English

Strichartz estimates and low regularity solutions of 3D relativistic Euler equations

Analysis of PDEs 2024-11-05 v3

Abstract

We study the low regularity well-posedness for Cauchy problem of 3D relativistic Euler equations. Firstly, we introduce a new decomposition for relativistic velocity and derive new transport equations for vorticity, which both play a crucial role in energy and Strichartz estimates. According to Smith-Tataru's approach, we then establish a Strichartz estimate of linear wave equations endowed with the acoustic metric. This leads us to prove a complete local well-posedness result if the initial logarithmic enthalpy, velocity, and modified vorticity (h0,\bu0,\bw0)Hs×Hs×Hs0(2<s0<s)(h_0, \bu_0, \bw_0) \in H^s \times H^s \times H^{s_0} (2<s_0<s). Therefore, we give an affirmative answer to "Open Problem D" proposed by Disconzi. Moreover, for (h0,\bu0,\bw0)H2+×H2+×H2(h_0,{\bu}_0,\bw_0) \in H^{2+} \times H^{2+} \times H^2, by frequency truncation, there is a stronger Strichartz estimate for solutions on a short-time-interval. By semi-classical analysis and induction method, these solutions can be extended from short time intervals to a regular time interval, and a uniform Strichartz estimate with loss of derivatives can be obtained. This allows us to prove the local well-posedness of 3D relativistic equations if (h0,\bu0,\bw0)H2+×H2+×H2(h_0,{\bu}_0,\bw_0) \in H^{2+} \times H^{2+} \times H^2.

Keywords

Cite

@article{arxiv.2401.12796,
  title  = {Strichartz estimates and low regularity solutions of 3D relativistic Euler equations},
  author = {Huali Zhang},
  journal= {arXiv preprint arXiv:2401.12796},
  year   = {2024}
}

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R2 v1 2026-06-28T14:24:46.260Z