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PreprintCC BY 4.0arXiv

Quark deconfinement as a natural trigger of Type-I critical collapse: black holes from neutron stars deemed stable

Abstract

Spherically symmetric general-relativistic simulations show that a first-order hadron--quark phase transition can collapse radially stable neutron stars into black holes, even when a stable hybrid star of the same baryon mass exists. The dynamical threshold lies 0.12 M⊙ in baryon mass below the static one, so black holes can be lighter than the heaviest stable star. The threshold is a Type-I critical point: near it, the star lingers at an unstable hybrid star of equal baryon mass for a time set by that star's unstable mode. The effect persists within a narrower window for finite conversion rates.

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BibTeX
@misc{borthakur2026quark,
  title = {{Quark deconfinement as a natural trigger of Type-I critical collapse: black holes from neutron stars deemed stable}},
  author = {Hrishikesh Borthakur and Ritam Mallick},
  howpublished = {arXiv},
  year = {2026},
  month = nov,
  doi = {10.48550/arxiv.2611.04679},
  eprint = {2611.04679},
  archivePrefix = {arXiv},
  url = {https://arxiv.org/abs/2611.04679},
  note = {CC BY 4.0},
}
RIS
TY  - UNPB
TI  - Quark deconfinement as a natural trigger of Type-I critical collapse: black holes from neutron stars deemed stable
AU  - Hrishikesh Borthakur
AU  - Ritam Mallick
PY  - 2026
DA  - 2026/11/03
PB  - arXiv
DO  - 10.48550/arxiv.2611.04679
UR  - https://arxiv.org/abs/2611.04679
AB  - Spherically symmetric general-relativistic simulations show that a first-order hadron--quark phase transition can collapse radially stable neutron stars into black holes, even when a stable hybrid star of the same baryon mass exists. The dynamical threshold lies 0.12 M_⊙ in baryon mass below the static one, so black holes can be lighter than the heaviest stable star. The threshold is a Type-I critical point: near it, the star lingers at an unstable hybrid star of equal baryon mass for a time set by that star's unstable mode. The effect persists within a narrower window for finite conversion rates.
ER  -