
In this article, we focus on the BV regularity of the adapted entropy solutions of the conservation laws whose flux function contains infinitely many discontinuities with possible accumulation points. It is well known that due to discontinuities of the flux function in the space variable, the total variation of the solution can blow up to infinity in finite time. We establish the existence of total variation bounds for certain classes of fluxes and the initial data. Furthermore, we construct two counterexamples, which exhibit BV blow-up of the entropy solution. These counterexamples not only demonstrate that these assumptions are essential, but also show that the BV-regularity result of [S. S. Ghoshal, J. Differential Equations, 258 (3), 980-1014, 2015] does not hold true when the spatial discontinuities of the flux are infinite.
Citation: Shyam Sundar Ghoshal, John D. Towers, Ganesh Vaidya. BV regularity of the adapted entropy solutions for conservation laws with infinitely many spatial discontinuities[J]. Networks and Heterogeneous Media, 2024, 19(1): 196-213. doi: 10.3934/nhm.2024009
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In this article, we focus on the BV regularity of the adapted entropy solutions of the conservation laws whose flux function contains infinitely many discontinuities with possible accumulation points. It is well known that due to discontinuities of the flux function in the space variable, the total variation of the solution can blow up to infinity in finite time. We establish the existence of total variation bounds for certain classes of fluxes and the initial data. Furthermore, we construct two counterexamples, which exhibit BV blow-up of the entropy solution. These counterexamples not only demonstrate that these assumptions are essential, but also show that the BV-regularity result of [S. S. Ghoshal, J. Differential Equations, 258 (3), 980-1014, 2015] does not hold true when the spatial discontinuities of the flux are infinite.
In this article, we consider the following initial value problem for scalar conservation laws in one space dimension:
ut+A(x,u)x=0for(x,t)∈R×(0,∞), | (1.1) |
u(x,0)=u0(x)forx∈R. | (1.2) |
It is assumed that the flux function A(x,⋅) is C2 and uniformly convex, i.e., there exists a positive constant C such that Auu(x,⋅)≥C>0 for all x∈R. It is to be noted that as a function of the space variable, the function A(x,u) can have infinitely many spatial discontinuities with possible accumulation points.
Conservation laws with discontinuous flux [2,3,4,5,7,9,11,12,14,15,23,24,25,29,30] has been a subject of immense interest to the mathematical community, as it is known to model various real-world problems. Examples include, the hydrodynamic limit of interacting particle systems with discontinuous speed parameter [13], sedimentation [14], petroleum industry and polymer flooding [29], two-phase flow in heterogeneous porous medium [6], clarifier thickener units used in wastewater treatment plants and mineral processing [10], and traffic flow on highways with changing surface conditions [15], etc. One of the classical studies of this IVP with the flux having spatial heterogeneities come from the seminal paper of Kruzkov [26], which studies its well-posedness for sufficiently smooth flux A. However, in practice, the flux function A appearing in the IVP modelling real-life applications, may not be smooth and may have spatial discontinuities. Since the flux contains spatial discontinuities, the Kruzkov entropy condition does not make sense and hence a different notion for uniqueness, incorporating the non-smooth structure of the flux is required. Owing to this, the notion of an adapted entropy solution is used to single out a unique solution for IVPs with non-smooth flux. The notion of adapted entropy condition was introduced by Audusse and Perthame in [8] for unimodal and monotone fluxes and later it was generalized in [27] to a more general class of fluxes of the type A(x,u)=g(β(x,u)) with g, a continuous function and β, Caratheodory function (i.e. β measurable in the x variable and continuous in the u variable). The existence of the entropy solutions was established via the convergence of numerical approximations in, [28] using front tracking approximations for monotone convex fluxes, and in [31] using finite volume approximations for possibly non–convex monotone fluxes. Additionally, the convergence of finite volume approximations for unimodal fluxes was studied in [18] using a singular mapping technique. In addition, Ghoshal et al. [20,21] extended the results for a Locally Lipschitz g and BV spatial β, using a β− TVD (Total Variation Diminishing) property. Further, Ghoshal et al. [22] also extended the results using the front tracking approximations for fluxes with flat regions. In this article, we describe the existence and non-existence of total variation bounds on the solution for uniformly convex flux A(x,⋅).
Total variation plays a pivotal role in the study of hyperbolic conservation laws. In the case of homogeneous flux i.e., A(x,u)=f(u), using the Lax–Oleinik formula, it can be shown that if the flux function is C2 and uniformly convex, i.e., f″≥C>0, then the entropy solution u(t,⋅)∈BVloc(R) for any initial data u0∈L∞(R). In other words, a C2 uniformly convex flux induces a BV regularizing effect on the entropy solution. For a locally Lipschitz flux (homogeneous), this result is not true in general. However, front tracking and finite volume approximations indicate that, t↦TV(u(t,⋅)) is non-increasing. Thus, the total variation of the solution at any time t>0 cannot be greater than the total variation of the initial data. On the other hand, for a two flux problem with A(x,u)=H(−x)g(u)+H(x)f(u), where f and g are C2 and convex, the authors in [1] construct counterexamples to show that the total variation of the entropy solution (see [1, Def. 2.4] with A=θg and B=θf) blows up in finite time, even for BV initial data.
Furthermore, results produced by the finite volume method [9] suggest that the total variation of the entropy solution away from the interface x=0 remains bounded, i.e., u(t,⋅)∈BVloc(R∖{0}). Also, the BV smoothing effect away from the interface for two flux problems with uniformly convex flux is discussed in [17]. Surprisingly, if f(θf)=g(θg), the existence of BV bounds was proved in [16] using an explicit formula for the two flux problem obtained in [5]. Furthermore, the regularity of the solutions in BVs space for conservation laws with discontinuous flux were recently investigated in [19].
These results can be naturally extended for the case of finitely many discontinuities and hence we have the existence of uniform BV bounds on the solution.
In the present article, we will show that results on BV bounds for the case when F is unimodal and has infinitely many spatial discontinuities are completely different from the case of finitely many spatial discontinuities. At this point, we would like to mention that the case where A(x,⋅) does not contain critical points is relatively simpler and BV bounds can be easily obtained using finite volume [31] and front tracking [28] approximations provided u0∈BV(R).
Hence, the question of whether a BV bound on the solution for fluxes having critical points in the u-variable and infinitely many spatial discontinuities is interesting and nontrivial. In this article, we provide a sufficient condition on the initial data to obtain a BV bound for the entropy solution for uniformly convex fluxes. In the later part of this article, we construct two counterexamples to demonstrate that the conditions are essential. Note that the flux A(x,⋅) considered in the current article has the same minimum for each x and is uniformly convex. By providing two examples in Sections 3.2 and 3.3, we show that the BV-regularity results of [16] can not hold when the flux F has infinitely many discontinuities. The example in Section 3.3 further shows that even if we assume uniform convexity of the flux, the TV (Total Variation) of the entropy solution can blow up. The construction of the example in Section 3.3 is novel and it contains new ideas which differ from previous constructions [1,16].
Throughout this article, we assume that the flux function A(x,u) satisfies the following assumptions.
A-1 The function x↦A(x,u) is measurable, u↦A(x,u) is uniformly convex and there exists uM∈BV(R) such that the following holds:
minu∈RA(x,u)=A(x,uM(x))=0. |
A-2 There exists (h1,h2)∈C0(R)2 such that for all x∈R, we have h1(u)≤A(x,u)≤h2(u). In addition, hi for i=1,2 are strictly decreasing and then increasing functions with |h1(±∞)|=+∞.
A-3 There exists a continuous function η:R→R and a BV function a:R→R such that
|A(x,u)−A(y,u)|≤η(u)|a(x)−a(y)|∀x,y,u∈R. |
Remark 2.1. A typical example of a flux function satisfying the above hypothesis (see [8]) is given by
A(x,u)=(u−uM(x))2. |
In view of the above hypothesis, we define the following:
Definition 2.1. A function k:R→R is said to be a stationary state, if u(x,t)=k(x) is the weak solution to the IVP (1.1) and (1.2), with u0(x)=k(x). For α>0, we work with two types of stationary states namely, k±α:R→R such that A(x,k±α(x))=α with k+α(x)∈(uM(x),∞) and k−α(x)∈(−∞,uM(x)). On the other hand, for α=0, we have k+0=k−0=uM. We define Sα to be the set of all stationary states corresponding to height α≥0.
Definition 2.2 (Adapted Entropy Condition, [8]). A function u∈L∞(R×[0,T])∩C([0,T],L1loc(R)) is an adapted entropy solution of the Cauchy problem if it satisfies the following inequality in the sense of distribution:
∂t|u(x,t)−k±α(x)|+∂x[sgn(u−k±α(x))(A(x,u)−α)]≤0, | (2.1) |
for α≥0. Or equivalently, for all 0≤ϕ∈C∞c(R×[0,T))
∫R×[0,T]|u(x,t)−kα(x)|ϕt(x,t)+sgn(u(x,t)−kα(x))(A(x,u(x,t))−α)ϕx(x,t)dxdt+∫R|u0(x)−kα(x)|ϕ(0,x)dx≥0. |
Theorem 2.1. [Uniqueness [8,27]] Let u,v be entropy solutions to the IVP (1.1) and (1.2) with initial data u0,v0∈L∞(R). Assume that the flux A(x, u) satisfies the hypotheses (A-1) and (A-2). Then, there exists M>0 such that the following holds,
b∫a|u(x,t)−v(x,t)|dx≤b+Mt∫a−Mt|u0(x)−v0(x)|dx, | (2.2) |
for −∞≤a<b≤∞ and t∈[0,T].
For our BV regularity result established in Theorem 3.1, we employ approximate solutions constructed using a wave front tracking algorithm. The front tracking algorithm can be summarized as follows:
Step−I Approximate the initial data u0 by a piecewise constant function uδ0 with finitely many discontinuities such that uδ0→u0 in L1loc(R) as δ→0 and
TV(uδ0)≤C, |
for some C>0.
Step−II Approximate A(x,u) by Aδ(x,u) such that x↦Aδ(x,⋅) is piecewise constant with finitely many discontinuities and for fixed x, the function u→Aδ(x,u) is piecewise linear convex such that Aδ(x,u)→A(x,u) for a.e. x∈R. In addition, the stationary states kδ,±α corresponding to the flux Aδ should satisfy kδ,±α(x)→k±α(x) for a.e. x∈R.
Step−III Solve the following initial value problem,
ut+(Aδ(x,u))x=0for(x,t)∈R×(0,∞), | (2.3) |
u(x,0)=uδ0(x)forx∈R, | (2.4) |
and denote the solution by uδ. More specifically, at each discontinuity point of uδ0, and at each discontinuity point of x↦Aδ(u,x), use the Riemann solver to obtain a solution uδ(⋅,τ) until the time τ at which the a discontinuity (front) of uδ interacts with other discontinuities of uδ or with the spatial discontinuities of the flux Aδ. Solve the initial value problem (IVP) given by Eq (2.3), at this interaction time t=τ, using uδ(⋅,τ) as the initial data. Repeat this procedure until the next interaction, and continue in this manner.
Theorem 2.2. Suppose u0∈BV(R)∩L1(R) and A(⋅,⋅) satisfies the assumptions (A-1)–(A-3). Then, there exists a unique adapted entropy solution to Eq (1.1) corresponding to the initial data u0.
Proof. The proof can be done as in [22]. Since A(x,⋅) is uniformly convex, the proof is even simpler. Due to the strict convexity assumption, the number of fronts does not increase at any interactions (interactions in the interior as well as on the interface). This implies that the front tracking approximations can be continued for all time t>0. On the other hand, the singular map Ψ is invertible and the TVD property of Ψ(⋅,u(t,⋅)) gives the desired compactness. Thus, repeating the arguments in [22], the entire sequence of front tracking approximations converge to the unique entropy solution.
This section is devoted to the study of BV regularity of adapted entropy solution. In the next subsection, we introduce a condition on initial data to get a TV bound on entropy solution when the fluxes are uniformly convex. Later, we give two counter-examples to show that neither the additional condition on initial data (Λ(u0)<∞) nor the uniform convexity assumption on flux can be relaxed.
To obtain a BV regularity of entropy solutions, we need an assumption on initial data which is stronger than BV. This is introduced below:
Let b∈L∞(R) and −∞<x1<⋯<xn+1<∞. We define a sequence {Δwj}1≤j≤n as follows,
Δwj:={|b(xj)−b(xj+1)| if A(xj,⋅)=A(xj+1,⋅),|b(xj)−uM(xj)|+|b(xj+1)−uM(xj+1)| if A(xj,⋅)≠A(xj+1,⋅), | (3.1) |
for 1≤j≤n. We define Λ(b) as follows,
Λ(b):=sup{n∑j=1Δwj;−∞<x1<⋯<xn+1<∞ and Δwj is defined as in (3.1)} | (3.2) |
and the set X:={b∈L∞(R);Λ(b)<∞}. Since uM∈BV(R), we observe that X⊂BV(R). If x↦A(x,⋅) is piecewise constant then Eq (3.2) can be simplified in the following way: let −∞=z0<z1<⋯<zn<zn+1=∞ be discontinuity points of x↦A(x,u). We can write
Λ(b)=n∑k=0TV(zk,zk+1)(b)+n∑k=1[|b(zk−)−uM(zk−)|+|b(zk+)−uM(zk+)|]. |
Remark 3.1. Suppose uM∈BV(R), then Λ(b)<∞ implies TV(b)<∞ but the converse is not true. Furthermore, if A is homogeneous then Λ(b)=TV(b).
Theorem 3.1. Let A(⋅,⋅) satisfy (A-1)–(A-3). Additionally, we assume that A(⋅,x)∈C2(R) and ∂uuA(⋅,x)≥C1 for all x∈R where C1>0 does not depend on x. Let u be an adapted entropy solution to Eqs (1.1) and (1.2) with initial data u0 such that Λ(u0)<∞ where Λ is defined as in Eq (3.2). Then we have
TV(u(⋅,t))≤TV(uM)+C3Λ(u0)fort>0, |
whereC2=sup{‖A(⋅,x)‖C2[−M,M],x∈R} and C3:=(C2C1)32.
Before the proof of Theorem 3.1, here we prove a property of uniform convex flux in the following lemma.
Lemma 3.1. For a closed interval I⊂R, let f,g∈C2(I) such that f′′,g′′∈[C1,C2] for C2>C1>0. Additionally, assume that f(θf)=g(θg)=0. Then we have
|g−1+(a)−g−1+(b)|≤C3|f−1+(a)−f−1+(b)|fora,b∈IwhereC3=(C2C1)32. |
Proof. Suppose f(u1)=g(u2) with u1>θf,u2>θg. Now, we observe that
f(u1)=f(θf)+f′(θf)(u1−θf)+f′′(u∗)2|u1−θf|2≥C12|u1−θf|2,g(u2)=g(θg)+g′(θg)(u2−θg)+g′′(u∗)2|u2−θg|2≤C22|u2−θg|2. |
Subsequently, we have
C12|u1−θf|2≤C22|u2−θg|2. |
Therefore, we have
(u1−θf)≤(C2C1)12(u2−θg). |
Notice that
f′(f−1+(p))=f′(f−1+(p))−f′(θf)=(f−1+(p)−θf)1∫0f′′(λf−1+(p)+(1−λ)θf)dλ≤(C2C1)32(g−1+(p)−θg)1∫0g′′(λg−1+(p)+(1−λ)θg)dλ=(C2C1)32g′(g−1+(p)). |
Hence, we have
g−1+(a)−g−1+(b)=(a−b)1∫01g′(g−1+(λa+(1−λ)b))dλ≤(C2C1)32(a−b)1∫01f′(f−1+(λa+(1−λ)b))dλ=(C2C1)32(f−1+(a)−f−1+(b)). |
Proof of Theorem 3.1. We prove the estimate for the approximate solution uδ, and then we show that the estimates are uniform over δ. Let uδ be the approximate solution to Eq (1.1) obtained via wave front tracking. Note that there is no affine part on A(⋅,x) for all x∈R due to ∂uuA(x,u)≥C1. Due to uniform convexity no new state arises away from the interface for time t>0. Since there is no linear part in the flux, no rarefaction wave occurs at the interface for t>0. Therefore, for a time t0>0 and x∈R, there exists y(x)∈R such that Aδ(uδ(x,t0),x)=Aδ(uδ0(y(x)),y(x)). Suppose −∞=x0<x1<⋯<xm<xm+1=∞ are discontinuity points of x↦A(⋅,x). Let z1,z2∈(xi,xi+1) for some 0≤i≤m. Now, there are two cases
1. y(z1),y(z2)∈(xj,xj+1) for some 0≤j≤m. Then by Lemma 3.1 we have
|uδ(z1,t0)−uδ(z2,t0)|≤C3|uδ0(y(z1))−uδ0(y(z2))|. | (3.3) |
2. y(z1)∈(xj,xj+1),y(z2)∈(xk,xk+1) for some 0≤j≠k≤m. Then by Lemma 3.1 and the triangle inequality, we have
|uδ(z1,t0)−uδ(z2,t0)|≤|uδ(z1,t0)−uδM(z1)|+|uδ(z2,t0)−uδM(z2)|+|uδM(z1)−uδM(z2)|≤C3[|uδ0(y(z1))−uδM(y(z1))|+|uδ0(y(z2))−uδM(y(z2))|]+|uδM(z1)−uδM(z2)|. | (3.4) |
Suppose z∈(xi,xi+1) for 0≤i≤m−1, then by Lemma 3.1, we have
|uδ(z,t0)−uδM(z)|≤C3|uδ0(y(z))−uδM(y(z))|. | (3.5) |
Combining Eqs (3.3), (3.4) and (3.5) with definition Eq (3.2) of Λ we conclude Theorem 3.1.
In this section, we wish to construct an example of an adapted entropy solution such that u(⋅,1)∉BVloc(R) for a flux satisfying (A-1)–(A-3) and an initial datum u0∈BV(R) with Λ(u0)<∞. We also assume that the flux possesses C2 regularity in the state variable, that is, for a.e. x∈R, u↦A(x,u) is a C2-function (but not necessarily uniformly convex). Note that this result is special for fluxes having infinitely many spatial discontinuities since for a flux A with finitely many discontinuities and satisfying (A-1)–(A-3), we have TV(u(⋅,t))<∞ for BV initial data (see [16]).
Proposition 3.1. There exists a flux A satisfying (A-1)–(A-3) and an initial datum u0 such that Λ(u0)<∞ such that the corresponding entropy solution to (1.1) has TV blow up at some finite time T0>0.
Construction: Let us consider two sequences {yn}n≥0 and {zn}n≥1 such that they satisfy
yn−1<zn<yn for n≥1 andlimn→∞yn=limn→∞zn=z∗ for some z∗∈R. | (3.6) |
Now we consider the following flux,
A(x,u):=∞∑n=1fn(u)χ(yn−1,zn](x)+∞∑n=1gn(u)χ(zn,yn](x)+f1χ(−∞,y0](x)+u2χ(z∗,∞](x) | (3.7) |
where fn,gn are defined as follows
fn(u)=2n3/2u2+u4 and gn(u)=u4. |
Note that u↦A(x,u) is a C2-function for a.e. x∈R. Hence (A-1) is satisfied. Observe that A(x,u) satisfies (A-2), with h1(u)=u4,h2(u)=2u4 and uM≡0. Note that (A-3) is verified for A(x,u) with the following choice of η,a
η(u):=2u2 and a(x):=∞∑n=11n32χ(yn−1,zn](x)+1χ(−∞,y0](x). |
Loosely speaking, |(gn)−1+(fn(u))|≥u12n−38 gives a possible blow up in the solution.
We consider an initial datum defined as follows,
un0(x):={0 if yn−1<x<x1n,an if x1n<x<x2n,0 if x2n<x<zn,0 if zn<x<yn. |
We observe that rarefaction wave arises at x1n and shock wave is generated at x2n with shock speed λn where λn is calculated as follows
λn=fn(an)−fn(0)an−0=2ann32+a3n. | (3.8) |
Assume that at time t=tn the shock curve hits the interface; therefore, we have x2n+tnλn=zn. Since the speed of the extreme right characteristic of the rarefaction wave f′n(an) is bigger than an, we need to give sufficient gap between x1n and x2n such that before time t=1 it does not hit the shock wave and the interface at zn. Hence, the following inequality must hold:
zn−x1n≥f′n(an). | (3.9) |
Now after the shock wave from x2n hits the interface at zn it generates another shock wave from (zn,tn)∈R×R+. Note that this new shock wave has states bn,0 on its left and right respectively where bn=(gn)−1+(fn(an)). We want this shock wave not to meet the interface at yn before time t=1. Hence we must have
ξn(1−tn)+zn<yn, | (3.10) |
where ξn is the shock speed between bn,0, that is,
ξn=gn(bn)−gn(0)bn−0=b3n. | (3.11) |
If we are able to choose such x1n,x2n,zn,yn then the solution has the following structure up to time t=1, (see Figure 2)
1. For t∈[0,tn] we have
un(x,t):={0 if x<x1n,(f′n)−1(x−x1n/t) if x1n<x<x1n+f′n(an)t,an if x1n+f′n(an)t<x<x2n+λnt,0 if x2n+λnt<x<zn,0 if zn<x<yn, |
where λn is defined as in Eq (3.8).
2. For t∈[tn,1] we have
un(x,t):={0 if x<x1n,(f′n)−1(x−x1n/t) if x1n<x<x2n+f′n(an)t,an if x2n+f′n(an)t<x<zn,bn if zn<x<zn+ξn(t−tn),0 if zn+ξn(t−tn)<x<yn |
where ξn is defined as in Eq (3.11) and bn is defined as follows,
bn=(gn)−1+(fn(an)). |
Finally, we choose
an=1n1+δ,x2n−x1n=8nδ+52+8n3+3δ and zn−x2n=(4nδ+52+2n3+3δ)(1−1n2), |
where δ>0. Next we choose
yn−zn=2(2n2δ+72+1n4+4δ)34≤6(1n2δ+72)34 and x1n=yn−1+1n2. |
Note that
yn−1<x1n<x2n<zn<yn. |
Note that x2n−x1n=f′n(an). Hence, we have zn−x1n=zn−x2n+x2n−x1n>f′(an) since zn−x2n>0. Therefore, Eq (3.9) is satisfied. Observe that yn−zn=2((gn)−1+(fn(an)))3=2ξn>ξn(1−tn) since ξn>0 and 0<1−tn<1. Hence, the condition (3.10) is satisfied. Now we note that
yn−yn−1=yn−zn+zn−x2n+x2n−x1n+x1n−yn−1≤6(1n2δ+72)34+(4nδ+52+2n3+3δ)(1−1n2)+8nδ+52+8n3+3δ+1n2≤1n2+22nδ+52+8n218. |
Thus, there exists an y∞ such that yn→y∞. Set z∗=y∞ and y0=0 in Eq (3.7).
Note that TV(un0)≤n−1−δ and TV(un(⋅,1))≥|bn|. Observe that
|bn|=[2n2δ+72+1n4+4δ]14≥1n78+δ2. |
Note if we take an initial datum u0(x)=∞∑k=1uk0(x)1(yk−1,yk)(x), then u(x)=∞∑k=1uk(x)1(yk−1,yk)(x) will be the adapted entropy solution to Eq (1.1). Since TV(uk0)≤k−1−δ and supp(uk0),k≥1 are mutually disjoint, we have TV(u0)<∞. We observe that supp(uk(⋅,1)),k≥1 are mutually disjoint. Therefore, we have,
TV(u(⋅,1))≥∑k≥11k78+δ2. | (3.12) |
Now we choose, δ∈(0,4−1). Then, we have 78+δ2<1. Hence, TV(u(⋅,1))=∞.
In Section 3.2, we presented an example exhibiting a BV blow-up of entropy solutions corresponding to an initial datum u0 for which the quantity Λ(u0) is finite but the flux as a function of the state variable is not necessarily uniformly convex. In contrast to the previous section, we now construct an example starting from BV initial data and a uniformly convex flux such that the entropy solution has a TV blow-up at some finite time T. More precisely, we construct a flux and a BV initial data for which the quantity Λ(u0) is not finite.
Proposition 3.2. There exists a flux A satisfying (A-1)–(A-3) and an initial datum u0 such that ∂uuA(x,u)∈[C1,C2] for some C2>C1>0 and the corresponding entropy solution to Eq (1.1) has TV blow up at some finite time T0>0.
Proof. We start by constructing a flux A satisfying conditions (A-1)–(A-3) and the initial datum, for which the above proposition holds true: Let g(u)=u2 and for any n∈N, let
fn(u):={u2 if u≤−1n2/3,u2+u2n1/4−3n13/12u4+3n29/12u6−n15/4u8 if −1n2/3≤u≤1n2/3,u2 if u≥1n2/3,, |
which implies that
f′n(u)={2u if u≤−1n2/3,2u+2un1/4−12n13/12u3+18n29/12u5−8n15/4u7 if −1n2/3≤u≤1n2/3,2u if u≥1n2/3. |
and
f′′n(u)={2 if u≤−1n2/3,2+2n1/4−36n13/12u2+90n29/12u4−56n15/4u6 if −1n2/3≤u≤1n2/3,2 if u≥1n2/3.. |
Hence fn∈C2(R) for n≥1. Note that there exists n0∈N such that f′′n(u)≥1 for n≥n0. Suppose {an},{bn} are two sequences such that 0<an+1<bn+1<an. We consider a flux A as follows
A(x,u):={fn(u) for an≤x≤bn for n≥n0,g(u) otherwise. |
We choose an=1n2/3 and bn=an+1n2n. We approximate A by AN as follows
AN(x,u):={fn(u) for an≤x≤bn with n0≤n≤N,g(u) otherwise. |
By the choice of fn(u)=g(u) for |u|≥n−2/3. Consider the following data
u0(x):={0 for x<0,1 for x>0. | (3.13) |
Now, we analyze the characteristics. We track the paths traveled by the characteristics emanating from x=0,t=0 to get structural information about adapted entropy solution to Eq (1.1) corresponding to flux AN and data u0 as in Eq (3.13).
Let uN be the adapted entropy solution to Eq (1.1) with flux AN and data u0. Note that initially a rarefaction arises at x=0 and then it travels through the interfaces, and there is no interaction between waves. We observe that since n0≥4, fn=g=u2 for u=1, no wave arises from interfaces at t=0+ for x>0. Let LN:[0,2]→R be the path traveled by the characteristic arising from x=0 with speed 2wN with wN:=(N+1)−2/3.
Note that LN is a piecewise linear curve originating from x=0 (see Figure 3). We get LN(0)=0 and wish to estimate LN(1). Let vN,k∈[0,∞) be defined such that g(wN)=fm(vN,k). Suppose LN(t)∈[ak,bk] for t∈[tk,t′k]. Therefore, we have f′k(vN,k)(t′k−tk)=bk−ak. Suppose t′′k>tk is such that bk−ak=(t′′k−tk)g′(wN). We obtain
|t′′k−t′k|=(bk−ak)|f′k(vN,k)−g′(wN)|f′k(vN,k)g′(wN). |
Subsequently, we have
g′(wN)|t′′k−t′k|=(bk−ak)|f′k(vN,k)−g′(wN)|f′k(vN,k). |
Let L(˜tN)=aN/2; then we have
|1−˜tN|≤N∑k=[N2]+1(bk−ak)|f′k(vN,k)−g′(wN)|f′k(vN,k)g′(wN). |
Note that 1(N+1)2/3≥12(N/2)2/3 for N≥n1 for some n1>1. Subsequently, we have k2/3(N+1)2/3≥12. Now we observe that
fk(12(N+1)2/3)=12(N+1)4/3(1+1k1/4(1−k4/34(N+1)4/3)3)≤g(wN)124/3(1+116k1/4)≤g(wN)=fk(vN,k). |
Hence, we get wN2≤vN,k for N/2+1≤k≤N. Since (1−k4/3u2)3≥0 for |u|≤k−2/3 we have fk(wN)≥fk(vN,k), therefore wN≥vN,k. This shows that
|f′(vN,k)−g′(wN)|≤|wN−vN,k|+ˉCk1/4vN,k≤˜CwN. |
Hence,
|1−˜tN|≤N∑k=N2+1˜Ck2kwN=˜C(N+1)2/3N∑k=N2+11k2k≤˜C1(N+1)2/32NN2N+1≤˜C22NNN+13. | (3.14) |
Therefore,
|L(1)−2(N+1)2/3|≤˜C|1−˜tN|wN≤˜C32NNN+1. | (3.15) |
Let um be the entropy solution to Eq (1.1) with data u0 as in Eq (3.13) and flux Am. It will be now shown that the adapted entropy solution um agrees with uN in some subset of R×[0,1] for sufficiently large m. Due to the fact that fm=g for u≥(N+1)−2/3, then characteristic with speed 2(N+1)−2/3 travels through LN(1) for m≥N+1 and we observe the following:
um(x,t)=uN(x,t) for (x,t)∈DN | (3.16) |
where DN is defined as (see Figure 3)
DN:=(−∞,0]×[0,1]∪{(x,t),x≥LN(t),t∈[0,1]}. |
We now calculate the variation |uN(am+,1)−uN(am−,1)|, where uN is the adapted entropy solution to Eq (1.1) corresponding to flux AN and data u0.
Let the characteristic corresponding to u=12m2/3, originating from x=0 move through path Q(t). Note that Q(t) is analogous to L(t). By a similar argument as in Eq (3.15), we obtain
|Q(1)−am|≤˜C2m2m+1. |
Suppose Q(t) hits x=bm−1 and x=am at time t=˜t1 and t=˜t2 respectively. Suppose uN(am−)=˜wN, then we have,
am−bm−1=2wN(˜t2−˜t1) and am−bm−1=2˜wN(1−˜t1). |
Since ˜t2≥1 we get wN≤˜wN. Then we have
|1wN−1˜wN|≤˜t2−1am−bm−1. | (3.17) |
Note that
am−bm−1=12n2/3−12(n+1)2/3−1(n+1)2n+2≥13(n+1)5/3−1(n+1)2n+2≥16(n+1)5/3. |
By a similar argument as in Eq (3.14) we have
|˜t2−1|≤Bm2m+1. |
Hence, from Eq (3.17), we obtain
1−wN˜wN≤24Bm5/3m2m+112m2/3≤12Bm2m. |
Then, we get
1−12Bm2m≤wm˜wm. |
For sufficiently large m, that is there exists an m0>1 such that 1−12Bm2m≥12 for m≥m0. Therefore, ˜wm≤2wm. Hence, we get
|wm−˜wm|≤2w2m˜t2−1am−bm−1≤24Bm2m+23. |
Suppose fm(˜vm)=g(˜wm). Note that there exists m1>1 such that |˜wm−wm|≤16m2/3. Then we note that 13m2/3≤˜wm≤12m2/3. Subsequently, we get
fm(˜wm)=fm(12m2/3)=14m4/3(1+18m1/4)≥14m4/3=g(˜wm)=fm(˜vm). |
Thus, we get ˜wm≥˜vm. Note that
fm(13n2/3)=19m4/3(1+49m1/4)≤29m4/3≤g(˜wm)=fm(˜vm). |
Hence, 1/3≤˜vmm2/3≤1/2. Therefore,
˜w2m=14m4/3=fm(˜vm)=v2m(1+(1−m2/3vm)3m1/4)≤v2m(1+827m1/4). |
Hence,
|˜wm−˜vm|=˜wm−˜vm≥˜wm(√1+827m1/4−1√1+827m1/4)≥127m1/4(12m2/3−Bm2m+23). |
Therefore, we obtain for N≥2m+1,
|uN(am+,1)−uN(am−,1)|≥127m1/4(12m2/3−Bm2m+23). | (3.18) |
Finally, we show that um converges to an adapted entropy solution to Eq (1.1) for initial data u0 defined as in Eq (3.13) as m→∞. Note that ||uN−um||L1(R×[0,1])≤˜BN−2/3 for all m≥N. Therefore, {um}m≥1 is a Cauchy sequence in L1(R×[0,1]). Hence, there exists a u∈L1(R×[0,1]) such that um→u in L1(R×[0.1]). We also note that AN(x,⋅)=A(x,⋅) for x∈R∖[0,bN]. This implies k±α,N(x)=k±α(x) for x∈R∖[0,bN] and we get k±α,N→0 as N→∞. Since uN is an adapted entropy solution, uN→u in L1(R×[0,T]), k±α,N→k±α,AN(x,u)→A(x,u) for a.e. x∈R, we get u as the adapted entropy solution to Eq (1.1) for data u0 as in Eq (3.13) with flux A(x,u). By using Eq (3.16), we note that u(x,t)=uN(x,t) for (x,t)∈DN. From Eq (3.18) we get
|u(am+,1)−u(am−,1)|≥127m1/4(12m2/3−Bm2m+23). |
Hence we have TV(u(⋅,1))=∞.
Remark 3.2. Let u0 be defined as in Eq (3.13). Due to the finite speed of propagation we can consider a data ˜u0=u0χ[−M,M] for some large M>0 and the solution gives a TV blow up at time t=1.
The authors declare that they have not used Artificial Intelligence (AI) tools in the creation of this article.
The authors declare that there are no conflicts of interest.
SSG and GV would like to thank the Department of Atomic Energy, Government of India, under project no. 12-R & D-TFR-5.01-0520 for support. SSG acknowledges the Inspire faculty-research grant DST/INSPIRE/04/2016/000237. A part of this work was carried out during the GV's tenure of the ERCIM 'Alain Bensoussan' Fellowship Programme at NTNU.
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