dc.contributorUniversidade Estadual Paulista (Unesp)
dc.contributorYonsei Univ
dc.contributorAsia Pacific Ctr Theoret Phys
dc.date.accessioned2018-11-26T17:55:01Z
dc.date.available2018-11-26T17:55:01Z
dc.date.created2018-11-26T17:55:01Z
dc.date.issued2018-08-22
dc.identifierPhysical Review C. College Pk: Amer Physical Soc, v. 98, n. 2, 14 p., 2018.
dc.identifier2469-9985
dc.identifierhttp://hdl.handle.net/11449/164556
dc.identifier10.1103/PhysRevC.98.025206
dc.identifierWOS:000442475700008
dc.identifierWOS000442475700008.pdf
dc.identifier0845658462496715
dc.identifier0000-0003-2132-8251
dc.description.abstractWe study the properties of the Delta isobar in the symmetric and asymmetric nuclear matter using the QCD sum rules approach based on the energy dispersion relation. Allowing for different continuum thresholds for the polarization tensors with different dimensions, we find stable masses for the Delta in both the vacuum and the medium. Compared to the nucleon case, we find that the vector repulsion is smaller for the Delta while the scalar attraction is similar (75 MeV vector repulsion and 200 MeV scalar attraction in the symmetric matter). The smaller vector repulsion can be understood using the Pauli principle and a constituent quark model. Also, the isospin dependence of the quasiparticle energy, which mainly comes from the vector self-energy, is quite weak. We also allow for an explicit pi - N continuum contribution to the polarization function but find its effect to be minimal Phenomenological consequences of our results are discussed.
dc.languageeng
dc.publisherAmer Physical Soc
dc.relationPhysical Review C
dc.relation1,443
dc.rightsAcesso aberto
dc.sourceWeb of Science
dc.titleQCD sum rules for the Delta isobar in neutron matter
dc.typeArtículos de revistas


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