Résumé
The Carrollian fluid equations arise as the (Formula presented.) limit of the relativistic fluid equations and have recently experienced a surge of activity in the flat-space holography community. However, the rigorous mathematical well-posedness theory for these equations does not appear to have been previously studied. This paper is the third in a series in which we initiate the systematic analysis of the Carrollian fluid equations. In the present work, we prove the global-in-time existence of bounded entropy solutions to the isentropic Carrollian fluid equations in one spatial dimension for a particular constitutive law ((Formula presented.)). Our method is to use a vanishing viscosity approximation for which we establish a compensated compactness framework. Using this framework we also prove the compactness of entropy solutions in (Formula presented.), and establish a kinetic formulation of the problem. This global existence result in (Formula presented.) extends the (Formula presented.) theory presented in [2].
| langue originale | Anglais |
|---|---|
| Numéro d'article | e70186 |
| journal | Journal of the London Mathematical Society |
| Volume | 111 |
| Numéro de publication | 6 |
| Les DOIs | |
| état | Publié - 1 juin 2025 |
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