849 research outputs found

    Heavy Quark Spin Symmetry and Heavy Baryons: Electroweak Decays

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    Heavy quark spin symmetry is discussed in the context of single and doubly heavy baryons. A special attention is paid to the constraints/simplifications that this symmetry imposes on the non-relativistic constituent quark model wave functions and on the b->c semileptonic decays of these hadrons.Comment: Presented at the 21st European Conference on Few-Body Problems in Physics, Salamanca, Spain, 30 August - 3 September 201

    Assembly of mitochondrial proteins

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    Study of the leptonic decays of pseudoscalar B,DB, D and vector B,DB^*, D^* mesons and of the semileptonic BDB\to D and BDB\to D^* decays

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    We present results for different observables in weak decays of pseudoscalar and vector mesons with a heavy cc or bb quark. The calculations are done in a nonrelativistic constituent quark model improved at some instances by heavy quark effective theory constraints. We determine pseudoscalar and vector meson decay constants that within a few per cent satisfy fVMV/fPMP=1f_V M_V/f_P M_P=1, a result expected in heavy quark symmetry when the heavy quark masses tend to infinity. We also analyze the semileptonic BDB\to D and BDB\to D^* decays for which we evaluate the different form factors. Here we impose heavy quark effective theory constraints among form factors that are not satisfied by a direct quark model calculation. The value of the form factors at zero recoil allows us to determine, by comparison with experimental data, the value of the Vcb|V_{cb}| Cabbibo-Kobayashi-Maskawa matrix element. From the BDB\to D semileptonic decay we get Vcb=0.040±0.006|V_{cb}|=0.040\pm0.006 in perfect agreement with our previous determination based on the study of the semileptonic ΛbΛc\Lambda_b\to \Lambda_c decay and also in excellent agreement with a recent experimental determination by the DELPHI Collaboration. We further make use of the partial conservation of axial current hypothesis to determine the strong coupling constants gBBπ(0)=60.5±1.1g_{B^*B\pi}(0)=60.5\pm 1.1 and gDDπ(0)=22.1±0.4g_{D^*D\pi}(0)=22.1\pm0.4. The ratio R=(gBBπ(0)fBMD)/(gDDπ(0)fDMB)=1.105±0.005R=(g_{B^*B\pi}(0) f_{B^*}\sqrt{M_D})/ (g_{D^*D\pi}(0) f_{D^*}\sqrt{M_B})=1.105\pm0.005 agrees with the heavy quark symmetry prediction of 1.Comment: 19 Latex pages,6 figures, references added, corrected typos, content enlarge

    Masses and semileptonic decays of doubly heavy baryons in a nonrelativistic quark model

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    We evaluate masses and semileptonic decay widths for the ground state of doubly heavy Ξ\Xi and Ω\Omega baryons in the framework of a nonrelativistic quark model. We solve the three-body problem by means of a variational ansatz made possible by heavy-quark spin symmetry constraints. Our masses are comparable to the ones obtained in relativistic calculations and we get one of the best agreements with lattice data. Our simple wave functions are used to evaluate semileptonic decays of doubly heavy Ξ,Ξ(J=1/2)\Xi, \Xi'(J=1/2) and Ω,Ω(J=1/2)\Omega, \Omega'(J=1/2) baryons. Our results for the decay widths are in reasonable agreement with calculations done in a relativistic calculation in the quark-diquark approximation. We also check that our wave functions comply with what it is expected in the infinite heavy quark mass limit.Comment: 3 latex pages, two tables. To appear in the INPC07 proceeding

    Mixing angle of doubly heavy baryons in QCD

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    We calculate the mixing angles between the spin--1/2, Ξbc\Xi_{bc}--Ξbc\Xi^\prime_{bc} and Ωbc\Omega_{bc}--Ωbc\Omega^\prime_{bc} states of doubly heavy baryons within the QCD sum rules method. It is found that the mixing angles are large and have the values φΞbc=160±50\varphi_{\Xi_{bc}} = 16^0 \pm 5^0 and φΩbc=180±60\varphi_{\Omega_{bc}} = 18^0 \pm 6^0, respectively. The mixing angles are slightly smaller compared to the predictions of the non--relativistic quark model, φΞbc=25.50\varphi_{\Xi_{bc}} = 25.5^0 and φΩbc=25.90\varphi_{\Omega_{bc}} = 25.9^0.Comment: 6 Page

    Masses and semileptonic decays of doubly heavy baryons in a nonrelativistic quark model

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    We evaluate masses and semileptonic decay widths for the ground state of doubly heavy Ξ\Xi and Ω\Omega baryons in the framework of a nonrelativistic quark model. We solve the three-body problem by means of a variational ansatz made possible by heavy-quark spin symmetry constraints. Our masses are comparable to the ones obtained in relativistic calculations and we get one of the best agreements with lattice data. Our simple wave functions are used to evaluate semileptonic decays of doubly heavy Ξ,Ξ(J=1/2)\Xi, \Xi'(J=1/2) and Ω,Ω(J=1/2)\Omega, \Omega'(J=1/2) baryons. Our results for the decay widths are in reasonable agreement with calculations done in a relativistic calculation in the quark-diquark approximation. We also check that our wave functions comply with what it is expected in the infinite heavy quark mass limit.Comment: 3 latex pages, two tables. To appear in the INPC07 proceeding

    Proceedings of the 2nd Iberian Nuclear Astrophysics Meeting on Compact Stars

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    This volume contains most of the links to the presentations delivered at this international workshop. This meeting was the second in the series following the previous I Encuentro Ib\'erico de Compstar, held at the University of Coimbra, Portugal in 2010. The main purpose of this meeting was to strengthen the scientific collaboration between the participants of the Iberian and the rest of the southern European branches of the European Nuclear Astrophysics network, formerly, COMPSTAR. This ESF (European Science Foundation) supported network has been crucial in helping to make a broader audience for the the most interesting and relevant research lines being developed currently in Nuclear Astrophysics, especially related to the physics of neutron stars. The program of the meeting was tailored to theoretical descriptions of the physics of neutron stars although some input from experimental observers and other condensed matter and optics areas of interest was also included.Comment: Journal of Physics: Conference Series Volume 342 (2012), Proceedings of the 2nd Iberian Nuclear Astrophysics Meeting on Compact Stars, 22-23 September 2011, Salamanca-Spain. Editors, M. A. Perez-Garcia, J. Pons and C. Albertus Editor
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