The sun as a detector of gravitational waves

Details The sun as a detector of gravitational waves The sun as a detector of gravitational waves

Mar 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984natur.308..165c&link_type=abstract

Nature (ISSN 0028-0836), vol. 308, March 8, 1984, p. 165, 166.

Physics

4

Gravitational Waves, Solar Oscillations, Damping, Radiation Absorption, Radiative Transfer

Scientific paper

The absorption rate of external gravitational radiation by the sun is shown to be orders of magnitude less than that required to overcome radiative damping by the core. The study was spurred by suggestions that the solar 160 min oscillation is caused by gravitational radiation emitted by the binary system Geminga. The damping rate due to reemission of the absorbed radiation is estimated by means of the quadrupole formula for the gravity wave luminosity. The absorption cross-section is calculated to be 0.4 percent of the solar cross-section, indicating that the oscillation cannot be caused by gravitational radiation from a nearby binary system.

Affiliated with

Also associated with

No associations

Rating

The sun as a detector of gravitational waves 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 The sun as a detector of gravitational waves, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The sun as a detector of gravitational waves will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1043317