Volume 508 - QCD at the Extremes (QCDEX2025) - Session: Parton Densities and TMDs at low scales, including saturation and recombination.
Neutron star as a signal for quark-gluon plasma formation
A. Khatri* and S.S. Singh
*: corresponding author
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Supplementary files:
Pre-published on: November 19, 2025
Published on: —
Abstract
Studying neutron stars can help us understand the early formation of the universe. To understand and describe neutron stars, an appropriate equation of state that satisfies bulk nuclear matter properties is necessary. This study explores the quark matter equation of state by applying the Density Dependent Quark Mass model which is an extension of the MIT Bag model. The equation of state such as pressure, energy density, entropy, specific heat and speed of sound are calculated for a range of temperatures. The model results provide QGP equation of state, and the velocity of sound is shown in comparison to the Lattice QCD result.
DOI: https://doi.org/10.22323/1.508.0019
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