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Gravitational radiation in infinite derivative gravity and connections to effective quantum gravity

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Gravitational radiation in infinite derivative gravity and connections to effective quantum gravity. / Edholm, James.
In: Physical Review D, Vol. 98, No. 4, 044049, 28.08.2018.

Research output: Contribution to Journal/MagazineJournal articlepeer-review

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Edholm J. Gravitational radiation in infinite derivative gravity and connections to effective quantum gravity. Physical Review D. 2018 Aug 28;98(4):044049. doi: 10.1103/PhysRevD.98.044049

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Bibtex

@article{14d5ce7caea847ceade5f2837d127029,
title = "Gravitational radiation in infinite derivative gravity and connections to effective quantum gravity",
abstract = "The Hulse-Taylor binary provides possibly the best test of GR to date. We find the modified quadrupole formula for infinite derivative gravity (IDG). We investigate the backreaction formula for propagation of gravitational waves, found previously for effective quantum gravity (EQG) for a flat background and extend this calculation to a de Sitter background for both EQG and IDG. We put tighter constraints on EQG using new LIGO data. We also find the power emitted by a binary system within the IDG framework for both circular and elliptical orbits and use the example of the Hulse-Taylor binary to show that IDG is consistent with GR.",
author = "James Edholm",
note = "{\textcopyright} 2018 American Physical Society",
year = "2018",
month = aug,
day = "28",
doi = "10.1103/PhysRevD.98.044049",
language = "English",
volume = "98",
journal = "Physical Review D",
issn = "1550-7998",
publisher = "American Physical Society",
number = "4",

}

RIS

TY - JOUR

T1 - Gravitational radiation in infinite derivative gravity and connections to effective quantum gravity

AU - Edholm, James

N1 - © 2018 American Physical Society

PY - 2018/8/28

Y1 - 2018/8/28

N2 - The Hulse-Taylor binary provides possibly the best test of GR to date. We find the modified quadrupole formula for infinite derivative gravity (IDG). We investigate the backreaction formula for propagation of gravitational waves, found previously for effective quantum gravity (EQG) for a flat background and extend this calculation to a de Sitter background for both EQG and IDG. We put tighter constraints on EQG using new LIGO data. We also find the power emitted by a binary system within the IDG framework for both circular and elliptical orbits and use the example of the Hulse-Taylor binary to show that IDG is consistent with GR.

AB - The Hulse-Taylor binary provides possibly the best test of GR to date. We find the modified quadrupole formula for infinite derivative gravity (IDG). We investigate the backreaction formula for propagation of gravitational waves, found previously for effective quantum gravity (EQG) for a flat background and extend this calculation to a de Sitter background for both EQG and IDG. We put tighter constraints on EQG using new LIGO data. We also find the power emitted by a binary system within the IDG framework for both circular and elliptical orbits and use the example of the Hulse-Taylor binary to show that IDG is consistent with GR.

U2 - 10.1103/PhysRevD.98.044049

DO - 10.1103/PhysRevD.98.044049

M3 - Journal article

VL - 98

JO - Physical Review D

JF - Physical Review D

SN - 1550-7998

IS - 4

M1 - 044049

ER -