[Submitted on 11 Jun 2025] (cross-list from astro-ph.HE)
Locating the QCD critical point with neutron-star observations
Christian Ecker🇩🇪 · Niko Jokela🇫🇮 · Matti Järvinen🇰🇷
We present a probabilistic model for the QCD critical endpoint (CEP) and the equation of state (EOS) at -equilibrium, constrained by neutron-star observations. Using a hybrid framework that combines the holographic V-QCD model with an effective van der Waals description of nuclear matter, we generate a large ensemble of EOSs incorporating nuclear theory uncertainties. Constraining this ensemble with neutron-star mass-radius data and tidal deformability measurements from gravitational waves, we identify a strong first-order deconfinement transition at zero temperature, with a transition strength of and onset density . The resulting posterior yields credible intervals for the CEP location: , .
- Comments:
- 9 pages, 5 figures
- Subjects:
- High Energy Astrophysical Phenomena (astro-ph.HE); General Relativity and Quantum Cosmology (gr-qc); High Energy Physics — Phenomenology (hep-ph); High Energy Physics — Theory (hep-th); Nuclear Theory (nucl-th)
- arXiv:
- 2506.10065 [pdf]