The Road to Prediction: Toward Gravitational Wave Signatures from Core Collapse Supernovae

Details The Road to Prediction: Toward Gravitational Wave Signatures from Core Collapse Supernovae The Road to Prediction: Toward Gravitational Wave Signatures from Core Collapse Supernovae

Oct 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aipc..686...29m&link_type=abstract

THE ASTROPHYSICS OF GRAVITATIONAL WAVE SOURCES. AIP Conference Proceedings, Volume 686, pp. 29-39 (2003).

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Gravitational Radiation, Magnetic Fields, And Other Observations, Wave Generation And Sources, Supernovae

Scientific paper

Gravitational waves from a core collapse supernova will result from a number of phenomena that may occur during the explosion. An exciting prospect stems from the fact that waves from these different phenomena will occur at different amplitudes and frequencies, providing, with a successful detection and analysis, evidence of them and the opportunity to perform a detailed comparison of model predictions and gravitational wave observations. The latter would serve both to help us understand supernova phenomenology and to develop realistic three-dimensional supernova models. We present a brief ``state of supernova theory'' and discuss the outstanding research issues that must be addressed to both ascertain the core collapse supernova mechanism and predict core collapse supernova gravitational wave signatures.

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