Radiating Love: adiabatic tidal fluxes and modes up to next-to-next-to-leading post-Newtonian order

A bstract We present the analytical evaluation of the gravitational energy and angular momentum flux with tidal effects for inspiraling compact binaries, at the next-to-next-to-leading post-Newtonian (2PN) order, within the diagrammatic Effective Field Theory approach. We first compute the stress-energy tensor for a binary system, which requires the evaluation of two-point Feynman integrals, up to two loops. Then we extract the multipole moments of the system, which we present for generic orbits in center-of-mass coordinates, and which are needed to evaluate the total gravitational energy and the angular momentum flux for generic orbits. Finally, we provide the expressions for gauge invariant quantities for circular orbits, such as the fluxes, mode amplitudes, and phase of the emitted gravitational wave. Our results are useful for updating previous theoretical studies, as well as related phenomenological analyses and waveform models.

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Publication Details

Journal
Journal of High Energy Physics
Published
2025-05-02
DOI
https://doi.org/10.1007/jhep05(2025)008
Citations
6
Primary Topic
Pulsars and Gravitational Waves Research
Type
article
Field-Weighted Citation Impact
6.93

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article

Radiating Love: adiabatic tidal fluxes and modes up to next-to-next-to-leading post-Newtonian order

Manoj K. Mandal, Raj Patil, Jan Steinhoff, Pierpaolo Mastrolia
6 citations
Journal of High Energy Physics
Pulsars and Gravitational Waves Research
6.93
article

Radiating Love: adiabatic tidal fluxes and modes up to next-to-next-to-leading post-Newtonian order

Manoj K. Mandal, Raj Patil, Jan Steinhoff, Pierpaolo Mastrolia
article en
6 citations

Abstract

A bstract We present the analytical evaluation of the gravitational energy and angular momentum flux with tidal effects for inspiraling compact binaries, at the next-to-next-to-leading post-Newtonian (2PN) order, within the diagrammatic Effective Field Theory approach. We first compute the stress-energy tensor for a binary system, which requires the evaluation of two-point Feynman integrals, up to two loops. Then we extract the multipole moments of the system, which we present for generic orbits in center-of-mass coordinates, and which are needed to evaluate the total gravitational energy and the angular momentum flux for generic orbits. Finally, we provide the expressions for gauge invariant quantities for circular orbits, such as the fluxes, mode amplitudes, and phase of the emitted gravitational wave. Our results are useful for updating previous theoretical studies, as well as related phenomenological analyses and waveform models.

Journal of High Energy PhysicsVol. 2025(5)
University of Padua (IT), Humboldt-Universität zu Berlin (DE), Istituto Nazionale di Fisica Nucleare, Sezione di Padova (IT), Max Planck Institute for Gravitational Physics (DE)
Deutsche Forschungsgemeinschaft
Openalex Percentile: Top 3%
Pulsars and Gravitational Waves Research
6.93
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