Gravitational waves from rotational core collapse in the conformally flat spacetime approximation

Details Gravitational waves from rotational core collapse in the conformally flat spacetime approximation Gravitational waves from rotational core collapse in the conformally flat spacetime approximation

Oct 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aipc..586..757d&link_type=abstract

RELATIVISTIC ASTROPHYSICS: 20th Texas Symposium. AIP Conference Proceedings, Volume 586, pp. 757-759 (2001).

Astronomy and Astrophysics

Astrophysics

Supernovae, Hydrodynamics, Mathematical Procedures And Computer Techniques, Approximation Methods, Equations Of Motion, Neutron Stars, Relativity And Gravitation

Scientific paper

We have developed an axisymmetric general relativistic hydrodynamic code based upon an approximation scheme recently proposed by Wilson and coworkers, in which the 3-metric γij is conformally flat, thus reducing the mathematical complexity of the Einstein metric equations to a set of 5 coupled elliptic equations. Applications of our code to rotational supernova core collapse are presented. We also discuss first results concerning the emission of gravitational waves. .

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