Characterization of echoes: A Dyson-series representation of individual pulses

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Characterization of echoes : A Dyson-series representation of individual pulses. / Correia, Miguel R.; Cardoso, Vitor.

In: Physical Review D, Vol. 97, No. 8, 084030, 17.04.2018.

Research output: Contribution to journalJournal articleResearchpeer-review

Harvard

Correia, MR & Cardoso, V 2018, 'Characterization of echoes: A Dyson-series representation of individual pulses', Physical Review D, vol. 97, no. 8, 084030. https://doi.org/10.1103/PhysRevD.97.084030

APA

Correia, M. R., & Cardoso, V. (2018). Characterization of echoes: A Dyson-series representation of individual pulses. Physical Review D, 97(8), [084030]. https://doi.org/10.1103/PhysRevD.97.084030

Vancouver

Correia MR, Cardoso V. Characterization of echoes: A Dyson-series representation of individual pulses. Physical Review D. 2018 Apr 17;97(8). 084030. https://doi.org/10.1103/PhysRevD.97.084030

Author

Correia, Miguel R. ; Cardoso, Vitor. / Characterization of echoes : A Dyson-series representation of individual pulses. In: Physical Review D. 2018 ; Vol. 97, No. 8.

Bibtex

@article{1e1a43492da84c809bbdcd7407e83999,
title = "Characterization of echoes: A Dyson-series representation of individual pulses",
abstract = "The ability to detect and scrutinize gravitational waves from the merger and coalescence of compact binaries opens up the possibility to perform tests of fundamental physics. One such test concerns the dark nature of compact objects: are they really black holes? It was recently pointed out that the absence of horizons-while keeping the external geometry very close to that of General Relativity-would manifest itself in a series of echoes in gravitational wave signals. The observation of echoes by LIGO/Virgo or upcoming facilities would likely inform us on quantum gravity effects or unseen types of matter. Detection of such signals is in principle feasible with relatively simple tools but would benefit enormously from accurate templates. Here we analytically individualize each echo waveform and show that it can be written as a Dyson series, for arbitrary effective potential and boundary conditions. We further apply the formalism to explicitly determine the echoes of a simple toy model: the Dirac delta potential. Our results allow to read off a few known features of echoes and may find application in the modeling for data analysis.",
author = "Correia, {Miguel R.} and Vitor Cardoso",
year = "2018",
month = apr,
day = "17",
doi = "10.1103/PhysRevD.97.084030",
language = "English",
volume = "97",
journal = "Physical Review D",
issn = "2470-0010",
publisher = "American Physical Society",
number = "8",

}

RIS

TY - JOUR

T1 - Characterization of echoes

T2 - A Dyson-series representation of individual pulses

AU - Correia, Miguel R.

AU - Cardoso, Vitor

PY - 2018/4/17

Y1 - 2018/4/17

N2 - The ability to detect and scrutinize gravitational waves from the merger and coalescence of compact binaries opens up the possibility to perform tests of fundamental physics. One such test concerns the dark nature of compact objects: are they really black holes? It was recently pointed out that the absence of horizons-while keeping the external geometry very close to that of General Relativity-would manifest itself in a series of echoes in gravitational wave signals. The observation of echoes by LIGO/Virgo or upcoming facilities would likely inform us on quantum gravity effects or unseen types of matter. Detection of such signals is in principle feasible with relatively simple tools but would benefit enormously from accurate templates. Here we analytically individualize each echo waveform and show that it can be written as a Dyson series, for arbitrary effective potential and boundary conditions. We further apply the formalism to explicitly determine the echoes of a simple toy model: the Dirac delta potential. Our results allow to read off a few known features of echoes and may find application in the modeling for data analysis.

AB - The ability to detect and scrutinize gravitational waves from the merger and coalescence of compact binaries opens up the possibility to perform tests of fundamental physics. One such test concerns the dark nature of compact objects: are they really black holes? It was recently pointed out that the absence of horizons-while keeping the external geometry very close to that of General Relativity-would manifest itself in a series of echoes in gravitational wave signals. The observation of echoes by LIGO/Virgo or upcoming facilities would likely inform us on quantum gravity effects or unseen types of matter. Detection of such signals is in principle feasible with relatively simple tools but would benefit enormously from accurate templates. Here we analytically individualize each echo waveform and show that it can be written as a Dyson series, for arbitrary effective potential and boundary conditions. We further apply the formalism to explicitly determine the echoes of a simple toy model: the Dirac delta potential. Our results allow to read off a few known features of echoes and may find application in the modeling for data analysis.

U2 - 10.1103/PhysRevD.97.084030

DO - 10.1103/PhysRevD.97.084030

M3 - Journal article

VL - 97

JO - Physical Review D

JF - Physical Review D

SN - 2470-0010

IS - 8

M1 - 084030

ER -

ID: 299200438