Complete equation of state for neutron stars using the relativistic Hartree-Fock approximation

Tsuyoshi Miyatsu, Sachiko Yamamuro, Ken'ichiro Nakazato, Myung Ki Cheoun

研究成果: 書籍/レポート タイプへの寄稿会議への寄与

抄録

We construct the equation of state in a wide-density range for neutron stars within relativistic Hartree-Fock approximation. The properties of uniform and nonuniform nuclear matter are studied consistently. The tensor couplings of vector mesons to baryons due to exchange contributions (Fock terms) are included, and the change of baryon internal structure in matter is also taken into account using the quark-meson coupling model. The Thomas-Fermi calculation is adopted to describe nonuniform matter, where the lattice of nuclei and the neutron drip out of nuclei are considered. Even if hyperons exist in the core of a neutron star, we obtain the maximum neutron-star mass of 1.95M , which is consistent with the recently observed massive pulsar, PSR J1614-2230. In addition, the strange vector (φ) meson also plays a important role in supporting a massive neutron star.

本文言語英語
ホスト出版物のタイトルOrigin of Matter and Evolution of Galaxies 2013 - Proceedings of the 12th International Symposium on Origin of Matter and Evolution of Galaxies, OMEG 2013
出版社American Institute of Physics Inc.
ページ420-425
ページ数6
ISBN(印刷版)9780735412286
DOI
出版ステータス出版済み - 2014
イベント12th International Symposium on Origin of Matter and Evolution of Galaxies, OMEG 2013 - Tsukuba, 日本
継続期間: 11月 18 201311月 21 2013

出版物シリーズ

名前AIP Conference Proceedings
1594
ISSN(印刷版)0094-243X
ISSN(電子版)1551-7616

その他

その他12th International Symposium on Origin of Matter and Evolution of Galaxies, OMEG 2013
国/地域日本
CityTsukuba
Period11/18/1311/21/13

!!!All Science Journal Classification (ASJC) codes

  • 物理学および天文学一般

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