Neutrons stars as non-accelerator hadron physics laboratory

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4525

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DC Field	Value	Language
dc.contributor.author	Datta, B	-
dc.date.accessioned	2009-06-08T15:02:43Z	-
dc.date.available	2009-06-08T15:02:43Z	-
dc.date.issued	1995	-
dc.identifier.citation	Cowsik, R. ed., Proceedings of International Conference on non-accelerator particle physics., Indian Institute of Astrophysics, Bangalore, 2 - 9 Jan, 1994, India, pp. 364 – 371	en
dc.identifier.isbn	981-02-1811-7	-
dc.identifier.uri	http://hdl.handle.net/2248/4525	-
dc.description.abstract	Neutron stars are extremely compact stellar objects, with density that of atomic nucleus and higher. The composition of neutron stars is believed to be mostly neutrons, with admixtures of protons, electrons and perhaps hyperons in the core. We discuss the behaviour of hadronic matter at high densities, with emphasis on the constraints on the equation of state using observational data.	en
dc.language.iso	en	en
dc.publisher	World Scientific	en
dc.rights	Restricted Access	-
dc.subject	Neutrons Stars	en
dc.subject	Non-Accelerator	en
dc.title	Neutrons stars as non-accelerator hadron physics laboratory	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

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