Spin-spin interaction in the spin-precession equations

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

3

Post-Newtonian Approximation, Perturbation Theory, Related Approximations, Wave Generation And Sources, Binary And Multiple Stars

Scientific paper

One of the most active field of research in general relativity is the description of the spin properties of astrophysical objects. The main tool in the description of the gravitational waves emitted by compact binary systems in the inspiral era is the post-Newtonian (PN) approximation, where spin effects, namely, spin-orbit and spin-spin interactions, become important in higher orders. These interactions are described with coupled differential equations in general, but the PN approximation scheme gives the opportunity to solve them order by order. In the present work the effects of the spin-orbit and spin-spin interactions are described in the spin-precession equations with the use of the PN approximation up to 1.5 PN order. The decoupled angular equations describing the evolution of the direction of the spin vectors are given, and they are solved both in the eccentric and circular orbit cases. Since the spin-precession equations do not have a Newtonian contribution it is nontrivial to determine the relative order of the different variables. This analysis is also included up to the order of the spin-spin interaction.

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

Spin-spin interaction in the spin-precession equations 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 Spin-spin interaction in the spin-precession equations, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Spin-spin interaction in the spin-precession equations will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1724181

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