Influence of the Effective Mass Modification of Weak Interacting Light Boson on the Properties of Neutron Stars

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DC Field	Value	Language
dc.contributor.author	Sulaksono, Anto	-
dc.contributor.author	Agrawal, B. K.	-
dc.date.accessioned	2016-02-21T11:52:09Z	-
dc.date.available	2016-02-21T11:52:09Z	-
dc.date.issued	2013-03	-
dc.identifier.issn	14325411	-
dc.identifier.other	10.1007/s00601-012-0419-x	en_US
dc.identifier.uri	http://paper.sci.ui.ac.id/jspui/handle/2808.28/34	-
dc.description.abstract	The influence of modification of the effective mass of weakly interacting light boson (WILB) present in the compact hyperonic stars are investigated within the framework of the extended relativistic mean field model. It is found that the bulk properties of the hyperonic stars are compatible with the provided recent observational constraints, if the presence of the WILBs with appropriate effective mass is considered.	en_US
dc.language.iso	en_US	en_US
dc.publisher	Springer Vienna	en_US
dc.relation.ispartofseries	Volume 54;Issue 1	-
dc.source	Few-Body Systems, March 2013, Volume 54, Issue 1, pp 501-504	en_US
dc.source.uri	http://link.springer.com/article/10.1007%2Fs00601-012-0419-x	en_US
dc.title	Influence of the Effective Mass Modification of Weak Interacting Light Boson on the Properties of Neutron Stars	en_US
dc.type	Article	en_US
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