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Details on the gravitational-wave emission from rotating gravitational collapse in 3D

MPG-Autoren
http://pubman.mpdl.mpg.de/cone/persons/resource/persons20670

Rezzolla,  Luciano
Astrophysical Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society;

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JoP_66_1_012045.pdf
(beliebiger Volltext), 378KB

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Zitation

Baiotti, L., Hawke, I., Rezzolla, L., & Schnetter, E. (2007). Details on the gravitational-wave emission from rotating gravitational collapse in 3D. Journal of Physics: Conference Series, 66(1): 012045. doi:10.1088/1742-6596/66/1/012045.


Zitierlink: http://hdl.handle.net/11858/00-001M-0000-0012-C3A3-1
Zusammenfassung
We here provide details on the numerical study of the gravitational-wave emission from the gravitational collapse to black holes of rotating neutron stars in three dimensions. More specifically, we concentrate on the use of mesh-refined grids, either fixed or progressive, as well as on the use of the excision techniques and of the advantages that result when this is not employed.