Analytic approximations, perturbation theory, effective field theory methods and their applications
DOI10.1007/s10714-014-1682-6zbMath1291.83004arXiv1401.2193OpenAlexW2070156745MaRDI QIDQ2247800
No author found.
Publication date: 30 June 2014
Published in: General Relativity and Gravitation (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1401.2193
Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Research exposition (monographs, survey articles) pertaining to relativity and gravitational theory (83-02) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Exact solutions to problems in general relativity and gravitational theory (83C15) Approximation procedures, weak fields in general relativity and gravitational theory (83C25)
Related Items (3)
Cites Work
- Unnamed Item
- Unnamed Item
- Black hole stereotyping: induced gravito-static polarization
- Classical space-times from the S-matrix
- Next-to-next-to-leading order spin–orbit effects in the gravitational wave flux and orbital phasing of compact binaries
- Next-to-next-to-leading order post-Newtonian spin(1)-spin(2) Hamiltonian for self-gravitating binaries
- Radiation reaction at the level of the action
- High-Accuracy Comparison Between the Post-Newtonian and Self-Force Dynamics of Black-Hole Binaries
- Next-to-leading-order spin–orbit effects in the motion of inspiralling compact binaries
- Relativistic Closed-Form Hamiltonian for Many-Body Gravitating Systems in the Post-Minkowskian Approximation
- High-accuracy gravitational waveforms for binary black hole mergers with nearly extremal spins
- The reduced Hamiltonian for next-to-leading-order spin-squared dynamics of general compact binaries
- Tensor-multi-scalar theories of gravitation
- Exact Solutions of Einstein's Field Equations
- Next-to-next-to-leading order spin–orbit effects in the equations of motion of compact binary systems
- Compact binary coalescence parameter estimations for 2.5 post-Newtonian aligned spinning waveforms
- Next‐to‐next‐to‐leading order post‐Newtonian linear‐in‐spin binary Hamiltonians
- Next-to-leading tail-induced spin–orbit effects in the gravitational radiation flux of compact binaries
- Time-domain inspiral templates for spinning compact binaries in quasi-circular orbits described by their orbital angular momenta
- Effective field theory methods to model compact binaries
- Gravitational radiation from post-Newtonian sources and inspiralling compact binaries
This page was built for publication: Analytic approximations, perturbation theory, effective field theory methods and their applications
