Physics
Scientific paper
Sep 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008mgm..conf.1728y&link_type=abstract
"THE ELEVENTH MARCEL GROSSMANN MEETING On Recent Developments in Theoretical and Experimental General Relativity, Gravitation an
Physics
Scientific paper
The distance-redshift relation via gravitational waves in the clumpy universe is simulated numerically by taking account of the effects of gravitational lensing. It is assumed that all of the matter in the universe takes the form of randomly distributed point masses, each of which has the identical mass ML. Calculations are carried out in the two extreme cases: λ ≫ GML/c2 and λ ≪ GML/c2, where λ denotes the wavelength of gravitational waves. In the former, the distance-redshift relation for the fully homogeneous and isotropic universe is reproduced with small distance dispersion, whereas, in the latter, the distance dispersion is larger. This result suggests that we might obtain the information about the typical mass of lens objects through the distance-redshift relation gleaned through observation of gravitational waves of various wavelengths.
Kozaki Hiroshi
nakao Ken-ichi
Takahashi Ryuichi
Yoo Chul-Moon
No associations
LandOfFree
Lensing Effects on Gravitational Waves in a Clumpy 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 Lensing Effects on Gravitational Waves in a Clumpy Universe, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Lensing Effects on Gravitational Waves in a Clumpy Universe will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1337973