Dark spinor inflation -- theory primer and dynamics

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dc.creatorBoehmer, Christian G.
dc.date2008-04-03
dc.date2008-05-16
dc.date.accessioned2026-07-07T11:33:29Z
dc.date.available2026-07-07T11:33:29Z
dc.descriptionInflation driven by a single dark spinor field is discussed. We define the notion of a dark spinor field and derive the cosmological field equations for such a matter source. The conditions for inflation are determined and an exactly solvable model is presented. We find the power spectrum of the quantum fluctuation of this field and compare the results with scalar field inflation.
dc.description13 pages; typo in Eq. (12) corrected, minor improvements
dc.identifierhttps://arxiv.org/abs/0804.0616
dc.identifierhttp://arxiv.org/abs/0804.0616
dc.identifierPhys.Rev.D77:123535,2008
dc.identifierdoi:10.1103/PhysRevD.77.123535
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/197913
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Theory
dc.titleDark spinor inflation -- theory primer and dynamics
dc.typetext

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