Effective field theory calculation of conservative binary dynamics at third post-Newtonian order

Details Effective field theory calculation of conservative binary dynamics at third post-Newtonian order Effective field theory calculation of conservative binary dynamics at third post-Newtonian order

2011-04-06

arxiv.org/abs/1104.1122v3

Phys.Rev.D84:044031,2011

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

24 pages, 6 figures. Typos corrected and references added in v2. Typos corrected in v3

Scientific paper

10.1103/PhysRevD.84.044031

We reproduce the two-body gravitational conservative dynamics at third post-Newtonian order for spin-less sources by using the effective field theory methods for the gravitationally bound two-body system, proposed by Goldberger and Rothstein. This result has been obtained by automatizing the computation of Feynman amplitudes within a Mathematica algorithm, paving the way for higher-order computations not yet performed by traditional methods.

Affiliated with

Also associated with

No associations

Rating

Effective field theory calculation of conservative binary dynamics at third post-Newtonian order 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 Effective field theory calculation of conservative binary dynamics at third post-Newtonian order, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Effective field theory calculation of conservative binary dynamics at third post-Newtonian order will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-418206