Greybody factors, reflectionless scattering modes, and echoes of ultracompact horizonless objects

Motivated by a recently discovered connection between the greybody factors of black holes and the ringdown signal, we investigate the greybody factors of ultracompact horizonless objects, also elucidating their connection to echoes. The greybody factor of ultracompact objects features both low-frequency resonances and high-frequency quasireflectionless scattering modes, which become purely reflectionless in the presence of symmetric cavity potentials, as might be the case for a wormhole. We show these high-frequency (quasi)reflectionless scattering modes, rather than low-frequency resonances, to be directly responsible for the echoes in the time-domain response of ultracompact objects or of black holes surrounded by matter fields localized at large distances.

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Publication Details

Journal
Physical review. D/Physical review. D.
Published
2025-04-18
DOI
https://doi.org/10.1103/physrevd.111.084051
Citations
15
Primary Topic
Pulsars and Gravitational Waves Research
Type
article
Field-Weighted Citation Impact
17.32

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article

Greybody factors, reflectionless scattering modes, and echoes of ultracompact horizonless objects

Sumanta Chakraborty, Shauvik Biswas, Paolo Pani, Romeo Felice Rosato
15 citations
Physical review. D/Physical review. D.
Pulsars and Gravitational Waves Research
17.32
article

Greybody factors, reflectionless scattering modes, and echoes of ultracompact horizonless objects

Sumanta Chakraborty, Shauvik Biswas, Paolo Pani, Romeo Felice Rosato
article en
15 citations

Abstract

Motivated by a recently discovered connection between the greybody factors of black holes and the ringdown signal, we investigate the greybody factors of ultracompact horizonless objects, also elucidating their connection to echoes. The greybody factor of ultracompact objects features both low-frequency resonances and high-frequency quasireflectionless scattering modes, which become purely reflectionless in the presence of symmetric cavity potentials, as might be the case for a wormhole. We show these high-frequency (quasi)reflectionless scattering modes, rather than low-frequency resonances, to be directly responsible for the echoes in the time-domain response of ultracompact objects or of black holes surrounded by matter fields localized at large distances.

Physical review. D/Physical review. D.Vol. 111(8)
Indian Association for the Cultivation of Science (IN), Istituto Nazionale di Fisica Nucleare, Sezione di Roma I (IT), Sapienza University of Rome (IT)
Ministero dell’Istruzione, dell’Università e della Ricerca, Sapienza Università di Roma, Ministero dell'Università e della Ricerca, Science and Engineering Research Board, Instituto Nazionale di Fisica Nucleare
Openalex Percentile: Top 1%
Pulsars and Gravitational Waves Research
17.32
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