83,705 research outputs found

    Near field pressure fluctuations in a circular jet

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    The vortical structures in shear layers govern many dynamic aspects of the jet, including entrainment of mass, transfer of momentum and noise generation. These structures develop from instability waves and undergo a merging process. Vortex merging reduces the time scale and increases the length scale of the shear layer. At the same time pressure fluctuations are induced by the unsteady motion. These pressure perturbations can exert high level dynamic loading on nearby structures, and radiate to the far field as noise. In this study, the generation mechanism of the pressure fluctuations and the radiation process are examined

    Noncommutative D-Brane in Non-Constant NS-NS B Field Background

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    We show that when the field strength H of the NS-NS B field does not vanish, the coordinates X and momenta P of an open string endpoints satisfy a set of mixed commutation relations among themselves. Identifying X and P with the coordinates and derivatives of the D-brane world volume, we find a new type of noncommutative spaces which is very different from those associated with a constant B field background.Comment: 11 pages, Latex, minor modification

    Supersymmetric reduced models with a symmetry based on Filippov algebra

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    Generalizations of the reduced model of super Yang-Mills theory obtained by replacing the Lie algebra structure to Filippov nn-algebra structures are studied. Conditions for the reduced model actions to be supersymmetric are examined. These models are related with what we call \{cal N}_{min}=2 super pp-brane actions.Comment: v3: In the previous versions we overlooked that Eq.(3.9) holds more generally, and missed some supersymmetric actions. Those are now included and modifications including a slight change in the title were made accordingly. 1+18 page

    Decay constants and radiative decays of heavy mesons in light-front quark model

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    We investigate the magnetic dipole decays VPγV\to P\gamma of various heavy-flavored mesons such as (D,D,Ds,Ds,ηc,J/ψ)(D,D^*,D_s,D^{*}_s,\eta_c, J/\psi) and (B,B,Bs,Bs,ηb,Υ)(B,B^*,B_s,B^*_s,\eta_b,\Upsilon) using the light-front quark model constrained by the variational principle for the QCD-motivated effective Hamiltonian. The momentum dependent form factors FVP(q2)F_{VP}(q^2) for VPγV\to P\gamma^* decays are obtained in the q+=0q^+=0 frame and then analytically continued to the timelike region by changing q{\bf q}_\perp to iqi{\bf q}_\perp in the form factors. The coupling constant gVPγg_{VP\gamma} for real photon case is then obtained in the limit as q20q^2\to 0, i.e. gVPγ=FVP(q2=0)g_{VP\gamma}=F_{VP}(q^2=0). The weak decay constants of heavy pseudoscalar and vector mesons are also calculated. Our numerical results for the decay constants and radiative decay widths for the heavy-flavored mesons are overall in good agreement with the available experimental data as well as other theoretical model calculations.Comment: 9 pages, 3figures, added few more references, typos correcte

    Charged lepton mixing and oscillations from neutrino mixing in the early Universe

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    Charged lepton mixing as a consequence of neutrino mixing is studied for two generations e,μe,\mu in the temperature regime mμTMWm_\mu \ll T \ll M_W in the early Universe. We state the general criteria for charged lepton mixing, critically reexamine aspects of neutrino equilibration and provide arguments to suggest that neutrinos may equilibrate as mass eigenstates in the temperature regime \emph{prior} to flavor equalization. We assume this to be the case, and that neutrino mass eigenstates are in equilibrium with different chemical potentials. Charged lepton self-energies are obtained to leading order in the electromagnetic and weak interactions. The upper bounds on the neutrino asymmetry parameters from CMB and BBN without oscillations, combined with the fit to the solar and KamLAND data for the neutrino mixing angle, suggest that for the two generation case there is resonant \emph{charged lepton} mixing in the temperature range T5GeVT \sim 5 \mathrm{GeV}. In this range the charged lepton oscillation frequency is of the same order as the electromagnetic damping rate.Comment: 17 pages, 2 figs, same results with more discussions on quantum Zeno effect. To appear in Astroparticle Physic
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