$\bar K$-Nuclear Deeply Bound States?

dc.creatorGal, Avraham
dc.date2006-04-25
dc.date.accessioned2026-07-07T10:46:59Z
dc.date.available2026-07-07T10:46:59Z
dc.descriptionFollowing the prediction by Akaishi and Yamazaki of relatively narrow $\bar K$-nuclear states, deeply bound by over 100 MeV where the main decay channel $\bar K N \to πΣ$ is closed, several experimental signals in stopped $K^-$ reactions on light nuclei have been interpreted recently as due to such states. In this talk I review (i) the evidence from $K^-$-atom data for a {\it deep} $\bar K$-nucleus potential, as attractive as $V_{\bar K}(ρ_0) \sim -(150 - 200)$ MeV at nuclear matter density, that could support such states; and (ii) the theoretical arguments for a {\it shallow} potential, $V_{\bar K}(ρ_0) \sim -(40 - 60)$ MeV. I then review a recent work by Mareš, Friedman and Gal in which $\bar K$-nuclear bound states are generated dynamically across the periodic table, using a RMF Lagrangian that couples the $\bar K$ to the scalar and vector meson fields mediating the nuclear interactions. Substantial polarization of the core nucleus is found for light nuclei, with central nuclear densities enhanced by almost a factor of two. The binding energies and widths calculated in this dynamical model differ appreciably from those calculated for a static nucleus. These calculations provide a lower limit of $Γ_{\bar K} \sim 50 \pm 10$ MeV on the width of nuclear bound states for $\bar K$ binding energy in the range $B_{\bar K} = 100 - 200$ MeV.
dc.descriptionAn updated expanded version of a talk first given in SNP'04, Osaka, July 2004. Presented at ISHIP 2006, Frankfurt, April 2006, to be published in Int. J. Mod. Phys. E
dc.identifierhttps://arxiv.org/abs/nucl-th/0604067
dc.identifierhttp://arxiv.org/abs/nucl-th/0604067
dc.identifierInt.J.Mod.Phys.E16:891-903,2007
dc.identifierdoi:10.1142/S0218301307006368
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/183422
dc.subjectNuclear Theory
dc.title$\bar K$-Nuclear Deeply Bound States?
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