Utilize este identificador para referenciar este registo:
https://hdl.handle.net/10316/115131
Campo DC | Valor | Idioma |
---|---|---|
dc.contributor.author | Huang, Chun | - |
dc.contributor.author | Raaijmakers, Geert | - |
dc.contributor.author | Watts, Anna L | - |
dc.contributor.author | Tolos, Laura | - |
dc.contributor.author | Providência, Constança | - |
dc.date.accessioned | 2024-05-14T10:47:03Z | - |
dc.date.available | 2024-05-14T10:47:03Z | - |
dc.date.issued | 2024 | - |
dc.identifier.issn | 0035-8711 | pt |
dc.identifier.issn | 1365-2966 | pt |
dc.identifier.uri | https://hdl.handle.net/10316/115131 | - |
dc.description.abstract | Measurements of neutron star mass and radius or tidal deformability deliver unique insight into the equation of state (EOS) of cold dense matter. EOS inference is very often done using generalized parametric or non-parametric models, which deliver no information on composition. In this paper, we consider a microscopic nuclear EOS model based on a field theoretical approach. We show that current measurements from NICER and gravitational wave observations constrain primarily the symmetric nuclear matter EOS. We then explore what could be delivered by measurements of mass and radius at the level anticipated for future large-area X-ray timing telescopes. These should be able to place very strong limits on the symmetric nuclear matter EOS, in addition to constraining the nuclear symmetry energy that determines the proton fraction inside the neutron star. | pt |
dc.language.iso | eng | pt |
dc.publisher | Oxford University Press | pt |
dc.relation | info:eu-repo/grantAgreement/UIDP/04564/2020/PT | pt |
dc.relation | info:eu-repo/grantAgreement/FCT/3599-PPCDT/2022.06460.PTDC/PT | pt |
dc.relation | UIDB/04564/2020 | pt |
dc.rights | openAccess | pt |
dc.rights.uri | http://creativecommons.org/licenses/by/4.0/ | pt |
dc.subject | dense matter | pt |
dc.subject | equation of state | pt |
dc.subject | stars: neutron | pt |
dc.subject | X-rays: general | pt |
dc.title | Constraining a relativistic mean field model using neutron star mass–radius measurements I: nucleonic models | pt |
dc.type | article | - |
degois.publication.firstPage | 4650 | pt |
degois.publication.lastPage | 4665 | pt |
degois.publication.issue | 4 | pt |
degois.publication.title | Monthly Notices of the Royal Astronomical Society | pt |
dc.relation.publisherversion | https://academic.oup.com/mnras/ | pt |
dc.peerreviewed | yes | pt |
dc.identifier.doi | 10.1093/mnras/stae844 | pt |
degois.publication.volume | 529 | pt |
dc.date.embargo | 2024-01-01 | * |
uc.date.periodoEmbargo | 0 | pt |
item.openairetype | article | - |
item.fulltext | Com Texto completo | - |
item.languageiso639-1 | en | - |
item.grantfulltext | open | - |
item.cerifentitytype | Publications | - |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
crisitem.project.grantno | Center for Physics of the University of Coimbra | - |
crisitem.author.researchunit | CFisUC – Center for Physics of the University of Coimbra | - |
crisitem.author.orcid | 0000-0001-6464-8023 | - |
Aparece nas coleções: | I&D CFis - Artigos em Revistas Internacionais FCTUC Física - Artigos em Revistas Internacionais |
Ficheiros deste registo:
Ficheiro | Descrição | Tamanho | Formato | |
---|---|---|---|---|
stae844.pdf | 2.91 MB | Adobe PDF | Ver/Abrir |
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