Quasi-static and dynamic photon bubbles in cold atom clouds

Detalhes bibliográficos
Autor(a) principal: Rodrigues, João D.
Data de Publicação: 2022
Outros Autores: Giampaoli, Ruggero, Rodrigues, José-António, Ferreira, António V., Terças, Hugo, Mendonça, José T.
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Científico de Acesso Aberto de Portugal (Repositórios Cientìficos)
Texto Completo: http://hdl.handle.net/10400.1/17963
Resumo: Turbulent radiation flow is ubiquitous in many physical systems where light–matter interaction becomes relevant. Photon bubble instabilities, in particular, have been identified as a possible source of turbulent radiation transport in astrophysical objects such as massive stars and black hole accretion disks. Here, we report on the experimental observation of a photon bubble instability in cold atomic gases, in the presence of multiple scattering of light. Two different regimes are identified, namely, the growth and formation of quasi-static structures of depleted atom density and increased photon number, akin to photon bubbles in astrophysical objects, and the destabilisation of these structures in a second regime of photon bubble turbulence. A two-fluid theory is developed to model the coupled atom–photon gas and to describe both the saturation of the instability in the regime of quasi-static bubbles and the low-frequency turbulent phase associated with the growth and collapse of photon bubbles inside the atomic sample. We also employ statistical dimensionality reduction techniques to describe the low-dimensional nature of the turbulent regime. The experimental results reported here, along with the theoretical model we have developed, may shed light on analogue photon bubble instabilities in astrophysical scenarios. Our findings are consistent with recent analyses based on spatially resolved pump–probe measurements.
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spelling Quasi-static and dynamic photon bubbles in cold atom cloudsCold atomsInstabilitiesPhoton bubble turbulenceMagneto-optical trapsRadiation trappingDiffusive light transportTurbulent radiation flow is ubiquitous in many physical systems where light–matter interaction becomes relevant. Photon bubble instabilities, in particular, have been identified as a possible source of turbulent radiation transport in astrophysical objects such as massive stars and black hole accretion disks. Here, we report on the experimental observation of a photon bubble instability in cold atomic gases, in the presence of multiple scattering of light. Two different regimes are identified, namely, the growth and formation of quasi-static structures of depleted atom density and increased photon number, akin to photon bubbles in astrophysical objects, and the destabilisation of these structures in a second regime of photon bubble turbulence. A two-fluid theory is developed to model the coupled atom–photon gas and to describe both the saturation of the instability in the regime of quasi-static bubbles and the low-frequency turbulent phase associated with the growth and collapse of photon bubbles inside the atomic sample. We also employ statistical dimensionality reduction techniques to describe the low-dimensional nature of the turbulent regime. The experimental results reported here, along with the theoretical model we have developed, may shed light on analogue photon bubble instabilities in astrophysical scenarios. Our findings are consistent with recent analyses based on spatially resolved pump–probe measurements.MDPISapientiaRodrigues, João D.Giampaoli, RuggeroRodrigues, José-AntónioFerreira, António V.Terças, HugoMendonça, José T.2022-07-12T09:22:48Z2022-04-302022-06-23T12:11:22Z2022-04-30T00:00:00Zinfo:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articleapplication/pdfhttp://hdl.handle.net/10400.1/17963engAtoms 10 (2): 45 (2022)10.3390/atoms100200452218-2004info:eu-repo/semantics/openAccessreponame:Repositório Científico de Acesso Aberto de Portugal (Repositórios Cientìficos)instname:Agência para a Sociedade do Conhecimento (UMIC) - FCT - Sociedade da Informaçãoinstacron:RCAAP2023-07-24T10:30:06Zoai:sapientia.ualg.pt:10400.1/17963Portal AgregadorONGhttps://www.rcaap.pt/oai/openaireopendoar:71602024-03-19T20:07:44.650077Repositório Científico de Acesso Aberto de Portugal (Repositórios Cientìficos) - Agência para a Sociedade do Conhecimento (UMIC) - FCT - Sociedade da Informaçãofalse
dc.title.none.fl_str_mv Quasi-static and dynamic photon bubbles in cold atom clouds
title Quasi-static and dynamic photon bubbles in cold atom clouds
spellingShingle Quasi-static and dynamic photon bubbles in cold atom clouds
Rodrigues, João D.
Cold atoms
Instabilities
Photon bubble turbulence
Magneto-optical traps
Radiation trapping
Diffusive light transport
title_short Quasi-static and dynamic photon bubbles in cold atom clouds
title_full Quasi-static and dynamic photon bubbles in cold atom clouds
title_fullStr Quasi-static and dynamic photon bubbles in cold atom clouds
title_full_unstemmed Quasi-static and dynamic photon bubbles in cold atom clouds
title_sort Quasi-static and dynamic photon bubbles in cold atom clouds
author Rodrigues, João D.
author_facet Rodrigues, João D.
Giampaoli, Ruggero
Rodrigues, José-António
Ferreira, António V.
Terças, Hugo
Mendonça, José T.
author_role author
author2 Giampaoli, Ruggero
Rodrigues, José-António
Ferreira, António V.
Terças, Hugo
Mendonça, José T.
author2_role author
author
author
author
author
dc.contributor.none.fl_str_mv Sapientia
dc.contributor.author.fl_str_mv Rodrigues, João D.
Giampaoli, Ruggero
Rodrigues, José-António
Ferreira, António V.
Terças, Hugo
Mendonça, José T.
dc.subject.por.fl_str_mv Cold atoms
Instabilities
Photon bubble turbulence
Magneto-optical traps
Radiation trapping
Diffusive light transport
topic Cold atoms
Instabilities
Photon bubble turbulence
Magneto-optical traps
Radiation trapping
Diffusive light transport
description Turbulent radiation flow is ubiquitous in many physical systems where light–matter interaction becomes relevant. Photon bubble instabilities, in particular, have been identified as a possible source of turbulent radiation transport in astrophysical objects such as massive stars and black hole accretion disks. Here, we report on the experimental observation of a photon bubble instability in cold atomic gases, in the presence of multiple scattering of light. Two different regimes are identified, namely, the growth and formation of quasi-static structures of depleted atom density and increased photon number, akin to photon bubbles in astrophysical objects, and the destabilisation of these structures in a second regime of photon bubble turbulence. A two-fluid theory is developed to model the coupled atom–photon gas and to describe both the saturation of the instability in the regime of quasi-static bubbles and the low-frequency turbulent phase associated with the growth and collapse of photon bubbles inside the atomic sample. We also employ statistical dimensionality reduction techniques to describe the low-dimensional nature of the turbulent regime. The experimental results reported here, along with the theoretical model we have developed, may shed light on analogue photon bubble instabilities in astrophysical scenarios. Our findings are consistent with recent analyses based on spatially resolved pump–probe measurements.
publishDate 2022
dc.date.none.fl_str_mv 2022-07-12T09:22:48Z
2022-04-30
2022-06-23T12:11:22Z
2022-04-30T00:00:00Z
dc.type.status.fl_str_mv info:eu-repo/semantics/publishedVersion
dc.type.driver.fl_str_mv info:eu-repo/semantics/article
format article
status_str publishedVersion
dc.identifier.uri.fl_str_mv http://hdl.handle.net/10400.1/17963
url http://hdl.handle.net/10400.1/17963
dc.language.iso.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv Atoms 10 (2): 45 (2022)
10.3390/atoms10020045
2218-2004
dc.rights.driver.fl_str_mv info:eu-repo/semantics/openAccess
eu_rights_str_mv openAccess
dc.format.none.fl_str_mv application/pdf
dc.publisher.none.fl_str_mv MDPI
publisher.none.fl_str_mv MDPI
dc.source.none.fl_str_mv reponame:Repositório Científico de Acesso Aberto de Portugal (Repositórios Cientìficos)
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