Gravitational Waves and Compact Objects: From Theory to Data Analysis

A special issue of Universe (ISSN 2218-1997). This special issue belongs to the section "Gravitation".

Deadline for manuscript submissions: closed (30 November 2021) | Viewed by 2204

Special Issue Editors


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Guest Editor
1. Departamento de Astronomía y Astrofísica, Universitat de València, Dr. Moliner 50, 46100 Burjassot, València, Spain
2. Departamento de Matemática da Universidade de Aveiro and Centre for Research and Development in Mathematics and Applications (CIDMA), Campus de Santiago, 3810-183 Aveiro, Portugal
Interests: numerical relativity; black holes and exotic compact objects; boson stars; gravitational waves

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Guest Editor
Instituto Galego de Física de Altas Enerxías (IGFAE), University of Santiago de Compostela, Praza do Obradoiro, 0, 15705 Santiago de Compostela, A Coruña, Spain
Interests: gravitational-wave astronomy; black-hole ringdown; data analysis; exotic compact objects

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Guest Editor
Departamento de Astronomía y Astrofísica, Universitat de València, C/Dr Moliner 50, 46100 Burjassot, Valencia, Spain
Interests: gravitational-wave astronomy; data analysis; core-collapse supernova

Special Issue Information

Dear Colleagues,

Gravitational-wave astronomy is opening a new window into the strong field regime of gravity. To this day, the LIGO-Virgo-KAGRA (LVK) collaboration has detected over 50 gravitational-wave events, all of them consistent with black holes and neutron stars. Such outstanding achievement relies heavily on two fundamental pillars: numerical relativity and data analysis. The true (classical and quantum) nature of the observed compact objects remains, however, elusive due to several reasons. First, although the gravitational-wave data so far are well fitted by the Kerr hypothesis, no sufficiently developed alternative gravitational waveforms exist to challenge the prevailing black-hole binary merger interpretation. Second, current observations do not yet allow for a detailed observation of the characteristic ringdown emission from the remnant objects of these mergers, therefore providing strong evidence in favour or against the Kerr hypothesis. Alternative models of compact objects with unique features (ecos, UCOs) have been proposed, but numerical studies can be undertaken to study their properties and stability, and obtain the gravitational radiation emitted by such objects. These shall lead to their discovery of these exotic objects or to constraints on their populations. On the other hand, new data analysis techniques shall be needed to correctly identify the source of the gravitational waves detected by the LVK. A meeting point of these different fields would greatly improve our understanding of current and future gravitational-wave events.

This Special Issue aims to review current and future prospects of numerical relativity, gravitational waves, the physics of compact objects, and data analysis. In particular, of great interest are investigations involving the merger and ringdown stages of compact mergers, where strong gravity effects shall allow to resolve the nature of the involved objects. Therefore, novel ideas beyond the current binary black hole framework are especially welcome, both theoretical and experimental.

Dr. Nicolas Sanchis-Gual
Dr. Juan Calderón-Bustillo
Dr. Alejandro Torres-Forne
Guest Editors

Manuscript Submission Information

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Keywords

  • gravitational waves
  • numerical relativity
  • data analysis
  • black holes
  • compact objects

Published Papers (1 paper)

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Research

17 pages, 869 KiB  
Article
Aspects of Gauss-Bonnet Scalarisation of Charged Black Holes
by Carlos A. R. Herdeiro, Alexandre M. Pombo and Eugen Radu
Universe 2021, 7(12), 483; https://0-doi-org.brum.beds.ac.uk/10.3390/universe7120483 - 07 Dec 2021
Cited by 18 | Viewed by 1699
Abstract
The general relativity vacuum black holes (BHs) can be scalarised in models where a scalar field non-minimally couples to the Gauss-Bonnet (GB) invariant. Such GB scalarisation comes in two flavours, depending on the GB sign that triggers the phenomenon. Hereafter these two cases [...] Read more.
The general relativity vacuum black holes (BHs) can be scalarised in models where a scalar field non-minimally couples to the Gauss-Bonnet (GB) invariant. Such GB scalarisation comes in two flavours, depending on the GB sign that triggers the phenomenon. Hereafter these two cases are termed GB± scalarisation. For vacuum BHs, only GB+ scalarisation is possible in the static case, while GB scalarisation is spin induced. But for electrovacuum BHs, GB is also charged induced. We discuss the GB scalarisation of Reissner-Nordström and Kerr-Newman BHs, discussing zero modes and constructing fully non-linear solutions. Some comparisons with GB+ scalarisation are given. To assess the generality of the observed features, we also briefly consider the GB± scalarisation of stringy dilatonic BHs and coloured BHs which provide qualitative differences with respect to the electrovacuum case, namely on the distribution and existence of regions triggering GB scalarisation. Full article
(This article belongs to the Special Issue Gravitational Waves and Compact Objects: From Theory to Data Analysis)
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