1. Introduction
We investigate the, so-called, dissipative Aw–Rascle system

on
$\mathbb{T}^3 \times (0,T)$, where
$\mathbb{T}^3 $ is a three-dimensional torus. The unknown of the system are the density
$\varrho(t,x)$ and the desired velocity of motion
$\textbf{w}(t,x)$. The actual velocity of motion u is given by the relation:

where
$\nabla p(\varrho)$ is the velocity offset, with a given offset function
$p(\cdot) \in C^5(\mathbb{R}_+)$.
System (1.1) is supplemented with the initial data

The purpose of the article is to prove local-in-time existence of regular solutions to system (1.1) under the following assumptions on the data

We may also assume less regularity of ϱ 0 at the price of additional assumption on well-prepared data, more precisely

Our goal is to prove local in time existence of regular solutions to (1.1) Note that, using (1.2), we can rewrite (1.1) as

which is the equivalent formulation as long as the solution remains sufficiently regular. Moreover, assuming ϱ > 0 we can further transform this system to obtain

subject to the initial data

System (1.1) with closure relation (1.2) was recently considered by Acaves et al. [Reference Aceves-Sanchez, Bailo, Degond and Mercier1] in the context of pedestrian flow. Their offset function was actually singular with respect to (w.r.t.) density

This offset function acts as a barrier to ensure that the density remains below its maximum ϱ max, which models the formation of congestion within the crowd. For an up-to-date overview of the literature on the macroscopic models of crowds, we refer to the recent overview articles [Reference Bellomo and Brezzi5–Reference Bellomo, Liao, Quaini, Russo and Siettos7].
The dissipative Aw–Rascle system is a model inspired by the one-dimensional Aw–Rascle road traffic model. For derivation of this model and its qualitative analysis, we refer to [Reference Aw, Klar, Rascle and Materne3, Reference Aw and Rascle4]. The offset function (1.9) was actually originally proposed for that model in the work of Berthelin et al. [Reference Berthelin, Degond, Delitata and Rascle8], as a remedy to the lack of uniform bound for the density.
The classical Aw–Rascle model for traffic differs from the dissipative Aw–Rascle system (1.1), not only in its spatial dimension but also because it uses a scalar offset, i.e.,
$ u=w-p(\varrho)$. Incorporating the offset in the form of gradient (1.2) resolves the dimension discrepancy in the closure relation between the velocities u and w. However, the whole system changes its character from hyperbolic to mixed hyperbolic-parabolic type due to additional dissipation effect in the continuity equation (1.7a). While for description of the multi-lane traffic, first order systems seem to be a more suitable [Reference Agrawal, Kanagaraj and Treiber2, Reference Herty, Fazekas and Visconti20, Reference Tumash, Canudas-de-Wit and Monache33], and it was demonstrated in [Reference Aceves-Sanchez, Bailo, Degond and Mercier1] that system (1.1) and (1.2) correctly capture the fundamental diagram for the pedestrian flow.
The mathematical properties of the dissipative Aw–Rascle system have been explored for the first time in [Reference Chaudhuri, Gwiazda and Zatorska10]. The authors demonstrated the existence and weak-strong uniqueness of Young-measure solutions to the system (1.1) and (1.2) with
$p(\varrho)=\varrho^\gamma$, γ > 0. Their result states that the measure-valued solution coincides with the strong solution emanating from the same initial data, as long as the latter exists. However, the existence of regular solutions was assumed rather than proven, which motivates the current article. Our aim is to address this gap. Initially, we will focus on a generalization of the offset function
$p(\varrho)=\varrho^\gamma$ considered in [Reference Chaudhuri, Gwiazda and Zatorska10], followed by an analysis of the well-posedness for two other forms: the singular offset function (1.9) and a non-local offset function defined as
$p(\varrho) = K(x) * \varrho$. These variations are inspired not only by the aforementioned pedestrian flow model [Reference Aceves-Sanchez, Bailo, Degond and Mercier1] but also by models that address lubrication effects [Reference Lefebvre-Lepot and Maury25] and collective behaviors [Reference Kim22, Reference Peszek and Poyato31], as discussed in [Reference Chaudhuri, Mehmood, Perrin and Zatorska11–Reference Chaudhuri, Peszek, Szlenk and Zatorska13, Reference Mehmood26] and related literature.
Lastly, it is important to mention that the well-posedness of the system (1.1) and (1.2) has been previously examined in the framework of weak solutions. Using the method of convex integration, it was shown in [Reference Chaudhuri, Feireisl and Zatorska9] that any initial data
$(\varrho_0,\textbf{u}_0)\in C^2(\mathbb{T}^3)\times C^3(\mathbb{T}^3)$ can connect to any terminal data
$(\varrho_T,\textbf{u}_T)\in C^2(\mathbb{T}^3)\times C^3(\mathbb{T}^3)$ consistent with mass and momentum conservation, via a weak solution belonging the class

The corresponding ill-posedness result clearly shows that the existence of so-called wild solutions extends beyond the hyperbolic systems of conservation laws and, in particular, to those experiencing dissipation that degenerates in vacuum.
In this article, we extend the energy estimates approach developed for the compressible Navier–Stokes equations (see [Reference Valli and Zajaczkowski34], [Reference Zajaczkowski35], [Reference Danchin and Mucha14], [Reference Danchin and Mucha15], [Reference Kreml, Nečasová and Piasecki23], among others) to systems of mixed hyperbolic-parabolic type, which exhibit dissipation in the continuity equation but lack it in the momentum equation. We prove the local existence of regular solutions to system (1.1) by applying the method of successive approximations. We restrict ourselves to direct energy approach in L 2 framework. Alternative Lp approach, which has been developed for the compressible Navier–Stokes system in [Reference Mucha and Zajaczkowski28]–[Reference Mucha and Zajaczkowski29] and, with entirely different techniques based on
${\mathcal R}$-bounded solution operators in [Reference Enomoto and Shibata17], would be another possibility in context of regular solutions to (1.1), but we leave this direction for future investigation.
The main difficulty here is to derive Lp estimates for a linear transport equation. The approach is based on an explicit solution formula obtained by the method of characteristics. Partial results of this type have been used in the theory of compressible Navier–Stokes equations (see among others [Reference Mucha and Zajaczkowski28], [Reference Valli and Zajaczkowski34], [Reference Zajaczkowski35], [Reference Kreml, Nečasová and Piasecki23]), but a consistent Lp theory for transport equations is still missing. Here we address this issue proving quite a general result (lemma 2.2), which may be of independent interest. The dissipativity in (1.6b) gives parabolic estimates, but a delicate part is to ensure positivity of the solution at each step of the iteration. This issue is addressed in lemma 2.3.
1.1. Notation
Before stating our main result, we shall introduce the notation used in the article.
• Throughout the article, by
$E(\cdot)$ we denote a positive, continuous function such that
$E(0)=0$ and
$\phi(\cdot)$ denotes a continuous, positive function.
• We use standard notation
$L_p(\mathbb{T}^3)$ and
$W^1_p(\mathbb{T}^3)$ for Lebesgue and Sobolev spaces on the torus, respectively, and
$H^k(\mathbb{T}^3):=W^k_2(\mathbb{T}^3)$. Next,
$L_p(0,T;X)$, where X is a Banach space, denotes a Bochner space.
• For T > 0 and
$k \in \mathbb N$ let us also denote
(1.10)\begin{equation} \begin{aligned} &{\mathcal X}_k(T):=L_2(0,T;H^k(\mathbb{T}^3)) \cap L_\infty(0,T;H^{k-1}(\mathbb{T}^3)),\\ & {\mathcal Y}_k(T):=\{f\in L_\infty(0,T;H^k(\mathbb{T}^3)): \; f_t \in L_\infty(0,T;H^{k-1}(\mathbb{T}^3)),\\ & {\mathcal V}_k(T):=\{g \in L_2(0,T;H^{k+1}(\mathbb{T}^3)) \cap L_\infty(0,T;H^k(\mathbb{T}^3)):\\ & \quad \quad \quad \quad \quad \;g_t \in L_2(0,T;H^{k-1}(\mathbb{T}^3)) \} \end{aligned} \end{equation}
with norms defined in a natural way as appropriate sums of norms.
Since all spaces are considered on the torus, we shall sometimes skip indication of the domain in the definition of space and write Lp instead of
$L_p(\mathbb{T}^3)$, etc. We are now in a position to state our main result.
Theorem 1.1. Assume the initial data satisfies
$\varrho_0 \gt 0$, and either (1.4) or (1.5). Assume, moreover, that the pressure is an increasing function of the density of class C 5. Then there exists T > 0 such that system (1.7) admits a unique solution
$(\varrho,{\textbf{w}}) \in {\mathcal V}_3(T)\times {\mathcal Y}_3(T)$ with the estimate

in case of (1.4) or

in case of (1.5).
The strategy of the proof involves two main steps:
• construction of solutions to a suitable approximation of system (1.7),
• proof of convergence.
We aim to approximate solutions (1.7) by solutions to the iterative scheme defined as

At each step of the iteration, having
$(\varrho^n,\textbf{w}^n)$ we set
$\textbf{u}^n=\textbf{w}^n-\nabla p(\varrho^n)$ and solve the second equation of (1.11) for
$\textbf{w}^{n+1}$. Next we use
$\textbf{w}^{n+1}$ to determine
$\varrho^{n+1}$ from the first equation. Therefore, each step of iteration is decoupled to solving separate linear problems

with given
$(\bar{\textbf{w}},\bar{\varrho})$ and

with given
$\bar{\textbf{u}}$. Convergence of this iterative scheme is then proved using the Banach fixed point theorem.
The article is organized as follows. In §2, we first solve the linear problems corresponding to the iterative scheme described above in (1.12) and (1.13). Next, in §3, we prove the convergence of the iterative scheme using the contraction argument. Finally, in §4, we discuss the existence results for general singular and non-local offset functions; we formulate and prove our other main results—theorems 4.1 and 4.3.
2. Linear theory
In this section, we solve linear problems corresponding to (1.12) and (1.13).
2.1. Linear transport equation
Consider the linear transport equation

with given vector field v and unknown scalar valued η. Our goal is to prove the existence of a solution to (2.1) in the regularity framework corresponding to theorem 1.1. We will use the explicit form of the solution in Lagrangian coordinates given by

The first step is, therefore, to investigate the regularity properties of solutions to (2.2). For this purpose, we shall repeatedly use a basic fact that if a matrix is close to identity in the
$L_\infty$ in space-time norm, then the same holds for its inverse. In particular, using the notation E(T), we have

for any function
$A:(0,T)\times \mathbb{T}^3 \to \mathbb{R}^{3\times 3}$. The following result improves [Reference Kreml, Nečasová and Piasecki23, Lemma 3.2]:
Lemma 2.1. Assume
$\textbf{v} \in L_2(0,T;H^3(\mathbb{T}^3))$. Then there exists a continuous, positive function
$\phi(\cdot)$ denotes such that the solution to (2.2) satisfies









Proof. The first assertion was proved in [Reference Kreml, Nečasová and Piasecki23, Lemma 3.2]. The second is derived and used in the proof of the aforementioned result. Then (2.6) results from (2.3), while (2.7) follows from the fact that the entries of the inverse an invertible matrix A are smooth functions of the entries of A

In order to prove the bounds for higher derivatives observe that differentiating the solution formula

with respect to y we obtain

which is equivalent to

Differentiating this identity in y, we obtain

Multiplying the component corresponding to
$\partial^2_{y_i y_j} X$ by
$|\partial^2_{y_i y_j} X|^4 \partial^2_{y_i y_j} X$, summing over
$i,j$ and integrating over
$\mathbb{T}^3$ we get

By (2.4), for small T and any function f of the time variable with values in
$L_p(\mathbb{T}^3)$ for
$1 \leq p \lt \infty$, we have

and similarly

By (2.15), (2.16), and Sobolev imbedding, applying (2.4) to the first term of the RHS of (2.14) we get

The assumed integrability of v allows to conclude (2.9) by Gronwall inequality:

This proves (2.9), which immediately implies (2.10). A remark is due here. In derivation of (2.9), we assumed for simplicity that

which does not hold since we don’t have Poincaré inequality. To make the proof fully precise, we would have to replace
$\|\nabla_y^2 X\|_{L_6(\mathbb{T}^3)}$ by
$\|\nabla_y X\|_{W^1_6(\mathbb{T}^3)}$ which is easy—it is enough to write estimate for
$\frac{\partial}{\partial t}\|\nabla_y X\|_{L_6(\mathbb{T}^3)}^6$. Therefore to avoid additional obvious terms, we assume (2.17). Similar simplification is also used later in the proof.
In order to prove (2.11), we differentiate (2.13) in y obtaining

Multiplying the equation corresponding to
$\partial^3_{y_i y_j y_k} X$ by
$\partial^3_{y_i y_j y_k} X$ and summing over all
$i,j,k$ we get

from which, by Sobolev imbedding, (2.4), (2.15), and (2.16), we obtain

and by Gronwall inequality we conclude (2.11), which implies (2.12).
Now we are in a position to prove a series of estimates for the transport equation (2.1). As they may be of independent interest, we prove them in a possibly general form.
Lemma 2.2. Assume
$\textbf{v} \in {\mathcal X}_3(T)$ defined in (1.10) and
$\eta_0 \in H^3(\mathbb{T}^3)$. Then the solution to (2.1) satisfies










Proof. We have

Differentiating this identity in y, we obtain

which, by lemma 2.1, implies

from which we obtain (2.18). Similarly, using (2.8), we obtain (2.19). In order to estimate
$\nabla_x^2 \eta$, we differentiate (2.28) in y to obtain

for
$j,k \in \{1,2,3\}$. Rewriting the above system as

for
$k,j \in \{1,2,3\}$, which is a linear system of nine equations for the unknown derivatives
$\frac{\partial^2 \eta}{\partial x_i\partial x_l}(t,X)$. In order to solve it, we observe that the diagonal of this system corresponds to
$(i,l)=(j,k)$, which means that on the diagonal we have terms
$\frac{\partial X_k}{\partial y_k}\frac{\partial X_j}{\partial y_j}$, while all entries outside the diagonal contains the terms which are not on the diagonal of
$\nabla_y X$. Therefore, by (2.4), all terms on the diagonal of system (2.30) are close to 1 for short times, while all other terms are small. Therefore, system (2.30) is uniquely solvable and we obtain


Next, by (2.9)

and finally

Combining (2.31), (2.32), (2.33), and (2.34), we obtain (2.20). Next, by (2.10) and (2.29), we have

Combining this estimate with (2.31), (2.33), and (2.34), we arrive at (2.21). Next, similarly to (2.32), we obtain

and, in analogy to (2.33), we have

Combining (2.35), (2.36), and (2.34) with p = 2, we obtain (2.22). Next, by (2.10) and (2.29), we have

which combined with (2.36) and (2.34) for p = 2 gives (2.23).
In order to estimate the third order derivatives, we differentiate (2.30) w.r.t. ym, which yields

where
$X=X(t,y)$ or
$X=X(s,y)$ according to (2.30). Similarly as in case of (2.30), it is a system of 27 linear equations for the third order derivatives of η. On the diagonal, we have terms corresponding to
$(i,l,n)=(j,k,m)$, which, again by (2.4), are close to one, while all other entries are small for small times. Therefore, (2.37) is uniquely solvable and we obtain

Let us estimate the RHS of (2.38). For the second term, by (2.9) and (2.20), we have

and for the third, by (2.11) and (2.18)

It remains to estimate the terms with g. By (2.11), we have

Next, by (2.9),

and finally

Combining (2.38)–(2.42) and applying Sobolev imbedding to estimate all terms containing g by a single norm, we obtain

which together with estimates on lower order derivatives of η completes the proof of (2.24).
In order to prove of (2.25) observe that, for any finite p, by (2.9) and (2.21) we have

Similarly by (2.11) and (2.19), we obtain

For the terms with g on the RHS of (2.38), we use the estimates (2.40)–(2.42). Combining them with (2.43)–(2.44), we obtain

which completes the proof of (2.25). Now we can use (2.1) to prove the estimates for ηt. First we immediately get

Next we differentiate (2.1) in the space variable to obtain

By (2.18), we have

by (2.20)

by (2.19)

and finally by (2.21)

so altogether we obtain

Finally we differentiate (2.45) once more in space:

For the first term we have, by (2.18),

and, by (2.19),

For the second term, by (2.20),

and by (2.21)

Finally, to estimate the last term, we apply (2.24) to get

and (2.25) to obtain

Combining (2.46), (2.47), (2.50), (2.52), and (2.54), we obtain (2.26). Finally, (2.48), (2.49), (2.51), (2.53), and (2.55) allow to conclude (2.27), which completes the proof.
2.2. Linear continuity equation with dissipation
In this section, we investigate the linear problem

Concerning the regularity of the data, we keep in mind that the above system corresponds to the first equation of (1.7). Therefore, taking into account lemma 2.2, it is sufficient to assume
$\textbf{v} \in L_\infty(0,T;H^3(\mathbb{T}^3))$. The parabolic maximal regularity then leads to the following result.
Lemma 2.3. Assume
$\varrho_0 \in H^2(\mathbb{T}^3)$,
$\textbf{v} \in L_\infty(0,T;H^2(\mathbb{T}^3))$,
$\mathfrak{a} \in L_\infty(0,T;W^1_\infty(\mathbb{T}^3)) \cap L_2(0,T;H^2(\mathbb{T}^3))$ with
$\mathfrak{a} \geq c \gt 0$, and
$\mathfrak{b} \in L_2(0,T;H^1(\mathbb{T}^3))$. Then (2.56) admits a unique solution satisfying

If
$\varrho_0 \in H^3(\mathbb{T}^3)$,
$\mathfrak{b} \in L_2(0,T;H^2(\mathbb{T}^3))$
$\textbf{v} \in L_\infty(0,T;H^3(\mathbb{T}^3))$ and
$\mathfrak{a} \in L_\infty(W^1_\infty(\mathbb{T}^3)) \cap L_2(0,T;H^3(\mathbb{T}^3))$ with
$\mathfrak{a} \geq c \gt 0$, then

Moreover, if we assume

and the initial data is strictly positive, i.e.,
$\inf_{x\in \mathbb{T}^3} \varrho_0 \gt 0$ then we have

Remark 1.
Clearly, the constant C in (2.57) and (2.58) depends on c and it goes to infinity when c → 0.
Proof. Rewriting (2.56) as

we immediately obtain the bound

The above estimate (2.62) is a direct consequence of parabolic regularity theorem in
$L^2-$ setup (see Ladyženskaya, Solonikov, and Ural’ceva [Reference Ladyženskaja, Solonnikov and Ural’ceva24, Chapter 3], even for more general boundary conditions). Differentiating (2.61) in xi, we obtain

therefore

Under the assumed regularity of v and
$\mathfrak{a}$, using (2.62) we can find appropriate bound on
$\|F_1\|_{L_2(0,T;L_2(\mathbb{T}^3))}$. Namely,

We have

which gives

which together with (2.63) implies (2.57).
Next, let α be any multi-index with
$|\alpha|=2$. Applying D α to (2.61), we obtain

where

In order to prove (2.58), we have to estimate the
$L_2(0,T;L_2(\mathbb{T}^3))$ norm of
$F_2^\alpha$. We have

Combining these estimates with Sobolev imbedding, we obtain

The terms with
$\mathfrak{a}$ can be treated as follows

which together with Sobolev imbedding yields

Combining (2.65) and (2.66) with the maximal regularity estimate for (2.64), we obtain

Combining this estimate with (2.62) and (2.63), we obtain (2.58).
It remains to prove (2.60) under additional assumption (2.59). Consider a function
$\psi : \mathbb{R} \rightarrow \mathbb{R}$ as

Clearly,
$\psi \in C^{1}(\mathbb{R})$ with

Let
$t \in [0,T]$, define
$K= \underline{\varrho_0}:= \min_{x \in \mathbb{T}^3} \varrho_0 \gt 0 $,
$M:=\|\operatorname{div} \left( \textbf{v}-\mathbf{b} \right)(t) \|_{L_\infty(\mathbb{T}^3)}$. Now, we consider a function
$h_z:[0,T)\rightarrow \mathbb{R}$ as

where
$\displaystyle \widetilde{K}= {K}\exp\left( -Mt \right) $. Since,
$\varrho \in {\mathcal V}_3(T) $, a straightforward computation yields

Using Eq. (2.56), assumption (2.59), and integration by parts, we obtain

From the assumption on
$\mathfrak{a}$, we get

Moreover, the choice of ψ and M gives

Now the identity
$ \lambda \psi^{\prime \prime}(\lambda)= \psi^\prime(\lambda) $ for
$\lambda\in \mathbb{R}$ implies

Here, we apply Grönwall’s inequality along with
$\inf_{x\in \mathbb{T}^3} \varrho_0 =K$ to deduce

Therefore, we have
$ \varrho(t) \geq \widetilde{K}= \exp{\left( -Mt \right)} \inf_{x\in \mathbb{T}^3} \varrho_0 \gt 0$ in
$(0,T)\times \mathbb{T}^3 $.
Next, we state another lemma, related to the maximum and minimal principles of (2.56) with b = 0.
Lemma 2.4. Assume
$\varrho_0 \in H^2(\mathbb{T}^3)$,
$\textbf{v} \in L_\infty(0,T;H^2(\mathbb{T}^3))$, and
$\mathfrak{a} \in L_\infty(0,T;W^1_\infty) \cap L_2(0,T;H^2(\mathbb{T}^3))$ with
$\mathfrak{a} \geq c \gt 0$. Then the unique solution of (2.56) with
$\mathfrak{b}=0$ admits satisfying

for
$0\leq t \leq T$.
Proof. Sketch of proof
The proof is similar to the proof non-negativity property in lemma 2.3 and extensively used in literatures like Novotný and Straskraba [Reference Novotný and Straškraba30, Proposition 7.39], Feireisl and Novotny [Reference Feireisl and Novotný19, Lemma 3.1], where they have consider a special case with a is constant. For the sake of completeness, we just highlight the key steps:
• Define :
$R=(\sup_{\mathbb{T}^3}\varrho_0) \exp\left(\int_0^t \Vert \operatorname{div} \mathbf{v}(s) \Vert_{L_\infty(\mathbb{T}^3) } \; ds\right). $
• Then R satisfies
$R^{\prime}(t)- \Vert \operatorname{div} \mathbf{v}(t) \Vert_{L_\infty(\mathbb{T}^3)} R(t) =0$ with
$R(0)= \sup_{\mathbb{T}^3}\varrho_0$.
• Now consider
$W(t,x)= \varrho(t,x)- R(t)$ and it satisfies
(2.69)\begin{align} \partial_t W + \operatorname{div}(W\textbf{v} ) -\operatorname{div}(\mathfrak{a} \nabla \varrho) \leq 0 \text{a.e. in }(0,T) \times \mathbb{R}^d , \end{align}
with
$W(0,x)= \varrho_0- \sup_{\mathbb{T}^3}\varrho_0\leq 0 $.
• Now we test Eq. (2.69) with
$\Psi^{\prime}(W)$ and integrating over space to obtain
\begin{align*} \frac{d}{dt} \int_{\mathbb{T}^3} \Psi(W) + 2 \int_{\mathbb{T}^3} \mathfrak{a} \Psi^{\prime \prime }(W) |\nabla W|^2 \leq \Vert \operatorname{div} \mathbf{v}\Vert_{L_\infty(\mathbb{T}^3) } \Psi(W) \end{align*}
where
\begin{equation*}\mathit{\Psi(\lambda)}= \begin{cases} \frac{1}{2}\lambda^2, & \lambda\geq 0\\ 0, &\lambda \lt 0.\\ \end{cases}\end{equation*}
• Since,
$\Psi(0)\leq 0$, from Grönwall’s inequality, we conclude
\begin{equation*} \varrho(t,x) \leq \sup_{\mathbb{T}^3}\varrho_0 \exp\left(\int_0^t \Vert \operatorname{div} \mathbf{v}(s) \Vert_{L_\infty(\mathbb{T}^3) } \; ds\right).\end{equation*}
For the other side of the inequality (2.68), we need to consider

and proceed analogously by considering

We have collected all the necessary tools to use in order to prove the convergence of iterative scheme (1.11).
3. Convergence of the iterative scheme
3.1. Boundedness of the sequence of approximations
The estimates from the previous section allow us to show
Lemma 3.1. Let
$({\textbf{w}}^n,\varrho^n)$ be the sequence defined in (1.11) with
${\textbf{u}}^1(t,x) = \textbf{u}_0(x)$ for
$(t,x) \in (0,T)\times \mathbb{T}^3$ and initial data satisfying (1.4) or (1.5). There exists
$M=M(\|\varrho_0\|_{H^4(\mathbb{T}^3)},\|\textbf{u}_0\|_{H^3(\mathbb{T}^3)})$ in case of (1.4) or
$M=M(\|\varrho_0\|_{H^3(\mathbb{T}^3)},\|\textbf{u}_0+\nabla p(\varrho_0)\|_{H^3(\mathbb{T}^3)})$ in case of (1.5) and
$T=T(M) \gt 0$ such that

where the spaces
${\mathcal Y}_k(T)$ and
${\mathcal V}_k(T)$ are defined in (1.10).
Proof. Recall that
$\phi(\cdot)$ denotes an increasing, positive function, precise form of which may vary from line to line. For the purpose of this proof, we also introduce more precise notation
$\phi_1,\phi_2,\phi_3$ to denote given, increasing, positive functions. The first equation of system (1.11) is exactly (2.56) with b = 0,
$\varrho=\varrho^{n+1},\textbf{v}=\textbf{w}^{n+1}$, and
$\mathfrak{a}=\varrho^n p'(\varrho^n)$, while the subequation of the second line of (1.11) corresponding to the ith component of
$\textbf{w}^{n+1}$ is nothing but (2.1) with g = 0,
$\eta=\textbf{w}^{n+1}_i$, and
$\textbf{v}=\textbf{u}^n$.
By lemma 2.2, recalling that
$\textbf{u}^n=\textbf{w}^n+\nabla p(\varrho^n)$ we have

In order to use (2.58) to estimate
$\|\varrho^{n+1}\|_{{\mathcal V}_3(T)}$, we need to have a closer look at
$\mathfrak{a}(\varrho)=\varrho p'(\varrho)$

where Q is some polynomial, a precise form of which is not relevant. We have
$\varrho \in L_\infty( (0,T)\times \mathbb{T}^3)$. Therefore, as
$p \in C^5$,

and

These bounds with an obvious estimate on
$\|\nabla \mathfrak{a}(\varrho)\|_{L_2(0,T;L_2(\mathbb{T}^3))}$ imply

Obviously, we also have

Applying (2.58) to the first equation of (1.11), we obtain

which together with (3.3), (3.4), and (3.2) gives

Let us take

where C(T) is the constant from (3.5). Then, assuming that

for sufficiently small T we can assure that

which together with (3.2) and (3.5) implies

thus we have (3.1).
3.2. Contraction argument. Proof of theorem 1.1
Lemma 3.2. Let us denote

Then, under the assumptions of lemma 3.1, we have

where notation E(t) is described in §1.1.
Proof. Subtracting (1.11) for
$(\textbf{w}^{n+1},\varrho^{n+1})$ and
$(\textbf{w}^{n},\varrho^{n})$, we obtain

where

Each equation of the second line of (3.7) corresponds to (2.1) with
$g \sim \delta \textbf{u}^n \nabla \textbf{w}^n$. Therefore, taking into account (3.2), we can differentiate the right hand side in space only twice. For this purpose, we show contraction in lower regularity then the estimate (3.2). This approach is well known in the regularity theory of the compressible and inhomogeneous Navier–Stokes systems to overcome the limitations coming from the presence of the gradient of the density in the continuity equation (see among others [Reference Hoff21], [Reference Mucha and Piasecki27], [Reference Piasecki and Pokorný32], [Reference Danchin and Mucha14], [Reference Danchin and Mucha15], [Reference Danchin, Mucha and Piasecki16]). Combining (2.18) and (2.22) for
$\eta_0=0$, we obtain

which applied to (3.7) implies

The first equation of (3.7) is (2.56) with
$\textbf{v}=\textbf{w}^{n+1}$,
$\mathfrak{a}=\varrho^n p'(\varrho^n)$,
$b=R_n$, and
$\varrho_0=0$.
Therefore, (2.57) implies

As
$p(\cdot)$ is sufficiently smooth, we have

By (3.1), we have

and

Therefore choosing T sufficiently small, we can ensure that

Choosing such T and adding (3.10) to (3.9), we obtain

Recalling (3.8), we have

The last term can be estimated directly:

Let us proceed with A 1. We estimate the second order derivatives, which are the most restrictive. We have

The first two terms have the same structure and can be bounded as follows applying (3.1):

For the third term, we have

and the same estimate holds for the fourth one. Next,

and finally, for the last term, we have

Plugging the above estimates into (3.12), we obtain and observing that A 1 and A 2 have the same structure due to assumed regularity of the pressure we obtain

which together with (3.13) gives

Now in order to close the contraction argument, it is enough to estimate the second term on the RHS of (3.11). Recalling (1.2), we have

We have

We again apply (3.1) to obtain

which gives

Next,

Let us focus on the last term:

The lack of small constant is not a problem, since the term which we are estimating is already multiplied by a small constant in (3.11). The other terms in (3.17) can be estimated similarly, here we even get additional smallness in time. Summing up, we obtain

Similarly, we can show

Combining (3.16), (3.18), and (3.19), we get

Plugging (3.14) and (3.20) into (3.11), we finally conclude (3.6).
Now we complete the proof of theorem 1.1 in a standard way. Inequality (3.6) implies

On the other hand, the estimate (3.1) implies existence of a subsequence, which we can still denote
$(\textbf{w}^n,\varrho^n)$

Setting
$\textbf{u}=\textbf{w}-\nabla p(\varrho)$ we easily verify that the limit satisfies (1.7).
4. Existence theory for general velocity offsets
The goal of this section is to extend the previous result to the case of different velocity offset functions
$p(\varrho)$.
• Singular offset: As mentioned in the introduction, Aceves et al. [Reference Aceves-Sanchez, Bailo, Degond and Mercier1] derive a variant of dissipative Aw–Rascle system from a microscopic model of pedestrian dynamics. This corresponds to (1.7) with the offset function in the form (1.9). Drawing motivation from this, we consider a more general offset function and the system (1.6), namely
(4.1)\begin{align} p(\varrho)= a \frac{\varrho^\alpha}{(1-\varrho)^\beta} \text{ with } a \gt 0,\; \alpha \gt 0 \text{ and }\; \beta \gt 1. \end{align}
Similar form was considered in [Reference Chaudhuri, Navoret, Perrin and Zatorska12] where the existence of regular solutions for certain approximation of this function was proven in one space dimension. The authors also performed the singular limit passage a → 0 obtaining in the limit the hard congestion system. Similar limit has been postulated in the multi-dimensional case, see [Reference Aceves-Sanchez, Bailo, Degond and Mercier1], but to our knowledge it has not yet been proved rigorously. Nevertheless, it is expected that in the hard congestion limit, in the saturated region where ϱ = 1, one cannot expect a regular solution due to appearance of extra forcing term. Therefore here we keep a a positive constant, which results in restriction to unsaturated flow provided that the initial density is strictly below 1. This case is discussed in §4.1.
• Non-local velocity offset: It turns out that considering the non-local offset function
(4.2)\begin{align} p(\varrho)=K \ast \varrho, \end{align}
where K is some non-local kernel, leads to reformulation of the system that generalizes the pressureless Euler-alignment model, see [Reference Chaudhuri, Peszek, Szlenk and Zatorska13] for further details. Unfortunately, we are not able to apply our construction along with the linear theory (described in §2 and 3) directly to the system (1.7) with (4.2). Instead, we consider a system where the offset function
$p(\varrho)$ is a combination of local and a particular non-local component that corresponds to the Newtonian potential, i.e.,
\begin{equation*} - \Delta K \ast \varrho \approx \varrho .\end{equation*}
More precisely, the closure relation is now of the form
\begin{align*} \textbf{w}=\textbf{u}+ \nabla p(\varrho) + \nabla \Phi_\varrho \text{with } p \in C^5(\mathbb{R}_{+}) \,\,\, \text{and }- \Delta \Phi_\varrho = \varrho - \lt \varrho \gt , \end{align*}
where
$ \lt \varrho \gt =\frac{1}{|\mathbb{T}^3|}\int_{\mathbb{T}^3}\varrho\,{\rm d} {x}$, and so (1.7) can be rewritten as follows
\begin{equation*} \begin{cases} \partial_{t} \varrho+\operatorname{div}(\varrho{\textbf{w}})-\operatorname{div}(\varrho \left( \nabla p(\varrho) + \nabla \Phi_\varrho \right))=0, \qquad \qquad \qquad \qquad \qquad \hfill \textrm{(4.4a)}\\ \partial_{t}(\varrho{\textbf{w}})+\operatorname{div}(\varrho{\textbf{w}}\otimes\textbf{w})=\operatorname{div}(\varrho{\textbf{w}}\otimes \nabla p(\varrho))+\operatorname{div}(\varrho{\textbf{w}} \otimes \nabla \Phi_\varrho ),\, \qquad \hfill \textrm{(4.4b)}\\ - \Delta \Phi_\varrho = \varrho - \lt \varrho \gt .\,\, \qquad \qquad \qquad \qquad \qquad \qquad \qquad \qquad \qquad \qquad \hfill \textrm{(4.4c)} \end{cases} \end{equation*}
This case is discussed in §4.2.
4.1. Construction for the system with singular velocity offset
Here, we consider (1.6a)–(1.6b) with (4.1). Moreover, along with the hypothesis on initial data (1.4) or (1.5), we need

Theorem 4.1. Assume the initial data satisfies (1.4) or (1.5) with (4.5). Then there exists T > 0 such that system (1.7) admits a unique solution
$(\varrho,\textbf{w}) \in {\mathcal V}_3(T)\times {\mathcal Y}_3(T)$ with the estimate

in case of (1.4) or

in case of (1.5).
The proof of the theorem 4.1 consists of two parts: the proof of boundedness of approximate solutions and the compactness argument. The iteration scheme for this case is the same as in (1.11), but the proof of analogue of lemma 3.1 requires some alterations that we explain below. The contraction argument is similar to the one described in §3.2, more precisely lemma 3.2, and we skip the details here.
The main lemma for the uniform bounds reads:
Lemma 4.2. Let
$({\textbf{w}}^n,\varrho^n)$ be the sequence defined in (1.11) with
${\textbf{u}}^1(t,x) = \textbf{u}_0(x)$ for
$(t,x) \in (0,T)\times \mathbb{T}^3$. There exists
$M=M(\|\varrho_0\|_{H^4(\mathbb{T}^3)},\|\textbf{u}_0\|_{H^3(\mathbb{T}^3)})$ in case of (1.4) or
$M=M(\|\varrho_0\|_{H^3(\mathbb{T}^3)},\|\textbf{u}_0+\nabla p(\varrho_0)\|_{H^3(\mathbb{T}^3)})$ in case of (1.5) and
$T(=T(M)) \gt 0$ such that

where the spaces
${\mathcal Y}_k(T)$ and
${\mathcal V}_k(T)$ are defined in (1.10). More precisely, it holds that there exists
$0 \lt \vartheta \lt 1$ such that

Proof. Similarly to lemma (3.1), we prove this lemma with the help of an induction hypothesis: we interpret the first equation in (1.11) as Eq. (2.56) with
$\mathfrak{b}=0$,
$\varrho=\varrho^{n+1},\textbf{v}=\textbf{w}^{n+1}$, and
$\mathfrak{a}=\varrho^n p'(\varrho^n)$, while the ith row of the second equation in (1.11) as (2.1) with g = 0,
$\eta=\textbf{w}^{n+1}_i$ and
$\textbf{v}=\textbf{u}^n$.
Clearly, there exists
$0 \lt \vartheta \lt 1$ such that

Now, we assume that
$(\varrho_n, \textbf{w}_n)$ satisfy (4.6) along with (4.7). This yields,

and
$\mathfrak{a} \in L_\infty(0,T;W^1_\infty(\mathbb{T}^3)) \cap L_2(0,T;H^2(\mathbb{T}^3))$. Here, we perform the similar estimates for
$ \textbf{w}^{n+1} $ and obtain

Similarly, for
$ \varrho^{n+1} $, we have

Applying lemma 2.4, we obtain

for
$t\in (0,T)$. Because

with C independent of time, we further deduce

We set

where C(T) is the constant from (4.9). Assuming that

for sufficiently small T, we can show that

This in turn, along with (4.8) and (4.9), implies

thus we have the first part of (4.6). Finally, we choose a sufficiently small T depending only on M, such that from (4.10) we obtain that

This finishes the proof.
4.2. Construction for the system with non-local velocity offset
In this part, we prove the following existence result for system (4.4):
Theorem 4.3. Assume the initial data satisfies (1.4) or (1.5). Then there exists T > 0 such that system (4.4) admits a unique solution
$(\varrho,\textbf{w}, \Phi_\varrho) \in {\mathcal V}_3(T)\times {\mathcal Y}_3(T) \times {\mathcal V}_5(T)$ with the estimate

in case of (1.4) or

in case of (1.5).
Again the proof of the above theorem is similar to the proof of theorem 1.1.
In this case, however, we use the following iteration scheme for construction of the approximate solution:

where
$\displaystyle - \Delta \Phi_{\varrho_0} = \varrho_0 - \lt \varrho_0 \gt $,
$(\varrho^0,\textbf{w}^0,\Phi_0)=(\varrho_0,\textbf{u}_0+\nabla p(\varrho_0)+ \nabla \Phi_{\varrho_0}, \Phi_{\varrho_0})$ and

The key observation is that the equation for
$\Phi_{n+1}$ in this scheme is an elliptic equation. Therefore, the regularity class for
$\{\Phi_n\}$ is higher. Additionally, we have uniform bounds for the approximate sequence
$ (\varrho^{n}, \textbf{w}^n, \Phi_n) $ in spaces
${\mathcal V}_3(T)\times {\mathcal Y}_3(T) \times {\mathcal V}_5(T)$, as stated in the following Lemma.
Lemma 4.4. Let
$(\textbf{w}^n,\varrho^n,\Phi_n)$ be the sequence defined in (4.11) with
$\textbf{u}^1(t,x) = \textbf{u}_0(x)$ for
$(t,x) \in (0,T)\times \mathbb{T}^3$. There exists
$M=M(\|\varrho_0\|_{H^4(\mathbb{T}^3)},\|\textbf{u}_0\|_{H^3(\mathbb{T}^3)})$ in case of (1.4) or
$M=M(\|\varrho_0\|_{H^3},\|\textbf{u}_0+\nabla p(\varrho_0)\|_{H^3(\mathbb{T}^3)})$ in case of (1.5) and
$T=T(M) \gt 0$ such that

where the spaces
${\mathcal Y}_k(T)$ and
${\mathcal V}_k(T)$ are defined in (1.10).
Proof. Sketch of the proof
The key steps of the proof are the following.
• The bounds on
$\|\textbf{w}^{n+1}\|_{{\mathcal Y}_3(T)}$ and
$\|\varrho^{n+1}\|_{{\mathcal V}_3(T)}$ are obtained by calculations similar to proof of lemma 3.1, but keeping in mind that the relation between wn and un has been modified (4.12). Ultimately, we obtain
(4.13)\begin{align} & \|\textbf{w}^{n+1}\|_{{\mathcal Y}_3(T)}\leq \phi(\sqrt{{T}}\|\textbf{u}^n\|_{{\mathcal X}_3(T)})\nonumber\\ & =\phi_1\left(\sqrt{{T}}(\|\textbf{w}^n(t)\|_{{\mathcal Y}_3(T)}+\|\varrho^n\|_{{\mathcal V}_3(T)} + \| \Phi_n \|_{{\mathcal V}_5(T) } )\right) , \end{align}
and
(4.14)\begin{equation} \begin{aligned} & \|\varrho^{n+1}\|_{{\mathcal V}_3(T)} \\ & \leq \phi_2(\|\varrho_0\|_{H^3(\mathbb{T}^3)}) \left[C(T)+ T\|\varrho^{n+1}\|_{{\mathcal V}_3(T)}\right. \\ & \left. \Big[ \phi_1\Big(\sqrt{{T}}(\|\textbf{w}^n(t)\|_{{\mathcal Y}_3(T)}+\|\varrho^n\|_{{\mathcal V}_3(T)} +\| \Phi_n \|_{{\mathcal V}_5(T) } )\right)\\ & +\phi_3(\|\varrho^n\|_{L_\infty( (0,T) \times \mathbb{T}^3)})\left( \|\varrho^n\|_{{\mathcal V}_3(T)}+\| \Phi_n \|_{{\mathcal V}_5(T)} \right) \Big]\Big]. \end{aligned} \end{equation}
• The estimate of
$ \|\Phi_{n+1} \|_{{\mathcal V}_5(T)} $ follows from the elliptic regularity estimates for the solutions of the problem
\begin{equation*}- \Delta \Phi_{n+1} = \varrho^{n+1} - \lt \varrho^{n+1} \gt .\end{equation*}
Following Evans [Reference Evans18, Chapter 6], we obtain
(4.15)\begin{align} \| \Phi_{n+1} \|_{{\mathcal V}_5(T) } \leq C_{\rm ell} \| \varrho^{n+1} \|_{{\mathcal V}_3(T) }. \end{align}
• The strict positivity of
$\varrho^{n+1}$ is a direct consequence of lemma 2.3, where we use the particular form of
$\mathfrak{b} = \operatorname{div}(\varrho^{n} \nabla \Phi_{n} )$ in the first line of (4.11), i.e.,
\begin{align*} \varrho^{n+1}_t+{\rm div}\,(\varrho^{n+1} \textbf{w}^{n+1} ) -{\rm div}\,(\varrho^n p'( \varrho^n)\nabla\varrho^{n+1})=\mathfrak{b}= {\rm div}\,(\varrho^{n+1} \nabla\Phi_{n} ). \end{align*}
• Now we combine estimates (4.13)–(4.15) and choose
\begin{equation*} M=2(1+C_{\rm ell}) \max\{\sup_{s\in[0,1]}\phi_1(s),\phi_2(\|\varrho_0\|_{H^3(\mathbb{T}^3)})C(T)\}, \end{equation*}
where C(T) is the constant from (4.14) and C ell is from (4.15). Now, assuming that
\begin{equation*} \|\textbf{w}^n\|_{{\mathcal Y}_3(T)}+\|\varrho^n\|_{{\mathcal V}_3(T)}+ \|\Phi_{n} \|_{{\mathcal V}_5(T)} \leq M, \end{equation*}
for sufficiently small T, first we can show that
\begin{align*} &\phi_1(\sqrt{T}(\|\textbf{w}^n\|_{{\mathcal Y}_3(T)}+\|\varrho^n\|_{{\mathcal V}_3(T)}+\|\Phi_{n+1} \|_{{\mathcal V}_5(T)} )\leq\frac{M}{2}\\ & T\phi_2(\|\varrho_0\|_{H^3(\mathbb{T}^3)})\left[ \|\textbf{w}^{n+1}\|_{{\mathcal Y}_3(T)}+\phi_3(\|\varrho^n\|_{L_\infty( (0,T) \times \mathbb{T}^3)})\right. \\ & \left. \left( \|\varrho^n\|_{{\mathcal V}_3(T)}+\|\Phi_{n} \|_{{\mathcal V}_5(T)} \right) \right] \leq \frac{1}{2}. \end{align*}
This, along with (4.8) and (4.9), implies
\begin{equation*} \|\textbf{w}^{n+1}\|_{{\mathcal Y}_3(T)}+\|\varrho^{n+1}\|_{{\mathcal V}_3(T)}+\|\Phi_{n+1} \|_{{\mathcal V}_5(T)}\leq M, \end{equation*}
and the proof is complete.
The second part of the proof of theorem 4.3 is to provide an analogue of the contraction argument described in §3.2. We denote

The system of difference equation corresponding to (4.11) is thus

where

Performing the estimates similar to those from the proof of lemma 3.2, for the term

We can show the following lemma:
Lemma 4.5. Under the assumptions of lemma 4.4, we have

where E(t) is described in §1.1.
This concludes the contraction argument and also the proof of theorem 4.3.
Acknowledgements
The work of N.C. was funded by the ‘Excellence Initiative Research University (IDUB)’ program at the University of Warsaw. T.P.’s work was supported by the National Science Centre (NCN) project 2022/45/B/ST1/03432. The work of N.C. and E.Z. was supported by the EPSRC Early Career Fellowship no. EP/V000586/1.