Probing the central engine of long gamma-ray bursts and hypernovae with gravitational waves and neutrinos

Abstract

There are the two common candidates as the viable energy source for the central engine of long gamma-ray bursts (GRBs) and hypernovae (HNe), neutrino annihilation and magnetic fields. We investigate gravitational wave (GW) emission accompanied by these two mechanisms. Especially, we focus on GW signals produced by neutrinos from a hyper-accreting disk around a massive black hole. We show that neutrino-induced GWs are detectable for $\sim$1 Mpc events by LISA and $\sim$ 100 Mpc by DECIGO/BBO, if the central engine is powered by neutrinos. The GW signals depend on the viewing angle and they are anti-correlated with neutrino ones. But, simultaneous neutrino detections are also expected, and helpful for diagnosing the explosion mechanism when later electromagnetic observations enable us to identify the source. GW and neutrino observations are potentially useful for probing choked jets that do not produce prompt emission, as well as successful jets. Even in non-detection cases, observations of GWs and neutrinos could lead to profitable implications for the central engine of GRBs and HNe.

14 pages, 9 figures, version to appear in PRD (with minor changes)

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• High-Energy Multi-Messenger Transient Astrophysics
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• Neutrino Pair Annihilation in Collapsars; Ray-Tracing Method in Special Relativity
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• Anisotropic multimessenger signals from black hole neutrino-dominated accretion flows with outflows in binary compact object mergers
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• Gravitational Waves from the Propagation of Long Gamma-Ray Burst jets
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• Neutrino Acceleration by Bulk Matter Motion and Explosion Mechanism of Gamma-Ray Bursts
• Gravitational memory signal from neutrino self-interactions in supernova
• Neutrinos and gravitational waves from magnetized neutrino-dominated accretion discs with magnetic coupling
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• Collapsar Disk Outflows III: Detectable Neutrino and Gravitational Wave Signatures
• Gravitational Wave Memory from Accelerating Relativistic Jets in Multiple Thick Shell Scenarios