Gravitational Waves from Neutrino Emission Asymmetries in Core-collapse Supernovae

Vartanyan, David; Burrows, Adam

doi:10.3847/1538-4357/abafac

Gravitational Waves from Neutrino Emission Asymmetries in Core-collapse Supernovae

Journal Article · Mon Sep 28 00:00:00 EDT 2020 · The Astrophysical Journal (Online)

DOI:https://doi.org/10.3847/1538-4357/abafac· OSTI ID:1852587

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Univ. of California (United States). Department of Physics and Astronomy; OSTI
Princeton Univ., NJ (United States). Department of Astrophysical Sciences

We present a broadband spectrum of gravitational waves (GWs) from core-collapse supernovae (CCSNe) sourced by neutrino emission asymmetries for a series of full 3D simulations. The associated GW strain probes the long-term secular evolution of CCSNe and small-scale turbulent activity and provides insight into the geometry of the explosion. For nonexploding models, both the neutrino luminosity and the neutrino gravitational waveform will encode information about the spiral SASI. The neutrino memory will be detectable for a wide range of progenitor masses for a galactic event. Our results can be used to guide near-future decihertz and long-baseline GW detection programs, including aLIGO, the Einstein Telescope, and DECIGO.

View Accepted Manuscript (DOE)

Research Organization:: Argonne National Lab. (ANL), Argonne, IL (United States); Univ. of California, Oakland, CA (United States); Univ. of California, San Diego, CA (United States)

Sponsoring Organization:: USDOE Office of Science (SC)

Grant/Contract Number:: AC02-06CH11357; AC03-76SF00098; SC0018297

OSTI ID:: 1852587

Alternate ID(s):: OSTI ID: 23031359

Journal Information:: The Astrophysical Journal (Online), Journal Name: The Astrophysical Journal (Online) Journal Issue: 2 Vol. 901; ISSN 1538-4357

Publisher:: IOP PublishingCopyright Statement

Country of Publication:: United States

Language:: English

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