Published February 5, 2021 | Version v1
Journal article

Scattering of axial gravitational wave pulses by monopole black holes and QNMs: a semianalytic approach

  • 1. Stanford Institute for Theoretical Physics, Stanford University, Stanford, California 94305 (United States)

Description

We study scattering of short Gaussian pulses of axial gravitational waves by a spherically symmetric black hole that has swallowed one or more global monopoles. We qualitatively show how the response of the black hole to the impinging pulses depends both on the number of monopoles the black hole has swallowed and on the symmetry breaking scale of the model which gave rise to the monopoles. We use semianalytical methods to determine the corresponding quasinormal modes that get excited by the impinging pulses and that get imprinted in the black hole's response to the pulses. When generalized to the case of rotating black holes, such modes are also expected to show up in various other dynamical processes such as the ringdown phase of a binary black hole merger in case at least one of the companion black holes of the binary has swallowed one or more global monopoles. (paper)

Availability note (English)

Available from http://dx.doi.org/10.1088/1361-6382/abce46

Additional details

Identifiers

Publishing Information

Journal Title
Classical and Quantum Gravity
Journal Volume
38
Journal Issue
3
Journal Page Range
[20 p.]
ISSN
0264-9381
CODEN
CQGRDG

INIS

Country of Publication
United Kingdom
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
53071050
Subject category
S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
Descriptors DEI
BLACK HOLES; GRAVITATIONAL WAVES; PULSES; SCATTERING; SYMMETRY BREAKING