Constraints to Coupling Constants of the Omega- and Sigma-Mesons with Dibaryons

dc.creatorFaessler, Amand
dc.creatorBuchmann, A. J.
dc.creatorKrivoruchenko, M. I.
dc.date1997-06-27
dc.date.accessioned2026-07-07T11:11:16Z
dc.date.available2026-07-07T11:11:16Z
dc.descriptionThe effect of narrow dibaryon resonances to nuclear matter and structure of neutron stars is investigated in the mean-field theory (MFT) and in the relativistic Hartree approximation (RHA). The existence of massive neutron stars imposes constraints to the coupling constants of the omega- and sigma-mesons with dibaryons. We conclude that the experimental candidates to dibaryons d1(1920) and d'(2060) if exist form in nuclear matter a Bose condensate stable against compression. This proves stability of the ground state for nuclear matter with a Bose condensate of the light dibaryons.
dc.description10 pages, 6 figures
dc.identifierhttps://arxiv.org/abs/nucl-th/9706080
dc.identifierhttp://arxiv.org/abs/nucl-th/9706080
dc.identifierPhys.Rev.C56:1576-1581,1997
dc.identifierdoi:10.1103/PhysRevC.56.1576
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/191039
dc.subjectNuclear Theory
dc.titleConstraints to Coupling Constants of the Omega- and Sigma-Mesons with Dibaryons
dc.typetext

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