2,787 research outputs found

    Branching ratio and CP asymmetry of Bs→π+π−B_s \to \pi^+ \pi^- decays in the perturbative QCD approach

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    In this paper, we calculate the decay rate and CP asymmetry of the Bs→π+π−B_s \to \pi^+\pi^- decay in perturbative QCD approach with Sudakov resummation. Since none of the quarks in final states is the same as those of the initial BsB_s meson, this decay can occur only via annihilation diagrams in the standard model. Besides the current-current operators, the contributions from the QCD and electroweak penguin operators are also taken into account. We find that (a) the branching ratio is about 4×10−74 \times 10^{-7}; (b) the penguin diagrams dominate the total contribution; and (c) the direct CP asymmetry is small in size: no more than 33% ; but the mixing-induced CP asymmetry can be as large as ten percent testable in the near future LHC-b experiments.Comment: 12 pages, 4 figures included, RevTe

    Branching ratios of B+→D(∗)+K(∗)0B^+ \to D^{(*)+}K^{(*)0} decays in perturbative QCD approach

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    We study the rare decays B+→D(∗)+K(∗)0B^+ \to D^{(*)+}K^{(*)0}, which can occur only via annihilation type diagrams in the standard model. We calculate all of the four modes, B→PP,VP,PV,VVB \to PP, VP, PV, VV, in the framework of perturbative QCD approach and give the branching ratios of the order about 10−610^{-6}.Comment: 18 pages, 1 figure, Revte

    Study of color suppressed modes B0→Dˉ(∗)0η(â€Č)B^0 \to \bar D^{(*)0} \eta^{(\prime)}

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    The color suppressed modes B0→Dˉ(∗)0η(â€Č)B^0 \to \bar D^{(*)0} \eta^{(\prime)} are analyzed in perturbative QCD approach. We find that the dominant contribution is from the non-factorizable diagrams. The branching ratios calculated in our approach for B0→Dˉ(∗)0ηB^0 \to \bar D^{(*)0} \eta agree with current experiments. By neglecting the gluonic contribution, we predict the branching ratios of B0→Dˉ(∗)0ηâ€ČB^0 \to \bar D^{(*)0} \eta' are at the comparable size of B0→Dˉ(∗)0π0B^0 \to \bar D^{(*)0} \pi^0, but smaller than that of B0→Dˉ(∗)0ηB^0 \to \bar D^{(*)0} \eta .Comment: revtex, 5 pages, axodraw.st

    Lambda and Anti-Lambda Hypernuclei in Relativistic Mean-field Theory

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    Several aspects about Λ\Lambda-hypernuclei in the relativistic mean field theory, including the effective Λ\Lambda-nucleon coupling strengths based on the successful effective nucleon-nucleon interaction PK1, hypernuclear magnetic moment and Λˉ\bar\Lambda-hypernuclei, have been presented. The effect of tensor coupling in Λ\Lambda-hypernuclei and the impurity effect of Λˉ\bar\Lambda to nuclear structure have been discussed in detail.Comment: 8 pages, 2 figures, Proceedings of the Sendai International Symposium "Strangeness in Nuclear and Hadronic Systems SENDAI08

    f(R) Gravities, Killing Spinor Equations, "BPS" Domain Walls and Cosmology

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    We derive the condition on f(R) gravities that admit Killing spinor equations and construct explicit such examples. The Killing spinor equations can be used to reduce the fourth-order differential equations of motion to the first order for both the domain wall and FLRW cosmological solutions. We obtain exact "BPS" domain walls that describe the smooth Randall-Sundrum II, AdS wormholes and the RG flow from IR to UV. We also obtain exact smooth cosmological solutions that describe the evolution from an inflationary starting point with a larger cosmological constant to an ever-expanding universe with a smaller cosmological constant. In addition, We find exact smooth solutions of pre-big bang models, bouncing or crunching universes. An important feature is that the scalar curvature R of all these metrics is varying rather than a constant. Another intriguing feature is that there are two different f(R) gravities that give rise to the same "BPS" solution. We also study linearized f(R) gravities in (A)dS vacua.Comment: 37 pages, discussion on gravity trapping in RSII modified, typos corrected, further comments and references added; version to appear in JHE

    Study of pure annihilation type decays B→Ds∗KB \to D_s^{*} K

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    In this work, we calculate the rare decays B0→Ds∗−K+B^0 \to D_s^{*-} K^+ and B+→Ds∗+Kˉ0B^+ \to D_s^{*+} \bar{K}^0 in perturbative QCD approach with Sudakov resummation. We give the branching ratio of 10−510^{-5} for B0→Ds∗−K+B^0 \to D_s^{*-}K^+, which will be tested soon in BB factories. The decay B+→Ds∗+Kˉ0B^+ \to D_s^{*+} \bar{K}^0 has a very small branching ratio at O(10−8){\cal O}(10^{-8}), due to the suppression from CKM matrix elements ∣Vub∗Vcd∣|V_{ub}^* V_{cd}|. It may be sensitive to new physics contributions.Comment: 14 pages, 1 figur

    Critical and Non-Critical Einstein-Weyl Supergravity

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    We construct N=1 supersymmetrisations of some recently-proposed theories of critical gravity, conformal gravity, and extensions of critical gravity in four dimensions. The total action consists of the sum of three separately off-shell supersymmetric actions containing Einstein gravity, a cosmological term and the square of the Weyl tensor. For generic choices of the coefficients for these terms, the excitations of the resulting theory around an AdS_4 background describe massive spin-2 and massless spin-2 modes coming from the metric; massive spin-1 modes coming from a vector field in the theory; and massless and massive spin-3/2 modes (with two unequal masses) coming from the gravitino. These assemble into a massless and a massive N=1 spin-2 multiplet. In critical supergravity, the coefficients are tuned so that the spin-2 mode in the massive multiplet becomes massless. In the supersymmetrised extensions of critical gravity, the coefficients are chosen so that the massive modes lie in a "window" of lowest energies E_0 such that these ghostlike fields can be truncated by imposing appropriate boundary conditions at infinity, thus leaving just positive-norm massless supergravity modes.Comment: 29 page

    Revisiting the B {\to} {\pi} {\rho}, {\pi} {\omega} Decays in the Perturbative QCD Approach Beyond the Leading Order

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    We calculate the branching ratios and CP asymmetries of the B→πρB \to \pi \rho, πω\pi\omega decays in the perturbative QCD factorization approach up to the next-to-leading-order contributions. We find that the next-to-leading-order contributions can interfere with the leading-order part constructively or destructively for different decay modes. Our numerical results have a much better agreement with current available data than previous leading-order calculations, e.g., the next-to-leading-order corrections enhance the B0→π0ρ0B^0\rightarrow \pi^0\rho^0 branching ratios by a factor 2.5, which is helpful to narrow the gaps between theoretic predictions and experimental data. We also update the direct CP-violation parameters, the mixing-induced CP-violation parameters of these modes, which show a better agreement with experimental data than many of the other approaches.Comment: 23 pages, 4 figures, 4 table

    Spectrum of Higher Derivative 6D Chiral Supergravity

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    Gauged off-shell Maxwell-Einstein supergravity in six dimensions with N=(1,0) supersymmetry has a higher derivative extension afforded by a supersymmetrized Riemann squared term. This theory admits a supersymmetric Minkowski x S^2 compactification with a U(1) monopole of unit charge on S^2. We determine the full spectrum of the theory on this background. We also determine the spectrum on a non-supersymmetric version of this compactification in which the monopole charge is different from unity, and we find the peculiar feature that there are massless gravitini in a representation of the S^2 isometry group determined by the monopole charge.Comment: typos correcte
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