4 research outputs found

    Stability of Non-Abelian Black Holes

    Full text link
    Two types of self-gravitating particle solutions found in several theories with non-Abelian fields are smoothly connected by a family of non-trivial black holes. There exists a maximum point of the black hole entropy, where the stability of solutions changes. This criterion is universal, and the changes in stability follow from a catastrophe-theoretic analysis of the potential function defined by black hole entropy.Comment: 4 Figures to be sent on request,8 pages, WU-AP/33/9

    One-Loop Amplitudes in Euclidean Quantum Gravity

    Full text link
    This paper studies the linearized gravitational field in the presence of boundaries. For this purpose, ζ\zeta-function regularization is used to perform the mode-by-mode evaluation of BRST-invariant Faddeev-Popov amplitudes in the case of flat Euclidean four-space bounded by a three-sphere. On choosing the de Donder gauge-averaging term, the resulting ζ(0)\zeta(0) value is found to agree with the space-time covariant calculation of the same amplitudes, which relies on the recently corrected geometric formulas for the asymptotic heat kernel in the case of mixed boundary conditions. Two sets of mixed boundary conditions for Euclidean quantum gravity are then compared in detail. The analysis proves that one cannot restrict the path-integral measure to transverse-traceless perturbations. By contrast, gauge-invariant amplitudes are only obtained on considering from the beginning all perturbative modes of the gravitational field, jointly with ghost modes.Comment: 26 pages, plain TeX, no figure

    Chiral bag boundary conditions on the ball

    Get PDF
    Local boundary conditions for spinor fields are expressed in terms of a 1-parameter family of boundary operators, and find applications ranging from (supersymmetric) quantum cosmology to the bag model in quantum chromodynamics. The present paper proves that, for massless spinor fields on the Euclidean ball in dimensions d=2,4,6, the resulting zeta(0) value is independent of such a theta parameter, while the various heat-kernel coefficients exhibit a theta-dependence which is eventually expressed in a simple way through hyperbolic functions and their integer powers.Comment: 30 pages, REVTe

    Strings, p-branes and Skyrmions in curved space

    No full text
    SIGLEAvailable from British Library Document Supply Centre- DSC:DX84887 / BLDSC - British Library Document Supply CentreGBUnited Kingdo
    corecore