6 research outputs found

    Flavour changing neutral currents and CP violating processes in generalized supersymmetric theories

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    We consider supersymmetric extensions of the standard model with general non-universal soft breaking terms. We analyse in a model-independent way the constraints on these terms at the electroweak energy scale coming from gluino mediated flavour (F) changing neutral current and CP-violating processes. We have computed the complete ΔF=1\Delta F=1 and ΔF=2\Delta F=2 effective hamiltonian for gluino mediated processes, including for the first time the effect of box diagrams in the evaluation of ϵ/ϵ\epsilon^{\prime}/\epsilon. We present numerical results for the constraints on these non-universal soft breaking terms for different values of the parameters, extending the analysis also to the leptonic sector. A comparison with previous results in the literature is given.Comment: LaTeX, 17 pages, 3 uuencoded figure

    Chiral Logs in Quenched QCD

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    The quenched chiral logs are examined on a 163×2816^3 \times 28 lattice with Iwasaki gauge action and overlap fermions. The pion decay constant fπf_{\pi} is used to set the lattice spacing, a=0.200(3)fma = 0.200(3) {\rm fm}. With pion mass as low as 180MeV\sim 180 {\rm MeV}, we see the quenched chiral logs clearly in mπ2/mm_{\pi}^2/m and fPf_P, the pseudoscalar decay constant. We analyze the data to determine how low the pion mass needs to be in order for the quenched one-loop chiral perturbation theory (χ\chiPT) to apply. With the constrained curve-fitting method, we are able to extract the quenched chiral log parameter δ\delta together with other low-energy parameters. Only for mπ300MeVm_{\pi} \leq 300 {\rm MeV} do we obtain a consistent and stable fit with a constant δ\delta which we determine to be 0.24(3)(4) (at the chiral scale Λχ=0.8GeV\Lambda_{\chi}=0.8 {\rm GeV}). By comparing to the 123×2812^3 \times 28 lattice, we estimate the finite volume effect to be about 2.7% for the smallest pion mass. We also fitted the pion mass to the form for the re-summed cactus diagrams and found that its applicable region is extended farther than the range for the one-loop formula, perhaps up to mπ500600m_{\pi} \sim 500-600 MeV. The scale independent δ\delta is determined to be 0.20(3) in this case. We study the quenched non-analytic terms in the nucleon mass and find that the coefficient C1/2C_{1/2} in the nucleon mass is consistent with the prediction of one-loop χ\chiPT\@. We also obtain the low energy constant L5L_5 from fπf_{\pi}. We conclude from this study that it is imperative to cover only the range of data with the pion mass less than 300MeV\sim 300 {\rm MeV} in order to examine the chiral behavior of the hadron masses and decay constants in quenched QCD and match them with quenched one-loop χ\chiPT\@.Comment: 37 pages and 24 figures, pion masses are fitted to the form for the re-summed cactus diagrams, figures added, to appear in PR

    Interacting new agegraphic viscous dark energy with varying GG

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    We consider the new agegraphic model of dark energy with a varying gravitational constant, GG, in a non-flat universe. We obtain the equation of state and the deceleration parameters for both interacting and noninteracting new agegraphic dark energy. We also present the equation of motion determining the evolution behavior of the dark energy density with a time variable gravitational constant. Finally, we generalize our study to the case of viscous new agegraphic dark energy in the presence of an interaction term between both dark components.Comment: 12 pages, accepted for publication in IJTP (2010

    Black Holes in Bulk Viscous Cosmology

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    We investigate the effects of the accretion of phantom energy with non-zero bulk viscosity onto a Schwarzschild black hole and show that black holes accreting viscous phantom energy will lose mass rapidly compared to the non-viscous case. When matter is incorporated along with the phantom energy, the black holes meet with the same fate as bulk viscous forces dominate matter accretion. If the phantom energy has large bulk viscosity, then the mass of the black hole will reduce faster than in the small viscosity case.Comment: 20 pages, 3 figures, accepted for publication in Int. J. Theor. Phy
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