Charm and bottom baryon decays in the Bethe-Salpeter approach: Heavy to heavy semileptonic transitions

Detalles Bibliográficos
Parent link:Physical Review D: particles, fields, gravitation, and cosmology.— , 1970-
Vol. 59, iss. 7.— 1999.— [074016]
Outros autores: Ivanov M. A., Korner J. G., Lyubovitskiy (Lyubovitskij) V. E. Valery Efimovich, Rusetsky A. G.
Summary:Title screen
Charm and bottom baryons and mesons are studied within the framework of a relativistically covariant 3D reduction of the Bethe-Salpeter equation. We carry out an analysis of semileptonic decays of heavy hadrons within this framework using explicit oscillator-type wave functions where we calculate Isgur-Wise functions, decay rates and asymmetry parameters. Within this model we also study the effect of interactions between the light quarks inside the heavy baryon and how they affect the values of the computed heavy baryon observables. We also elaborate on the role of relativistic effects in the calculation of the heavy baryon Isgur-Wise function.
Режим доступа: по договору с организацией-держателем ресурса
Publicado: 1999
Subjects:
Acceso en liña:https://doi.org/10.1103/PhysRevD.59.074016
Formato: Electrónico Capítulo de libro
KOHA link:https://koha.lib.tpu.ru/cgi-bin/koha/opac-detail.pl?biblionumber=656774
Descripción
Summary:Title screen
Charm and bottom baryons and mesons are studied within the framework of a relativistically covariant 3D reduction of the Bethe-Salpeter equation. We carry out an analysis of semileptonic decays of heavy hadrons within this framework using explicit oscillator-type wave functions where we calculate Isgur-Wise functions, decay rates and asymmetry parameters. Within this model we also study the effect of interactions between the light quarks inside the heavy baryon and how they affect the values of the computed heavy baryon observables. We also elaborate on the role of relativistic effects in the calculation of the heavy baryon Isgur-Wise function.
Режим доступа: по договору с организацией-держателем ресурса
DOI:10.1103/PhysRevD.59.074016