Bose Fermi Supersymmetry with Bogoliubov transforms in Cosmology

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dc.creatorPatwardhan, Ajay
dc.date2006-11-04
dc.date.accessioned2026-07-07T07:32:12Z
dc.date.available2026-07-07T07:32:12Z
dc.descriptionField theory including Supersymmetry and Bose Fermi Symmetry is an active subject of particle physics and cosmology. Recent and expected observational evidence gives indicators for the creation and destruction of normal and supersymmetric dark matter in the universe. This paper uses Bogoliubov transforms in supersymmetric and Bose Fermi form for obtaining the vaccuum expectation values at any two times in cosmological and black hole geometries. The isotropic Robertson Walker and slightly anisotropic Bianchi I geometry mode functions have a differential equation form analogous to the supersymmetric Hamiltonian. The condition for mixed and distinct representations for bosonic and fermionic fields of normal and supersymmetric partner particles are found.
dc.description11 pages, no figures. Visitor, Institute of Mathematical Sciences, Chennai; ajay@imsc.res.in
dc.identifierhttps://arxiv.org/abs/hep-th/0611044
dc.identifierhttp://arxiv.org/abs/hep-th/0611044
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/119030
dc.subjectHigh Energy Physics - Theory
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleBose Fermi Supersymmetry with Bogoliubov transforms in Cosmology
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