Abstract
We show that the Hunter–Saxton equation \(u_t+uu_x=\frac{1}{4}\big (\int _{-\infty }^x \hbox {d}\mu (t,z)- \int ^{\infty }_x \hbox {d}\mu (t,z)\big )\) and \(\mu _t+(u\mu )_x=0\) has a unique, global, weak, and conservative solution \((u,\mu )\) of the Cauchy problem on the line.
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1 Introduction
The Hunter–Saxton (HS) equation [14] reads
Here u is an \(H^1({\mathbb {R}})\) function for each time t, and \(\mu (t)\) is a nonnegative Radon measure. Derived in the context of modeling liquid crystals, the HS equation has turned out to have considerable interest mathematically. It has, for example, a geometric interpretation [17,18,19,20,21], convergent numerical methods [9, 12], and a stochastic version [11], in addition to numerous extensions and generalizations [24, 25], too many to mention here. The first comprehensive study appeared in [15, 16]. While the HS equation was originally derived on differential form
where, in the case of smooth functions, \(\mu \) equal to \(u_x^2\) will automatically satisfy the second equation, we prefer to work on the integrated version. Note that there are several ways to integrate this equation, say
for which the uniqueness of conservative solutions on the half-line has been established in [5], but we prefer the more symmetric form. For us, it is essential to introduce a measure \(\mu (t)\) on the line such that for almost all times \(\hbox {d}\mu =\hbox {d}\mu _\mathrm{ac}=u_x^2 \hbox {d}x\). The times t when \(\hbox {d}\mu \ne u_x^2 \hbox {d}x\) will precisely be the times when uniqueness can break down. Our task here is to analyze this situation in detail and restore uniqueness by carefully selecting particular solutions called conservative solutions. The aim of this paper is to show the following uniqueness result (Theorems 3.6 and 5.10):
For any initial data \((u_0, \mu _0)\in {\mathcal {D}}\) the Hunter–Saxton equation has a unique global conservative weak solution \((u,\mu )\in {\mathcal {D}}\). Here \({\mathcal {D}}\) is given in Definition 2.2.
In the case of the so-called dissipative solutions, where energy is removed exactly at the times when the measure \(\mu \) ceases to be absolutely continuous, the uniqueness question has been addressed in [7] by showing the uniqueness of the characteristics.
The problem at hand can be illustrated by the following explicit example [6]. Consider the trivial case \(u_0=0\), which clearly has \(u(t,x)=0\) as one solution. However, as can be easily verified, also
is a solution for any \(\alpha \ge 0\), with \(\mu (0)=\alpha \delta _0\) and \(\hbox {d} \mu (t)=4 t^{-2} {\mathbb {I}}_{(-\alpha t^2/8, \alpha t^2/8)}(x)\hbox {d}x\) for \(t\not =0\). Here \({\mathbb {I}}_A\) is the indicator (characteristic) function of the set A. Thus, the initial value problem is not well-posed without further constraints.
Furthermore, it turns out that the solution u of the HS equation may develop singularities in finite time in the following sense: Unless the initial data are monotonously increasing, we find
Past wave breaking there are at least two different classes of solutions, denoted conservative (energy is conserved) and dissipative (where energy is removed locally) solutions, respectively, and this dichotomy is the source of the interesting behavior of solutions of the equation (but see also [8, 10]). We will in this paper consider the so-called conservative case where the associated energy is preserved.
The natural approach to solve the HS equation is by the use of characteristics, i.e., to solve the equation
However, in this case the function \(u=u(t,x)\) will in general only be Hölder and not Lipschitz continuous. This is the crux of the problem. Thus, we cannot expect uniqueness of solutions of this equation. Indeed, it is precisely in the case where uniqueness fails that the HS equation encounters singularities. See [3, 5, 7, 26,27,28]. We will reformulate the HS equation in new variables, the aim being to identify variables where the singularities disappear.
Rewriting the HS equation, using characteristics, yields a linear system of differential equations [4],
where \(C=\mu (0,{\mathbb {R}})=\mu (t,{\mathbb {R}})\). Here \(\check{U}(t,\xi )=u(t,\check{y}(t,\xi ))\) and \(\check{H}(t,\xi )=\int _{-\infty }^{\check{y}(t,\xi )}u_x^2(t,x)\hbox {d}x\). This system describes weak, conservative solutions and can be integrated to yield
Here we may recover \((u,\mu )\) from \(u(t,x)=\check{U}(t,\xi )\) for some \(\xi \) such that \(x=\check{y}(t,\xi )\) and \(\mu =\check{y}_\#(\check{H}_\xi )\hbox {d}\xi \). In particular, it has been shown in [4] that given any initial data \((u_0,\mu _0)\in {\mathcal {D}}\) there exists at least one conservative solution and this solution satisfies (1.4). On the other hand, the question of uniqueness of conservative solutions has not been addressed. This question can also be rephrased as: Do all conservative solutions satisfy (1.4)?
In [6], we introduced a new set of coordinates, which allowed us, in contrast to [4], to construct a Lipschitz metric d, which is not based on equivalence classes. The underlying system of differential equations, which has been derived using pseudo-inverses and the system (1.4), is surprisingly simple, but forced us to impose an additional first moment conditionFootnote 1, \(\int _{\mathbb {R}}(1+\left| x\right| )\hbox {d}\mu _0<\infty \), on the measure. To be more specific, d satisfies
for any two weak, conservative solutions \((u_i,\mu _i)\in {\mathcal {D}}\), which satisfy the additional condition \(\int _{\mathbb {R}}(1+\left| x\right| )\hbox {d}\mu _{i,0}<\infty \). The new coordinates are defined as follows. Let \(\chi (t,\eta )=\sup \{x\mid \mu (t, (-\infty ,x))<\eta \}\) and \({\mathcal {U}}(t,\eta )=u(t,\chi (t,\eta ))\) and introduce \({\hat{\chi }}(t,\eta )=\chi (t,C \eta )\) and \({\hat{{\mathcal {U}}}}(t,\eta )={\mathcal {U}}(t,C \eta )\) where \(C=\mu (t,{\mathbb {R}})\). Then we define
However, a closer look reveals that one explicitly associates to any initial data the weak conservative solution computed using (1.4). Thus, the question if all weak conservative solutions satisfy (1.4) is never addressed.
Furthermore, to study stability questions for conservative solutions the coordinates from [6] seem to be favorable, but not for investigating the uniqueness. The main difficulty stems from the fact that for each \(t\in {\mathbb {R}}\), the function \(F(t,x)=\mu (t,(-\infty ,x))\), where \(\mu \) denotes a positive, finite Radon measure, is increasing but not necessarily strictly increasing. This means, in particular, that its spatial inverse \(\chi (t,\eta )\) might have jumps. Time evolution of increasing functions with possible jumps can lead to the same problems as for conservation laws. What happens to jumps as time evolves? Do they satisfy some kind of Rankine–Hugoniot condition or do they behave more like rarefaction waves? In [6] this issue has been resolved by using the system (1.4) to show that any jump preserves position and height. Thus, the associated system for \((\chi (t,\eta ), {\mathcal {U}}(t,\eta ))\) cannot be treated using the classical ODE theory, but only in a weak sense with some additional constraints. Hence, these new variables would not simplify the study of uniqueness questions.
Given a conservative solution \((u,\mu )\), define the quantities
Then one can derive, see Theorem 3.4, that these quantities satisfy
In contrast to u(t, x), the function \(U(t,\xi )\) is Lipschitz continuous, and hence, the above system can be solved uniquely using the method of characteristics, which is sufficient to ensure the uniqueness of conservative solutions. In particular, it can be shown that by applying the method of characteristics the above system turns into (1.4), see Remark 3.5.
Although the uniqueness question is successfully addressed, the above system has one main drawback: The definition of the function \(y(t,\xi )\) is far from unique. On the other hand, the above system can be used to find other equivalent formulations of the Hunter–Saxton equation, which might be advantageous for addressing, e.g., stability questions. As an illustration, we here introduce a novel set of coordinates, which can be studied on its own, without relying on special properties of solutions to (1.4) and which avoids the formation of jumps but requires to impose additional moment conditions. The main idea is to introduce an auxiliary measure \(\nu \), such that \(G(t,x)=\nu (t,(-\infty ,x))\) is strictly increasing for each \(t\in {\mathbb {R}}\). To that end, define the auxiliary function (the power n to be fixed later)
which will be a smooth function for all Radon measures \(\mu \) and let
Provided \((u,\mu )\) is a weak, conservative solution of the HS equation, which satisfies an additional moment condition, see (5.2), we show, cf. Theorem 5.9, that the triplet \((\chi (t,\eta ), {\mathcal {U}}(t,\eta ), {\mathcal {P}}(t,\eta ))\) satisfies
where
In particular, \(h(t,\eta )\) is continuous w.r.t. time and Lipschitz continuous w.r.t. space, so that the above system has a unique solution and can be solved by applying the method of characteristics. This is sufficient to ensure the uniqueness of conservative solutions that satisfy an additional moment condition, cf. Theorem 5.10.
2 Background
In this section, we introduce the concept of weak conservative solutions for the Hunter–Saxton equation. Afterward, we show that there indeed exists at least one weak conservative solution to every admissible initial data. We use \({\mathcal {C}}_c^\infty \) to denote smooth functions with compact support and \({\mathcal {C}}_0^\infty \) to denote smooth functions that vanish at infinity.
As a starting point, we introduce the spaces we work in.
Definition 2.1
Let E be the vector space defined by
equipped with the norm \(\left\| f\right\| _{E}=\left\| f\right\| _{L^\infty } + \left\| f'\right\| _{L^2}\).
Furthermore, let
Write \({\mathbb {R}}\) as \({\mathbb {R}}=(-\infty ,1)\cup (-1,\infty )\) and consider the corresponding partition of unity \(\psi ^+\) and \(\psi ^-\), i.e., \(\psi ^+\) and \(\psi ^-\) belong to \(C^\infty ({\mathbb {R}})\), \(\psi ^-+\psi ^+\equiv 1\), \(0\le \psi ^\pm \le 1\), \({{\,\mathrm{supp}\,}}(\psi ^-)\subset (-\infty ,1)\), and \({{\,\mathrm{supp}\,}}(\psi ^+)\subset (-1,\infty )\). Furthermore, introduce the linear mapping \({\mathcal {R}}_1\) from \(H_1^1({\mathbb {R}})\) to E defined as
and the linear mapping \({\mathcal {R}}_2\) from \(H_2^1({\mathbb {R}})\) to E defined as
The mappings \({\mathcal {R}}_1\) and \({\mathcal {R}}_2\) are linear, continuous, and injective. Accordingly introduce \(E_1\) and \(E_2\), the images of \(H_1^1({\mathbb {R}})\) and \(H_2^1({\mathbb {R}})\) by \({\mathcal {R}}_1\) and \({\mathcal {R}}_2\), respectively, i.e.,
The corresponding norms are given by:
and
Note that the mappings \({\mathcal {R}}_1\) and \({\mathcal {R}}_2\) are also well-defined for all \(({\bar{f}}, a)\in L^2_1({\mathbb {R}})=L^2({\mathbb {R}})\times {\mathbb {R}}\) and \(({\bar{f}}, a, b)\in L_2^2({\mathbb {R}})=L^2({\mathbb {R}})\times {\mathbb {R}}^2\). Accordingly, let
equipped with the norms
and
respectively.
With these spaces in mind, we can define next the admissible set of initial data.
Definition 2.2
(Eulerian coordinates) The space \({\mathcal {D}}\) consists of all pairs \((u,\mu )\) such that
-
\(u\in E_2\),
-
\(\mu \in {\mathcal {M}}^+({\mathbb {R}})\),
-
\(\mu ((-\infty ,\, \cdot \,))\in E_1^0\),
-
\(\hbox {d}\mu _\mathrm{ac}=u_x^2 \hbox {d}x\),
where \({\mathcal {M}}^+({\mathbb {R}})\) denotes the set of positive, finite Radon measures on \({\mathbb {R}}\).
A weak conservative solution is not only a weak solution of the Hunter–Saxton equation, but has to satisfy several additional conditions, which make it possible to single out a unique, energy-preserving solution.
Definition 2.3
We say that \((u,\mu )\) is a weak conservative solution of the Hunter–Saxton equation with initial data \((u(0,\, \cdot \,),\mu (0,\, \cdot \,))\in {\mathcal {D}}\) if
-
(i)
At each fixed t, we have \(u(t,\, \cdot \,)\in E_2\).
-
(ii)
At each fixed t, we have \(\mu (t,(-\infty , \, \cdot \,))\in E^0_1\) and \(\hbox {d}\mu _\mathrm{ac}(t)=u_x^2(t,\, \cdot \,)\hbox {d}x\).
-
(iii)
The pair \((u,\mu )\) satisfies for any \(\phi \in {\mathcal {C}}_c^\infty ([0,\infty )\times {\mathbb {R}})\)
$$\begin{aligned}&\int _0^\infty \int _{{\mathbb {R}}}\Big [ u\phi _t+\frac{1}{2} u^2\phi _x \nonumber \\&\quad +\frac{1}{4} \left( \int _{-\infty }^x \hbox {d}\mu (t)-\int _x^\infty \hbox {d}\mu (t)\right) \phi \Big ] \hbox {d}x \hbox {d}t = -\int _{{\mathbb {R}}} u\phi |_{t=0} \hbox {d}x, \end{aligned}$$(2.3a)$$\begin{aligned}&\int _0^\infty \int _{{\mathbb {R}}} (\phi _t+u\phi _x)\hbox {d}\mu (t) \hbox {d}t =-\int _{{\mathbb {R}}}\phi |_{t=0}\hbox {d}\mu (0). \end{aligned}$$(2.3b) -
(iv)
The function u(t, x) defined on \([0,T]\times {\mathbb {R}}\) is Hölder continuous and the map \(t\mapsto u(t,\, \cdot \,)\) is Lipschitz continuous from [0, T] into \(E^0_2\).
-
(v)
There exists a set \({\mathcal {N}}\subset {\mathbb {R}}\) with \({{\,\mathrm{meas}\,}}({\mathcal {N}})=0\) such that for every \(t\not \in {\mathcal {N}}\) the measure \(\mu (t)\) is absolutely continuous and has density \(u_x^2(t,\, \cdot \,)\) w.r.t. the Lebesgue measure.
-
(vi)
The family of Radon measures \(\{ \mu (t)\mid t\in {\mathbb {R}}\}\) depends continuously on time w.r.t. the topology of weak convergence of measures.
Note that the family \(\{\mu (t) \mid t\in {\mathbb {R}}\}\) provides a measure-valued solution w to the linear transport equation
Thus, one has that \(\mu (t,{\mathbb {R}})=\mu (0,{\mathbb {R}})\) for all \(t\in {\mathbb {R}}\).
In [4], weak conservative solutions in \({\mathcal {D}}\) have been constructed. A closer look at their construction reveals that the following theorem holds.
Theorem 2.4
For any initial data \((u_0,\mu _0)\in {\mathcal {D}}\), the Hunter–Saxton equation has a global conservative weak solution \((u,\mu )\) in the sense of Definition 2.3.
In other words, all the properties stated in Definition 2.3 are satisfied for the conservative solutions constructed in [4]. However, some of them are better hidden than others. This is especially true for (iv) and (vi), which we show here.
We start by recalling the set of Lagrangian coordinates.
Definition 2.5
(Lagrangian coordinates) The set \({\mathcal {F}}\) consists of all triplets \((\check{y},\check{U},\check{H})\) such that
-
\((\check{y}-{{\,\mathrm{Id}\,}}, \check{U},\check{H})\in E_2\times E_2\times E_1\),
-
\((\check{y}-{{\,\mathrm{Id}\,}}, \check{U},\check{H})\in [W^{1,\infty }({\mathbb {R}})]^3\),
-
\(\displaystyle {\lim _{\xi \rightarrow -\infty }} \check{H}(\xi )=0\),
-
\(\check{y}_\xi \ge 0\), \(\check{H}_\xi \ge 0\) a.e.,
-
there exists \(c>0\) such that \(\check{y}_\xi +\check{H}_\xi \ge c>0\) a.e.,
-
\(\check{U}_\xi ^2=\check{y}_\xi \check{H}_\xi \) a.e..
Note that there cannot be a one-to-one correspondence between Eulerian and Lagrangian coordinates. Instead, one has that each element in Eulerian coordinates corresponds to an equivalence class in Lagrangian coordinates. Furthermore, all elements belonging to one and the same equivalence class can be identified using so-called relabeling functions.
Definition 2.6
(Relabeling functions) We denote by \({\mathcal {G}}\) the group of homeomorphisms f from \({\mathbb {R}}\) to \({\mathbb {R}}\) such that
where \({{\,\mathrm{Id}\,}}\) denotes the identity function.
Let \(X_1=(\check{y}_1,\check{U}_1,\check{H}_1)\) and \(X_2=(\check{y}_2,\check{U}_2,\check{H}_2)\) in \({\mathcal {F}}\). Then, \(X_1\) and \(X_2\) belong to the same equivalence class if there exists a relabeling function \(f\in {\mathcal {G}}\) such that
Furthermore, let
Then \({\mathcal {F}}_0\) contains exactly one representative of each equivalence class in \({\mathcal {F}}\). Note that if \(X=(\check{y},\check{U},\check{H})\in {\mathcal {F}}_0\) and \(f\in {\mathcal {G}}\), then one has
This implies that for each \(X=(\check{y},\check{U},\check{H})\in {\mathcal {F}}\) one has that \(\check{y}+\check{H}\in {\mathcal {G}}\).
Whether or not a function is a relabeling function, can be checked using the following lemma, which is taken from [13].
Lemma 2.7
(Identifying relabeling functions) If f is absolutely continuous, \(f-{{\,\mathrm{Id}\,}}\in W^{1,\infty }({\mathbb {R}})\), \(f_\xi -1\in L^2({\mathbb {R}})\), and there exists \(c\ge 1\) such that \(\frac{1}{c}\le f_\xi \le c\) almost everywhere, then \(f\in {\mathcal {G}}\).
In [4], one rewrites the Hunter–Saxton equation, with the help of a generalized method of characteristics as a linear system of differential equations, cf. (1.4),
where \(C=\mu (0,{\mathbb {R}})=\mu (t,{\mathbb {R}})\). This system of differential equations does not preserve \({\mathcal {F}}_0\), but respects equivalence classes. It can be integrated to yield
with initial data determined as introduced next in (2.8).
The connection between the pairs \((u,\mu )\in {\mathcal {D}}\) and the triplet \((\check{y},\check{U},\check{H})\in {\mathcal {F}}\) is given by the following definitions.
Definition 2.8
Let the mapping \(L:{\mathcal {D}}\rightarrow {\mathcal {F}}_0\) be defined by \(L(u,\mu )=(\check{y},\check{U},\check{H})\), where
Definition 2.9
Let the mapping \(M:{\mathcal {F}}\rightarrow {\mathcal {D}}\) be defined by \(M(\check{y},\check{U},\check{H})=(u,\mu )\), whereFootnote 2
Now we can finally focus on showing that the weak conservative solutions constructed in [4] satisfy Definition 2.3 (iv) and (vi).
2.1 On the Hölder continuity in the definition of weak conservative solutions
In [4], a generalized method of characteristics was used to construct weak conservative solutions as outlined above. This ansatz yields solutions u that are Hölder continuous with respect to space and time, but not Lipschitz continuous. Indeed, assume we are given a solution \((u,\mu )\) with corresponding Lagrangian coordinates \((\check{y}, \check{U}, \check{H})\) satisfying (2.6). Choose two points \((t_1,x_1)\) and \((t_2,x_2)\). Then, we can find \(\xi _1\) and \(\xi _2\) such that
Thus, we have
As far as the first term on the right-hand side is concerned, we have
where we have used that \(-\frac{1}{4} C\le \frac{1}{2}\check{H}(t,\xi )-\frac{1}{4} C\le \frac{1}{4} C\). For the second term observe that the time variable is the same, but not the space variable. In particular, we have
Here we used that \(u_x\in L^2({\mathbb {R}})\) and \(\hbox {d}\mu _\mathrm{ac}=u_x^2\hbox {d}x\) combined with the Cauchy–Schwarz inequality. Similar considerations yield
thus one ends up with Hölder continuity with Hölder exponent \(\frac{1}{2}\).
An important consequence of the above observation is the following. The solution to the ODE
would be unique if the function \(u(t,\, \cdot \,)\) were Lipschitz continuous. According to (2.14), this function is Hölder continuous with exponent \(\frac{1}{2}\), which leads to the possibility that there might exist several weak conservative solutions to one and the same initial data.
Moreover, one has, in general, that
and hence every time wave breaking occurs, the Lipschitz continuity is lost.
2.2 On the Lipschitz continuity in the definition of weak conservative solutions
In [4], a generalized method of characteristics was used to construct weak conservative solutions. The same approach has been used in [23], see also [6], in the case of the two-component Hunter–Saxton system, which generalizes the HS equation. However, there is a slight, but important difference in the solution spaces.
The one used in [23] is bigger, since one only assumes \(u(t,\, \cdot \,)\in L^\infty ({\mathbb {R}})\) and \(F(t,\, \cdot \,)\in L^\infty ({\mathbb {R}})\) instead of \(u(t,\, \cdot \,)\in E_2^0\) and \(F(t,\, \cdot \,)\in E_1^0\) . Thus, one would expect that the mapping \(t\mapsto u(t,\, \cdot \,)\) is Lipschitz continuous from [0, T] into \(L^\infty ({\mathbb {R}})\). Yet, a closer look at
where
reveals that \(u_t(t,\, \cdot \,)\) cannot be uniformly bounded in \(L^\infty ({\mathbb {R}})\), since \(u_x(t,\, \cdot \,)\) does not belong to \(L^\infty ({\mathbb {R}})\) and hence \(t\mapsto u(t,\, \cdot \,)\) is not Lipschitz continuous from [0, T] into \(L^\infty ({\mathbb {R}})\).
The smaller solution space used in [4] and here, on the other hand, is the correct choice, since the right-hand side of (2.15) belongs to \(E_2^0\) and hence the mapping \(t\mapsto u(t,\, \cdot \,)\) is Lipschitz continuous from [0, T] into \(E_2^0\).
2.3 On the continuity in the topology of weak convergence of measures in the definition of weak conservative solutions
In [4], a generalized method of characteristics was used to construct weak conservative solutions as outlined above. This ansatz yields measures \(\mu \), such that the mapping \(t\mapsto \mu (t,\, \cdot \,)\) is locally Lipschitz continuous if we equip the set of positive Radon measures with the Kantorovich–Rubinstein norm, which generates the weak topology [1].
Denote by \(\mathrm{BL}({\mathbb {R}})\) the space of all bounded and Lipschitz continuous functions equipped with the norm
Then, the Kantorovich–Rubinstein norm of \(\mu \in {\mathcal {M}}^+({\mathbb {R}})\) is given by
Given a solution \((u,\mu )\) with corresponding Lagrangian coordinates \((\check{y}, \check{U}, \check{H})\), which satisfy (2.6). Let \(\phi \in \mathrm{BL}({\mathbb {R}})\) such that \(\left\| \phi \right\| \le 1\). Then, we have
Recalling (2.6), we have
Thus,
for all \(\phi \in \mathrm{BL}({\mathbb {R}})\) such that \(\left\| \phi \right\| \le 1\), and, in particular,
which proves the local Lipschitz continuity, since \(\left\| \check{U}(s,\, \cdot \,)\right\| _{L^\infty }\) can be uniformly bounded on any bounded time interval.
Note that we cannot expect global Lipschitz continuity in time due to the last term in the above inequality.
3 Uniqueness of weak conservative solutions via Lagrangian coordinates
The main goal of this section is to present the proof of Theorem 3.6. To be a bit more precise, we will show that the characteristic equation
has a unique solution and thereby establish rigorously that each weak conservative solution satisfies the system of ordinary differential equations (2.6) in Lagrangian coordinates. The pair \((u,\mu )\) will be a solution in the sense of Definition 2.3. In particular, this means that the function u(t, x) is Hölder continuous in (t, x), and the map \(t\mapsto u(t,\, \cdot \,)\) is Lipschitz continuous from [0, T] into \(E^0_2\), the set of locally square integrable functions with possible non-vanishing asymptotics at \(\pm \infty \). The measure \(\mu (t)\) is finite, \(\mu (t,{\mathbb {R}})=C\), absolutely continuous and has density \(u_x^2(t,\, \cdot \,)\) w.r.t. the Lebesgue measure, except on a set \({\mathcal {N}}\) of zero measure. Furthermore, no moment condition is assumed on the measure here.
Given a weak conservative solution \((u,\mu )\in {\mathcal {D}}\), let
where F(t, x) is given by (2.16). Then, \(y(t,\, \cdot \,):{\mathbb {R}}\rightarrow {\mathbb {R}}\) is non-decreasing, \(y(t,\, \cdot \,)\le {{\,\mathrm{Id}\,}}\), and Lipschitz continuous with Lipschitz constant at most one [13, Thm. 3.8]. Furthermore, define
Note that \({\tilde{H}}(t,\, \cdot \,): {\mathbb {R}}\rightarrow [0,C]\) is non-decreasing (since \(y(t,\, \cdot \,)\) has Lipschitz constant at most one) and continuous. For completeness, we introduce for later use
For each time t, we have that
which implies that
Subtracting \(y(t,\xi )\) in the above inequality, we end up with
Remark 3.1
Note that we made a particular choice in the above calculations,
i.e., \(X(t, \, \cdot \,)=(y(t,\, \cdot \,),U(t,\, \cdot \,), {\tilde{H}}(t,\, \cdot \,))\in {\mathcal {F}}_0\) for all t. However, we could have chosen any representative of the corresponding equivalence class. Indeed, pick f(t, x) such that \(f(t,\, \cdot \,)\in {\mathcal {G}}\) for all t and replace \(y(t,\xi )\), \(U(t,\xi )\), and \({\tilde{H}}(t,\xi )\) by
\({\tilde{H}}_1(t,\xi )=f(t,\xi )-y_1(t,\xi )\), and \(U_1(t,\xi )=u(t,y_1(t,\xi ))\), respectively. Then
i.e., \(X_1(t,\, \cdot \,)=(y_1(t,\, \cdot \,), U_1(t,\, \cdot \,), {\tilde{H}}_1(t,\, \cdot \,))\in {\mathcal {F}}\) for all t. In particular, one has
3.1 The differential equation satisfied by the characteristics \(y(t,\xi )\)
Recall that u(t, x) is a weak solution to
and hence we obtain, by computing \(u(t,\, \cdot \,)\) along characteristics, that
Thus, for every characteristic x(s) given by
we have
Recall that due to the Hölder continuity of u the equation (3.7) will in general not have a unique solution. This estimate, together with the Hölder continuity of the weak conservative solution, helps us to refine the estimate for \(\vert x(t)-x(s)\vert \). Indeed, by assumption we know that there exists a constant D such that
Thus, every characteristic x(t) given through (3.7), satisfies
Recalling (3.8), we end up with
Integration then yields for all s and t in [0, T] that
Here M denotes some positive constant, which is independent of s and t. Furthermore, using (3.8), there exists a positive constant N such that
We are now ready to turn our attention toward the equation
In the case of a classical solution, one has that \(F(t,x(t))=F(s,x(s))\). In our more general case, one has
We will show this estimate in the next lemma. For simplicity, we let \(s=0\) and only consider the right inequality.
Lemma 3.2
In the above notation, we have the following result
Proof
We have that \(\mu (t,{\mathbb {R}})=C\) for all t. We will first show that for a given \(\varepsilon >0\), we can find an \(M>0\) such that
To that end, we first observe that for \(t=0\) we can find an \({\tilde{M}}_0>0\) such that
Let \(\delta \) be a small positive number to be decided later. Since \(u(t,\, \cdot \,)\in E_2\) for all \(t\in [0,T]\), we can find \(u_{\pm \infty }(t)\), \(x_\delta \), and \({\tilde{x}}_\delta \) such that
Next choose \(x_1<x_2<x_3<x_4\) such that
and pick functions \(\psi _1,\psi _2\in C^\infty ({\mathbb {R}})\) with
Define
which clearly satisfies \(\psi (t,\, \cdot \,)\in C^{\infty }_c({\mathbb {R}})\) for \(t\in [0,T]\). We then find
Furthermore, using that \((u,\mu )\) is a weak solution and \(\psi \) is a test function, we get
Direct computations yield
with
This implies for all \(t\in [0,T]\), using (3.14),
Choosing \(\delta \le \varepsilon /(2TC(\left\| \psi _1'\right\| _{L^\infty }+\left\| \psi _2'\right\| _{L^\infty }))\) and \(M=\max \{{\tilde{M}}_0, \left| x_\varepsilon \right| , \left| {\tilde{x}}_\varepsilon \right| , \left| x_2\right| , \left| x_3\right| \}\), we see that
Let \(\phi \in C^\infty ({\mathbb {R}})\) with \({{\,\mathrm{supp}\,}}(\phi _x)\subseteq [-{\tilde{M}},{\tilde{M}}]\) and \(\phi _x\ge 0\), such that \(\phi (x)=\phi (-\infty )\) for \(x\le -{\tilde{M}}\) with \(\phi (-\infty )=-\int _{{\mathbb {R}}}\phi _x(z) \hbox {d}z\), and \(\phi (x)=0\) for \(x\ge {\tilde{M}}\). Introduce \({\bar{\phi }}\in C^\infty ([0,T]\times {\mathbb {R}})\) such that
Fix a constant b. Then we find, since \(\phi (x-bt)-{\bar{\phi }}(t,x)\in C^\infty _c([0,T]\times {\mathbb {R}})\), that
By (3.13), the terms in the next to last line can be made arbitrarily small by increasing M, so that
If we choose \(b\ge u\) a.e., then \(\int _0^t \int (u-b)\phi _x \hbox {d}\mu (s) \mathrm{d}s\le 0\), which together with
yields
from which we conclude
\(\square \)
For any \(t\in {\mathbb {R}}\), introduce the strictly increasing function \(L(t,\, \cdot \,):{\mathbb {R}}\rightarrow {\mathbb {R}}\) given by
which satisfies, cf. (3.2) and (3.4),
Then,
and choosing \(x(s)=y(s,\xi )\), we get
Recalling that \(L(t,\, \cdot \,)\) is strictly increasing we end up with
Since \(\xi \mapsto y(t,\xi )\) is Lipschitz with Lipschitz constant at most one, it follows that \(y(t,\xi )\) is Lipschitz and hence differentiable almost everywhere in \([0,T]\times {\mathbb {R}}\).
Next we aim at computing \(y_t(t,\xi )\), using (3.10), and deriving the differential equation for \(y(t,\xi )\). One has, combining (3.10) and the analysis used to derive (3.12),
We can derive this estimate as follows. For simplicity, let \(s=0\) and consider only the right estimate.
Lemma 3.3
In the above notation, we have the following result
Proof
Given an \(\varepsilon >0\), we can find, as in the proof of Lemma 3.2, an \(M>0\) such that
Let \(\psi \in C^\infty ({\mathbb {R}})\) with \({{\,\mathrm{supp}\,}}(\psi _x)\subseteq [-{\tilde{M}},{\tilde{M}}]\) and \(\psi _x\ge 0\). Let \(\phi =\phi (t,x)\) satisfy \(\phi _t+g \phi _x=0\), with initial data \(\phi |_{t=0}=\psi \) for some given continuous function \(g=g(t,x)\). Introduce \({\bar{\phi }}\in C^\infty ([0,T]\times {\mathbb {R}})\) such that
Then we find, since \(\phi -{\bar{\phi }}\in C^\infty _c([0,T]\times {\mathbb {R}})\), that
By (3.18), the terms in the next to last line can be made arbitrarily small by increasing M, so that
Let \({\bar{x}}\in {\mathbb {R}}\) and consider the Hölder continuous function \(g(t,x)=u(0,{\bar{x}})+ D(t+\vert x-{\bar{x}}\vert )^{1/2}\), which satisfies \(g\ge u\) a.e. by (3.9). Furthermore, let \(\xi =\xi (t,z)\) solve \(\xi _t=g(t,\xi )\) with initial condition \(\xi (0,z)=z\). Then \(\phi (t, \xi (t, z))=\phi (0, \xi (0,z))=\psi (z)\) if \(\xi (t,\, \cdot \,)\) is a strictly increasing function. To see this, observe that one has if \(\xi (t,z_2)>\xi (t,z_1)\) for \(z_2>z_1\),
which implies
and thus \(\xi (t,\, \cdot \,)\) and \(\phi (t,\, \cdot \,)\) are strictly increasing functions.
Since \(g\ge u\) a.e., we have \(\int _0^t \int (u-g)\phi _x \hbox {d}\mu (s) \mathrm{d}s\le 0\), which together with
implies
from which we conclude
It remains to estimate \(\xi (t,z)-\xi (0,z)\). Integrating the differential equation for \(\xi (t,z)\), we find
where \(L=\vert u(0,{\bar{x}})\vert +\vert \xi (0,z)-{\bar{x}}\vert + \frac{D^2}{4}+\frac{T}{2}\). Thus,
which by the Gronwall inequality implies
or
Plugging this estimate into the integral representation of the solution, we find
Introducing \({\tilde{M}}=D(1+Le^T)\), (3.19) reads
A close look reveals that \({\tilde{M}}=D(1+(\vert u(0,{\bar{x}})\vert +\vert \xi (0,z)-{\bar{x}}\vert +\frac{D^2}{4}+\frac{T}{2})e^T)\), which means that \({\tilde{M}}\) depends linearly on \(\vert \xi (0,z)-{\bar{x}}\vert \). On the other hand, one has for \(z=\xi (0,z)={\bar{x}}\),
where \(M=D(1+(\left\| u(0,\, \cdot \,)\right\| _{L^\infty }+\frac{D^2}{4}+\frac{T}{2})e^T)\). Since the above argument holds for any choice of \({\bar{x}}\in {\mathbb {R}}\), we end up with
\(\square \)
Recalling (3.15), (3.16), and choosing \(x(s)=y(s,\xi )\), we get
and, applying (3.16) once more,
Since \(L(t,\, \cdot \,)\) is strictly increasing, we end up with
Note that the above inequality implies that
since combining (3.9) and (3.17) yields
Thus, one has
and it is left to compute
Recalling (3.21), the above equality (3.22) holds since \(y(t,\, \cdot \,)\) is Lipschitz continuous with Lipschitz constant at most one. Moreover, note that for \(u(t,y(t,\xi ))\not =0\), one has
This result also remains valid in the case \(u(t,y(t,\xi ))=0\). Hence, we conclude that \(y(t,\xi )\) satisfies
Furthermore, recalling (3.2), direct computations yield
3.2 The differential equation satisfied by \(U(t,\xi )\)
To begin with, we have a closer look at the system of differential equations, given by (3.23) and (3.24), which reads, using (3.3)
This systems of equations can be solved (uniquely) by the method of characteristics, if the differential equation
has a unique solution and \(k_\zeta (t,\, \cdot \,)\) is strictly positive for all \(t\in [0,T]\). According to the classical ODE theory, (3.26) has for each fixed \(\zeta \) a unique solution if the function \(U(t,\xi )=u(t,y(t,\xi ))\) is continuous with respect to time and Lipschitz with respect to space. The continuity with respect to time is an immediate consequence of (3.21). To establish the Lipschitz continuity with respect to space is a bit more involved. A closer look at (3.2) and (3.4) reveals that one has
and
This means especially, given \(\xi \in {\mathbb {R}}\), there exist \(\xi ^-\le \xi \le \xi ^+\) such that
and
In view of Definition 2.3 (v), we then have for \(\xi _1< \xi _2\) such \(y(t,\xi _1)\not =y(t,\xi _2)\) that
since both \(y(t,\, \cdot \,)\) and \({\tilde{H}}(t,\, \cdot \,)\) are Lipschitz continuous in space with Lipschitz constant at most one. Thus, (3.26) has a unique solution. Furthermore, if \(k(0,\zeta )=\zeta \) for all \(\zeta \in {\mathbb {R}}\) and \(\zeta _1<\zeta _2\), we have, as long as the function \(k(t,\, \cdot \,)\) remains non-decreasing that
which yields
Thus, \(k(t,\, \cdot \,)\) not only remains strictly increasing, it is also Lipschitz continuous with Lipschitz constant \(e^t\) and hence according to Rademacher’s theorem differentiable almost everywhere. In particular, one has that
Introducing
we have from (3.25)
In particular, one has
and (3.2) turns into
Furthermore, note that \({\bar{y}}(t,\zeta )\) is a characteristic due to (3.28a). Introducing
the system (3.28) reads
The above system can be extended to the system (2.6), which has been introduced in [4] and which describes conservative solutions in the sense of Definition 2.3, if we can show that
As an immediate consequence, one then obtains the uniqueness of global weak conservative solutions.
The proof of (3.30) is based on an idea that has been used in [2]. According to the definition of a weak solution, one has for all \(\phi \in {\mathcal {C}}_c^\infty ([0,\infty )\times {\mathbb {R}})\) that
Note that in the above equality, one can replace \(\phi \in {\mathcal {C}}_c^\infty ([0,\infty )\times {\mathbb {R}})\) by \( \phi (t,x)\) such that \(\phi (t,\, \cdot \,) \in {\mathcal {C}}_c^\infty ({\mathbb {R}})\) for all t and \(\phi (\, \cdot \,,x)\in {\mathcal {C}}^1({\mathbb {R}})\) for all x.
To prove that \({\bar{U}}(t,\zeta )\) is Lipschitz, we have to make a special choice of \(\phi (t,x)\). Let
where \(\psi \) is a standard Friedrichs mollifier. Our choice is motivated by the following observation,
and hence
Direct calculations then yield
Introduce the function
and note that \(F_\mathrm{ac}(\tau ,\, \cdot \,)\) is absolutely continuous. Moreover, one has
and
which implies
For the last two terms, observe that for every \(\tau \not \in {\mathcal {N}}\), i.e., for almost every \(\tau \in [0,T]\) one has
and
Thus, the dominated convergence theorem yields
In particular,
i.e., \({\bar{U}}(t,\zeta )\) is Lipschitz continuous with respect to time, and
for all \((t,\zeta )\) in \([0,T]\times {\mathbb {R}}\). Moreover, one has, using (3.27) and (3.29)
i.e., \({\bar{U}}(t,\zeta )\) is Lipschitz continuous with respect to space.
The final step is to derive the differential equation for \(U(t,\xi )\) from (3.31). Recall that we have the relation
Since \(k(t,\, \cdot \,)\) is continuous and strictly increasing, there exists a continuous and strictly increasing function \(o(t,\, \cdot \,)\) such that
Now, given \(\xi \in {\mathbb {R}}\), there exists a unique \(\zeta \in {\mathbb {R}}\) such that \(k(t,\zeta )=\xi \), and thus,
By definition, we have that \(o(t,\, \cdot \,)\) is continuous and strictly increasing and hence differentiable almost everywhere. Furthermore, one has that \(o(t,\, \cdot \,)\) satisfies
by (3.27), which yields
Since u(t, x) can be uniformly bounded on \([0,T]\times {\mathbb {R}}\), it follows that \(o(t,\xi )\) is Lipschitz with respect to both space and time on \([0,T]\times {\mathbb {R}}\) and by Rademacher’s theorem differentiable almost everywhere. Moreover, direct calculations yield
For every \(t\in [0,T]\), \(o(t,\, \cdot \,)\) is strictly increasing and continuous, and combining (3.33) and (3.34), one has
Furthermore, both \({\bar{U}}\) and o are Lipschitz with respect to both space and time on \([0,T]\times {\mathbb {R}}\), and hence, both U and \({\bar{U}}\) are Lipschitz and hence differentiable almost everywhere on \([0,T]\times {\mathbb {R}}\). Using (3.31) and (3.36), we finally end up with
Following closely [4] one can show that for each time t the triplet \((y,U,{\tilde{H}})\) belongs to \({\mathcal {F}}_0\). Furthermore, the system given by (3.25) and (3.37) can be uniquely solved in \({\mathcal {F}}_0\) with the help of the method of characteristics. Thus, we have shown the following result.
Theorem 3.4
Given a weak conservative solution \((u,\mu )\) to the Hunter–Saxton equation. Then, the functions \(y(t,\xi )\), \(U(t,\xi )\), and \({\tilde{H}}(t,\xi )\) defined in (3.1), (3.2), and (3.3), respectively, satisfy the following system of differential equations
which can be solved uniquely in \({\mathcal {F}}_0\) with the help of the method of characteristics. In particular, applying the method of characteristics yields the system of ordinary differential equations (2.6), which describes the weak conservative solutions constructed in [4].
Remark 3.5
Note that the above system of differential equations (3.38) is related to the system (1.4) by relabeling. Indeed, denote by \((\check{y}, \check{U}, \check{H})\) the classical Lagrangian solution with initial data in \({\mathcal {F}}_0\), which solves (1.4), as introduced in [4].
Applying the method of characteristics to (3.38), will yield a unique solution, since the characteristic equation
can be solved uniquely and \(k(t,\, \cdot \,)\) is strictly increasing, see the beginning of this subsection. Thus, we are led to investigating the system
where \(({\hat{y}}, {\hat{U}}, {\hat{H}})(t,\zeta )=( y, U, {\tilde{H}})(t,k(t,\zeta ))\) with initial data
While the last three equations coincide with the ones in (1.4), which suggests
the role of the first equation has to be clarified to prove (3.40). By construction, one has that
which implies that
and in particular, \(k(t,\, \cdot \,)\) is the relabeling function connecting \((y, U, {\tilde{H}})(t,\, \cdot \,)\in {\mathcal {F}}_0\) with \(({\hat{y}}, {\hat{U}}, {\hat{H}})(t,\, \cdot \,)\in {\mathcal {F}}\) for every \(t\in {\mathbb {R}}\). Furthermore, since \(k(t,\zeta )\) can be recovered using \({\hat{y}}(t,\zeta )\) and \({\hat{H}}(t,\zeta )\), system (3.39) can be reduced to (1.4) and hence one obtains the weak conservative solutions constructed in [4].
We have proved the following theorem.
Theorem 3.6
For any initial data \((u_0, \mu _0)\in {\mathcal {D}}\), the Hunter–Saxton equation has a unique global conservative weak solution \((u,\mu )\in {\mathcal {D}}\) in the sense of Definition 2.3.
4 Introduction of an auxiliary function
As a preparation for rewriting the Hunter–Saxton equation in a set of coordinates, which shares the essential features with the Lagrangian coordinates, while at the same time avoiding equivalence classes, we introduce an, at the moment, auxiliary function p(t, x).
According to the definition of a weak solution, one has for all \(\phi \in {\mathcal {C}}_c^\infty ([0,\infty )\times {\mathbb {R}})\) that
Furthermore, recall that \(F(t,x)=\mu (t,(-\infty ,x))\). If we would use the change of variables from [6], which is based on the pseudo-inverse of F, one difficulty turns up immediately. The function \(F(t,\, \cdot \,)\) might have intervals, where it is constant and that would especially mean that its inverse would have jumps. The classical method of characteristics implies that these intervals, where \(F(t,\, \cdot \,)\) is constant, will change their position (i.e., they move to the right or to the left), but their length remains unchanged. This would imply that one has to deal with jumps in the inverse, and hence, the involved change of variables does not simplify the problem we are interested in. Therefore, a change of variables, for proving the existence and uniqueness of conservative solutions of the HS equation, while at the same time avoiding equivalence classes, should not be based on the inverse of F, but the inverse of a strictly increasing and bounded function. This is where p(t, x) will come into the play.
Let \(n\in {\mathbb {N}}\). Introduce the nonnegative function
with
We note the following elementary result.
Lemma 4.1
Let \(n\in {\mathbb {N}}\) and \(K_n\) be given by (4.3). Then \(K_n\in L^p({\mathbb {R}})\cap {\mathcal {C}}^\infty _0({\mathbb {R}})\) for all \(1\le p\le \infty \). Note that
The jth derivative \(K_n^{(j)}\) satisfies
where \(q_{n,j}(x)\) denotes a polynomial with degree not exceeding \(2^{j+1}n-2n-j\).
Thus, \(p_n(t,\, \cdot \,)=K_n\star \mu (t)\in {\mathcal {C}}^\infty _0({\mathbb {R}})\cap H^s({\mathbb {R}})\) for any integer \(s\ge 1\).
Proof
Clearly \(K_n^{(j)}=q_{n,j}r^{-2^j n}\) for some polynomial \(q_{n,j}\) where \(r=1+x^2\). It remains to estimate the degree of \(q_{n,j}\). We prove this by induction. Observe first that \(\deg (q_{n,0})=0\) and \(\deg (r^n)=2n\). We find in general
Assume that \(\deg (q_{n,j})\le 2^{j+1}n-2n-j\) for some j. Then, we note
Furthermore, one has
and therefore \(p_n(t,x)\) not only belongs to \({\mathcal {C}}^\infty _0({\mathbb {R}})\), but \(p_n(t,\, \cdot \,)\) in \(H^s({\mathbb {R}})\) for any integer \(s\ge 1\). \(\square \)
Remark 4.2
We will drop the subscript n in the notation, and the value of n will only be fixed later. Thus, we write
What can we say about the time evolution of the function p(t, x)? We have two main ingredients: On the one hand the definition of p(t, x). Consider \(\psi \in {\mathcal {C}}_c^\infty ({\mathbb {R}})\) such that \({{\,\mathrm{supp}\,}}(\psi )\subset (-1,T+1)\), \(\psi \equiv 1\) on [0, T], and \(0\le \psi \le 1 \). If we define \(\phi (t,x)=\psi (t)K(x)\), then \(\phi (t,x)\in {\mathcal {C}}^\infty ([0,\infty )\times {\mathbb {R}})\), and it can be approximated by admissible test functions. On the other hand, we have the definition of a weak solution (4.1), which implies
Note that the above equation implies that the function p(t, x) is locally Lipschitz continuous with respect to time, if
can be uniformly bounded. Therefore, observe that
Furthermore, since u(t, x) is a weak solution to
we have that
Thus, Rademacher’s theorem yields that the function
from [0, T] to \({\mathbb {R}}\) is Lipschitz continuous (or locally Lipschitz continuous on \([0,\infty )\times {\mathbb {R}}\)) and hence differentiable almost everywhere on the finite interval [0, T]. In fact, one has from (4.4) and Definition 2.3 that
for all \((t,x)\in [0,T]\times {\mathbb {R}}\). Indeed, use (4.4) as a starting point, which reads in Lagrangian coordinates \((\check{y}, \check{U}, \check{H})\),
Recalling (2.6), direct calculations yield
which implies
for all \((t,x)\in [0,T]\times {\mathbb {R}}\).
Note that combining (4.5), (3.6), and Lemma 4.1, one has
For later use, note that, we have
and
where B is independent of time. A closer look reveals that
Furthermore, Lemma 4.1 implies that \(p_x(t,\cdot )\in {\mathcal {C}}_0^\infty ({\mathbb {R}})\) and
Finally, note the following useful expression
Thus, the function
is differentiable almost everywhere on \([0,T]\times {\mathbb {R}}\) and satisfies
Here we used, in the last step, (3.2) and (3.23). Note that \(g(t,\xi )\) is not only differentiable on \([0,T]\times {\mathbb {R}}\), but even Lipschitz continuous.
5 Uniqueness in a new set of coordinates
In this section, we will rewrite the Hunter–Saxton equation in a set of coordinates, which shares the essential features with the Lagrangian coordinates, while at the same time avoids equivalence classes. However, there is a price to pay: we have to impose an additional moment condition.
Given \(\gamma >2\) and a weak conservative solution \((u,\mu )\) in the sense of Definition 2.3, such that
Using the reformulation of the Hunter–Saxton equation in Lagrangian coordinates, whose time evolution is given by (2.6) and that \(f_\gamma (x)=\vert x\vert ^\gamma \) is convex for \(\gamma >2\), it follows that
We can see this as follows.
for a constant \({\tilde{C}}\), using (2.7c), (2.9b) and the estimate
Moreover, recalling the definition of p(t, x), cf. (4.2) and introducing the nonnegative measure
we have that (5.2) implies for any \(n\ge \gamma \),
For details, we refer to Lemma A.3.
Furthermore, let
where F(t, x) is given by (2.16). Then for all \(t\in {\mathbb {R}}\) the function \(G(t,\, \cdot \,)\) is strictly increasing and satisfies
Last but not least introduce \(\chi (t,\, \cdot \,)\) the (pseudo) inverse of \(G(t,\, \cdot \,)\), i.e.,
Then \(\chi (t,\, \cdot \,):[0,B+C]\rightarrow {\mathbb {R}}\) is strictly increasing for every \(t\not \in {\mathcal {N}}\). Furthermore, since the function \(G(t,\, \cdot \,)\) is of bounded variation, it can have at most countably many jumps, which implies that \(\chi (t,\, \cdot \,)\) can have at most countably many intervals where it is constant. On the other hand, the function \(\chi (t,\, \cdot \,)\) has no jumps since the function \(G(t,\, \cdot \,)\), in contrast to \(F(t,\, \cdot \,)\), is strictly increasing.
Our first goal is to show that
where \(y(t,\xi )\) is given by (3.1) and \(\ell (t,\, \cdot \,):[0,B+C]\rightarrow {\mathbb {R}}\) is a strictly increasing function to be determined next. Note that combining (4.13) and (5.5) one has
and therefore (3.5) can be rewritten as
Introducing (cf. (3.2) and (4.13))
we end up with
Since \(H(t,\, \cdot \,):{\mathbb {R}}\rightarrow [0, B+C]\) is strictly increasing (as \({\tilde{H}}\) is non-decreasing and g is strictly increasing) and continuous, it is invertible with inverse \(\ell (t,\, \cdot \,)\), i.e.,
This is the function sought in (5.8). Furthermore,
Since \(y(t,\, \cdot \,)\) is surjective and non-decreasing, we end up with
Remark 5.1
Recall Remark 3.1 and the notation therein. Assume
where \(X(t,\, \cdot \,)\in {\mathcal {F}}_0\) and \(f(t,\, \cdot \,)\in {\mathcal {G}}\), i.e., \(X(t, \, \cdot \,)\) and \(X_1(t,\, \cdot \,)\) belong to the same equivalence class. Then, following the same lines as above and denoting the inverse of \(f(t,\, \cdot \,)\) by \(f^{-1}(t,\, \cdot \,)\), we would have ended up with
and
Thus, we obtain the same function \(\chi (t,\eta )\) independent of which representative in the corresponding equivalence class we choose. This is in contrast to some of the following steps, where relabeling will play a crucial role. In particular, it is then of great importance, which representative we choose from the equivalence class.
5.1 Differentiability of \(\chi (t,\eta )\) with respect to time
Next, we want to study the time evolution of \(\chi (t,\eta )\). On the one hand, we will see that \(\chi (t,\eta )\) behaves like a characteristic. On the other hand, we expect \(\chi _t(t,\, \cdot \,)\in L^\gamma ([0,B+C])\), since one has
To begin with, we aim at showing that \(\chi (t,\eta )\) is differentiable with respect to time in the following sense: We establish that \(\chi (\, \cdot \,,\eta )\) is Lipschitz continuous and show that for each \(t\in [0,T]\) one has that
exists for almost every \(\eta \in [0,B+C]\). The dominated convergence theorem then implies that \(\chi _t(t,\, \cdot \,)\in L^\gamma ([0,B+C])\).
To establish that \(\chi (t,\eta )\) is Lipschitz with respect to time, a relabeling argument will be the key. We will show that \((y+H)(t,\, \cdot \,)\) is a relabeling function denoted \(v(t,\, \cdot \,)\). To that end, observe that combining (3.2) and (5.9) yields
Introducing the function
where \(g(t,\xi )\) is given by (4.13), we end up with
Combining (4.9), (4.10), and \(0\le y_\xi (t,\xi )\le 1\), we have that \(v(t,\, \cdot \,)\) satisfies all assumptions of Lemma 2.7, and hence, \(v(t,\, \cdot \,):{\mathbb {R}}\rightarrow {\mathbb {R}}\) is a relabeling function. Thus, \(v(t,\, \cdot \,):{\mathbb {R}}\rightarrow {\mathbb {R}}\) is strictly increasing and continuous, which implies that there exists a unique, strictly increasing and continuous function \(w(t,\, \cdot \,):{\mathbb {R}}\rightarrow {\mathbb {R}}\) such that
In particular, one has
Introducing
the relation (5.15) rewrites as
Since both \(H(t,\, \cdot \,)\) and \(w(t,\, \cdot \,)\), and hence \({\hat{H}}(t,\, \cdot \,)\), are strictly increasing and continuous, there exists a unique, strictly increasing and continuous function \({\hat{\ell }}(t,\, \cdot \,):[0,B+C]\rightarrow {\mathbb {R}}\) such that
Recalling (5.16) and (5.17), we have that
Thus, cf. Remark 5.1,
and
which, together with (5.18), implies
An important consequence of the above equality is that we can choose whether we want to study the differentiability of \(\chi (t,\eta )={\hat{\ell }}(t,\eta )-\eta \) or of \({\hat{\ell }}(t,\eta )\) with respect to time. Since \({\hat{\ell }}(t,\, \cdot \,)\) is the inverse to \({\hat{H}}(t,\, \cdot \,)\), it seems advantageous to study \({\hat{\ell }}(t,\eta )\) in detail. The basis will be a good understanding of the relabeling function \(v(t,\eta )\) and its inverse \(w(t,\eta )\).
5.1.1 The Lipschitz continuity of \(w(t,\xi )\)
We proceed by showing that the function \(w(t,\xi )\) is Lipschitz continuous, which then implies that both \({\hat{y}}(t,\xi )\) and \({\hat{H}}(t,\xi )\) are differentiable almost everywhere. A closer look at (5.14) reveals that \(v(t,\xi )\) is Lipschitz continuous and hence differentiable almost everywhere on \([0,T]\times {\mathbb {R}}\). In particular, (4.14), (4.9), and \(0\le y_\xi (t,\xi )\le 1\) yield
which satisfies
by applying in addition (3.6) and (3.2). Now, given \(\xi \in {\mathbb {R}}\), there exists a unique \(\eta \in {\mathbb {R}}\) by (5.16), such that
Thus, we can write
By definition, we have that \(w(t,\, \cdot \,)\) is continuous and strictly increasing. In particular, one has that \(w(t,\, \cdot \,)\) is differentiable almost everywhere and
Combined, with (5.24), this yields
Furthermore, one has
This finishes the proof of the Lipschitz continuity of \(w(t,\xi )\), which implies by Rademacher’s theorem that \(w(t,\xi )\) is differentiable almost everywhere on \([0,T]\times {\mathbb {R}}\). Since also y, \({\tilde{H}}\), and g are Lipschitz continuous on \([0,T]\times {\mathbb {R}}\), (5.9) and (5.17) imply that \({\hat{H}}\) and \({\hat{y}}\) are differentiable almost everywhere on \([0,T]\times {\mathbb {R}}\).
5.1.2 The Lipschitz continuity of \({\hat{\ell }}(\, \cdot \,,\eta )\)
We are now ready to show the Lipschitz continuity of \({\hat{\ell }}(\, \cdot \,,\eta )\), which immediately implies that \(\chi (\, \cdot \,,\eta )\) is Lipschitz continuous by (5.21). In view of (5.19), we start by having a closer look at \({\hat{H}}(t,\xi )\). By (5.16), we have that
and, using (5.9), (3.24), and (4.14) that
Combing the above equations and recalling (4.15), (5.17), (5.18), and (5.22), we get
If we can show that the term on the right-hand side can be bounded by a multiple of \({\hat{H}}_\xi \), then we are led to sub- and supersolutions, which solve a transport equation. Recalling (5.9), (4.13), and (3.6), we have that
Here we have used that
which combines (4.13), (5.9), (5.17), \(0\le {\tilde{H}}_\xi (t,\xi )\le 1\), and \(w_\xi (t,\xi )\ge 0\). In particular, one obtains that
where \(A=3(\left\| u(0,\, \cdot \,)\right\| _{L^\infty }+\frac{1}{4}CT)\). Applying the method of characteristics, we end up with the following estimate
Now, following the same lines as before, we have: Given \(\eta \in [0,B+C]\), there exists a unique \({\hat{\eta }}\in {\mathbb {R}}\) such that
Furthermore, we have
since \({\hat{\ell }}(t,\, \cdot \,)\) is strictly increasing, and (cf. (5.21))
This finishes the proof of the Lipschitz continuity of \({\hat{\ell }}(\, \cdot \,,\eta )\). Note that \(\chi (t,\, \cdot \,):[0,B+C]\rightarrow {\mathbb {R}}\) and hence 2A can be seen as a dominating function. This observation is essential since the differential equation for \(\chi \) has to be considered in \(L^\gamma ([0,B+C])\).
5.1.3 The time derivative of \(\chi _t(t,\eta )\)
It is left to compute, cf. (5.21),
for almost every \(\eta \in [0,B+C]\).
5.1.4 The time derivative of \(\ell (t,\eta )\)
To begin with, we will show that
exists for almost every \(\eta \in [0,B+C]\) and compute its value. Since \(\ell (t,\, \cdot \,)\) is the inverse of \(H(t,\, \cdot \,)\), cf. (5.11), we start by having a closer look at \(H(t,\xi )\). Recall (3.21), which implies that
and, combined with (3.20), that there exists a positive constant \({\tilde{M}}\) such that
Applying (3.2), the above inequality reads
As the following lemma shows a similar estimate holds for \(H(t,\xi )\). The proof relies on a detailed investigation of the function \(g(t,\xi )\) and can be found in Lemma A.1.
Lemma 5.2
(i) Let \(g(t,\xi )\) be given by (4.13). Then, there exists a positive constant \({\bar{M}}\) such that
(ii) Let \(H(t,\xi )\) be defined by (5.9). Then
Since both \(H(t,\, \cdot \,)\) and its inverse \(\ell (t,\, \cdot \,)\) are strictly increasing and continuous, we have that there exists a unique \(\eta (s)\) such that
and replacing \(\xi \) by \(\ell (s,\eta )\) in Lemma 5.2 (ii), we have
Furthermore, note that the above inequality implies that \(\eta (s)\rightarrow \eta \) as \(s\rightarrow t\) and hence \(\ell (s,\eta )\rightarrow \ell (t,\eta )\) as \(s\rightarrow t\) by (5.32).
Thus, we have
if all the above limits exist.
The first limit is of the form
since \(\eta (s)\rightarrow \eta \) as \(s\rightarrow t\). Moreover, \(\ell (t,\, \cdot \,)\) is strictly increasing and continuous and hence differentiable almost everywhere. Thus, the above limit exists for almost every \(\eta \in {\mathbb {R}}\) and equals \(\ell _\eta (t,\eta )\).
For the second limit, keep in mind that both \(u(t,\, \cdot \,)\) and \(p(t,\, \cdot \,)\) are continuous and that \(\ell (s,\eta )\rightarrow \ell (t,\eta )\) as \(s\rightarrow t\). The estimate (5.33) then implies that
Here we used (5.8), (4.13), (5.9). Introducing
we end up with
where
Using once more that \(u(t,\, \cdot \,)\) is continuous and that \(\ell (s,\eta )\rightarrow \ell (t,\eta )\) as \(s\rightarrow t\), we get
Combining (5.34)–(5.39), we have shown that for a given t, one has for almost every \(\eta \in [0,B+C]\) that
where \(h(t,\eta )\) is given by (5.38). This completes the computation of \(\ell _t(t,\eta )\).
It is left to show, cf. (5.28), that
exists for almost every \(\eta \in [0,B+C]\) and to compute its value. Recall (5.31) and (5.32), which imply
Using (5.37) and (5.38), we thus end up with
Combining (5.28), (5.40), (5.41), and (5.21) finally yields that for each \(t\in [0,T]\)
for almost every \(\eta \in [0,B+C]\) and the function \(h(t,\eta )\) is given by (5.38). This completes the computation of \(\chi _t(t,\eta )\).
To summarize, we showed with the help of the dominated convergence theorem that
Actually we showed that
which is a limiting process in \(L^\gamma ([0,B+C])\). Thus, the correct Banach space to work in is \(L^\gamma ([0, B+C])\). This might be surprising at first sight since only \(\chi _t(t,\, \cdot \,)\) belongs to \(L^\gamma ([0,B+C])\) but not \(\chi _\eta (t,\, \cdot \,)\). On the other hand, one has that the function \(g(t,\ell (t,\, \cdot \,))\) is non-decreasing and hence differentiable almost everywhere. Furthermore, (5.9) and (5.11) imply that \(g(t,\ell (t,\, \cdot \,))\) is Lipschitz continuous with Lipschitz constant at most one and for almost every \(\eta \in [0,B+C]\) it follows that
Thus,
using (5.43), which is finite, cf. (4.10) and which implies that \(h\chi _\eta (t,\, \cdot \,)\in L^\gamma ([0,B+C])\). Thus, we will not study (5.42) pointwise, but as a differential equation in \(L^\gamma ([0,B+C])\).
Theorem 5.3
The function \(\chi (t,\, \cdot \,)\) satisfies for almost all t the following differential equation in \(L^\gamma ([0,B+C])\)
where
Furthermore, the mapping \(t\mapsto \chi (t,\, \cdot \,)\) is continuous from [0, T] into \(L^\gamma ([0,B+C])\).
Remark 5.4
The above computations are based on error estimates. This idea is also used when proving the chain rule in the classical setting for functions of several variables. However, one cannot use the chain rule here. Namely, writing
one is tempted to look at \(\chi (t,\eta )\) as a composition of two functions, since \(v(t,\xi )\) is differentiable almost everywhere with respect to both time and space. However, \(v_t(t,\xi )\) and \(v_\xi (t,\xi )\) are not continuous with respect to time and space, and this fact prevents us from using the following splitting
together with a limiting process based on the existence of the partial derivatives of v. Furthermore, \(\ell (t,\eta )\) is not differentiable almost everywhere, we only know that for fixed t, the derivatives \(\ell _t(t,\eta )\) and \(\ell _\eta (t,\eta )\) exist for almost every \(\eta \).
Remark 5.5
An alternative derivation of the differential equation for \(\chi (t,\eta )\): By the weak formulation, we have cf. (2.3b), (4.5), and (5.3), that
for any test function \(\phi \in {\mathcal {C}}_c^\infty ([0,\infty )\times {\mathbb {R}})\). Using (5.5) and changing the coordinates according to (5.7) and (5.36), we end up with
First of all note that using integration by parts (for the integral with respect to \(\eta \)) in the triple integral, we obtain
Furthermore, the right-hand side of (5.46) can be rewritten as
Combining the last two equation with (5.46), we have
Now we are ready to read off the differential equation for \(\chi (t,\eta )\), since the above equality is equivalent to
where \(h(t,\eta )\) is given by (5.38). Since the above equality must hold for any test function \(\phi \), we end up with
5.2 Differentiability of \({\mathcal {U}}(t,\eta )\) with respect to time
To begin with, we have a closer look at the differential equation (5.44), which reads
where \(h(t,\eta )\) is given by (5.45). This equation can be solved (uniquely) by the method of characteristics, if the differential equation
has a unique solution and \(m_\theta (t,\, \cdot \,)\) is strictly positive for all \(t\in [0,T]\). According to the classical ODE theory, (5.47) has for each fixed \(\theta \) a unique solution, if the function \(h(t,\eta )\) is continuous with respect to time and Lipschitz with respect to space. This is the result of the next lemma, whose proof can be found in Lemma A.2. Hence (5.47) has a unique solution.
Lemma 5.6
Consider the function h defined by (5.45). Then
-
(i)
\(t\mapsto h(t,\eta )\) is continuous;
-
(ii)
\(\eta \mapsto h(t,\eta )\) is Lipschitz and satisfies
$$\begin{aligned} \vert h(t,\eta _2)-h(t,\eta _1)\vert \le \big (1+2n\left\| u(0,\, \cdot \,)\right\| _{L^\infty }+C+\frac{n}{2} Ct\big )\vert \eta _2-\eta _1\vert . \end{aligned}$$(5.48)
For the method of characteristics to be well-defined, we must check that solutions to (5.47) are strictly increasing. If \(m(0,\theta )=\theta \) for all \(\theta \in [0,B+C]\) and \(\theta _1<\theta _2\), we have, using (5.48), as long as the function \(m(t,\, \cdot \,)\) remains non-decreasing, that
where \(B(t)=1+2n\left\| u(0,\, \cdot \,)\right\| _{L^\infty }+C+\frac{n}{2}Ct\), which yields
Thus \(m(t,\, \cdot \,)\) not only remains strictly increasing, it is also Lipschitz continuous with Lipschitz constant \(\hbox {e}^{\int _0^t B(s)\mathrm{d}s}\) and hence according to Rademacher’s theorem differentiable almost everywhere. In particular, one has that
Thus \(m(t,\, \cdot \,)\) is strictly increasing.
Introducing
we have from (5.44)
and hence \({\bar{\chi }}(t,\eta )\) is a characteristic. Introducing
equation (5.51) reads
To take a next step toward deriving the differential equation for \({\mathcal {U}}(t,\eta )\), we want to show that \({\bar{{\mathcal {U}}}}(t,\theta )\) satisfies
where
The proof of (5.53) is again based on an idea that has been used in [2]. According to the definition of a weak solution, one has, see (2.3a) and (5.5), for all \(\phi \in {\mathcal {C}}_c^\infty ([0,\infty )\times {\mathbb {R}})\) that
In the above equality, one can replace \(\phi \in {\mathcal {C}}_c^\infty ([0,\infty )\times {\mathbb {R}})\) by \(\phi (t,x)\) such that \(\phi (t,\, \cdot \,)\in {\mathcal {C}}_c^\infty ({\mathbb {R}})\) for all t and \(\phi (\, \cdot \,,x)\in {\mathcal {C}}^1({\mathbb {R}})\).
5.2.1 The Lipschitz continuity of \({\bar{{\mathcal {U}}}}(t,\, \cdot \,)\)
To prove that \({\bar{{\mathcal {U}}}}(t,\theta )\) is Lipschitz with respect to time, we have to make a special choice of \(\phi (t,x)\). Let
where \(\psi \) is a standard Friedrichs mollifier. Our choice is motivated by the following observation,
and hence
Direct calculations then yield, using (5.51)
Introduce the function
and note that \(G_\mathrm{ac}(\tau ,\, \cdot \,)\) is absolutely continuous. Moreover, one has
and
which implies
For the next term, observe
which implies
For the last two terms, observe that for every \(\tau \not \in {\mathcal {N}}\), i.e., for almost every \(\tau \in [0,T]\) one has, using (5.7), that
and
Thus, the dominated convergence theorem, using (5.56) and (5.55), yields that
Furthermore, the continuity of \(m(t,\theta )\), \({\bar{\chi }}(t,\theta )\), and p(t, y) with respect to time, implies that
for all \((t,\theta )\in [0,T]\times [0, B+C]\). Thus, \({\bar{{\mathcal {U}}}}(\, \cdot \,,\eta )\) will be Lipschitz on [0, T], if we can show that the right-hand side of (5.57) can be uniformly bounded on [0, T]. Since \(p(t,\, \cdot \,) \in L^1({\mathbb {R}})\), cf. (4.10), the claim follows if \(m(t,\, \cdot \,)\) can be bounded. Therefore, recall that \(m(t,\theta )\) satisfies (5.47) with the initial condition \(m(0,\theta )=\theta \), which implies that it suffices to show that \(\left\| h(t,\, \cdot \,)\right\| _{L^\infty }\) can be bounded by a function, which is at most growing linearly. Using (5.45), (5.36), (3.6), Lemma 4.1, and (4.2), we have
and thus \(\left\| h(t,\, \cdot \,)\right\| _{L^\infty }\) grows at most linearly. This finishes the proof of the uniform Lipschitz continuity in time of \({\bar{{\mathcal {U}}}}(t,\theta )\).
As a closer look reveals the differential equation (5.57) holds pointwise. Thus, one can either look at \({\bar{{\mathcal {U}}}}(t,\, \cdot \,)\) as a function in \(L^\gamma ([0,B+C])\) or in \(L^\infty ([0,B+C])\). Furthermore, the mapping \(t\mapsto {\bar{{\mathcal {U}}}}(t,\, \cdot \,)\) is continuous from [0, T] into \(L^\gamma ([0,B+C])\).
5.2.2 The differential equation for \({\mathcal {U}}(t,\eta )\)
In view of (5.44), it remains to derive the differential equation for \({\mathcal {U}}(t,\eta )\) from (5.57). Recall that we have by (5.52) the relation
Since \(m(t,\, \cdot \,)\) is continuous and strictly increasing, cf. (5.49), there exists a unique, continuous and strictly increasing function \(n(t,\, \cdot \,)\) such that
Now, given \(\eta \in [0,B+C]\), there exists a unique \(\theta \in [0,B+C]\), such that
By definition, we have that \(n(t,\, \cdot \,)\) is continuous, strictly increasing, and hence differentiable almost everywhere. Furthermore, one has that \(n(t,\, \cdot \,)\) satisfies
by (5.49), which yields
Since \(h(t,\eta )\) can be uniformly bounded on \([0,T]\times [0, B+C]\), see (5.58), it follows that \(n(t,\eta )\) is Lipschitz with respect to both space and time on \([0,T]\times [0, B+C]\) and by Rademacher’s theorem differentiable almost everywhere. Moreover, direct calculations yield
Since \(n(t,\, \cdot \,)\) is strictly increasing for every \(t\in [0,T]\), combining (5.52) and (5.59) yields
Furthermore, using (5.36), (5.20), (3.3), and (5.52), one has
In Sect. 3.2, we showed that for every \(t\in [0,T]\), the function \(U(t,\, \cdot \,)\) is Lipschitz. Since \(\ell (t,\, \cdot \,)\) and \(m(t,\, \cdot \,)\) are strictly increasing, it follows that both \({\mathcal {U}}(t,\, \cdot \,)\) and \({\bar{{\mathcal {U}}}}(t,\, \cdot \,)\) are differentiable almost everywhere on \([0,B+C]\). Thus, for any \(t\in [0,T]\) one ends up with
for almost every \(\eta \in [0,B+C]\). This is the sought differential equation for \({\mathcal {U}}(t,\eta )\).
The correct Banach space to work in is \(L^\gamma ([0,B+C])\cap L^\infty ([0,B+C])\). To see this, introduce the function
Observe that (5.5) and (5.12) imply that \(g_2(t,\, \cdot \,)\) is Lipschitz continuous with Lipschitz constant at most \(1+C\), since
Thus, it follows that for any fixed \(t\in [0,T]\)
In particular, one has
and
which is finite, cf. (4.9) and (5.6), and which implies that \(h{\mathcal {U}}_\eta (t,\, \cdot \,)\in L^\gamma ([0,B+C])\cap L^\infty ([0,B+C])\).
To summarize, we showed the following theorem.
Theorem 5.7
The function \({\mathcal {U}}(t,\, \cdot \,)\) satisfies the following differential equation in \(L^\gamma ([0,B+C])\cap L^\infty ([0,B+C])\)
where
Furthermore, the mapping \(t\mapsto {\mathcal {U}}(t,\, \cdot \,)\) is continuous from [0, T] into \(L^\gamma ([0,B+C])\).
5.3 Differentiability of \({\mathcal {P}}(t,\eta )\) with respect to time
To close the system of differential equations (5.44) and (5.60), i.e.,
where
it remains to derive the differential equation satisfied by \({\mathcal {P}}(t,\eta )\), given by (5.36).
5.3.1 The Lipschitz continuity of \({\mathcal {P}}(t,\eta )\)
To begin with, we show that \({\mathcal {P}}(t,\eta )\) is Lipschitz continuous on \([0,T]\times [0,B+C]\) and hence differentiable almost everywhere on \([0,T]\times [0, B+C]\). Direct calculations yield
where we used that \(p(t,\, \cdot \,)\in {\mathcal {C}}_0^\infty ({\mathbb {R}})\) and \(p(\, \cdot \,, x)\) is differentiable almost every on the finite interval [0, T]. Furthermore, we took advantage of \(\chi (t,\, \cdot \,)\) being continuous and increasing and hence differentiable almost everywhere on \([0,B+C]\).
Combining (5.61) with (5.27) and (5.43) as well as (4.8) and (4.11), we end up with
i.e., \({\mathcal {P}}(t,\eta )\) is Lipschitz continuous on \([0,T]\times [0,B+C]\).
We are now ready to derive the differential equation satisfied by \({\mathcal {P}}(t,\eta )\). Therefore, note that (5.42) implies that for each \(t\in [0,T]\) one has
for almost every \(\eta \in [0,B+C]\), since \(p(t,\, \cdot \,)\in {\mathcal {C}}_0^\infty ({\mathbb {R}})\). Furthermore, one has for almost every \((t,\eta )\in [0,T]\times [0, B+C]\) that
if the two limits on the right-hand side exist. The first one exists and is given by (4.7). The second one, on the other hand, requires a closer look. Write
Following once more the argument leading to (4.4), recalling (3.6), (5.27), Lemma 4.1, and that \(p_x(t,\, \cdot \,)\in {\mathcal {C}}_0^\infty ({\mathbb {R}})\), we have
and
if the limit on the right-hand side exists. In view of (5.42), one has that for each \(t\in [0,T]\)
for almost every \(\eta \in [0,B+C]\). We find, using (5.44), (cf. (2.9b)), (4.5), (5.8), (5.9), (5.11), (4.14), that
The correct Banach space to work in is again \(L^\gamma ([0, B+C])\cap L^\infty ([0,B+C])\), since
To summarize, we showed the following theorem.
Theorem 5.8
The function \({\mathcal {P}}(t,\, \cdot \,)\), given by (5.36), satisfies for almost all t the following differential equation in \(L^\gamma ([0,B+C])\cap L^\infty ([0,B+C])\)
where
and
Furthermore, the mapping \(t\mapsto {\mathcal {P}}(t,\, \cdot \,)\) is continuous from [0, T] into \(L^\gamma ([0,B+C])\).
5.4 Summary
We have shown the following result.
Theorem 5.9
The functions \(\chi (t,\eta )\), \({\mathcal {U}}(t,\eta )\), and \({\mathcal {P}}(t,\eta )\) defined by (5.7) and (5.36), respectively, satisfy the following system of equations:
where
which can be uniquely solved using the method of characteristics in \(L^\gamma ([0,B+C])\times (L^\gamma ([0,B+C])\cap L^\infty ([0, B+C]))^2\).
We remark that Definition 2.3, which lists all properties that have to be satisfied by weak conservative solutions, requires
In our new coordinates, these conditions can be formulated in terms of \({\mathcal {U}}\chi _\eta (t,\eta )\) and \(\chi _\eta (t,\eta )\), whose time evolution cannot be described with the help of (5.66). On the other hand, the imposed moment condition (5.2), which is preserved with respect to time, implies (5.69). Indeed, let
which both exist and are finite. Thus, \(u(t,\, \cdot \,)\in E_2\), if and only if
by the definition of \(E_2\). Here we only consider one integral, since all of them can be investigated using similar ideas. One has
which is finite if \(\gamma >2\) and (5.2) is satisfied.
For the second condition, recall that
Thus, \(F(t,\, \cdot \,)\in E_1^0\) if and only if
by the definition of \(E_0^1\). Again we only consider one integral, since all of them can be considered using similar ideas. One has
which is finite if \(\gamma >2\) and (5.2) is satisfied.
We have proved the following theorem.
Theorem 5.10
Let \(\gamma >2\), then for any initial data \((u_0, \mu _0)\in {\mathcal {D}}\) such that
the Hunter–Saxton equation has a unique global conservative weak solution \((u,\mu )\in {\mathcal {D}}\) in the sense of Definition 2.3, which satisfies
Notes
Condition (2.15) in [6], here stated in terms of the measure \(\mu \).
The push-forward of a measure \(\nu \) by a measurable function f is the measure \(f_\#\nu \) defined by \(f_\#\nu (B)=\nu (f{^{-1}}(B))\) for all Borel sets B.
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Appendix A: Proof of Lemmas 5.2 and 5.6
Appendix A: Proof of Lemmas 5.2 and 5.6
Lemma A.1
(Lemma 5.2) (i) Let \(g(t,\xi )\) be given by (4.13). Then, there exists a positive constant \({\bar{M}}\) such that
(ii) Let \(H(t,\xi )\) be defined by (5.9). Then,
Proof
(i): We want to estimate
Recalling (4.13), we split the above difference into two terms as follows
\({\mathrm{I}}_1\): Since p(t, x) is continuously differentiable on \([0,T]\times {\mathbb {R}}\), we have by the mean value theorem that
for some m between \(y(s,\xi )\) and \(y(t,\xi +u(t,y(t,\xi ))(t-s))\). Furthermore, we find
for some constant M (that is increased during the calculation), using (4.8), (4.11), (5.29), and (3.6). In addition, we estimate
Finally, using (5.29) once more, there exists a positive constant \({\hat{M}}\) such that
\({\mathrm{I}}_2\): Using (3.1), (3.2), and (4.5), we can write
Next we will show that each of the terms \({\mathrm{II}}_1\), \({\mathrm{II}}_2\), and \({\mathrm{II}}_3\) is of order \(\vert t-s\vert ^{3/2}\). Therefore, it is important to keep in mind that \(0\le y_\xi \), \({\tilde{H}}_\xi \le 1\).
\({\mathrm{II}}_1\): Since u(t, x) is Hölder continuous with Hölder exponent \(\frac{1}{2}\) on \([0,T]\times {\mathbb {R}}\), we have, by (3.8) and (3.9), for all \(\tau \) between s and t that
and
\({\mathrm{II}}_2\): Since \(K(\, \cdot \,)\), given by (4.3), is smooth one has for all \(\tau \) between s and t that
and
\({\mathrm{II}}_3\): Here integration by parts will be the key. Indeed, one has
Recalling (3.24) and that \(0\le {\tilde{H}}_\xi \le 1\), we have for all \(\tau \) between s and t that
and
Thus, we have
Combining now all these estimates, we have that there exists a positive constant \(\check{M}\) such that
(ii): Combine (5.9), (5.30), and (A.1). \(\square \)
Lemma A.2
(Lemma 5.6) Consider the function h defined by (5.45). Then
-
(i)
\(t\mapsto h(t,\eta )\) is continuous;
-
(ii)
\(\eta \mapsto h(t,\eta )\) is Lipschitz and satisfies
$$\begin{aligned} \vert h(t,\eta _2)-h(t,\eta _1)\vert \le (1+2n\left\| u(0,\, \cdot \,)\right\| _{L^\infty }+C+\frac{n}{2}Ct)\vert \eta _2-\eta _1\vert . \end{aligned}$$(A.2)
Proof
(i) First, we establish the continuity with respect to time. Recalling (3.6), (3.9), (4.4), (4.9), and (5.27), we have
For the second term of \(h(t,\eta )\), note that one can write
Using (3.9), (5.27), and Lemma 4.1, one has
Last but not least, recalling (3.9), Lemma 4.1, (4.4), (4.10), and (5.27), we have
Thus, we have that \(h(t,\eta )\) is Hölder continuous with exponent \(\frac{1}{2}\) with respect to time.
(ii) To establish the Lipschitz continuity with respect to space is a bit more involved, but follows pretty much the same lines. As a closer look at (5.12) reveals, one has
This means especially given \(\eta \in [0,B+C]\), there exist \(\eta ^-\le \eta \le \eta ^+\) such that
and
In view of Definition 2.3 (v), (5.3), (4.11), and (5.5), we then have for \(\eta _1<\eta _2\) such that \(\chi (t,\eta _1)\not = \chi (t,\eta _2)\) that
As far as the second part is concerned, observe that (cf. (5.63))
and we have
Thus, we have that \(h(t,\eta )\) is Lipschitz continuous with respect to space with
\(\square \)
Lemma A.3
Given \(\gamma >2\) and a weak conservative solution \((u,\mu )\) in the sense of Definition 2.3, which satisfies
Then for any \(n\in {\mathbb {N}}\) such that \(n\ge \gamma \)
Proof
Due to (4.10), it suffices to show
Since \(p(t,\, \cdot \,)\) is nonnegative and both integrals can be estimated using the same ideas, we only present the details for the first one. Direct computations yield
In the above calculations, we used that \((a+b)^2\le 2(a^2+b^2)\) and that \((a+b)^2\le 2\max (a^2, b^2)\). \(\square \)
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Grunert, K., Holden, H. Uniqueness of conservative solutions for the Hunter–Saxton equation. Res Math Sci 9, 19 (2022). https://doi.org/10.1007/s40687-022-00314-6
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DOI: https://doi.org/10.1007/s40687-022-00314-6