Toward Black Hole Stars: Supermassive Black Hole Growth in Nuclear Clusters via Stellar-object and Gas Accretion

BibTeX Entry

@article{2026ApJ..1000L..21K,
  author = {{Kritos}, Konstantinos and {Silk}, Joseph},
  title = {{Toward Black Hole Stars: Supermassive Black Hole Growth in Nuclear Clusters via Stellar-object and Gas Accretion}},
  journal = {\apjl},
  keywords = {Stellar dynamics, Gravitational wave sources, Transient sources, 1596, 677, 1851},
  year = {2026},
  month = mar,
  volume = {1000},
  number = {1},
  eid = {L21},
  pages = {L21},
  doi = {10.3847/2041-8213/ae4c52},
  adsurl = {https://ui.adsabs.harvard.edu/abs/2026ApJ..1000L..21K},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System},
  dimensions = {true},
  lrdkeys = {early universe, heavy seed, super-eddington, theory},
  eprint = {2602.15929},
  archiveprefix = {arXiv},
  primaryclass = {astro-ph.HE},
  month_numeric = {3}
}

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