Radiation-reaction in the effective field theory approach to post-Minkowskian dynamics
From MaRDI portal
Publication:2696871
DOI10.1007/JHEP01(2023)140OpenAlexW4318614159MaRDI QIDQ2696871
Rafael A. Porto, Jakob Neef, Gregor Kälin
Publication date: 17 April 2023
Published in: Journal of High Energy Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2207.00580
Related Items (11)
Scattering amplitudes and \(N\)-body post-Minkowskian Hamiltonians in general relativity and beyond ⋮ Spin Supplementary condition in quantum field theory: covariant SSC and physical state projection ⋮ Machine learning post-Minkowskian integrals ⋮ Classical observables from the exponential representation of the gravitational S-matrix ⋮ Bootstrapping the relativistic two-body problem ⋮ The relation between KMOC and worldline formalisms for classical gravity ⋮ Large gauge effects and the structure of amplitudes ⋮ Classical gravitational observables from the eikonal operator ⋮ The sub-leading scattering waveform from amplitudes ⋮ Poincaré invariance of spinning binary dynamics in the post-Minkowskian Hamiltonian approach ⋮ Orbital precession and hidden symmetries in scalar-tensor theories
Uses Software
Cites Work
- The effective field theorist's approach to gravitational dynamics
- Transforming differential equations of multi-loop Feynman integrals into canonical form
- Analytic tools for Feynman integrals
- Progress in effective field theory approach to the binary inspiral problem
- On-shell heavy particle effective theories
- Testing binary dynamics in gravity at the sixth post-Newtonian level
- How to choose master integrals
- Classical gravitational scattering from a gauge-invariant double copy
- Radiative classical gravitational observables at \(\mathcal{O} (G^3)\) from scattering amplitudes
- FIESTA4: optimized Feynman integral calculations with GPU support
- \texttt{epsilon}: a tool to find a canonical basis of master integrals
- The \(\varepsilon\)-form of the differential equations for Feynman integrals in the elliptic case
- The amplitude for classical gravitational scattering at third post-Minkowskian order
- The eikonal approach to gravitational scattering and radiation at \(\mathcal{O} (G^3)\)
- Classical black hole scattering from a worldline quantum field theory
- Radiated momentum in the post-Minkowskian worldline approach via reverse unitarity
- SUSY in the sky with gravitons
- From boundary data to bound states. III: Radiative effects
- The fifth-order post-Newtonian Hamiltonian dynamics of two-body systems from an effective field theory approach
- From boundary data to bound states
- From boundary data to bound states. II: Scattering angle to dynamical invariants (with twist)
- The fifth-order post-newtonian Hamiltonian dynamics of two-body systems from an effective field theory approach: potential contributions
- Radiation reaction from soft theorems
- The 6th post-Newtonian potential terms at \(O( G_N^4)\)
- Black hole binary dynamics from the double copy and effective theory
- Observables and amplitudes for spinning particles and black holes
- Scattering of spinning black holes from exponentiated soft factors
- Maximal cuts and differential equations for Feynman integrals. An application to the three-loop massive banana graph
- Classical space-times from the S-matrix
- Reducing differential equations for multiloop master integrals
- Extremal black hole scattering at \(\mathcal{O} (G^3)\): graviton dominance, eikonal exponentiation, and differential equations
- Classical gravitational self-energy from double copy
- Tidal effects in quantum field theory
- Dynamics of binary systems to fourth post-Minkowskian order from the effective field theory approach
- Scalar QED as a toy model for higher-order effects in classical gravitational scattering
- All things retarded: radiation-reaction in worldline quantum field theory
- FIRE6: Feynman integral reduction with modular arithmetic
- FIESTA5: numerical high-performance Feynman integral evaluation
- Mathematical Aspects of Scattering Amplitudes
- The tune of love and thenature(ness)of spacetime
- Next-to-leading-order spin–orbit effects in the motion of inspiralling compact binaries
- Brownian Motion of a Quantum Oscillator
- INTRODUCTORY LECTURES ON THE EFFECTIVE ONE BODY FORMALISM
- Iterated path integrals
- Volumes of hyperbolic manifolds and mixed Tate motives
- Laser interferometer space antenna dynamics and controls model
- The quadrupole moment of compact binaries to the fourth post-Newtonian order: I. Non-locality in time and infra-red divergencies
- The quadrupole moment of compact binaries to the fourth post-Newtonian order: II. Dimensional regularization and renormalization
- The mass quadrupole moment of compact binary systems at the fourth post-Newtonian order
- High-Order Post-Newtonian Contributions to Gravitational Self-force Effects in Black Hole Spacetimes
- Effective field theory methods to model compact binaries
- Singularities and Discontinuities of Feynman Amplitudes
- Gravitational radiation from post-Newtonian sources and inspiralling compact binaries
- Bootstrapping the relativistic two-body problem
- \texttt{Libra}: a package for transformation of differential systems for multiloop integrals
- DiffExp, a Mathematica package for computing Feynman integrals in terms of one-dimensional series expansions
This page was built for publication: Radiation-reaction in the effective field theory approach to post-Minkowskian dynamics
