A TFD model for the Electrospheres of Bare Strange Quark Stars
Hai-Chuan Guo (CAS), Ren-Xin Xu (PKU), Cheng-Min Zhang (CAS)

TL;DR
This paper models the electron layer on bare strange quark stars, incorporating Dirac exchange-energy and magnetic field effects, to better understand surface electron distributions and electric fields.
Contribution
It introduces a TFD model that accounts for exchange-antisymmetry and magnetic fields in electrosphere structure analysis of bare strange stars.
Findings
Exchange-energy influences electron distribution
Magnetic fields significantly affect electrosphere structure
Model improves understanding of star surface electric fields
Abstract
We study the layer of electrons on bare strange star surfaces, taking the Dirac exchange-energy into account. Because electrons are fermions, the electron wave function must be of exchange-antisymmetry. The Dirac exchange-energy originates, consequently, from the exchange-antisymmetry of electron wave functions. This consideration may result in changing the electron distribution and the electric field on the surface of bare strange star. The strong magnetic field effect on the structures of the electrospheres is also discussed.
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Taxonomy
TopicsPulsars and Gravitational Waves Research · Astronomy and Astrophysical Research · Stellar, planetary, and galactic studies
