Stochastic gravitational-wave background from stellar core-collapse events - INSPIRE

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Stochastic gravitational-wave background from stellar core-collapse events

Bella Finkel
(
- Skidmore Coll.
)
,
Haakon Andresen
(
- Stockholm U., OKC
)
,
Vuk Mandic
(
- Minnesota U.
)

Oct 4, 2021

10 pages

Published in:

Phys.Rev.D 105 (2022) 6, 063022

Published: Mar 15, 2022

e-Print:

2110.01478 [gr-qc]

DOI:

10.1103/PhysRevD.105.063022 (publication)

View in:

ADS Abstract Service

reference search20 citations

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Abstract: (APS)

We estimate the stochastic gravitational-wave background arising from all stellar core-collapse events in the universe based on the gravitational-wave signal predictions of recent numerical simulations. We focus on waveforms from slowly or nonrotating stars and include rapidly rotating, highly massive progenitors as extreme case limits. Our most realistic estimates are more than one hundred times below the sensitivity of third-generation terrestrial gravitational-wave detectors and likely weaker than cosmological contributions to the stochastic gravitational-wave background.

Note:

10 pages, 3 figures

gravitational radiation: background
gravitational radiation: stochastic
family: 3
gravitational radiation detector
numerical calculations
sensitivity
star: collapse
rotation
wave function

References(89)

Figures(3)

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