Multiple physical elements to determine the gravitational-wave signatures of core-collapse supernovae

Kei Kotake

doi:10.1016/j.crhy.2013.01.008

Multiple physical elements to determine the gravitational-wave signatures of core-collapse supernovae
[Éléments physiques multiples déterminant les signatures des ondes gravitationnelles de supernovas à effondrement de cœur]

Kei Kotake ^1,²

¹ Division of Theoretical Astronomy, National Astronomical Observatory of Japan, 2-21-1, Osawa, Mitaka, Tokyo 181-8588, Japan
² Center for Computational Astrophysics, National Astronomical Observatory of Japan, Mitaka, Tokyo 181-8588, Japan

Comptes Rendus. Physique, Gravitational waves / Ondes gravitationnelles, Volume 14 (2013) no. 4, pp. 318-351.

Résumé
Abstract

Nous passons en revue les progrès récents en matière de prédiction théorique dʼémission dʼondes gravitationnelles par les supernovae gravitationnelles. Après un bref survol des méthodes numériques, nous récapitulons les éléments physiques qui déterminent les signatures en ondes gravitationnelles considérées comme essentielles pour extraire les informations encore cachées à lʼobservation du mécanisme dʼexplosion de supernova. Nous concluons par un résumé des tâches urgents à accomplir pour que ce rêve devienne réalité.

We review recent progress in the theoretical predictions of gravitational waves (GWs) of core-collapse supernovae. Following a brief summary of the methods in the numerical modeling, we summarize multiple physical elements that determine the GW signatures which have been considered to be important in extracting the information of the long-veiled explosion mechanism from the observation of the GWs. We conclude with a summary of the most urgent tasks to make the dream come true.

Publié le : 2013-02-14

DOI : 10.1016/j.crhy.2013.01.008

Keywords: Supernovae, Radiation-hydrodynamics, Gravitational wave physics, Neutrino physics
Mots-clés : Supernovas, Hydrodynamique radiative, Physique des ondes gravitationnelles, Physique des neutrinos

Affiliations des auteurs :

Kei Kotake ^{1, 2}

¹ Division of Theoretical Astronomy, National Astronomical Observatory of Japan, 2-21-1, Osawa, Mitaka, Tokyo 181-8588, Japan
² Center for Computational Astrophysics, National Astronomical Observatory of Japan, Mitaka, Tokyo 181-8588, Japan

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Kei Kotake. Multiple physical elements to determine the gravitational-wave signatures of core-collapse supernovae. Comptes Rendus. Physique, Gravitational waves / Ondes gravitationnelles, Volume 14 (2013) no. 4, pp. 318-351. doi : 10.1016/j.crhy.2013.01.008. https://comptes-rendus.academie-sciences.fr/physique/articles/10.1016/j.crhy.2013.01.008/

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