35,226 research outputs found

    Comparison of techniques to reconstruct VHE gamma-ray showers from multiple stereoscopic Cherenkov images

    Get PDF
    For air showers observed simultaneously by more than two imaging atmospheric Cherenkov telescopes, the shower geometry is overconstrained by the images and image information should be combined taking into account the quality of the images. Different algorithms are discussed and tested experimentally using data obtained from observations of Mkn 501 with the HEGRA IACT system. Most of these algorithms provide an estimate of the accuracy of the reconstruction of shower geometry on an event-by-event basis, allowing, e.g., to select higher-quality subsamples for precision measurements.Comment: 14 Pages, 6 figures, Late

    Symmetry breaking: A tool to unveil the topology of chaotic scattering with three degrees of freedom

    Full text link
    We shall use symmetry breaking as a tool to attack the problem of identifying the topology of chaotic scatteruing with more then two degrees of freedom. specifically we discuss the structure of the homoclinic/heteroclinic tangle and the connection between the chaotic invariant set, the scattering functions and the singularities in the cross section for a class of scattering systems with one open and two closed degrees of freedom.Comment: 13 pages and 8 figure

    The intrinsic strangeness and charm of the nucleon using improved staggered fermions

    Full text link
    We calculate the intrinsic strangeness of the nucleon, - , using the MILC library of improved staggered gauge configurations using the Asqtad and HISQ actions. Additionally, we present a preliminary calculation of the intrinsic charm of the nucleon using the HISQ action with dynamical charm. The calculation is done with a method which incorporates features of both commonly-used methods, the direct evaluation of the three-point function and the application of the Feynman- Hellman theorem. We present an improvement on this method that further reduces the statistical error, and check the result from this hybrid method against the other two methods and find that they are consistent. The values for and found here, together with perturbative results for heavy quarks, show that dark matter scattering through Higgs-like exchange receives roughly equal contributions from all heavy quark flavors.Comment: 17 pages, 14 figure

    Top quark forward-backward asymmetry and charge asymmetry in left-right twin Higgs model

    Full text link
    In order to explain the Tevatron anomaly of the top quark forward-backward asymmetry AFBtA_{FB}^t in the left-right twin Higgs model, we choose to give up the lightest neutral particle of h^\hat{h} field as a stable dark matter candidate. Then a new Yukawa interaction for h^\hat{h} is allowed, which can be free from the constraint of same-sign top pair production and contribute sizably to AFBtA_{FB}^t. Considering the constraints from the production rates of the top pair (ttˉt\bar t), the top decay rates and ttˉt\bar{t} invariant mass distribution, we find that this model with such new Yukawa interaction can explain AFBtA_{FB}^t measured at the Tevatron while satisfying the charge asymmetry ACtA_{C}^t measured at the LHC.Moreover, this model predicts a strongly correlation between ACtA_{C}^t at the LHC and AFBtA_{FB}^t at the Tevatron, i.e., ACtA_{C}^t increases as AFBtA_{FB}^t increases.Comment: 17 pages, 9 figures; matches the published versio

    Black hole particle emission in higher-dimensional spacetimes

    Get PDF
    In models with extra dimensions, a black hole evaporates both in the bulk and on the visible brane, where standard model fields live. The exact emissivities of each particle species are needed to determine how the black hole decay proceeds. We compute and discuss the absorption cross-sections, the relative emissivities and the total power output of all known fields in the evaporation phase. Graviton emissivity is highly enhanced as the spacetime dimensionality increases. Therefore, a black hole loses a significant fraction of its mass in the bulk. This result has important consequences for the phenomenology of black holes in models with extra dimensions and black hole detection in particle colliders.Comment: 4 pages, RevTeX 4. v3: Misprints in Tables correcte

    Spin/Orbital Pattern-Dependent Polaron Absorption in Nd(1-x)Sr(x)MnO3

    Full text link
    We investigated optical properties of Nd(1-x)Sr(x)MnO3 (x= 0.40, 0.50, 0.55, and 0.65) single crystals. In the spin/orbital disordered state, their conductivity spectra look quite similar, and the strength of the mid-infrared absorption peak is proportional to x(1-x) consistent with the polaron picture. As temperature lowers, the Nd(1-x)Sr(x)MnO3 samples enter into various spin/orbital ordered states, whose optical responses are quite different. These optical responses can be explained by the spin/orbital ordering pattern-dependent polaron hopping.Comment: 3 figures (gzipped

    Optical Studies of a Layered Manganite La_{1.2}Sr_{1.8}Mn_2O_7 : Polaron Correlation Effect

    Full text link
    Optical conductivity spectra of a cleaved ab-plane of a La_{1.2}Sr_{1.8}Mn_2O_7 single crystal exhibit a small polaron absorption band in the mid-infrared region at overall temperatures. With decreasing temperature (T) to Curie temperature (T_C), the center frequency of the small polaron band moves to a higher frequency, resulting in a gap-like feature, and that it collapses to a lower frequency below T_C. Interestingly, with decreasing T, the stretching phonon mode hardens above T_C and softens below T_C. These concurring changes of lattice and electronic structure indicate that short range polaron correlation exist above T_C but disappear with a magnetic ordering.Comment: 4 pages including 5 figures. submitted to Phys. Rev.
    • …
    corecore