Linear momentum flux from inspiralling compact binaries in quasielliptical orbits at 2.5 post-Newtonian order

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Linear momentum flux from inspiralling compact binaries in quasielliptical orbits at 2.5 post-Newtonian order. / Kastha, Shilpa.

I: Physical Review D, Bind 105, Nr. 6, 064039, 23.03.2022.

Publikation: Bidrag til tidsskrift › Tidsskriftartikel › Forskning › fagfællebedømt

Harvard

Kastha, S 2022, 'Linear momentum flux from inspiralling compact binaries in quasielliptical orbits at 2.5 post-Newtonian order', Physical Review D, bind 105, nr. 6, 064039. https://doi.org/10.1103/PhysRevD.105.064039

APA

Kastha, S. (2022). Linear momentum flux from inspiralling compact binaries in quasielliptical orbits at 2.5 post-Newtonian order. Physical Review D, 105(6), [064039]. https://doi.org/10.1103/PhysRevD.105.064039

Vancouver

Kastha S. Linear momentum flux from inspiralling compact binaries in quasielliptical orbits at 2.5 post-Newtonian order. Physical Review D. 2022 mar. 23;105(6). 064039. https://doi.org/10.1103/PhysRevD.105.064039

Author

Kastha, Shilpa. / Linear momentum flux from inspiralling compact binaries in quasielliptical orbits at 2.5 post-Newtonian order. I: Physical Review D. 2022 ; Bind 105, Nr. 6.

Bibtex

@article{74708e8ce2b1438b889e4514e3a409b1,
title = "Linear momentum flux from inspiralling compact binaries in quasielliptical orbits at 2.5 post-Newtonian order",
abstract = "Emission of anisotropic gravitational radiation from a compact binary system leads to a flux of linear momentum. This results in recoil of the system. We investigate the rate of loss of linear momentum flux in the far zone of the source using various mass type and current type multipole moments for an inspiralling compact binary merger in quasielliptical orbits at 2.5 post-Newtonian order. We compute the linear momentum flux accurately up to O(e(t)) in a harmonic coordinate. A 2.5 post-Newtonian quasi-Keplarian representation of the parametric solution to the post-Newtonian equation of motion for the compact binary system has been adopted here. We also provide a closed form expression for the accumulated linear momentum from the remote past through the binary evolution.",
keywords = "GRAVITATIONAL-RADIATION RECOIL, SUPERMASSIVE BLACK-HOLE, SYSTEMS, MOTION, GENERATION, DYNAMICS, WAVES",
author = "Shilpa Kastha",
year = "2022",
month = mar,
day = "23",
doi = "10.1103/PhysRevD.105.064039",
language = "English",
volume = "105",
journal = "Physical Review D",
issn = "2470-0010",
publisher = "American Physical Society",
number = "6",

}

RIS

TY - JOUR

T1 - Linear momentum flux from inspiralling compact binaries in quasielliptical orbits at 2.5 post-Newtonian order

AU - Kastha, Shilpa

PY - 2022/3/23

Y1 - 2022/3/23

N2 - Emission of anisotropic gravitational radiation from a compact binary system leads to a flux of linear momentum. This results in recoil of the system. We investigate the rate of loss of linear momentum flux in the far zone of the source using various mass type and current type multipole moments for an inspiralling compact binary merger in quasielliptical orbits at 2.5 post-Newtonian order. We compute the linear momentum flux accurately up to O(e(t)) in a harmonic coordinate. A 2.5 post-Newtonian quasi-Keplarian representation of the parametric solution to the post-Newtonian equation of motion for the compact binary system has been adopted here. We also provide a closed form expression for the accumulated linear momentum from the remote past through the binary evolution.

AB - Emission of anisotropic gravitational radiation from a compact binary system leads to a flux of linear momentum. This results in recoil of the system. We investigate the rate of loss of linear momentum flux in the far zone of the source using various mass type and current type multipole moments for an inspiralling compact binary merger in quasielliptical orbits at 2.5 post-Newtonian order. We compute the linear momentum flux accurately up to O(e(t)) in a harmonic coordinate. A 2.5 post-Newtonian quasi-Keplarian representation of the parametric solution to the post-Newtonian equation of motion for the compact binary system has been adopted here. We also provide a closed form expression for the accumulated linear momentum from the remote past through the binary evolution.

KW - GRAVITATIONAL-RADIATION RECOIL

KW - SUPERMASSIVE BLACK-HOLE

KW - SYSTEMS

KW - MOTION

KW - GENERATION

KW - DYNAMICS

KW - WAVES

U2 - 10.1103/PhysRevD.105.064039

DO - 10.1103/PhysRevD.105.064039

M3 - Journal article

VL - 105

JO - Physical Review D

JF - Physical Review D

SN - 2470-0010

IS - 6

M1 - 064039

ER -

ID: 334654806