PreprintarXiv licencearXiv
Thermodynamic and structural properties of the thin atmosphere of a white dwarf
Abstract
We determine thermodynamic and structural properties of the Coulomb plasma (jellium) in the thin atmosphere of a white dwarf using the path integral Monte Carlo method within a general relativity description of the star.
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BibTeX
@misc{fantoni2026thermodynamic,
title = {{Thermodynamic and structural properties of the thin atmosphere of a white dwarf}},
author = {Riccardo Fantoni},
howpublished = {arXiv},
year = {2026},
month = oct,
doi = {10.48550/arxiv.2610.37708},
eprint = {2610.37708},
archivePrefix = {arXiv},
url = {https://arxiv.org/abs/2610.37708},
}
RIS
TY - UNPB
TI - Thermodynamic and structural properties of the thin atmosphere of a white dwarf
AU - Riccardo Fantoni
PY - 2026
DA - 2026/10/26
PB - arXiv
DO - 10.48550/arxiv.2610.37708
UR - https://arxiv.org/abs/2610.37708
AB - We determine thermodynamic and structural properties of the Coulomb plasma (jellium) in the thin atmosphere of a white dwarf using the path integral Monte Carlo method within a general relativity description of the star.
ER -