Limits on a stochastic gravitational wave background from observations of terrestrial and solar oscillations

Mathematics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

3

Background Radiation, Earth Movements, Gravitational Waves, Solar Oscillations, Vibration Mode, Astronomical Models, Limits (Mathematics), Relativity, Space Density, Stochastic Processes

Scientific paper

Realistic models of the Earth and Sun are used to calculate their respective responses to a homogeneous, isotropic background of gravitational radiation. Solar velocity data constrain the energy density of such a background at a frequency of 4 x 10-4 Hz to be less than 102, times the closure density of the universe, as does Earth seismic data at frequencies of 2 x 10-3 Hz and 2 x 10-2 Hz. With improved data soon to be available it is likely that both of these limits will be lowered to below closure density. Errors in previous analyses of the Earth are pointed out.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Limits on a stochastic gravitational wave background from observations of terrestrial and solar oscillations 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 Limits on a stochastic gravitational wave background from observations of terrestrial and solar oscillations, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Limits on a stochastic gravitational wave background from observations of terrestrial and solar oscillations will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1751501

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.