Rotational instabilities in post-collapse stellar cores

Details Rotational instabilities in post-collapse stellar cores Rotational instabilities in post-collapse stellar cores

Jun 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aipc..575..234d&link_type=abstract

ASTROPHYSICAL SOURCES FOR GROUND-BASED GRAVITATIONAL WAVE DETECTORS. AIP Conference Proceedings, Volume 575, pp. 234-245 (2001)

Astronomy and Astrophysics

Astrophysics

Supernovae, Relativity And Gravitation, Wave Generation And Sources

Scientific paper

A core-collapse supernova might produce large amplitude gravitational waves if, through the collapse process, the inner core can aquire enough rotational energy to become dynamically unstable. In this report I present the results of 3-D numerical simulations of core collapse supernovae. These simulations indicate that for some initial conditions the post-collapse inner core is indeed unstable. However, for the cases considered, the instability does not produce a large gravitational-wave signal. .

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