Magnetic moments of heavy baryons in the relativistic three-quark model
Journal Article
·
· Physical Review. D, Particles Fields
- Institut fuer Theoretische Physik, Universitaet Tuebingen, Auf der Morgenstelle 14, D-72076 Tuebingen (Germany)
- Bogoliubov Laboratory of Theoretical Physics, Joint Institute for Nuclear Research, 141980 Dubna (Russian Federation)
- Institut fuer Physik, Johannes Gutenberg-Universitaet, D-55099 Mainz (Germany)
The magnetic moments of ground state single, double and triple heavy baryons containing charm or bottom quarks are calculated in a relativistic three-quark model, which, in the heavy-quark limit, is consistent with heavy-quark effective theory and heavy hadron chiral perturbation theory. The internal quark structure of baryons is modeled by baryonic three-quark currents with a spin-flavor structure patterned according to standard covariant baryonic wave functions and currents used in QCD sum rule calculations.
- OSTI ID:
- 20782988
- Journal Information:
- Physical Review. D, Particles Fields, Vol. 73, Issue 9; Other Information: DOI: 10.1103/PhysRevD.73.094013; (c) 2006 The American Physical Society; Country of input: International Atomic Energy Agency (IAEA); ISSN 0556-2821
- Country of Publication:
- United States
- Language:
- English
Similar Records
Magnetic moments of heavy {xi}{sub Q} baryons in light cone QCD sum rules
Spin (1/2){sup +}, spin (3/2){sup +}, and transition magnetic moments of low lying and charmed baryons
Predictions for s-wave and p-wave heavy baryons from sum rules and the constituent quark model: Strong interactions
Journal Article
·
Sun Jun 01 00:00:00 EDT 2008
· Physical Review. D, Particles Fields
·
OSTI ID:20782988
Spin (1/2){sup +}, spin (3/2){sup +}, and transition magnetic moments of low lying and charmed baryons
Journal Article
·
Thu Apr 01 00:00:00 EDT 2010
· Physical Review. D, Particles Fields
·
OSTI ID:20782988
+1 more
Predictions for s-wave and p-wave heavy baryons from sum rules and the constituent quark model: Strong interactions
Journal Article
·
Sat Nov 01 00:00:00 EST 1997
· Physical Review, D
·
OSTI ID:20782988