
The primary purpose of fuel cell hybrid electric vehicles (FCHEVs) is to tackle the challenge of environmental pollution associated with road transport. However, to benefit from the enormous advantages presented by FCHEVs, an appropriate energy management system (EMS) is necessary for effective power distribution between the fuel cell and the energy storage systems (ESSs). The past decade has brought a significant increase in the number of FCHEVs, with different EMSs having been implemented due to technology advancement and government policies. These methods are broadly categorised into rule-based EMS methods, machine learning methods and optimisation-based control methods. Therefore, this paper presents a systematic literature review on the different EMSs and strategies used in FCHEVs, with special focus on fuel cell/lithium-ion battery hybrid electric vehicles. The contribution of this study is that it presents a quantitative evaluation of the different EMSs selected by comparing and categorising them according to principles, technology maturity, advantages and disadvantages. In addition, considering the drawbacks of some EMSs, gaps were highlighted for future research to create the pathway for comprehensive emerging solutions. Therefore, the results of this paper will be beneficial to researchers and electric vehicle designers saddled with the responsibility of implementing an efficient EMS for vehicular applications.
Citation: Samson Obu Showers, Atanda Kamoru Raji. State-of-the-art review of fuel cell hybrid electric vehicle energy management systems[J]. AIMS Energy, 2022, 10(3): 458-485. doi: 10.3934/energy.2022023
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The primary purpose of fuel cell hybrid electric vehicles (FCHEVs) is to tackle the challenge of environmental pollution associated with road transport. However, to benefit from the enormous advantages presented by FCHEVs, an appropriate energy management system (EMS) is necessary for effective power distribution between the fuel cell and the energy storage systems (ESSs). The past decade has brought a significant increase in the number of FCHEVs, with different EMSs having been implemented due to technology advancement and government policies. These methods are broadly categorised into rule-based EMS methods, machine learning methods and optimisation-based control methods. Therefore, this paper presents a systematic literature review on the different EMSs and strategies used in FCHEVs, with special focus on fuel cell/lithium-ion battery hybrid electric vehicles. The contribution of this study is that it presents a quantitative evaluation of the different EMSs selected by comparing and categorising them according to principles, technology maturity, advantages and disadvantages. In addition, considering the drawbacks of some EMSs, gaps were highlighted for future research to create the pathway for comprehensive emerging solutions. Therefore, the results of this paper will be beneficial to researchers and electric vehicle designers saddled with the responsibility of implementing an efficient EMS for vehicular applications.
We consider networks modeled by a directed graph where the dynamics on each edge are described by one-dimensional conservation laws. The dynamics are coupled at the vertices of the graph, called junctions. We are especially interested in (isentropic) gas dynamics, but there are many other applications for example in traffic, supply chains, data networks or blood circulation. This field became of interest to many researchers in the last two decades, see for example the overview by Bressan et al. [8]. A main challenge is posed by prescribing suitable coupling conditions at the junction. We consider novel conditions for the system of isentropic gas, also referred to as p-system.
The isentropic gas equations at a junction with
{∂tρk+∂x(ρkuk)=0∂t(ρkuk)+∂x(ρku2k+κργk)=0for a.e. t>0,x>0, | (1.1) |
where
The most challenging problem in modeling (gas) networks is to find physically correct coupling conditions. A first condition is usually conservation of mass at the junction
d∑k=1Akˉρkˉuk=0,for a.e. t>0, | (1.2) |
where
κˉργk=Hp(t),for k=1,…,d,a.e. t>0, | (1.3) |
equality of momentum flux [10,11]
ˉρkˉu2k+κˉργk=HMF(t),for k=1,…,d,a.e. t>0, | (1.4) |
and equality of stagnation enthalpy/Bernoulli invariant [28]
ˉu2k2+κγ−1ˉργ−1k=HSE(t),for k=1,…,d,a.e. t>0. | (1.5) |
Notice that the first two conditions are non-physically in the sense that energy may be produced at the junction [28]. Equality of stagnation enthalpy implies conservation of energy at the junction. We derive a coupling condition with dissipated energy at the junction. This is consistent with the isentropic gas equations where energy is also dissipated. The special situation with only two pipelines were studied in [13,21]
Usually existence and uniqueness of solutions to a generalization of the Riemann problem at the junction are studied locally in state space first. Reigstad [27] introduced a method to study existence and uniqueness almost globally in the subsonic region under a technical assumption. The results for the Riemann problem are used, to construct approximate solutions to the generalized Cauchy problem, usually by wave front tracking. See the book by Bressan [7] for a general introduction to the wave front tracking method. Colombo, Herty and Sachers [12] proved a general existence and uniqueness theorem for the generalized Cauchy problem by using this method. This theorem requires a transversality condition, subsonic data and sufficiently small total variation of the initial data.
Another approach to prove existence of solutions is the method of compensated compactness. This has been applied to a scalar traffic model [9] and the isentropic gas equations [22]. The method requires less assumptions on the regularity of the initial data but is restricted to systems with a large class of entropies. Moreover, less regularity of the solutions is obtained and the traces at the junction have to be considered carefully, see e.g. [5,22].
To supplement conservation of mass (1.2), we use an approach based on the kinetic model for isentropic gas and a maximum energy/entropy dissipation principle at the junction.
A kinetic model for the isentropic gas equations was introduced by Lions, Perthame and Tadmor [25]. The corresponding vector-valued BGK model were introduced by Bouchut [6]. For
∂tfkϵ+ξ∂xfkϵ=M[fkϵ]−fkϵϵ,for a.e. t>0,x>0,ξ∈R,k=1,…,d, | (1.6) |
with Maxwellian
Ψk[f1ϵ(t,0,⋅),…,fdϵ(t,0,⋅)](ξ)=fkϵ(t,0,ξ),for a.e. t>0,ξ>0. | (1.7) |
To select the function
Ψk[f1ϵ(t,0,⋅),…,fdϵ(t,0,⋅)](ξ)=M(ρϵ∗(t),0,ξ),for a.e. t>0,ξ>0. | (1.8) |
A formal limit argument leads to the definition of a generalized Riemann problem for
Definition 1. Let
(ρk,uk)(0+,x)=(ˆρk,ˆuk)∈D,for all x>0,k=1,…,d. |
(ρk,uk)(0+,x)={(ˆρk,ˆuk),x>0,(ρ∗,0),x<0, |
for all
d∑k=1Akˉρkˉuk=0, |
where
The set
Since the new coupling condition is based on restrictions of standard Riemann problems, we get a simple wave structure for the solutions in the sense of Definition 1. This structure allows us to prove existence and uniqueness of solutions globally in state space. We can use techniques by Reigstad [27] in the subsonic regime and extend them to the full state space. A general local existence and uniqueness result [12] for the Cauchy problem applies to the new condition. As a by-product we obtain Lipschitz continuous dependence on the initial data.
The coupling condition satisfies several properties regarding the energy/entropy dissipation. First, we obtain that entropy is non-increasing at the junction for a large class of symmetric entropies and in particular for the physical energy. A corollary of this property is a maximum principle on the Riemann invariants. More precisely, if the Riemann invariants of the initial data are bounded, then the Riemann invariants of the solution are bounded for all times. Furthermore, we prove a relation between the traces of the stagnation enthalpy at the junction.
We present an example in which the new coupling condition is the only condition leading to the physically correct wave types. The solutions to the generalized Riemann problem are computed numerically by using Newton's method. Furthermore, we study level sets associated to different coupling conditions and consider their geometry.
Our approach can be easily generalized to other hyperbolic systems. We extend it to full gas dynamics and obtain a similar coupling condition with an artificial density, zero speed and an artificial temperature at the junction. For more details and a brief literature overview see Section 8.
In Section 2, we recall several properties of the isentropic gas equations and the initial boundary value problem. In Section 3, we give a detailed motivation and a formal derivation of the coupling condition. Existence and uniqueness of solutions to the generalized Riemann problem will be proven in Section 4 and the corresponding results for the generalized Cauchy problem will be proven in Section 5. In Section 6, we derive several physical properties of the coupling condition, e.g. non-increasing energy, a maximum principle on the Riemann invariants and a relation for the traces of the stagnation enthalpy. Section 7 is devoted to numerical considerations. In Section 8, the extension of our approach to full gas dynamics is given. In Section 9, we finish with a conclusion.
The isentropic gas equations in one space dimension are given by
{∂tρ+∂x(ρu)=0∂t(ρu)+∂x(ρu2+κργ)=0a.e. t≥0,x∈R. | (2.1) |
Furthermore, we impose the entropy condition
∂tηS(ρ,u)+∂xGS(ρ,u)≤0a.e. t,x, | (2.2) |
for all (weak) entropy pairs
G′S=η′SF′,ηS(ρ=0,u)=0,η′S,ρ(ρ=0,u)=S(u), for all u∈R, | (2.3) |
and a suitable convex function
D={(x0,x1)∈R2|x0>0 or x0=x1=0}, | (2.4) |
χ(ρ,ξ)=cγ,κ(a2γργ−1−ξ2)λ+, | (2.5) |
θ=γ−12,λ=1γ−1−12,cγ,κ=a2/(γ−1)γJλ, | (2.6) |
Jλ=∫1−1(1−z2)λdz,aγ=2√γκγ−1. | (2.7) |
The isentropic gas equations admit the Riemann invariants
ω1=u−aγρθ,ω2=u+aγρθ, | (2.8) |
for
λ1(ρ,u)=u−√κγρθ,λ2(ρ,u)=u+√κγρθ, | (2.9) |
and the eigenvectors by
r1(ρ,u)=(1u−√κγρθ),r2(ρ,u)=(1u+√κγρθ), | (2.10) |
for
● subsonic if
● sonic if
● supersonic if
Next, we define several quantities corresponding to the kinetic (BGK) model for isentropic gas dynamics (1.6). The vector-valued Maxwellian
M[f](ξ)=M(ρf,uf,ξ) | (2.11) |
where
ρf=∫Rf0(ξ)dξ,ρfuf=∫Rf1(ξ)dξ | (2.12) |
and
M(ρ,u,ξ)=(χ(ρ,ξ−u),((1−θ)u+θξ)χ(ρ,ξ−u)). | (2.13) |
The kinetic entropies are defined by
HS(f,ξ)=∫RΦ(ρ(f,ξ),u(f,ξ),ξ,v)S(v)dvfor f∈D∖{0}, | (2.14) |
HS(0,ξ)=0, | (2.15) |
where
u(f,ξ)=f1/f0−θξ1−θ, | (2.16) |
ρ(f,ξ)=a−2γ−1γ((f1/f0−ξ1−θ)2+(f0cγ,κ)1/λ)1γ−1. | (2.17) |
The kernel
Φ(ρ,u,ξ,v)=(1−θ)2θcγ,κJλ1ω1<ξ<ω21ω1<v<ω2|ξ−v|2λ−1Υλ−1(z), | (2.18) |
z=(ξ+v)(ω1+ω2)−2(ω1ω2+ξv)(ω2−ω1)|ξ−v|, | (2.19) |
Υλ−1(z)=∫z1(y2−1)λ−1dy,z≥1. | (2.20) |
The kinetic Riemann invariants are given by
ω1=u(f,ξ)−aγρ(f,ξ)θ,ω2=u(f,ξ)+aγρ(f,ξ)θ, | (2.21) |
for
ηS(ρ,u)=∫Rχ(ρ,v−u)S(v)dv=∫RHS(M(ρ,u,ξ),ξ)dξ, | (2.22) |
GS(ρ,u)=∫R[(1−θ)u+θv] χ(ρ,v−u)S(v)dv | (2.23) |
=∫RξHS(M(ρ,u,ξ),ξ)dξ, | (2.24) |
for
η′S(ρ,u)=1Jλ∫1−1(1−z2)λ(S(u+aγρθz)+(θaγρθz−u)S′(u+aγρθz)S′(u+aγρθz))dz, | (2.25) |
for
H(f,ξ)=θ1−θξ22f0+θ2c1/λγ,κf1+1/λ01+1/λ+11−θ12f21f0−θ1−θξf1, | (2.26) |
and the corresponding macroscopic entropy pair is given by the physical energy and energy flux
η(ρ,u)=ρu22+κγ−1ργ,G(ρ,u)=ρu32+γκγ−1ργu. | (2.27) |
To construct solutions to the generalized Riemann problem, we need the (forward) Lax wave curves
R1(ρ0,u0):u=u0+aγρθ0−aγρθ,for ρ<ρ0, | (2.28) |
R2(ρ0,u0):u=u0−aγρθ0+aγρθ,for ρ>ρ0, | (2.29) |
and the shock curves are given by
S1(ρ0,u0):u=u0−√κ(ργ−ργ0)(ρ−ρ0)ρρ0,for ρ>ρ0, | (2.30) |
S2(ρ0,u0):u=u0−√κ(ργ−ργ0)(ρ−ρ0)ρρ0,for ρ<ρ0. | (2.31) |
We will use the notation
{(ρl,ul),x<0,(ρr,ur),x>0, | (2.32) |
where
In this subsection, we recall some basic properties of the initial boundary value problem. The sets
Definition 2. Let
(ρ,u)=RP(ρb,ub,ρr,ur)(0+),for a state (ρr,ur)∈D. |
Definition 3. Let
GS(ρ,u)−GS(ρb,ub)−η′S(ρb,ub)(F(ρ,u)−F(ρb,ub))≤0 |
for all entropy pairs
We recall the following result.
Proposition 1. ([23,Theorem 3.4]). Let
Next, we define subsets of
Definition 4. Let
●
●
●
●
We write
The sets
Next, we construct a solution which satisfies all properties in Definition 1 except of conservation of mass RP2. They will be used to construct the desired solution to Definition 1 later. To clarify that RP2 does not necessarily hold true, we denote the artificial density by
Lemma 1. Let
(ρk,uk)(0,x)={(ˆρk,ˆuk),x>0,(˜ρ∗,0),x<0, |
for a.e.
(i)
(ii)
(iii)
(iv)
(v)
(vi)
Proof. The existence and uniqueness of self-similar Lax solutions to Riemann problems is well-known. For Riemann problems with vacuum initial data see [26]. It remains to prove the properties for
In this section we give a physical motivation and formal derivation for the new coupling condition. Both are based on the kinetic model for isentropic gas and a maximum energy/entropy dissipation principle. First, we specify the kinetic coupling condition which conserves mass and dissipates as much energy as possible. In the second step, we consider the macroscopic limit of the kinetic coupling condition. This relaxation works only on a formal level since the currently available results for passing to the limit at the junction are not strong enough. Nevertheless, we are able to take the formal limit towards the macroscopic coupling condition. Finally, we also give an interpretation of the resulting conditions.
Since Dafermos [16] introduced the entropy rate admissibility criterion it is a natural approach to maximize the entropy dissipation in the field of hyperbolic conservation laws. This technique can be used to single out the physically correct solutions. We adapt this approach and aim to find the most dissipative kinetic coupling condition (with the constrained of conservation of mass). Since the physical energy is an entropy for the system of isentropic gas and is the physically relevant entropy, we maximize the energy dissipation.
We consider the kinetic BGK model of the isentropic gas equations which is given by
∂tfϵ+ξ∂xfϵ=M[fϵ]−fϵϵ,for a.e. t>0,x∈R,ξ∈R, | (3.1) |
where
Remark 1. The BGK model, its relaxation limit and boundary conditions were studied by Berthelin and Bouchut [3,4,5]. These results were extended to networks in [22]. Notice that our considerations are independent of the right hand side of the kinetic equation as long as the kinetic solution converges to an entropy solution of the macroscopic equation.
To couple the half-space solutions, we have to define a kinetic coupling condition
Ψ:L1μ((−∞,0)ξ,D)d→L1μ((0,∞)ξ,D)d;g↦Ψ[g]. | (3.2) |
The half-space solutions
Ψk[f1ϵ(t,0,⋅),…,fdϵ(t,0,⋅)](ξ)=fkϵ(t,0,ξ),for a.e. t>0,ξ>0. | (3.3) |
We are interested in kinetic coupling conditions which conserve mass. More precisely, we require that
d∑k=1Ak(∫∞0ξΨk0[g](ξ)dξ+∫0−∞ξgk0(ξ)dξ)=0, | (3.4) |
holds for all
d∑k=1Ak(∫∞0ξH(Ψk[g](ξ),ξ)dξ+∫0−∞ξH(gk(ξ),ξ)dξ). | (3.5) |
To find the unique minimizer of this functional, we use the convexity of the kinetic energy. More precisely, we use the sub-differential inequality (see e.g. [4])
H(g,ξ)≥H(M(ρ,u,ξ),ξ)+η′(ρ,u)(g−M(ρ,u,ξ)), | (3.6) |
for every
d∑k=1Ak∫∞0ξH(Ψk[g](ξ),ξ)dξ≥d∑k=1Ak∫∞0ξH(M(ρ∗,0,ξ),ξ)dξ+η′(ρ∗,0)[d∑k=1Ak(∫∞0ξΨk0[g](ξ)dξ−∫∞0ξM(ρ∗,0,ξ)dξ)]=d∑k=1Ak∫∞0ξH(M(ρ∗,0,ξ),ξ)dξ, | (3.7) |
where
d∑k=1Ak(∫∞0ξM0(ρ∗,0,ξ)dξ+∫0−∞ξgk0(ξ)dξ)=0. | (3.8) |
Such an
∫∞0ξM0(ρ∗,0,ξ)dξ=cγ,κ(aγρθ∗)γ+1γ−1∫10z(1−z2)λdz. | (3.9) |
The uniqueness follows from the strict convexity of
Theorem 1. The unique kinetic coupling condition
Ψ:L1μ((−∞,0)ξ,D)d→L1μ((0,∞)ξ,D)d;g↦Ψ[g] |
which conserves mass (3.4) and minimizes (3.5) is given by
Ψk[g](ξ):=M(ρ∗,0,ξ), | (3.10) |
where
According to [22], weak solutions to the kinetic BGK model on networks exist under suitable conditions on the initial data.
Instead of minimizing the kinetic energy, other kinetic entropies could be considered. Notice that every kinetic entropy
We take the formal limit at the junction with
∫RξHS(fkϵ(t,0,ξ),ξ)dξ−GS(ρϵ∗(t),0)−η′S(ρϵ∗(t),0)(∫Rξfkϵ(t,0,ξ)dξ−F(ρϵ∗(t),0))≤0, | (3.11) |
for
¯GS(ρk,uk)(t)−GS(ρ∗(t),0)−η′S(ρ∗(t),0)(¯F(ρk,uk)(t)−F(ρ∗(t),0))≤0, | (3.12) |
for a.e.
d∑k=1Ak¯ρkuk(t)=0,a.e. t>0, | (3.13) |
for the weak traces
We summarize that after formally taking the (strong) limit, the traces at
In this subsection, we restrict ourselves to the generalized Riemann problem since it is a building block for the Cauchy problem.
The new macroscopic coupling condition is an implicit condition compared to the known coupling conditions in the literature. The idea of the new coupling condition is to assume the existence of left hand states of zero speed, independent of
We made a particular choice by choosing
We interpret the macroscopic coupling condition by gas being stopped at the junction. Therefore, it is reasonable that we state a relation between the traces of the stagnation enthalpy at the junction. The stagnation enthalpy determines the enthalpy at a stagnation point after the gas is brought to a stop. This relation is given by inequalities depending on the signs of
We emphasis that the coupling condition does not coincide with the Rankine-Hugoniot conditions in the case
Summarizing, the derivation of the coupling condition by the kinetic model and the maximum energy dissipation principle at the junction lead to a choice of an artificial state of zero speed at the junction. Furthermore, the interpretation of the macroscopic coupling condition by particles stopped at the junction and redistributed is only possible with a state of zero speed. From a formal mathematical point of view, the proofs of the physical properties in Section 6 work only if the artificial state has zero speed. This observation is due to the structure of (3.12) and the fact that
In this section, we prove existence and uniqueness of solutions to the generalized Riemann problem. Our strategy is as follows. Due to Lemma 1, there exists a solution for a fixed artificial density
Proposition 2. Assume that initial data
Proof. First, we prove the continuity with respect to the artificial density at fixed
Step 1: First, we consider the boundary between
limρ↘˜ρ∗(ˉρk,ˉuk)=(ρα,uα)=limρ↗˜ρ∗(ˉρk,ˉuk), | (4.1) |
since the 2-wave curve, the 1-rarefaction curve and the curve defined by
Step 2: Next, we consider the boundary between
(ˉρk,ˉuk)(ρ)=(ˆρk,ˆuk), | (4.2) |
where
limρ↗˜ρ∗ˉρkˉuk=ˆρkˆuk, | (4.3) |
since the speed of the 2-shock tends to zero as
The continuity at
Lemma 2. ([27,Remark 1]). Along the reversed 2-wave curves monotonicity in
du0dρ0|W−2>0,for all(ρ,ρu)∈D∖{0}. | (4.4) |
The subscript denotes differentiation along the reversed
Proof. By the formula for the reversed 2-rarefaction wave, we have
du0dρ0|R−2=√κγργ−320>0. |
Along the reversed 2-shock curve, we get
du0dρ0|S−2=κ2ρ0ρ(1−γ)ργ−10ρ+γργ0−ργ+1ρ0√κ(ργ0−ργ)(ρ0−ρ)ρ0ρ=κ2ρ0ρ(u0−u)(ρρ0(ργ0−ργ)+γργ−10(ρ0−ρ))>0, |
since
In the subsonic regime, we can determine the artificial density by a function
Definition 5. Let
R∗(ρ,u)={(ρθ+uaγ)1/θ,if u≥0,R∗,with u=−√κ(ργ−Rγ∗)(ρ−R∗)ρR∗,R∗<ρ,if u<0. | (4.5) |
Notice that
(0,ρ]→(−∞,0],R∗↦−√κ(ργ−Rγ∗)(ρ−R∗)ρR∗, |
is bijective. By this definition we can reformulate RP1 in the subsonic regime by
R∗(ˉρk,ˉuk)(t)=HR∗(t),for k=1,…,d,for a.e. t>0. | (4.6) |
Compare the new condition (4.6) with the coupling conditions in (1.3 – 1.5) and note that they are different even in the subsonic regime.
Lemma 3. We have
dR∗dρ0|W−2>0,for all(ρ,u)∈D∖{0}. | (4.7) |
The subscript represents the differentiation along the reversed 2-wave curve.
Proof. For
dR∗dρ0=(ργ−320+1√κγdu0dρ0)(ρθ0+u0aγ)3−γγ−1>0, | (4.8) |
since
u0=−√κ(ργ0−Rγ∗)(ρ0−R∗)ρ0R∗ |
along the 2-wave curve gives
du0dρ0=κu0[γ(ργ−10−Rγ−1∗dR∗dρ0)(1R∗−1ρ0)+(ργ0−Rγ∗)(1ρ20−1R2∗dR∗dρ0)], |
or equivalently
dR∗dρ0=2u0κdu0dρ0+γργ−10(1ρ0−1R∗)+1ρ20(Rγ∗−ργ0)γRγ−1∗(1ρ0−1R∗)+1R2∗(Rγ∗−ργ0). |
The right hand side is strictly positive, since
Lemma 4. We have
dR∗dρ|λ1=0>0, |
where the subscript denotes the differentiation along the curve
Proof. We differentiate
dudρ=ddρ(√κγρθ)=√κγθργ−32>0. |
The result follows with (4.8).
Proposition 3. Fix initial data
Proof. Step 1: We consider the case
d(ˉρkˉuk)d˜ρ∗=dd˜ρ∗(√γκ(2γ+1)γ+1γ−1˜ργ+12∗)=√κγ(2γ+1)2γ−1˜ργ−12∗>0. |
Step 2: Next, we consider the case
dR∗dρ0|W−2>0, |
but this implies
dˉρkd˜ρ∗=dR−1∗(˜ρ∗)d˜ρ∗>0, |
where
d(ˉρkˉuk)d˜ρ∗=d(ˉρkˉuk)dˉρk⋅dˉρkd˜ρ∗. |
Therefore, it remains to prove
d(ˉρkˉuk)dˉρk|W−2>0. |
On
d(ˉρkˉuk)dˉρk=ˉuk+ˉρkdˉukdˉρk=ˉuk+√κγˉρθk=λ2(ˉρk,ˉuk)>0, |
since
d(ˉρkˉuk)dˉρk=ˉuk+ˉρkdˉukdˉρk=ˉuk+√κ2ˉρkˆρk(ˉuk−ˆuk)[γˉργk(ˉρk−ˆρk)+ˆρk(ˉργk−ˆργk)]=λ2(ˉρk,ˉuk)−√κγˉρθk+√κ2ˉρkˆρk(ˉuk−ˆuk)[γˉργk(ˉρk−ˆρk)+ˆρk(ˉργk−ˆργk)]=λ2(ˉρk,ˉuk)+√κ2ˉρkˆρk(ˉuk−ˆuk)⋅[γˉργk(ˉρk−ˆρk)+ˆρk(ˉργk−ˆργk)−2√γˉργk(ˉρk−ˆρk)√ˆρk(ˉργk−ˆργk)]=λ2(ˉρk,ˉuk)+√κ2ˉρkˆρk(ˉuk−ˆuk)[√γˉργk(ˉρk−ˆρk)−√ˆρk(ˉργk−ˆργk)]2>λ2(ˉρk,ˉuk)>0, |
for
Step 3: The strict monotonicity at the boundary between
Step 4: Finally, we consider the case
{(ˉρk,ˉuk)}=R2(ˆρk,ˆuk)∩{λ2=0}. |
Therefore,
Theorem 2. Assume that the initial states
Proof. For the solution
m(˜ρ∗)=d∑k=1Akˉρkˉuk. |
Since Proposition 2 and 3, the function
Step 1: We prove that there exist
m(ρ−)≤0≤m(ρ+). |
● We set
ρ−=argmin{ρ≥0|(ρ,0)∈W−2(ˆρk,ˆuk) for k=1,…,d}. |
Then, we have
● We set
ρ+=argmax{ρ≥0|(ρ,0)∈W−2(ˆρk,ˆuk) for k=1,…,d}. |
Then, we have
By the intermediate value theorem, we conclude that there exists
Step 2: We prove that
Since Riemann problems admit unique self-similar Lax solutions and
In this section, we prove existence and uniqueness of solutions to the Cauchy problem. This result is based on a general existence theorem by Colombo, Herty and Sachers [12] and holds true in a neighborhood of a subsonic solution. We also obtain Lipschitz continuous dependence on the initial data.
Definition 6. Fix
(ρk,uk)(0+,x)=(ˆρk,ˆuk)(x)∈D, |
for a.e.
(ˉρk,ˉuk)(t)∈V(ρ∗(t),0) |
for all
d∑k=1Akˉρkˉuk=0,for a.e. t>0. |
Theorem 3. Fix a vector of subsonic states
●
● for
● for
● if
Moreover, for every
Proof. Since
R∗(ˉρk,ˉuk)(t)=HR∗(t),for k=1,…,d, |
for a.e.
Ψ(U)=(∑dk=1AkρkukR∗(ρ1,u1)−R∗(ρ2,u2)⋮R∗(ρd−1,ud−1)−R∗(ρd,ud)). |
It remains to prove the transversality condition
det[D1Ψ(U0)⋅r2(ρ01,u01)⋯DdΨ(U0)⋅rd(ρ0d,u0d)]≠0, | (5.1) |
where
∂ρu∂ρ|W−2>0and∂R∗∂ρ|W−2>0 |
in the subsonic region. We deduce that
Dk(ρkuk)⋅r2(ρk,uk)>0andDkR∗(ρk,uk)⋅r2(ρk,uk)>0. |
This implies that the matrix involved in (5.1) has components with fixed sign which are given by
(+++⋯⋯++−0⋯⋯00+−⋱⋮⋮⋱⋱⋱⋱⋮⋮⋱⋱⋱00……0+−). |
A Laplace expansion implies that the determinant of this matrix has a fixed sign and is non-zero.
Remark 2. The existence and uniqueness result is restricted to subsonic initial data with sufficiently small total variation. The global result for the generalized Riemann problem and the large amount of inequalities for entropy fluxes at the junction (Propsition 4) motivate to prove a more general result. Notice that the method in [22] based on compensated compactness can be applied to the kinetic coupling condition (3.10). This result justifies the relaxation in the interior of the pipelines. Nevertheless, it is open how the traces relax at the junction and if the obtained macroscopic solution satisfies the coupling condition in Definition 6.
In this section, we prove some physical properties of the coupling condition. In particular, we prove that energy is non-increasing at the junction, a relation for the stagnation enthalpy and a maximum principle on the Riemann invariants.
Proposition 4. Assume that initial states
d∑k=1AkGS(ˉρk,ˉuk)≤0, |
for every convex
Proof. The case
GS(ˉρk,ˉuk)−GS(ρ∗,0)−η′S(ρ∗,0)(F(ˉρk,ˉuk)−F(ρ∗,0))≤0. |
Notice that
GS(ρ∗,0)=∫Rθvχ(ρ∗,v)S(v)dv=0,and∂ρuηS(ρ∗,0)=1Jλ∫1−1(1−z2)λS′(aγρθ∗z)dz=0, |
since the integrands are anti-symmetric. These observations together with conservation of mass at the junction give
0≥d∑k=1Ak[GS(ˉρk,ˉuk)−GS(ρ∗,0)−η′S(ρ∗,0)(F(ˉρk,ˉuk)−F(ρ∗,0))]=d∑k=1AkGS(ˉρk,ˉuk)−∂ρηS(ρ∗,0)(d∑k=1Akˉρkˉuk)=d∑k=1AkGS(ˉρk,ˉuk). |
An approximation argument leads to the result for general convex functions
Corollary 1 (Non-increasing energy). Assume that sufficiently regular initial data
(i) At the junction energy is non-increasing, i.e.
d∑k=1AkG(ˉρk,ˉuk)≤0,for a.e.t>0. |
(ii) At the junction the traces of the stagnation enthalpy
h(ρ,u)=u22+κγγ−1ργ−1 |
are related by
h(ˉρk,ˉuk)≤h(ρ∗,0)≤h(ˉρl,ˉul), |
for
Proof. Applying Proposition 4 to
d∑k=1AkG(ˉρk,ˉuk)≤0. |
Since
G(ˉρk,ˉuk)−∂ρη(ρ∗,0)ˉρkˉuk≤0. |
The result follows from dividing the inequality by
Corollary 2 (Maximum principle). Let
−ωM≤ω1(ˆρk,ˆuk)(x)<ω2(ˆρk,ˆuk)(x)≤ωM, |
for a.e.
−ωM≤ω1(ρk,uk)(t,x)<ω2(ρk,uk)(t,x)≤ωM, |
for a.e.
Proof. We define the symmetric, positive function
SM(v)=(−ωM−v)2++(v−ωM)2+,v∈R. |
As proven in [22], the definition of
ηSM(ρ,u)=0, if and only if −ωM≤ω1(ρ,u)<ω2(ρ,u)≤ωM. | (6.1) |
Furthermore, the divergence theorem and the entropy condition give
∫∞0ηSM(ρk,uk)(T,x)dx−∫∞0ηSM(ρk,uk)(0,x)dx−∫T0GSM(ρk,uk)(t,0)dt≤0, |
for
0≤d∑k=1Ak∫∞0ηSM(ρk,uk)(T,x)dx≤d∑k=1Ak∫∞0ηSM(ρk,uk)(0,x)dx=0. |
The result follows from (6.1).
We give an example in which the new coupling condition produces the physically correct wave types. This observation is based on the assumption of the appearance of turbulence at the junction. The other coupling conditions produce different wave types. Furthermore, we study level sets associated to unphysical coupling conditions. We will consider the coupling conditions with equal pressure, equal momentum flux, equal stagnation enthalpy and the artificial density coupling condition.
We consider the shallow water equations and set
The implementation is based on Newton's method applied to the coupling condition. The unknowns are the parameter of the reversed
We consider a three junction situation with one ingoing and two outgoing pipelines. The idea of this example is to assume that the sum of the momentum of the initial states is zero and the initial densities coincide. For this example we clearly get a stationary solution if we take the coupling condition with equal pressure. To make the example more concrete, we take the initial data in Table 1. The traces and energy dissipation of the numerical solutions are given in Table 2. The generalized Riemann problems are solved by the
pipeline | ||
1 | ||
2 | ||
3 |
Equal density | Equal momentum flux | Equal stagnation enthalpy | Equal artificial density | |||||
pipeline | ||||||||
1 | ||||||||
2 | ||||||||
3 | ||||||||
Energy dissipation |
pipeline | Equal density | Equal momentum flux | Equal stagnation enthalpy | Equal artificial density |
1 | no waves | rarefaction wave | rarefaction wave | shock |
2 | no waves | shock | shock | rarefaction wave |
3 | no waves | shock | shock | rarefaction wave |
We make the following observations:
● The
● The most energy is dissipated at the junction when the artificial density coupling condition is imposed.
● If the artificial density coupling condition is imposed, the momentum traces at the junction are smaller compared to the other coupling conditions. The momentum traces for the coupling conditions with equal pressure, equal momentum flux or equal stagnation enthalpy differ less strongly in comparison with each other.
In this section we consider the geometry of level sets corresponding to different coupling conditions. More precisely, we drop the condition on conservation of mass and compute the sets in which the attained boundary values may lie. For a solution to the generalized Riemann problem, the traces
{(ρ,ρu)∈D|H(ρ,u)=H(ρ0,u0)}, | (7.1) |
where
V(ρ∗,0),for suitable ρ∗≥0, |
which coincides with the definition in (7.1) in the subsonic case by taking
We make the following observations:
● The coupling conditions with equal momentum flux and stagnation enthalpy induce bounded level sets.
● The level sets induced by equal pressure, momentum flux and stagnation enthalpy are symmetric w.r.t. the
In this section, we apply the derivation technique to full gas dynamics. We compute the maximum entropy dissipating kinetic coupling condition for kinetic models with the standard Maxwellian, e.g. the Boltzmann equation, the linear Boltzmann equation or the Boltzmann BGK model. We maximize the entropy dissipation and not the energy dissipation since energy is conserved. Again, we define a macroscopic coupling condition which can be formally obtained by a macroscopic limit. Notice that the formal macroscopic limit of the kinetic Boltzmann (type) equations is given by the full compressible Euler equations. The aim of this section is to underline that the presented approach is quite general and can be adopted easily to other hyperbolic systems equipped by a kinetic model and an entropy. Furthermore, the obtained results are very similar to the results for the isentropic gas equations.
First, we recall some basic definitions and explain the setting. As before, we consider a network of one-dimensional pipelines. We assume that one of the kinetic equations mentioned above is satisfied in the interior of the pipelines. The kinetic Boltzmann (type) equations admit the standard Maxwellian
Mρ,u,θ(ξ)=ρ√2πθexp(−(u−ξ)22θ), | (8.1) |
for
Ψ:L1μ((−∞,0)ξ,[0,∞))d→L1μ((0,∞)ξ,[0,∞))d;g↦Ψ[g], | (8.2) |
which conserves mass and energy and dissipates as much entropy as possible. More precisely, we minimize
d∑k=1Ak∫∞0ξΨk[g](ξ)logΨk[g](ξ)dξ, | (8.3) |
with respect to
d∑k=1Ak(∫∞0ξΨk[g](ξ)dξ+∫0−∞ξgk(ξ)dξ)=0, | (8.4) |
d∑k=1Ak(∫∞0ξ3Ψk[g](ξ)dξ+∫0−∞ξ3gk(ξ)dξ)=0. | (8.5) |
The unique minimizer of this problem is given by
Ψk[g](ξ)=Mρ∗,0,θ∗(ξ),for ξ>0, | (8.6) |
where
Since
d∑k=1Ak∫∞0ξΨk[g](ξ)logΨk[g](ξ)dξ≥d∑k=1Ak(∫∞0ξMρ∗,0,θ∗(ξ)logMρ∗,0,θ∗(ξ)dξ)+d∑k=1Ak(∫∞0ξ[logMρ∗,0,θ∗(ξ)+1](Ψk[g](ξ)−Mρ∗,0,θ∗(ξ))dξ)=d∑k=1Ak∫∞0ξMρ∗,0,θ∗(ξ)logMρ∗,0,θ∗(ξ)dξ. | (8.7) |
The last step follows by
logMρ∗,0,θ∗(ξ)+1=logρ√2πθ+1−ξ22θ | (8.8) |
and (8.4 – 8.5). It can be easily checked that for every
d∑k=1Ak(∫∞0ξMρ∗,0,θ∗(ξ)logMρ∗,0,θ∗(ξ)dξ+∫0−∞ξg(ξ)logg(ξ)dξ)≤0. | (8.9) |
Next, we consider the macroscopic limit. As mentioned above, the kinetic equation converges formally towards the full Euler equations for ideal polytropic gas given by
{∂tρ+∂x(ρu)=0,∂t(ρu)+∂x(ρu2+ρθ)=0,∂t(ρu22+ρθ2)+∂x(ρu32+32ρuθ)=0,for a.e. t>0,x∈R, | (8.10) |
with density
∂t(ρlog(ρθ1/2))+∂x(ρulog(ρθ1/2))≤0,for a.e. t>0,x∈R. | (8.11) |
The full Euler equations on networks were studied before by several authors [14,15,19,24]. We summarize the main ideas of the constructed coupling conditions. Analogous to isentropic gas dynamics, conservation of mass at the junction is imposed
d∑k=1Akˉρkˉuk=0,a.e. t>0. | (8.12) |
Since energy is conserved in full gas dynamics, we additionally assume that energy is conserved at the junction, i.e.
d∑k=1Ak¯(ρu32+32ρuθ)k=0. | (8.13) |
There are more conditions needed to single out a unique solution. Most of them are a straight forward extension of a coupling condition for isentropic gas. We give a short overview of the coupling conditions in the literature:
Colombo and Mauri [15] introduced equality of momentum flux at the junction
¯(ρu2+ρθ)k=HMF(t),for a.e. t>0,k=1,…,d. | (8.14) |
Herty [19] used equality of pressure
ˉρkˉθk=Hp(t),for a.e. t>0,k=1,…,d. | (8.15) |
Networks consisting of
¯(u22+32θ)k=HSE(t),for a.e. t>0,k=1,…,d, | (8.16) |
and equality of entropy for traces with outgoing flow
log(ρθ1/2)=HS(t),for a.e. t>0, for ˉuk>0, | (8.17) |
withHS(t)=∑ˉuk<0Ak¯(ρulog(ρθ1/2))k∑ˉuk<0Akˉρkˉuk. | (8.18) |
These two conditions imply conservation of energy and entropy at the junction. Notice that conservation of entropy at the junction is not consistent with the fact that entropy can be dissipated in full gas dynamics.
In full gas dynamics an additional phenomena appears since the number of ingoing/outgoing characteristics at the junction can change in the subsonic region. This fact makes it more complicated to prove existence and uniqueness results. Nevertheless, we can use the formal arguments in Section 3 and the derivation in the previous subsection to define the following new coupling condition for full gas dynamics.
Definition 7. Fix initial data
(ρk,uk,θk)(0+,x)=(ˆρk,ˆuk,ˆθk)∈D3×3,for x>0,k=1,…,d; |
(ρk,uk,θk)(0+,x)={(ˆρk,ˆuk,ˆθk),x>0,(ρ∗,0,θ∗),x<0, |
for all
d∑k=1Akˉρkˉuk=0,for all t>0; |
d∑k=1Ak¯(ρu32+32ρuθ)k=0,for all t>0. |
Notice that this condition leads to conservation of mass and energy at the junction by definition. Furthermore, entropy is non-increasing at the junction by the entropy formulation of boundary conditions
d∑k=1Ak¯(ρulog(ρθ1/2))k≤0. | (8.19) |
Therefore, the new coupling condition satisfies some necessary physical properties.
We introduced a new coupling condition for isentropic gas and proved existence and uniqueness of solutions to the generalized Riemann and Cauchy problem.
The derivation of the coupling condition is based on the kinetic model and the selection of the unique kinetic coupling condition which conserves mass and dissipates as much energy as possible. The obtained kinetic coupling condition distributes the incoming kinetic data into all pipelines by the same Maxwellian with suitable artificial density and zero speed. Formal arguments lead to a corresponding macroscopic definition to the generalized Riemann problem. In this definition the artificial state with zero speed appears as the (left) initial state for a standard Riemann problem.
In addition to the derivation, we proved physical properties of the coupling condition. The coupling condition ensures that energy is non-increasing at the junction and leads to a maximum principle on the Riemann invariants. Furthermore, a relation of the traces of the stagnation enthalpy at the junction was given. Notice that these properties hold true due to the choice of an artificial state with zero speed.
We gave an example in which the new coupling condition is the only condition producing the physically correct wave types. The solutions to the generalized Riemann problems were computed numerically. Furthermore, we studied level sets related to different coupling conditions and their geometry.
Finally, we considered the coupling condition in view of the model hierarchy of gas dynamics by applying the same approach to full gas dynamics and Boltzmann (type) equations. We took the kinetic coupling conditions with conservation of mass and energy at the junction and maximize the entropy dissipation. This consideration leads to very similar results. In particular, we obtained an artificial state with suitable density and temperature and again with zero speed.
In summary, we defined a new coupling condition, derived several physical and mathematical properties and gave a motivation. Future research may consider more detailed numerical aspects and the rigorous justification of the considerations in Section 3.
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8. | Andrea Corli, Massimiliano D. Rosini, Ulrich Razafison, 2024, Mathematical Modeling of Chattering and the Optimal Design of a Valve*, 979-8-3503-1633-9, 76, 10.1109/CDC56724.2024.10886245 | |
9. | Andrea Corli, Ulrich Razafison, Massimiliano D. Rosini, Coherence of Coupling Conditions for the Isothermal Euler System, 2025, 0170-4214, 10.1002/mma.10847 |
pipeline | ||
1 | ||
2 | ||
3 |
Equal density | Equal momentum flux | Equal stagnation enthalpy | Equal artificial density | |||||
pipeline | ||||||||
1 | ||||||||
2 | ||||||||
3 | ||||||||
Energy dissipation |
pipeline | Equal density | Equal momentum flux | Equal stagnation enthalpy | Equal artificial density |
1 | no waves | rarefaction wave | rarefaction wave | shock |
2 | no waves | shock | shock | rarefaction wave |
3 | no waves | shock | shock | rarefaction wave |
pipeline | ||
1 | ||
2 | ||
3 |
Equal density | Equal momentum flux | Equal stagnation enthalpy | Equal artificial density | |||||
pipeline | ||||||||
1 | ||||||||
2 | ||||||||
3 | ||||||||
Energy dissipation |
pipeline | Equal density | Equal momentum flux | Equal stagnation enthalpy | Equal artificial density |
1 | no waves | rarefaction wave | rarefaction wave | shock |
2 | no waves | shock | shock | rarefaction wave |
3 | no waves | shock | shock | rarefaction wave |