Universal Relation in Dark Matter Admixed Neutron Star

Please use this identifier to cite or link to this item: http://hdl.handle.net/2080/4257

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DC Field	Value	Language
dc.contributor.author	Routaray, Pinku	-
dc.contributor.author	Das, H. C.	-
dc.contributor.author	Kumar, Bharat	-
dc.date.accessioned	2024-01-08T10:05:58Z	-
dc.date.available	2024-01-08T10:05:58Z	-
dc.date.issued	2023-12	-
dc.identifier.citation	67th DAE Symposium on Nuclear Physics, IIT Indore, India, 09-13 December 2023	en_US
dc.identifier.uri	http://hdl.handle.net/2080/4257	-
dc.description	Copyright belongs to proceeding publisher	en_US
dc.description.abstract	In the last decades, there have been no- table advancements in comprehending the properties of compact stars, such as mass, radius, and tidal deformability. These ad- vancements have enhanced the study of densely packed neutron stars (NS) and also provided limitations to several theoretical frameworks. Moreover, another mysterious topic is the possibility of dark matter (DM) inside the NS. There are several debatable issues regarding the nature and the mass of DM....	en_US
dc.subject	neutron star	en_US
dc.subject	Universal relation	en_US
dc.title	Universal Relation in Dark Matter Admixed Neutron Star	en_US
dc.type	Presentation	en_US
Appears in Collections:	Conference Papers

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