Internal composition of proto-neutron stars under strong magnetic fields-Reference-Cited by-同舟云学术

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Internal composition of proto-neutron stars under strong magnetic fields

Published:2016-08-10 Issue:4 Volume:94 Page:
ISSN:2470-0010
Container-title:Physical Review D
language:en
Short-container-title:Phys. Rev. D

Author:

Franzon B.,Dexheimer V.,Schramm S.

Funder

Conselho Nacional de Desenvolvimento Científico e Tecnológico

Deutscher Akademischer Austauschdienst

Human Genome Sciences

LOEWE Zentrum AdRIA

European Cooperation in Science and Technology

Publisher

American Physical Society (APS)

Link

http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevD.94.044018/fulltext

Reference91 articles.

1. The birth of neutron stars

2. Evolution of Proto–Neutron Stars

3. Composition and structure of protoneutron stars

Cited by 20 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Effects of finite temperature on the magnetized equation of state in neutron stars composed of a Bose-Einstein condensate;Physical Review C;2023-07-27

2. Methods for relativistic self-gravitating fluids: from binary neutron stars to black hole-disks and magnetized rotating neutron stars;General Relativity and Gravitation;2022-06

3. Effects of Magnetic Fields in Hot White Dwarfs;The Astrophysical Journal;2021-10-26

4. Quasi-universality of the magnetic deformation of neutron stars in general relativity and beyond;Astronomy & Astrophysics;2021-10

5. Frame-dragging effects in obliquely rotating magnetars;Journal of Astrophysics and Astronomy;2021-07-30

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