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(Referência obtida automaticamente do Web of Science, por meio da informação sobre o financiamento pela FAPESP e o número do processo correspondente, incluída na publicação pelos autores.)

Neutron star crustal properties from relativistic mean-field models and bulk parameters effects

Texto completo
Autor(es):
Dutra, M. [1] ; Lenzi, C. H. [1] ; de Paula, W. [1] ; Lourenco, O. [1]
Número total de Autores: 4
Afiliação do(s) autor(es):
[1] Inst Tecnol Aeronaut, DCTA, Dept Fis, BR-12228900 Sao Jose Dos Campos, SP - Brazil
Número total de Afiliações: 1
Tipo de documento: Artigo Científico
Fonte: EUROPEAN PHYSICAL JOURNAL A; v. 57, n. 8 AUG 2021.
Citações Web of Science: 0
Resumo

We calculate crustal properties of neutron stars, namely, mass (M-crust), radius (R-crust) and fraction of moment of inertia (Delta I/I) from parametrizations of hadronic relativistic mean-field (RMF) model consistent with symmetric and asymmetric nuclear matter constraints, as well as some stellar boundaries. We verify which one are also in agreement with restrictions of Delta I/I >= 1.4% and Delta I/I >= 7% related to the glitching mechanism observed in pulsars, such as the Vela one. The latter constraint explains the glitches phenomenon when entrainment effects are taken into account. Our findings indicate that these parametrizations pass in the glitching limit for a neutron star mass range of M <= 1.82 M-circle dot (Delta I/I >= 1.4%), and M <= 1.16 M-circle dot (Delta I/I >= 7%). We also investigate the influence of nuclear matter bulk parameters on crustal properties and find that symmetry energy is the quantity that produces the higher variations on Mcrust, Rcrust, and Delta I/I. Based on the results, we construct a particular RMF parametrization able to satisfy Delta I/I >= 7% even at M = 1.4 M-circle dot, the mass value used to fit data from the softer component of the Vela pulsar X-ray spectrum. The model also presents compatibility with observational data from PSR J1614-2230, PSR J0348 + 0432, and MSP J0740 + 6620 pulsars, as well as, with data from the Neutron Star Interior Composition Explorer (NICER) mission. (AU)

Processo FAPESP: 20/05238-9 - Diferentes abordagens no estudo da matéria fortemente interagente
Beneficiário:Odilon Lourenço da Silva Filho
Modalidade de apoio: Auxílio à Pesquisa - Regular
Processo FAPESP: 17/05660-0 - Estudos teóricos da estrutura e reações de núcleos exóticos e sistemas de muitos corpos
Beneficiário:Brett Vern Carlson
Modalidade de apoio: Auxílio à Pesquisa - Temático