New formula for gravitational-radiation energy loss in general relativity

Physics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

14

Energy Dissipation, Gravitational Waves, Relativity, Two Body Problem, Binary Stars, Equations Of State, Gravitational Wave Antennas, Pulsars

Scientific paper

Field contributions and Gauss's theorem for retarded functions lead to a new formula for gravitational-radiation energy loss. It clarifies the applicability of the quadrupole formula for systems with T super ik-dominated motion. Applied to the axially symmetric two-body problem with equation of state epsion = epsilon (e) for short free-fall times, the new formula yields the bulk-motion quadrupole-formula results. This contrasts an earlier larger flux with unconventional equation of state and that of critics claming a quadrupole-formula flux from internal motions. An order-of-magnitude estimate yields potential corrections of quadrupole-formula size after about 100 yr for the binary pulsar.

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

New formula for gravitational-radiation energy loss in general relativity 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 New formula for gravitational-radiation energy loss in general relativity, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and New formula for gravitational-radiation energy loss in general relativity will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1233291

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