Quasiradial oscillations of rotating hybrid neutron stars

Fuente: arXiv
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Main Authors: Zheng, Zi-Yue, Sun, Ting-Ting, Chen, Huan, Zheng, Xiao-Ping, Wei, Jin-Biao, Burgio, G. F., Schulze, H. -J.
Format: Preprint
Published: 2026
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author Zheng, Zi-Yue
Sun, Ting-Ting
Chen, Huan
Zheng, Xiao-Ping
Wei, Jin-Biao
Burgio, G. F.
Schulze, H. -J.
author_facet Zheng, Zi-Yue
Sun, Ting-Ting
Chen, Huan
Zheng, Xiao-Ping
Wei, Jin-Biao
Burgio, G. F.
Schulze, H. -J.
contents We investigate fundamental quasiradial oscillations in slow-rotation approximation of pure and hybrid neutron stars, employing equations of state of nuclear matter from Brueckner-Hartree-Fock theory or the relativistic mean field model, and of quark matter from the Dyson-Schwinger quark model, performing a Gibbs construction for the mixed phase in hybrid stars. Characteristic differences between neutron-star and hybrid-star fundamental quasiradial oscillation frequencies during spin-down are pointed out.
format Preprint
id arxiv_https___arxiv_org_abs_2605_23433
institution arXiv
publishDate 2026
record_format arxiv
spellingShingle Quasiradial oscillations of rotating hybrid neutron stars
Zheng, Zi-Yue
Sun, Ting-Ting
Chen, Huan
Zheng, Xiao-Ping
Wei, Jin-Biao
Burgio, G. F.
Schulze, H. -J.
Nuclear Theory
High Energy Astrophysical Phenomena
We investigate fundamental quasiradial oscillations in slow-rotation approximation of pure and hybrid neutron stars, employing equations of state of nuclear matter from Brueckner-Hartree-Fock theory or the relativistic mean field model, and of quark matter from the Dyson-Schwinger quark model, performing a Gibbs construction for the mixed phase in hybrid stars. Characteristic differences between neutron-star and hybrid-star fundamental quasiradial oscillation frequencies during spin-down are pointed out.
title Quasiradial oscillations of rotating hybrid neutron stars
topic Nuclear Theory
High Energy Astrophysical Phenomena
url https://arxiv.org/abs/2605.23433