The cosmological background in the Higgs scalar-tensor theory without Higgs particles

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dc.creatorFrommert, Hartmut
dc.creatorSchoor, Holger
dc.creatorDehnen, Heinz
dc.date1996-09-30
dc.date.accessioned2026-07-07T03:31:18Z
dc.date.available2026-07-07T03:31:18Z
dc.descriptionThe scalar background field and its consequences are discussed for the Friedmann type cosmological solutions of the scalar-tensor theory of gravity with the Higgs field of the Standard Model as the scalar gravitational field.
dc.description15 pages, no figures, LaTeX 2.09 file. Submitted to Nuclear Physics B
dc.identifierhttps://arxiv.org/abs/gr-qc/9609069
dc.identifierhttp://arxiv.org/abs/gr-qc/9609069
dc.identifierInt.J.Theor.Phys. 38 (1999) 725-735
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/35813
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Theory
dc.titleThe cosmological background in the Higgs scalar-tensor theory without Higgs particles
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