Statistical Physics of Dark and Normal Matter Distribution in Galaxy Formation : Dark Matter Lumps and Black Holes in Core and Halo of Galaxy

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dc.creatorPatwardhan, Ajay
dc.date2008-05-15
dc.date.accessioned2026-07-07T09:39:08Z
dc.date.available2026-07-07T09:39:08Z
dc.descriptionIn unified field theory the cosmological model of the universe has supersymmetric fields. Supersymmetric particles as dark and normal matter in galaxy clusters have a phase separation. Dark matter in halos have a statistical physics equation of state. Neutralino particle gas with gravitation can have a collapse of dark matter lumps. A condensate phase due to boson creation by annhillation and exchange can occur at high densities. The collapse of the boson condensate, including neutralinos, into the Schwarzschild radius creates dark matter black holes. Microscopic dark matter black holes can evaporate with Hawking effect giving gamma ray bursts and create a spectrum of normal particles. The phase separation of normal and dark matter in galaxy clusters and inside galaxies is given by statistical physics.
dc.description9 pages, Physics department, St Xaviers college, Mumbai. Visitor, Institute of Mathematical sciences, Chennai
dc.identifierhttps://arxiv.org/abs/0805.2360
dc.identifierhttp://arxiv.org/abs/0805.2360
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/161056
dc.subjectGeneral Physics
dc.titleStatistical Physics of Dark and Normal Matter Distribution in Galaxy Formation : Dark Matter Lumps and Black Holes in Core and Halo of Galaxy
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