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Please use this identifier to cite or link to this item: http://paper.sci.ui.ac.id/jspui/handle/2808.28/41
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dc.contributor.authorSulaksono, Anto-
dc.date.accessioned2016-02-21T16:51:23Z-
dc.date.available2016-02-21T16:51:23Z-
dc.date.issued2013-10-13-
dc.identifier.issn17426596-
dc.identifier.other10.1088/1742-6596/539/1/012003en_US
dc.identifier.urihttp://paper.sci.ui.ac.id/jspui/handle/2808.28/41-
dc.description.abstractThe influence of modification of one of the assumptions in standard non-rotating static neutron star calculation i.e., the anisotropic pressure of neutron star matter with hyperons in its core within the framework of extended relativistic mean field model is investigated. It is found that the maximum mass and the redshift predictions are quite compatible with the recent observational constraints if this assumption is relaxed.en_US
dc.language.isoen_USen_US
dc.publisherIOP Publishingen_US
dc.relation.ispartofseriesVolume 539;Conference 1-
dc.sourceJournal of Physics: Conference Series, Volume 539, conference 1 (Conference of Theoretical Physics and Nonlinear Phenomena (CTPNP) 2014: ''From Universe to String's Scale'' 15 February 2014, Surakarta, Indonesia)en_US
dc.source.urihttp://iopscience.iop.org/article/10.1088/1742-6596/539/1/012003en_US
dc.titleHyperons in anisotropic neutron staren_US
dc.typeArticleen_US
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