General Relativistic Mean Field Theory for Rotating Nuclei

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dc.creatorMadokoro, Hideki
dc.creatorMatsuzaki, Masayuki
dc.date1997-02-10
dc.date1997-04-16
dc.date.accessioned2026-07-07T11:11:05Z
dc.date.available2026-07-07T11:11:05Z
dc.descriptionWe formulate a general relativistic mean field theory for rotating nuclei starting from the special relativistic $σ- ω$ model Lagrangian. The tetrad formalism is adopted to generalize the model to the accelerated frame.
dc.description13 pages, REVTeX, no figures, submitted to Phys. Rev. Lett., the word `curved' is replaced by `non-inertial' or `accelerated' in several places to clarify the physical situation interested, some references are added, more detail discussions are given with omitting some redundant sentences
dc.identifierhttps://arxiv.org/abs/nucl-th/9702021
dc.identifierhttp://arxiv.org/abs/nucl-th/9702021
dc.identifierPhys.Rev.C56:2934-2937,1997
dc.identifierdoi:10.1103/PhysRevC.56.R2934
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/190976
dc.subjectNuclear Theory
dc.titleGeneral Relativistic Mean Field Theory for Rotating Nuclei
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