Mass-Critical Neutron Stars in the Hartree-Fock and Hartree-Fock-Bogoliubov Theories

Fuente: arXiv
Enregistré dans:
Détails bibliographiques
Auteurs principaux: Chen, Bin, Guo, Yujin, Nam, Phan Thành, Yang, Dong Hao Ou
Format: Preprint
Publié: 2025
Sujets:
Accès en ligne:
Tags: Ajouter un tag
Pas de tags, Soyez le premier à ajouter un tag!
_version_ 1866918147712352256
author Chen, Bin
Guo, Yujin
Nam, Phan Thành
Yang, Dong Hao Ou
author_facet Chen, Bin
Guo, Yujin
Nam, Phan Thành
Yang, Dong Hao Ou
contents We investigate the ground states of neutron stars and white dwarfs in the Hartree-Fock (HF) and Hartree-Fock-Bogoliubov (HFB) theories. It is known that the system is stable below a critical mass, which depends on the gravitational constant, while it becomes unstable if the total mass exceeds the critical mass. We prove that if the total mass is at the critical mass, then the HFB minimizers do not exist for any gravitational constant, while the HF minimizers exist for every gravitational constant except for a countable set, which is fully characterized by the Gagliardo-Nirenberg inequality for orthonormal systems. Our results complement the existence results in the sub-critical mass case established in [E. Lenzmann and M. Lewin, Duke Math. J., 2010].
format Preprint
id arxiv_https___arxiv_org_abs_2504_16462
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Mass-Critical Neutron Stars in the Hartree-Fock and Hartree-Fock-Bogoliubov Theories
Chen, Bin
Guo, Yujin
Nam, Phan Thành
Yang, Dong Hao Ou
Analysis of PDEs
Mathematical Physics
We investigate the ground states of neutron stars and white dwarfs in the Hartree-Fock (HF) and Hartree-Fock-Bogoliubov (HFB) theories. It is known that the system is stable below a critical mass, which depends on the gravitational constant, while it becomes unstable if the total mass exceeds the critical mass. We prove that if the total mass is at the critical mass, then the HFB minimizers do not exist for any gravitational constant, while the HF minimizers exist for every gravitational constant except for a countable set, which is fully characterized by the Gagliardo-Nirenberg inequality for orthonormal systems. Our results complement the existence results in the sub-critical mass case established in [E. Lenzmann and M. Lewin, Duke Math. J., 2010].
title Mass-Critical Neutron Stars in the Hartree-Fock and Hartree-Fock-Bogoliubov Theories
topic Analysis of PDEs
Mathematical Physics
url https://arxiv.org/abs/2504.16462