GWs from Supermassive Black Holes

Details GWs from Supermassive Black Holes GWs from Supermassive Black Holes

Dec 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998tx19.confe.473d&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

Based on recent determinations of mass function of Supermassive Black Holes (SMBH, with masses raging from 10^6-1010 M_odot), which are thought to be present in galaxies, we study the generation of gravitational waves (GWs) that could be produced during their formation. In particular, we discuss if the LISA antenna could detect the GWs produced during the formation of such SMBHs and provides clues to define their formation history. For example, whether the gravitational radiation observations could impose limits on the mass with which the SMBHs were formed, indicating the possibility that most of their present mass being a result of mass accretion or not.

Affiliated with

Also associated with

No associations

Rating

GWs from Supermassive Black Holes 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 Supermassive Black Holes, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and GWs from Supermassive Black Holes will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-769634