Semiclassical Equivalence of Two White Dwarf Models as Ground States of the Relativistic Hartree–Fock and Vlasov–Poisson energies

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초록

We are concerned with the semi-classical limit for ground states of the relativistic Hartree–Fock energies (HF) under a mass constraint, which are considered as the quantum mean-field model of white dwarfs (Lenzmann and Lewin in Duke Math J 152:257–315, 2010). In Jang and Seok (Kinet Relat Models 15:605–620, 2022), fermionic ground states of the relativistic Vlasov–Poisson energy (VP) are constructed as a classical mean-field model of white dwarfs, and are shown to be equivalent to the classical Chandrasekhar model. In this paper, we prove that as the reduced Planck constant ħ goes to the zero, the ħ-parameter family of the ground energies and states of (HF) converges to the fermionic ground energy and state of (VP) with the same mass constraint.

키워드

CHANDRASEKHAR THEORY; STELLAR COLLAPSE; STABILITY; LIMIT
제목
Semiclassical Equivalence of Two White Dwarf Models as Ground States of the Relativistic Hartree–Fock and Vlasov–Poisson energies
저자
Hong, Younghun; Jin, Sangdon; Seok, Jinmyoung
DOI
10.1007/s00023-024-01494-3
발행일
2025-07
유형
Article; Early Access
저널명
Annales Henri Poincare
권
26
호
7
페이지
2625 ~ 2653