Light hyperclusters and hyperons in low-density hot stellar matter
Main Author: | |
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Publication Date: | 2021 |
Other Authors: | , |
Format: | Other |
Language: | eng |
Source: | Repositórios Científicos de Acesso Aberto de Portugal (RCAAP) |
Download full: | https://hdl.handle.net/10316/95926 https://doi.org/10.1103/PhysRevC.104.035801 |
Summary: | 12 pages, 8 figures |
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Light hyperclusters and hyperons in low-density hot stellar matterNuclear Theoryastro-ph.HE12 pages, 8 figuresThe abundance of light nuclei and hyperons, that are produced in stellar environments such as supernova or binary mergers, is calculated within a relativistic mean-field model with density dependent couplings in low-density matter. Five light nuclei are considered, together with three light hyper-nuclei. We show that the presence of hyperons shifts the dissolution of clusters to larger densities, and increases the amount of clusters. This effect is larger the smaller the charge fraction, and the higher the temperature. The abundance of hyperons is also affected by the cluster formation: neutral and positively charged hyperons suffer a reduction, and the negatively charged ones an increase. We also observe that the dissolution of the less-abundant clusters occurs at larger densities due to smaller Pauli-blocking effects. Overall, hyper-nuclei set in at temperatures above 25 MeV, and depending on the temperature and chemical composition, they may be more abundant than $\alpha$-particles, or even more abundant than other heavier clusters.This work was partly supported by the FCT (Portugal) Projects No. UID/FIS/04564/2020 and No. POCI-01-0145-FEDER-029912, and by PHAROS COST Action CA16214. H.P. acknowledges Grant No. CEECIND/03092/2017 (FCT, Portugal).American Physical Society2021-06-23info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/otherhttps://hdl.handle.net/10316/95926https://hdl.handle.net/10316/95926https://doi.org/10.1103/PhysRevC.104.035801eng2469-99852469-9993http://arxiv.org/abs/2106.12245v1http://arxiv.org/abs/2106.12245v1http://arxiv.org/abs/2106.12245v1http://arxiv.org/abs/2106.12245v1https://journals.aps.org/prc/abstract/10.1103/PhysRevC.104.035801Custódio, TiagoPais, HelenaProvidência, Constançainfo:eu-repo/semantics/openAccessreponame:Repositórios Científicos de Acesso Aberto de Portugal (RCAAP)instname:FCCN, serviços digitais da FCT – Fundação para a Ciência e a Tecnologiainstacron:RCAAP2022-05-25T02:48:15Zoai:estudogeral.uc.pt:10316/95926Portal AgregadorONGhttps://www.rcaap.pt/oai/openaireinfo@rcaap.ptopendoar:https://opendoar.ac.uk/repository/71602025-05-29T05:44:17.309341Repositórios Científicos de Acesso Aberto de Portugal (RCAAP) - FCCN, serviços digitais da FCT – Fundação para a Ciência e a Tecnologiafalse |
dc.title.none.fl_str_mv |
Light hyperclusters and hyperons in low-density hot stellar matter |
title |
Light hyperclusters and hyperons in low-density hot stellar matter |
spellingShingle |
Light hyperclusters and hyperons in low-density hot stellar matter Custódio, Tiago Nuclear Theory astro-ph.HE |
title_short |
Light hyperclusters and hyperons in low-density hot stellar matter |
title_full |
Light hyperclusters and hyperons in low-density hot stellar matter |
title_fullStr |
Light hyperclusters and hyperons in low-density hot stellar matter |
title_full_unstemmed |
Light hyperclusters and hyperons in low-density hot stellar matter |
title_sort |
Light hyperclusters and hyperons in low-density hot stellar matter |
author |
Custódio, Tiago |
author_facet |
Custódio, Tiago Pais, Helena Providência, Constança |
author_role |
author |
author2 |
Pais, Helena Providência, Constança |
author2_role |
author author |
dc.contributor.author.fl_str_mv |
Custódio, Tiago Pais, Helena Providência, Constança |
dc.subject.por.fl_str_mv |
Nuclear Theory astro-ph.HE |
topic |
Nuclear Theory astro-ph.HE |
description |
12 pages, 8 figures |
publishDate |
2021 |
dc.date.none.fl_str_mv |
2021-06-23 |
dc.type.status.fl_str_mv |
info:eu-repo/semantics/publishedVersion |
dc.type.driver.fl_str_mv |
info:eu-repo/semantics/other |
format |
other |
status_str |
publishedVersion |
dc.identifier.uri.fl_str_mv |
https://hdl.handle.net/10316/95926 https://hdl.handle.net/10316/95926 https://doi.org/10.1103/PhysRevC.104.035801 |
url |
https://hdl.handle.net/10316/95926 https://doi.org/10.1103/PhysRevC.104.035801 |
dc.language.iso.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
2469-9985 2469-9993 http://arxiv.org/abs/2106.12245v1 http://arxiv.org/abs/2106.12245v1 http://arxiv.org/abs/2106.12245v1 http://arxiv.org/abs/2106.12245v1 https://journals.aps.org/prc/abstract/10.1103/PhysRevC.104.035801 |
dc.rights.driver.fl_str_mv |
info:eu-repo/semantics/openAccess |
eu_rights_str_mv |
openAccess |
dc.publisher.none.fl_str_mv |
American Physical Society |
publisher.none.fl_str_mv |
American Physical Society |
dc.source.none.fl_str_mv |
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FCCN, serviços digitais da FCT – Fundação para a Ciência e a Tecnologia |
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RCAAP |
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RCAAP |
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Repositórios Científicos de Acesso Aberto de Portugal (RCAAP) |
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Repositórios Científicos de Acesso Aberto de Portugal (RCAAP) |
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Repositórios Científicos de Acesso Aberto de Portugal (RCAAP) - FCCN, serviços digitais da FCT – Fundação para a Ciência e a Tecnologia |
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info@rcaap.pt |
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1833602455163633664 |