Bayesian Inference Applied to Pulsar's Models

Bayesian Inference Applied to Pulsar's Models

Author Marinho, Rubens M., Jr. Google Scholar
de Oliveira, Heitor O. Google Scholar
Magalhaes, Nadja S. Autor UNIFESP Google Scholar
Valentim, Rodolfo Autor UNIFESP Google Scholar
Coelho, Jaziel G. Google Scholar
Alves, Marcio E. S. Google Scholar
Abstract The goal of this work is to apply Bayesian statistics to the problem of pulsars in order to compute the Bayes factor and investigate which one among different EoS could better fit known pulsar data, regarding the rate of decrease of the angular velocity versus the angular velocity itself. We also find the posterior distribution and the best fit for some relevant parameters of the pulsar like the mass and the magnetic field.
Keywords Pulsar
Equation of State
Bayesian Statistics
xmlui.dri2xhtml.METS-1.0.item-coverage Singapore
Language English
Sponsor FAPESP
Coordenacao de Aperfeicoamento de Pessoal de Nivel Superior (CAPES)
Grant number FAPESP: 2013/26258-4
FAPESP: 2013/15088-0
Date 2017
Published in Proceedings Of The 7th International Workshop On Astronomy And Relativistic Astrophysics (Iwara 2016). Singapore, v. 45, p. -, 2017.
ISSN 2010-1945 (Sherpa/Romeo, impact factor)
Publisher World Scientific Publ Co Pte Ltd
Extent -
Origin http://dx.doi.org/10.1142/S2010194517600382
Access rights Closed access
Type Conference paper
Web of Science ID WOS:000410658500038
URI https://repositorio.unifesp.br/handle/11600/55460

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