2018
DOI: 10.1103/physrevd.98.036004
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Semileptonic decays of B(*) , D(*) into

Abstract: We perform a study of the B ðÃÞ , D ðÃÞ semileptonic decays, using a different method than in conventional approaches, where the matrix elements of the weak operators are evaluated and a detailed spin-angular momentum algebra is performed to obtain very simple expressions at the end for the different decay modes. Using only one experimental decay rate in the B or D sectors, the rates for the rest of decay modes are predicted and they are in good agreement with experiment. Some discrepancies are observed in the… Show more

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Cited by 22 publications
(46 citation statements)
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“…Work along the line of [41] is also done in [42] in the study of the semileptonic B, B * , D, D * decays intoνl and a pseudoscalar or vector meson. Once again, we can relate different reactions up to a global form factor.…”
Section: Introductionmentioning
confidence: 99%
“…Work along the line of [41] is also done in [42] in the study of the semileptonic B, B * , D, D * decays intoνl and a pseudoscalar or vector meson. Once again, we can relate different reactions up to a global form factor.…”
Section: Introductionmentioning
confidence: 99%
“…On the other hand, application of another kind of structure, photonic crystal (PhC) slab, in modulating polarization, is capturing interest nowadays [8][9][10][11]. Their simplicity in fabrication, designable band structures, and complex polarization features in the momentum space which are topologically linked with bound states in the continuum [10][11][12][13][14][15][16][17][18][19][20][21][22][23][24][25][26] are favorable for polarization modulation. However, the reported PhC slabs only support nearly linearly polarized resonances which only cover a small area on the Poincaré sphere.…”
mentioning
confidence: 99%
“…Since R = 0 cannot be a solution of Eq. (14), unless in the trivial case C 2 = 0 that we have already discussed in the previous section, this pole cannot be removed. Therefore, our solution exhibits a curvature singularity in r = 0 and cannot be interpreted as modelling a stellar configuration.…”
Section: Physical Interpretation Of the New Solutionsmentioning
confidence: 90%
“…The Tolman-Oppenheimer-Volkoff (TOV) approach is a valuable technique to integrate the Einstein field equations of general relativity for a fluid sphere in hydrostatic equilibrium [1][2][3]. Once a polytropic equation of state, relating pressure and energy density of the fluid, is assumed, the same system of differential equations can be applied in the construction of solutions representing gas clouds, stellar configurations, naked singularities, and wormholes [4][5][6][7][8][9][10][11][12][13][14][15]. Also black hole solutions can be understood as limiting-case solutions to the TOV system.…”
Section: Introductionmentioning
confidence: 99%