<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>g</mml:mi></mml:mrow></mml:math> -mode of neutron stars in pseudo-Newtonian gravity-Reference-Cited by-同舟云学术

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g -mode of neutron stars in pseudo-Newtonian gravity

Published:2023-09-05 Issue:6 Volume:108 Page:
ISSN:2470-0010
Container-title:Physical Review D
language:en
Short-container-title:Phys. Rev. D

Author:

Li Hong-Bo^ORCID,Gao Yong,Shao Lijing^ORCID,Xu Ren-Xin

Funder

National Natural Science Foundation of China

National Key Research and Development Program of China

Max-Planck-Gesellschaft

Center for High Performance Computing

Peking University

National SKA

Publisher

American Physical Society (APS)

Link

http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevD.108.064005/fulltext

Reference63 articles.

1. Gravitational-Wave Astronomy

2. The Non-radial Oscillations of Polytropic Stars

3. Exploring the relativistic regime with Newtonian hydrodynamics: an improved effective gravitational potential for supernova simulations

4. Exploring the relativistic regime with Newtonian hydrodynamics

5. Gravitational wave signatures ofab initiotwo-dimensional core collapse supernova explosion models for12–25 M⊙stars

Cited by 2 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. Radial and nonradial oscillations of inverted hybrid stars;Physical Review D;2024-03-15

2. Quasi-periodic oscillations during magnetar giant flares in the strangeon star model;Monthly Notices of the Royal Astronomical Society;2023-10-21

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