Worldline effective field theory of inspiralling black hole binaries in presence of dark photon and axionic dark matter

Abstract

We investigate the correction to the potential that gives rise to the bound orbits and radiation from non-spinning inspiralling binary black holes in a dark matter environment consisting of axion-like particles and dark photons using the techniques of Worldline Effective Field Theory. We compute the conservative dynamics up to $1$PN order for gravitational, electromagnetic, and Proca fields and up to $2$PN order for the scalar field. The effect of axion-electromagnetic coupling ($g_{a\gamma \gamma }$) arises to the conservative dynamics at $2.5$PN order and the kinetic mixing constant ($\gamma$) at $1$PN order. Furthermore, we calculate the radiation due to the various fields present in our theory. We find that the contribution of $g_{a\gamma \gamma }$ to the gravitational radiation appears at $N^{(7)}LO$ and to the scalar radiation appears at $N^{(5)}LO$. We also find that these radiative corrections due to the coupling $g_{a\gamma \gamma }$ vanishes for any orbit confined to a plane because of the existence of a binormal like term in effective radiative action but give rise to non-zero contributions for any orbit that lies in three dimensions. Last but not the least, $\gamma$ contributes to the gravitational radiation at $N^{(2)}LO$ and $N^{(4)}LO$.

arXiv comment89 pages, 19 figures, 4 tables, appendix updated, minor typos fixed, results remain unchanged

References in corpus (113)

• A direct empirical proof of the existence of dark matter
• WISPy Cold Dark Matter
• The QCD axion, precisely
• An Effective Field Theory of Gravity for Extended Objects
• A Search for Invisible Axion Dark Matter with the Axion Dark Matter Experiment
• Amplitudes, Observables, and Classical Scattering
• The Effective Field Theorist's Approach to Gravitational Dynamics
• The Strong CP Problem and Axions
• Gravitational radiation from inspiralling compact binaries completed at the third post-Newtonian order
• Spin effects in the inspiral of coalescing compact binaries
• The QCD Axion and Moduli Stabilisation
• Higher-order spin effects in the dynamics of compact binaries I. Equations of motion
• Higher-order spin effects in the dynamics of compact binaries II. Radiation field
• Effective Field Theories of Post-Newtonian Gravity: A comprehensive review
• Classical black hole scattering from a worldline quantum field theory
• Constraining the mass of dark photons and axion-like particles through black-hole superradiance
• Next to Leading Order Spin(1)Spin(1) Effects in the Motion of Inspiralling Compact Binaries
• Gravitational radiative corrections from effective field theory
• Classical Gravitational Bremsstrahlung from a Worldline Quantum Field Theory
• Strong CP problem and mirror world: the Weinberg Wilczek axion revisited
• Parameter estimation of inspiralling compact binaries using 3.5 post-Newtonian gravitational wave phasing: The non-spinning case
• Spin(1)Spin(2) Effects in the Motion of Inspiralling Compact Binaries at Third Order in the Post-Newtonian Expansion
• Dissipative Effects in the Worldline Approach to Black Hole Dynamics
• Dynamics of Binary Systems to Fourth Post-Minkowskian Order from the Effective Field Theory Approach
• Conservative Dynamics of Binary Systems at Fourth Post-Minkowskian Order in the Large-eccentricity Expansion
• Radiation Reaction and Gravitational Waves at Fourth Post-Minkowskian Order
• Gravitational field and equations of motion of spinning compact binaries to 2.5 post-Newtonian order
• Equivalence between the ADM-Hamiltonian and the harmonic-coordinates approaches to the third post-Newtonian dynamics of compact binaries
• Conservative dynamics of binary systems to fourth Post-Newtonian order in the EFT approach II: Renormalized Lagrangian
• Gravitational Bremsstrahlung and Hidden Supersymmetry of Spinning Bodies
• Factoring the Strong CP Problem
• The tail effect in gravitational radiation-reaction: time non-locality and renormalization group evolution
• The third and a half post-Newtonian gravitational wave quadrupole mode for quasi-circular inspiralling compact binaries
• A Model of Visible QCD Axion
• New derivation of a third post-Newtonian equation of motion for relativistic compact binaries without ambiguity
• Improved estimation of radiated axions from cosmological axionic strings
• Dark energy from the string axiverse
• Numerical Relativity and Astrophysics
• Spinning particles, axion radiation, and the classical double copy
• Topological Susceptibility and QCD Axion Mass: QED and NNLO corrections
• Binary dynamics from spin1-spin2 coupling at fourth post-Newtonian order
• Spin-squared Hamiltonian of next-to-leading order gravitational interaction
• The next-to-leading order gravitational spin(1)-spin(2) dynamics in Hamiltonian form
• Non-Relativistic Gravitation: From Newton to Einstein and Back
• Measuring the dark matter environments of black hole binaries with gravitational waves
• The Subhalo Mass Function and Ultralight Bosonic Dark Matter
• Spin induced multipole moments for the gravitational wave amplitude from binary inspirals to 2.5 Post-Newtonian order
• A Visible QCD Axion from an Enlarged Color Group
• Radiation-Reaction in the Effective Field Theory Approach to Post-Minkowskian Dynamics
• An even lighter QCD axion
• The Effect of Orbital Eccentricity on Gravitational Wave Background Radiation from Supermassive Black Hole Binaries
• Spin induced multipole moments for the gravitational wave flux from binary inspirals to third Post-Newtonian order
• Next-to-next-to-leading order gravitational spin-squared potential via the effective field theory for spinning objects in the post-Newtonian scheme
• Equivalence of ADM Hamiltonian and Effective Field Theory approaches at next-to-next-to-leading order spin1-spin2 coupling of binary inspirals
• Post-Newtonian dynamics and black hole thermodynamics in Einstein-scalar-Gauss-Bonnet gravity
• Conservative and radiative dynamics of spinning bodies at third post-Minkowskian order using worldline quantum field theory
• Post-Newtonian Gravitational and Scalar Waves in Scalar-Gauss-Bonnet Gravity
• Hadamard regularization of the third post-Newtonian gravitational wave generation of two point masses
• Multipole expansion at the level of the action
• On the Apparent Ambiguities in the Post-Newtonian Expansion for Binary Systems
• Dynamic Signatures of Black Hole Binaries with Superradiant Clouds
• Prospects for axion searches with Advanced LIGO through binary mergers
• Non-conservative effects on Spinning Black Holes from World-Line Effective Field Theory
• Scalar One-Loop Integrals using the Negative-Dimension Approach
• Higher-order-in-spin interaction Hamiltonians for binary black holes from Poincaré invariance
• Audible Axions
• Eccentricity evolution of compact binaries and applications to gravitational-wave physics
• Next-to-next-to-leading order gravitational spin-orbit coupling via the effective field theory for spinning objects in the post-Newtonian scheme
• Gravitational wave probes of axion-like particles
• Gravitational radiation from inspiralling compact objects: Spin effects to fourth Post-Newtonian order
• Towers of Gravitational Theories
• Non-linear multipole interactions and gravitational-wave octupole modes for inspiralling compact binaries to third-and-a-half post-Newtonian order
• The gravitational-wave memory from eccentric binaries
• Reduced Hamiltonian for next-to-leading order Spin-Squared Dynamics of General Compact Binaries
• First Constraints on Nuclear Coupling of Axionlike Particles from the Binary Neutron Star Gravitational Wave Event GW170817
• Constraints on Very Light Axions from Cavity Experiments
• Gravitational radiation from compact binary systems in screened modified gravity
• Radiation reaction for spinning bodies in effective field theory II: Spin-spin effects
• Radiation reaction for spinning bodies in effective field theory I: Spin-orbit effects
• Circularization vs. Eccentrification in Intermediate Mass Ratio Inspirals inside Dark Matter Spikes
• Spherical harmonic modes of 5.5 post-Newtonian gravitational wave polarizations and associated factorized resummed waveforms for a particle in circular orbit around a Schwarzschild black hol
• Black hole mass dynamics and renormalization group evolution
• Gravitational-wave amplitudes for compact binaries in eccentric orbits at the third post-Newtonian order: Tail contributions and post-adiabatic corrections
• Scalar Gravitational Radiation from Binaries: Vainshtein Mechanism in Time-dependent Systems
• Exploring the string axiverse and parity violation in gravity with gravitational waves
• Dark matter minispike: a significant enhancement of eccentricity for intermediate-mass-ratio-inspirals
• Effective field theory for gravitational radiation in scalar-tensor gravity
• New Solutions to the Strong CP Problem
• Gravitational Spin-Orbit Hamiltonian at NNNLO in the post-Newtonian framework
• Gravitational and electromagnetic radiation from binary black holes with electric and magnetic charges: Elliptical orbits on a cone
• Gravitational Quadratic-in-Spin Hamiltonian at NNNLO in the post-Newtonian framework
• Gravitational and electromagnetic radiation from binary black holes with electric and magnetic charges: Hyperbolic orbits on a cone
• Gravitational wave forms, polarizations, response functions and energy losses of triple systems in Einstein-Aether theory
• The Quadrupole Moment of Compact Binaries to the Fourth post-Newtonian Order: II. Dimensional Regularization and Renormalization
• Audible Axions with a Booster: Stochastic Gravitational Waves from Rotating ALPs
• Constraining properties of asymmetric dark matter candidates from gravitational-wave observations
• Axion dark matter search using arm cavity transmitted beams of gravitational wave detectors
• QCD Axion Dark Matter from a Late Time Phase Transition
• Axion Induced Oscillating Electric Dipole Moment of the Electron
• Angular momentum loss for eccentric compact binary in screened modified gravity
• Composite neutrinos and the QCD axion: baryogenesis, dark matter, small Dirac neutrino masses, and vanishing neutron EDM
• Study of eccentric binaries in Horndeski theory
• Horndeski gravity without screening in binary pulsars
• New results at 3PN via an effective field theory of gravity
• Energy extraction from AdS black holes via superradiance
• Eccentric-orbit EMRI radiation: Analytic forms of leading-logarithm and subleading-logarithm flux terms at high PN orders
• Small instantons and the strong CP problem in composite Higgs models
• Ultralight dark photon as a model for early universe dark matter
• On dual formulation of Axion solution to strong-CP problem
• On the Detection of QCD Axion Dark Matter by Coherent Scattering
• EFT approach to general relativity: correction to EIH Lagrangian due to electromagnetic charge
• Probing dark matter with polarimetry techniques
• Angular Momentum Loss for a Binary System in Einstein-Æther Theory

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• Probing dark matter halo profiles with multi-band observations of gravitational waves
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• Love beyond Einstein: Metric reconstruction and Love number in quadratic gravity using WEFT
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