GWs from BHs in an Explosive Scenario of Structure Formation of the Universe

Details GWs from BHs in an Explosive Scenario of Structure Formation of the Universe GWs from BHs in an Explosive Scenario of Structure Formation of the Universe

Dec 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998tx19.confe.474m&link_type=abstract

Abstracts of the 19th Texas Symposium on Relativistic Astrophysics and Cosmology, held in Paris, France, Dec. 14-18, 1998. Eds.:

Astronomy and Astrophysics

Astrophysics

Scientific paper

We study the generation of a stochastic background of gravitational waves (GWs) produced from a cosmological Population of core-collapse supernovae in an explosive scenario for the formation of the large-scale structures of the Universe. In this scenario the generation of a dense and turbulent shell of matter at high redshift quickly produces a Population of pre-galactic objects, which could form stellar black holes. We show that this scenario produces GWs that could be detectable by both laser interferometer and resonant mass detectors. Our results show that both, frequency and signal amplitude are dependent on the redshift when the explosive cycles occurred.

Affiliated with

Also associated with

No associations

Rating

GWs from BHs in an Explosive Scenario of Structure Formation of the Universe does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with GWs from BHs in an Explosive Scenario of Structure Formation of the Universe, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and GWs from BHs in an Explosive Scenario of Structure Formation of the Universe will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-769637