Neutrinos from Supernovae as a Trigger for Gravitational Wave Search

Abstract

Exploiting an improved analysis of the electronic antineutrinos signal from the explosion of a galactic core collapse supernova, we show that it is possible to identify within about ten milliseconds the time of the bounce, which is strongly correlated to the time of the maximum amplitude of the gravitational signal. This allows to precisely identify the gravitational wave burst timing.

4 pages, 2 figures

References in corpus (5)

• Delayed neutrino-driven supernova explosions aided by the standing accretion-shock instability
• 3D Collapse of Rotating Stellar Iron Cores in General Relativity including Deleptonization and a Nuclear Equation of State
• Generic Gravitational Wave Signals from the Collapse of Rotating Stellar Cores
• Improved analysis of SN1987A antineutrino events
• Results of the IGEC-2 search for gravitational wave bursts during 2005

Cited by in corpus (10)

• Supernova Neutrino Detection
• The Progenitor Dependence of the Preexplosion Neutrino Emission in Core-Collapse Supernovae
• Reconstructing the supernova bounce time with neutrinos in IceCube
• Comparative analysis of SN1987A antineutrino fluence
• Implication for the core collapse supernova rate from 21 years of data of the Large Volume Detector
• Searching for prompt signatures of nearby core-collapse supernovae by a joint analysis of neutrino and gravitational-wave data
• Constraining Absolute Neutrino Masses via Detection of Galactic Supernova Neutrinos at JUNO
• The likelihood for supernova neutrino analyses
• Signatures of collective and matter effects on supernova neutrinos at large detectors
• What is the issue with SN1987A neutrinos?