Confined gravitational waves for chiral matter with heat

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dc.creatorBulyzhenkov, I. E.
dc.date2008-04-24
dc.date2008-05-11
dc.date.accessioned2026-07-07T09:37:51Z
dc.date.available2026-07-07T09:37:51Z
dc.descriptionThe GR wave self-heating of geodesic massive bodies with constant thermo-gravimechanical energies increases the brightness-to-charge ratio along spiral radial transitions in the energy-to-energy gravitation. Paired confined gravitons locally warm accelerated matter that suggests the thermodynamical origin of electromagnetic outbursts with oscillating Wien's displacements. Damping of orbital periods by chiral GR waves is more efficient for neutron stars around giant companions than for binary pulsars.
dc.description2 pages
dc.identifierhttps://arxiv.org/abs/0804.3820
dc.identifierhttp://arxiv.org/abs/0804.3820
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/160605
dc.subjectGeneral Physics
dc.subjectSpace Physics
dc.titleConfined gravitational waves for chiral matter with heat
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