Thermodynamics of strongly magnetized dense quark matter from hard dense loop perturbation theory

Fuente: arXiv
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Main Authors: Satapathy, Sarthak, Sumit, Khan, Salman Ahamad
Format: Preprint
Published: 2025
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author Satapathy, Sarthak
Sumit
Khan, Salman Ahamad
author_facet Satapathy, Sarthak
Sumit
Khan, Salman Ahamad
contents We discuss the hard dense loop perturbation theory approach for studying the thermodynamics of strongly magnetized dense quark matter. The free energy of quarks and gluons have been calculated for one-loop quark and gluon self-energies, respectively. The longitudinal and transverse components of pressure, magnetization, second-order quark number susceptibility, and speed of sound have been computed, and their behavior with chemical potential and magnetic field has been analyzed. Our numerical results show that the longitudinal pressure increases with chemical potential and magnetic field, while for the transverse component, it is diminished. We also analyze the longitudinal component of the speed of sound at high chemical potentials, which approaches the speed of light in the asymptotic limit. The obtained results may be helpful in studying magnetized quark matter in the core of neutron stars and magnetars.
format Preprint
id arxiv_https___arxiv_org_abs_2503_00824
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Thermodynamics of strongly magnetized dense quark matter from hard dense loop perturbation theory
Satapathy, Sarthak
Sumit
Khan, Salman Ahamad
Nuclear Theory
High Energy Physics - Phenomenology
High Energy Physics - Theory
We discuss the hard dense loop perturbation theory approach for studying the thermodynamics of strongly magnetized dense quark matter. The free energy of quarks and gluons have been calculated for one-loop quark and gluon self-energies, respectively. The longitudinal and transverse components of pressure, magnetization, second-order quark number susceptibility, and speed of sound have been computed, and their behavior with chemical potential and magnetic field has been analyzed. Our numerical results show that the longitudinal pressure increases with chemical potential and magnetic field, while for the transverse component, it is diminished. We also analyze the longitudinal component of the speed of sound at high chemical potentials, which approaches the speed of light in the asymptotic limit. The obtained results may be helpful in studying magnetized quark matter in the core of neutron stars and magnetars.
title Thermodynamics of strongly magnetized dense quark matter from hard dense loop perturbation theory
topic Nuclear Theory
High Energy Physics - Phenomenology
High Energy Physics - Theory
url https://arxiv.org/abs/2503.00824