General Relativistic Shock Wave Solutions with Black Hole Formation: The Singular Isothermal Sphere Case

BibTeX Entry

@article{2026arXiv260629607C,
  author = {{Chen}, Chien-Ting J. and {Cai}, Michael J. and {Pacucci}, Fabio},
  title = {{General Relativistic Shock Wave Solutions with Black Hole Formation: The Singular Isothermal Sphere Case}},
  journal = {arXiv e-prints},
  keywords = {High Energy Astrophysical Phenomena, Cosmology and Nongalactic Astrophysics, Astrophysics of Galaxies, General Relativity and Quantum Cosmology},
  year = {2026},
  month = jun,
  eid = {arXiv:2606.29607},
  pages = {arXiv:2606.29607},
  archiveprefix = {arXiv},
  eprint = {2606.29607},
  primaryclass = {astro-ph.HE},
  adsurl = {https://ui.adsabs.harvard.edu/abs/2026arXiv260629607C},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System},
  dimensions = {true},
  lrdkeys = {early universe, heavy seed, jwst, theory},
  month_numeric = {6}
}

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