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Relativistic collision geometry and global near-vacuum solutions at critical transverse regularity

Abstract

We establish global well-posedness near vacuum for the relativistic Boltzmann equation with soft and hard potentials in the range γ∈(−2,1]. The initial data have critical Besov regularity of order 2/r in the transverse spatial variables for an admissible range of r depending on γ, together with weighted integrability in the longitudinal and momentum variables. The proof combines a fixed-direction div--curl lemma with bilinear collision estimates. In particular, to control the gain term, we combine localization to spherical caps with energy-weighted angular estimates. The key relativistic estimate controls the singularity associated with the first component of the post-collisional relative velocity. These bounds yield the required time decay.

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BibTeX
@misc{hu2026relativistic,
  title = {{Relativistic collision geometry and global near-vacuum solutions at critical transverse regularity}},
  author = {Xinfeng Hu and Shuangqian Liu and Haoran Peng and Yi Zhou},
  howpublished = {arXiv},
  year = {2026},
  month = oct,
  doi = {10.48550/arxiv.2610.40322},
  eprint = {2610.40322},
  archivePrefix = {arXiv},
  url = {https://arxiv.org/abs/2610.40322},
}
RIS
TY  - UNPB
TI  - Relativistic collision geometry and global near-vacuum solutions at critical transverse regularity
AU  - Xinfeng Hu
AU  - Shuangqian Liu
AU  - Haoran Peng
AU  - Yi Zhou
PY  - 2026
DA  - 2026/10/29
PB  - arXiv
DO  - 10.48550/arxiv.2610.40322
UR  - https://arxiv.org/abs/2610.40322
AB  - We establish global well-posedness near vacuum for the relativistic Boltzmann equation with soft and hard potentials in the range γ∈(−2,1]. The initial data have critical Besov regularity of order 2/r in the transverse spatial variables for an admissible range of r depending on γ, together with weighted integrability in the longitudinal and momentum variables. The proof combines a fixed-direction div--curl lemma with bilinear collision estimates. In particular, to control the gain term, we combine localization to spherical caps with energy-weighted angular estimates. The key relativistic estimate controls the singularity associated with the first component of the post-collisional relative velocity. These bounds yield the required time decay.
ER  -