Journal
PHYSICAL REVIEW D
Volume 92, Issue 6, Pages -Publisher
AMER PHYSICAL SOC
DOI: 10.1103/PhysRevD.92.063005
Keywords
-
Funding
- DOE at the University of Minnesota [DE-SC0011842]
- NSF at the University of Minnesota [PHY-1204944]
- NCN [Sonata Bis 2 (DEC-2012/07/E/ST9/01360)]
- Polish Science Foundation (FNP)
- French state funds [ANR-10-LABX-63]
- ANR within the Investissements dAvenir programme [ANR-11-IDEX-0004-02]
- French Agence Nationale pour la Recherche (ANR) via the grant VACOUL [ANR-2010-Blan-0510-01]
- Direct For Mathematical & Physical Scien
- Division Of Physics [1505870] Funding Source: National Science Foundation
Ask authors/readers for more resources
Superposition of gravitational waves generated by astrophysical sources is expected to give rise to the stochastic gravitational-wave background. We focus on the background generated by the ring-down of black holes produced in the stellar core collapse events, which is one of several mechanisms for gravitational wave production in the stellar core collapse process. We systematically study the parameter space in this model, including the most recent information about the star formation rate and about the population of black holes as a function of redshift and of metallicity. We find that the upcoming second and third generation gravitational-wave detectors will be able to observe this stochastic background if the black hole ring-down efficiency at producing gravitational waves is sufficiently high, namely similar to 10(-4) and similar to 10(-6) of the black hole rest energy, respectively.
Authors
I am an author on this paper
Click your name to claim this paper and add it to your profile.
Reviews
Recommended
No Data Available