/ 96 06 19 5 v 1 2 8 Ju n 19 96 Stochastic loop equations

ar X iv : h ep - t h / 96 06 10 4 v 1 1 7 Ju n 19 96 Non - Abelian Stokes Theorem and Quark - Monopole Interaction

We derive a new non-abelian Stokes theorem by rewriting the Wilson loop as a gauge-invariant area integral, at the price of integrating over an auxiliary field from the coset SU(N)/[(U(1)]N−1 space. We then introduce the relativistic quark-monopole interaction as a Wess–Zumino-type action, and extend it to the non-abelian case. We show that condensation of monopoles and confinement can be inves...

ar X iv : a st ro - p h / 96 06 17 9 v 1 2 9 Ju n 19 96 LECTURE 1 Coalescence of Binary Neutron Stars

ar X iv : h ep - t h / 96 06 18 6 v 1 2 7 Ju n 19 96 An Heterotic SUSY Version of one Non – Stable Integrability

By using Heterotic SUSY path integral, one version and generali zation of an integrability theorem due to Mayer is obtained.

ar X iv : h ep - t h / 96 06 06 9 v 1 1 2 Ju n 19 96 UAHEP 958 New Perturbative Solutions of the Kerr – Newman Dilatonic Black Hole Field Equations

This work describes new perturbative solutions to the classical, four-dimensional Kerr–Newman dilaton black hole field equations. Our solutions do not require the black hole to be slowly rotating. The unperturbed solution is taken to be the ordinary Kerr solution, and the perturbation parameter is effectively the square of the charge-to-mass ratio (Q/M) 2 of the Kerr–Newman black hole. We have ...

ar X iv : h ep - t h / 96 06 12 8 v 1 2 0 Ju n 19 96 ON THE EQUATION ∇ × a = κ a

We show that when correctly formulated the equation ∇ × a = κa does not exhibit some inconsistencies atributed to it, so that its solutions can represent physical fields. We want to look for solutions of Maxwell equations which describe stationary electromagnetic configurations – in the sense that the energy of the field does not propagate. In order to obtain one such stationary solution it is ...