Collapse of massive fields in anti-de Sitter spacetime

Gravitational collapse in asymptotically anti-de Sitter spacetime has a rich but poorly-understood structure. There are strong indications that some families of initial data form "bound" states, which are regular everywhere, while other families seem to always collapse to black holes. Here...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
Veröffentlicht in:arXiv.org 2015-05
Hauptverfasser: Okawa, Hirotada, Lopes, Jorge C, Cardoso, Vitor
Format: Artikel
Sprache:eng
Schlagworte:
Online-Zugang:Volltext
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
container_end_page
container_issue
container_start_page
container_title arXiv.org
container_volume
creator Okawa, Hirotada
Lopes, Jorge C
Cardoso, Vitor
description Gravitational collapse in asymptotically anti-de Sitter spacetime has a rich but poorly-understood structure. There are strong indications that some families of initial data form "bound" states, which are regular everywhere, while other families seem to always collapse to black holes. Here, we investigate the collapse of massive scalar fields in anti-de Sitter, with enlarged freedom in the initial data setup, such as several distinct wavepackets, gravitationally interacting with each other. Our results are fully consistent with previous findings in the literature: massive fields, which have a fully resonant spectra, collapse at (arbitrarily?) small amplitude for some classes of initial data, and form oscillating stars for others. We find evidence that initial data consisting on several wavepackets may allow efficient exchange of energy between them, and delay the collapse substantially, or avoid it altogether. When the AdS boundary is artificially changed so that the spectrum is no longer resonant, cascading to higher frequencies may still be present. Finally, we comment on the asymptotically flat counterparts.
format Article
fullrecord <record><control><sourceid>proquest</sourceid><recordid>TN_cdi_proquest_journals_2081626262</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2081626262</sourcerecordid><originalsourceid>FETCH-proquest_journals_20816262623</originalsourceid><addsrcrecordid>eNqNikEKwjAQAIMgWLR_WPBcSDdt7L0o3vVegt3AlrSp3dT3q-ADZA5zmNmoDI0pi6ZC3KlcZNBaoz1hXZtM2TaG4GYhiB5GJ8IvAs8UegGewE2Ji57gxinRAjK7ByUe6aC23gWh_Oe9Ol7O9_ZazEt8riSpG-K6TJ_UoW5Ki1_Mf9cbqpw1Bw</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>2081626262</pqid></control><display><type>article</type><title>Collapse of massive fields in anti-de Sitter spacetime</title><source>Free E- Journals</source><creator>Okawa, Hirotada ; Lopes, Jorge C ; Cardoso, Vitor</creator><creatorcontrib>Okawa, Hirotada ; Lopes, Jorge C ; Cardoso, Vitor</creatorcontrib><description>Gravitational collapse in asymptotically anti-de Sitter spacetime has a rich but poorly-understood structure. There are strong indications that some families of initial data form "bound" states, which are regular everywhere, while other families seem to always collapse to black holes. Here, we investigate the collapse of massive scalar fields in anti-de Sitter, with enlarged freedom in the initial data setup, such as several distinct wavepackets, gravitationally interacting with each other. Our results are fully consistent with previous findings in the literature: massive fields, which have a fully resonant spectra, collapse at (arbitrarily?) small amplitude for some classes of initial data, and form oscillating stars for others. We find evidence that initial data consisting on several wavepackets may allow efficient exchange of energy between them, and delay the collapse substantially, or avoid it altogether. When the AdS boundary is artificially changed so that the spectrum is no longer resonant, cascading to higher frequencies may still be present. Finally, we comment on the asymptotically flat counterparts.</description><identifier>EISSN: 2331-8422</identifier><language>eng</language><publisher>Ithaca: Cornell University Library, arXiv.org</publisher><subject>Asymptotic properties ; Eulers equations ; Gravitational collapse ; Relativity ; Spacetime</subject><ispartof>arXiv.org, 2015-05</ispartof><rights>2015. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.</rights><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>780,784</link.rule.ids></links><search><creatorcontrib>Okawa, Hirotada</creatorcontrib><creatorcontrib>Lopes, Jorge C</creatorcontrib><creatorcontrib>Cardoso, Vitor</creatorcontrib><title>Collapse of massive fields in anti-de Sitter spacetime</title><title>arXiv.org</title><description>Gravitational collapse in asymptotically anti-de Sitter spacetime has a rich but poorly-understood structure. There are strong indications that some families of initial data form "bound" states, which are regular everywhere, while other families seem to always collapse to black holes. Here, we investigate the collapse of massive scalar fields in anti-de Sitter, with enlarged freedom in the initial data setup, such as several distinct wavepackets, gravitationally interacting with each other. Our results are fully consistent with previous findings in the literature: massive fields, which have a fully resonant spectra, collapse at (arbitrarily?) small amplitude for some classes of initial data, and form oscillating stars for others. We find evidence that initial data consisting on several wavepackets may allow efficient exchange of energy between them, and delay the collapse substantially, or avoid it altogether. When the AdS boundary is artificially changed so that the spectrum is no longer resonant, cascading to higher frequencies may still be present. Finally, we comment on the asymptotically flat counterparts.</description><subject>Asymptotic properties</subject><subject>Eulers equations</subject><subject>Gravitational collapse</subject><subject>Relativity</subject><subject>Spacetime</subject><issn>2331-8422</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2015</creationdate><recordtype>article</recordtype><sourceid>ABUWG</sourceid><sourceid>AFKRA</sourceid><sourceid>AZQEC</sourceid><sourceid>BENPR</sourceid><sourceid>CCPQU</sourceid><sourceid>DWQXO</sourceid><recordid>eNqNikEKwjAQAIMgWLR_WPBcSDdt7L0o3vVegt3AlrSp3dT3q-ADZA5zmNmoDI0pi6ZC3KlcZNBaoz1hXZtM2TaG4GYhiB5GJ8IvAs8UegGewE2Ji57gxinRAjK7ByUe6aC23gWh_Oe9Ol7O9_ZazEt8riSpG-K6TJ_UoW5Ki1_Mf9cbqpw1Bw</recordid><startdate>20150501</startdate><enddate>20150501</enddate><creator>Okawa, Hirotada</creator><creator>Lopes, Jorge C</creator><creator>Cardoso, Vitor</creator><general>Cornell University Library, arXiv.org</general><scope>8FE</scope><scope>8FG</scope><scope>ABJCF</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>HCIFZ</scope><scope>L6V</scope><scope>M7S</scope><scope>PIMPY</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope><scope>PTHSS</scope></search><sort><creationdate>20150501</creationdate><title>Collapse of massive fields in anti-de Sitter spacetime</title><author>Okawa, Hirotada ; Lopes, Jorge C ; Cardoso, Vitor</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-proquest_journals_20816262623</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2015</creationdate><topic>Asymptotic properties</topic><topic>Eulers equations</topic><topic>Gravitational collapse</topic><topic>Relativity</topic><topic>Spacetime</topic><toplevel>online_resources</toplevel><creatorcontrib>Okawa, Hirotada</creatorcontrib><creatorcontrib>Lopes, Jorge C</creatorcontrib><creatorcontrib>Cardoso, Vitor</creatorcontrib><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>Materials Science &amp; Engineering Collection</collection><collection>ProQuest Central (Alumni Edition)</collection><collection>ProQuest Central UK/Ireland</collection><collection>ProQuest Central Essentials</collection><collection>ProQuest Central</collection><collection>Technology Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central Korea</collection><collection>SciTech Premium Collection</collection><collection>ProQuest Engineering Collection</collection><collection>Engineering Database</collection><collection>Publicly Available Content Database</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>ProQuest Central China</collection><collection>Engineering Collection</collection></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Okawa, Hirotada</au><au>Lopes, Jorge C</au><au>Cardoso, Vitor</au><format>book</format><genre>document</genre><ristype>GEN</ristype><atitle>Collapse of massive fields in anti-de Sitter spacetime</atitle><jtitle>arXiv.org</jtitle><date>2015-05-01</date><risdate>2015</risdate><eissn>2331-8422</eissn><abstract>Gravitational collapse in asymptotically anti-de Sitter spacetime has a rich but poorly-understood structure. There are strong indications that some families of initial data form "bound" states, which are regular everywhere, while other families seem to always collapse to black holes. Here, we investigate the collapse of massive scalar fields in anti-de Sitter, with enlarged freedom in the initial data setup, such as several distinct wavepackets, gravitationally interacting with each other. Our results are fully consistent with previous findings in the literature: massive fields, which have a fully resonant spectra, collapse at (arbitrarily?) small amplitude for some classes of initial data, and form oscillating stars for others. We find evidence that initial data consisting on several wavepackets may allow efficient exchange of energy between them, and delay the collapse substantially, or avoid it altogether. When the AdS boundary is artificially changed so that the spectrum is no longer resonant, cascading to higher frequencies may still be present. Finally, we comment on the asymptotically flat counterparts.</abstract><cop>Ithaca</cop><pub>Cornell University Library, arXiv.org</pub><oa>free_for_read</oa></addata></record>
fulltext fulltext
identifier EISSN: 2331-8422
ispartof arXiv.org, 2015-05
issn 2331-8422
language eng
recordid cdi_proquest_journals_2081626262
source Free E- Journals
subjects Asymptotic properties
Eulers equations
Gravitational collapse
Relativity
Spacetime
title Collapse of massive fields in anti-de Sitter spacetime
url https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2024-12-28T16%3A55%3A57IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest&rft_val_fmt=info:ofi/fmt:kev:mtx:book&rft.genre=document&rft.atitle=Collapse%20of%20massive%20fields%20in%20anti-de%20Sitter%20spacetime&rft.jtitle=arXiv.org&rft.au=Okawa,%20Hirotada&rft.date=2015-05-01&rft.eissn=2331-8422&rft_id=info:doi/&rft_dat=%3Cproquest%3E2081626262%3C/proquest%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=2081626262&rft_id=info:pmid/&rfr_iscdi=true