0. Choose fixed values for all parameters in the system except L1L_{1} and STS_{T}. Suppose that κR1\kappa R\geq 1. Let ϵ>0\epsilon>0. Then there exists a constant δ\delta with 0<δR0<\delta\leq R such that the following holds. If 0<L0<δ0<L_{0}<\delta there exists μ>0\mu>0 such that if STμS_{T}\geq\mu the inequality

|(ϕβαγST)N/2(κR+ν1κR)1N/2(L1)N/21F(logL1,ν1)1|<ϵ\left|\left(\frac{\phi\beta}{\alpha\gamma S_{T}}\right)^{-N/2}\left(\frac{\kappa R+\nu_{1}}{\kappa R}\right)^{1-N/2}(L_{1})^{N/2-1}F(\log L_{1},\nu_{1})-1\right|<\epsilon (67)

holds on the interval [logL0,δ][\log L_{0},\delta].

Proof To obtain the conclusion of the theorem it suffices to show that under the given assumptions η′′\eta^{\prime\prime} can be made as small as desired. That this is possible follows from the discussion above.

Note that this theorem implies, in particular, that for N>2N>2 and suitable values of L1L_{1} and STS_{T} there exists a range of L1L_{1} in which the response function is decreasing. The theorem also implies that in this regime the reponse function can be an increasing function of ν1\nu_{1}. This effect was not captured by the calculations of [5] since there ν1κR\frac{\nu_{1}}{\kappa R} was assumed to be so small as to be negligible.

Finally we examine the regime where L1/RL_{1}/R is small but the phosphatase is close to being completely activated. This means that S/STS/S_{T} is close to one. This holds provided C1C_{1} is sufficiently large compared to CC_{*}. It remains to check that such a regime actually occurs for some values of the parameters. It is possible to make j=0NCj\sum_{j=0}^{N}C_{j} large while keeping L1/RL_{1}/R constant. This can be done by making RR large. This makes aa_{-} large without making rr_{-} small. Hence it makes C1C_{1} large and hence SS close to STS_{T}. In this regime the function of r+r_{+} and rr_{-} occurring in the expression for CNC_{N} can be replaced by its limit for SSTS\to S_{T} and we again get a region where the slope of the graph of logCN\log C_{N} as a function logL1\log L_{1} is one but the line has been shifted compared to that obtained for L1/RL_{1}/R small.

In [5] these types of behaviour were exhibited numerically in the case N=5N=5 with biologically reasonable choices of the parameters. We found that changing these parameters a little allows similar observations to be made in the case N=3N=3. In the plot shown in Figure 3

Refer to caption
Figure 3: Log-log plot showing linearity of logC3\log C_{3} as a function of logL1\log L_{1} for small L1L_{1}, followed by decreasing, increasing, and saturation regimes. Parameters are α=1\alpha=1, ST=6×105S_{T}=6\times 10^{5}, β=5×102\beta=5\times 10^{2}, κ=104\kappa=10^{-4}, R=3×104R=3\times 10^{4}, b=4×102b=4\times 10^{-2}, γ=1.2×106\gamma=1.2\times 10^{-6}, ϕ=9×102\phi=9\times 10^{-2}, ν1=102\nu_{1}=10^{-2}.

the three regimes can be seen together with a fourth regime where L1/RL_{1}/R is no longer small. It is clear that a regime of this type must exist since the response function is globally bounded.

We now turn to the dependence of the response function on ν1\nu_{1}. It has been suggested in [9] that the kinetic proofreading model with negative feedback as studied here is not able to explain the presence of an optimal dissociation time, a biological effect confirmed by the experimental work of [10]. The plots of the response as a function of the dissociation time in that type of model in [9] show that it is increasing. Having an optimal dissociation time would require that there be a region where this function is decreasing. The response function being increasing as a function of the dissociation time corresponds to its being decreasing a function of ν1\nu_{1}. Here we have given an analytical proof in Theorem 2 that there exist parameters for which the response is an increasing function of ν1\nu_{1}, in contrast to the plots in [9]. Since the theorem is of limited help in finding explicit parameters for which this happens we also did a numerical search and identified parameters of this type. The results are displayed in Figure 4, where it is seen that FF has a maximum as a function of ν1\nu_{1} for fixed L1L_{1}, which corresponds to an optimal dissociation time.

Refer to caption   Refer to caption

Figure 4: C3C_{3} as a function of ν1\nu_{1} in model with N=3N=3, showing non-monotonic behaviour for some values of parameters. Left: linear scale, right: log-log scale. Parameters are α=101\alpha=10^{-1}, ST=107S_{T}=10^{7}, β=10\beta=10, κ=106\kappa=10^{-6}, R=105R=10^{5}, b=102b=10^{-2}, γ=104\gamma=10^{-4}, ϕ=102\phi=10^{-2}, L1=103L_{1}=10^{3}.

The conclusion of both the analytical and the numerical work is as follows. The claim that the kinetic proofreading model with feedback can only produce a response which is a decreasing function of the parameter ν1\nu_{1} is dependent on the parameter values chosen to do the simulations and not a general property of the model.

5 Including the antagonist

When the antagonist is included the output variable expressing the degree of activation of the T cell is CN+DNC_{N}+D_{N}. Now asymptotic expressions for this quantity will be derived. It has already been shown that for a steady state of the system (1)-(7) the quantities j=0NCj\sum_{j=0}^{N}C_{j} and j=0NDj\sum_{j=0}^{N}D_{j} can be expressed in terms of the parameters. The equation for SS can be solved to give the relation S=STC1+D1C1+D1+CS=S_{T}\frac{C_{1}+D_{1}}{C_{1}+D_{1}+C_{*}}. CjC_{j} solves the same difference equation as in the agonist-only case and DjD_{j} solves the difference equation obtained from that one by replacing ν1\nu_{1} by ν2\nu_{2}. The quantities rr_{-}, r+r_{+}, aa_{-} and a+a_{+} differ in the two cases. We can nevertheless proceed as in the former case to see that the solutions for CjC_{j} and DjD_{j} allow parametrizations in terms of these quantities as before. Note that using the equations (8) and (9) it is possible to eliminate the DjD_{j} from the equation for C0C_{0} and the CjC_{j} from the equation for D0D_{0}. Thus we have coupled equations for the CjC_{j} and DjD_{j} which can be analysed just as in the agonist-only case to express C1C_{1} and D1D_{1} as functions of SS and the parameters. We can also write CNC_{N} and DND_{N} as functions of Σ1\Sigma_{1} and Σ2\Sigma_{2} respectively. Proceeding as in the agonist-only case we get an expression for CN+DNC_{N}+D_{N} in the kinetic proofreading regime. The multiple of L1L_{1} obtained there as leading term is replaced by a linear combination of L1L_{1} and L2L_{2}.

Next the intermediate regime will be considered. For this it is necessary to define a new parameter η=max{ϕ+ν1b+γS}\eta=\max\{\frac{\phi+\nu_{1}}{b+\gamma S}\}. There are asymptotic expressions for rr_{-} and r+r_{+} where the leading terms are just as in the agonist-only case. In particular they are the same for CjC_{j} and DjD_{j}. Two asymptotic expressions for the quantity C1+D1C_{1}+D_{1} can be obtained.

C1+D1=CSST(1+O(η)),\displaystyle C_{1}+D_{1}=\frac{C_{*}S}{S_{T}}(1+O(\eta)), (68)
=r(κRL1κR+ν1+κRL2κR+ν2)(1+O(η)).\displaystyle=r_{-}\left(\frac{\kappa RL_{1}}{\kappa R+\nu_{1}}+\frac{\kappa RL_{2}}{\kappa R+\nu_{2}}\right)(1+O(\eta)). (69)

This gives an expression for rr_{-} in terms of SS. As in the agonist-only case this gives an expression for rr_{-} where the dependence on SS has been eliminated in leading order.

r=ϕCγST(κRL1κR+ν1+κRL2κR+ν2)1(1+O(η))r_{-}=\sqrt{\frac{\phi C_{*}}{\gamma S_{T}}\left(\frac{\kappa RL_{1}}{\kappa R+\nu_{1}}+\frac{\kappa RL_{2}}{\kappa R+\nu_{2}}\right)^{-1}}(1+O(\eta’)) (70)

where η\eta^{\prime} is defined in terms of η\eta as in the agonist-only case. Following the steps used in the agonist-only case leads to an expression for CN+DNC_{N}+D_{N} which is the same as that previously obtained for CNC_{N} except that the expression κRL1κR+ν1\frac{\kappa RL_{1}}{\kappa R+\nu_{1}} is replaced by κRL1κR+ν1+κRL2κR+ν2\frac{\kappa RL_{1}}{\kappa R+\nu_{1}}+\frac{\kappa RL_{2}}{\kappa R+\nu_{2}}. This leads in the end to an asymptotic expression for CN+DNC_{N}+D_{N} under a suitable assumption L1L_{1} and L2L_{2}. The assumption made in the agonist-only case can naturally be written as an assumption on κRL1κR+ν1\frac{\kappa RL_{1}}{\kappa R+\nu_{1}} and in the present case it is replaced by an assumption on κRL1κR+ν1+κRL2κR+ν2\frac{\kappa RL_{1}}{\kappa R+\nu_{1}}+\frac{\kappa RL_{2}}{\kappa R+\nu_{2}}. This implies that under certain circumstances CN+DNC_{N}+D_{N} increases when L2L_{2} increases and L1L_{1} is held fixed. An increase in the amount of self-antigen can lead to a decrease in the response to a foreign antigen.

6 Conclusions and outlook

In this paper some properties of the solutions of the model of [5] for T cell activation were proved. A new discovery was that already in the case of three phosphorylation sites (N=3N=3) there can exist more than one positive steady state for given values of the parameters. Another new observation is that damped oscillations can occur. It was also proved that, as suggested by the calculations in [5], the output variable CNC_{N} (concentration of the maximally phosphorylated receptor) is a decreasing function of the concentration L1L_{1} of antigen in some parts of parameter space. In an analogous way it was proved that under some circumstances the activation in response to an agonist can be decreased by increasing the concentration of the antagonist. It was proved that it can also happen that CNC_{N} is an increasing function of the dissociation constant ν1\nu_{1}. This abstract result was given a concrete illustration by a plot showing that CNC_{N} can have a local maximum as a function of ν1\nu_{1}.

The stability of the steady states was only determined analytically in the very special cases N=1N=1 and α\alpha close to zero. For N=3N=3 numerical calculations showed the occurrence of two stable steady states for certain values of the parameters. It was proved that damped oscillations occur but can there also be sustained oscillations (periodic solutions)? It is thus clear that there remain several aspects of the dynamics of this system which would profit from further investigations, analytical and numerical.

In immunology it is important to describe diverse situations including the course of different types of infectious disease, the development of autoimmune diseases and the destruction of tumour cells by the immune system. It would be unreasonable to expect that a simple mechanism could be the key to describing all these situations. One strategy to try to obtain more understanding is to choose one mechanism and to investigate which types of situations it suffices to describe. This may be done by combining mathematical models with experimental data. What are the restrictions under which the type of model studied in this paper might be appropriate? The first assumption is that in the situation to be explained the distinction between self and non-self takes place within an individual T cell. In other words it is assumed that it is not necessary to consider the population dynamics of the T cells involved or even the interaction of their population with that of other types of immune cells such as regulatory T cells or dendritic cells. A quite different type of mathematical model, where population effects are considered, can be found in [14]. In that case, in contrast to the lifetime dogma, the response depends on the rate of change of the antigen concentration. The second assumption which is important for the models studied here is that the distinction between self and non-self takes place on a sufficiently short time scale, say three minutes. On longer time scales there may be essential effects related to the spatial distribution of molecules on the T cell surface (formation of the immunological synapse) so that a description by means of ordinary differential equations may be insufficient. It may also happen that some T cell receptors become inactive on a longer time scale (limiting signalling model, cf. [10]).

In this paper we have concentrated on studying the mathematical properties of a particular model for the biological phenomenon of T cell activation with arbitrary values of the parameters. A complementary question is to what extent known experimental data on the parameters may further constrain the dynamics in this model. In addition it is important to know whether this model is consistent with all biological data and how it compares to other possible models for the same biological system. For a discussion of this we refer to [9], [6] and [10]. It was indicated in [10] that the situation where CNC_{N} is a decreasing function of ν1\nu_{1} cannot be reproduced using the model of [5]. Our results indicate that a failure of the model to reproduce this effect must depend not only on the model itself but on the choice of parameters used for simulations. At the same time it may be that this effect only occurs in experiments where the measurements are done on long time scales (many hours) and not on the time scale of the initial activation (a few minutes) for which the models of [1] and [5] were primarily intended. We plan to investigate these questions further elsewhere.

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