Rotating neutron stars: an invariant comparison of approximate and numerical space-time models-Reference-Cited by-同舟云学术

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Rotating neutron stars: an invariant comparison of approximate and numerical space-time models

Published:2005-04-11 Issue:3 Volume:358 Page:923-938
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:Monthly Notices of the Royal Astronomical Society

Author:

Berti E.,White F.,Maniopoulou A.,Bruni M.

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/358/3/923/3418058/358-3-923.pdf

Reference41 articles.

1. THE R-MODE INSTABILITY IN ROTATING NEUTRON STARS

2. Highly accurate calculation of rotating neutron stars

3. A millisecond pulsar

4. Making use of geometrical invariants in black hole collisions

5. A Radiation Scalar for Numerical Relativity

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1. Neutron stars in f(R,T) theory: slow rotation approximation;Journal of Cosmology and Astroparticle Physics;2024-09-01

2. Accretion disk in the Hartle–Thorne spacetime;The European Physical Journal Plus;2024-03-20

3. Rotating Massive Strangeon Stars and X-Ray Plateau of Short GRBs;Research in Astronomy and Astrophysics;2024-02-21

4. Rotating dark matter admixed neutron stars;Physical Review D;2023-11-13

5. Structure-preserving numerical simulations of test particle dynamics around slowly rotating neutron stars within the Hartle-Thorne approach;Physical Review D;2023-11-06

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