Quasi-normal Modes in de Sitter Space: Plane Wave Method

Recently, in the context of dS/CFT correspondence, quasinormal modes have been put forward to address certain features of this conjecture. In particular, it is argued that the dual states of quasi-normal modes are in fact the states of CFT$_3$ which are created by operator insertions. For a scalar f...

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Main Author: Tanhayi, M. Reza
Format: Text
Language:unknown
Published: arXiv 2014
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Online Access:https://dx.doi.org/10.48550/arxiv.1402.2893
https://arxiv.org/abs/1402.2893
id ftdatacite:10.48550/arxiv.1402.2893
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spelling ftdatacite:10.48550/arxiv.1402.2893 2023-05-15T18:22:48+02:00 Quasi-normal Modes in de Sitter Space: Plane Wave Method Tanhayi, M. Reza 2014 https://dx.doi.org/10.48550/arxiv.1402.2893 https://arxiv.org/abs/1402.2893 unknown arXiv https://dx.doi.org/10.1103/physrevd.90.064010 arXiv.org perpetual, non-exclusive license http://arxiv.org/licenses/nonexclusive-distrib/1.0/ General Relativity and Quantum Cosmology gr-qc High Energy Physics - Theory hep-th FOS Physical sciences article-journal Article ScholarlyArticle Text 2014 ftdatacite https://doi.org/10.48550/arxiv.1402.2893 https://doi.org/10.1103/physrevd.90.064010 2022-04-01T13:06:26Z Recently, in the context of dS/CFT correspondence, quasinormal modes have been put forward to address certain features of this conjecture. In particular, it is argued that the dual states of quasi-normal modes are in fact the states of CFT$_3$ which are created by operator insertions. For a scalar field in $dS_4$, quasi-normal modes which are singular on the past horizon of the south pole and decay exponentially towards the future have been considered in \cite{Ng:2012xp, Jafferis:2013qia}, these modes lie in two complex highest-weight representation of the dS$_4$ isometry group. In this work, we present a simple group representation analysis of these modes so that the de Sitter invariance is obviously manifest. By making use of the so-called plane wave method, we will show that the quasi-normal modes correspond to one class of the unitary irreducible representation of the de Sitter group. This consideration could be generalized straightforwardly for higher-spin fields and higher dimensions, in particular, we will study the quasinormal modes for gauge and spinor fields, and, in the case of a scalar field, the generalization to higher dimensions is also obtained. : 16 pages, typos corrected, references added, published version, To appear in Phys. Rev. D Text South pole DataCite Metadata Store (German National Library of Science and Technology) South Pole Sitter ENVELOPE(10.986,10.986,64.529,64.529)
institution Open Polar
collection DataCite Metadata Store (German National Library of Science and Technology)
op_collection_id ftdatacite
language unknown
topic General Relativity and Quantum Cosmology gr-qc
High Energy Physics - Theory hep-th
FOS Physical sciences
spellingShingle General Relativity and Quantum Cosmology gr-qc
High Energy Physics - Theory hep-th
FOS Physical sciences
Tanhayi, M. Reza
Quasi-normal Modes in de Sitter Space: Plane Wave Method
topic_facet General Relativity and Quantum Cosmology gr-qc
High Energy Physics - Theory hep-th
FOS Physical sciences
description Recently, in the context of dS/CFT correspondence, quasinormal modes have been put forward to address certain features of this conjecture. In particular, it is argued that the dual states of quasi-normal modes are in fact the states of CFT$_3$ which are created by operator insertions. For a scalar field in $dS_4$, quasi-normal modes which are singular on the past horizon of the south pole and decay exponentially towards the future have been considered in \cite{Ng:2012xp, Jafferis:2013qia}, these modes lie in two complex highest-weight representation of the dS$_4$ isometry group. In this work, we present a simple group representation analysis of these modes so that the de Sitter invariance is obviously manifest. By making use of the so-called plane wave method, we will show that the quasi-normal modes correspond to one class of the unitary irreducible representation of the de Sitter group. This consideration could be generalized straightforwardly for higher-spin fields and higher dimensions, in particular, we will study the quasinormal modes for gauge and spinor fields, and, in the case of a scalar field, the generalization to higher dimensions is also obtained. : 16 pages, typos corrected, references added, published version, To appear in Phys. Rev. D
format Text
author Tanhayi, M. Reza
author_facet Tanhayi, M. Reza
author_sort Tanhayi, M. Reza
title Quasi-normal Modes in de Sitter Space: Plane Wave Method
title_short Quasi-normal Modes in de Sitter Space: Plane Wave Method
title_full Quasi-normal Modes in de Sitter Space: Plane Wave Method
title_fullStr Quasi-normal Modes in de Sitter Space: Plane Wave Method
title_full_unstemmed Quasi-normal Modes in de Sitter Space: Plane Wave Method
title_sort quasi-normal modes in de sitter space: plane wave method
publisher arXiv
publishDate 2014
url https://dx.doi.org/10.48550/arxiv.1402.2893
https://arxiv.org/abs/1402.2893
long_lat ENVELOPE(10.986,10.986,64.529,64.529)
geographic South Pole
Sitter
geographic_facet South Pole
Sitter
genre South pole
genre_facet South pole
op_relation https://dx.doi.org/10.1103/physrevd.90.064010
op_rights arXiv.org perpetual, non-exclusive license
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
op_doi https://doi.org/10.48550/arxiv.1402.2893
https://doi.org/10.1103/physrevd.90.064010
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