Five-branes in heterotic brane-world theories
Physical Review D 65:6 (2002)
Abstract:
The effective action for five-dimensional heterotic M theory in the presence of five-branes is systematically derived from Hořava-Witten theory coupled to an M5-brane world-volume theory. This leads to a five-dimensional N=1 gauged supergravity theory on S1/ZFive-dimensional moving brane solutions with four-dimensional limiting behavior
Physical Review D Particles Fields Gravitation and Cosmology 66:12 (2002)
Abstract:
Under certain conditions some solutions to five-dimensional heterotic M theory can be accurately described by the four-dimensional action of the theory. We consider the connection between solutions of four- and five-dimensional heterotic M theory when moving five-branes are present in the bulk. We begin by describing how to raise the known four-dimensional moving brane solutions to obtain approximate solutions to the five-dimensional theory, presenting for the first time the metric template necessary for this procedure. We then present the first solutions to the five-dimensional theory containing moving five-branes. We then discuss the correspondence between solutions of the five- and four-dimensional actions as presented. Specifically, we show that our exact, five-dimensional solution only corresponds to one of the previously known four-dimensional solutions when the embedded five-brane is static. In other words, higher Kaluza-Klein modes are essential in the description of the five-brane’s motion in our new solution. © 2002 The American Physical Society.Glueball spectrum in O(a)-improved lattice QCD
Physical Review D 65:3 (2002)
Abstract:
We calculate the light "glueball" mass spectrum in NNo cosmological domain wall problem for weakly coupled fields
Physical Review D 65:2 (2002)
Abstract:
After inflation occurs, a weakly coupled scalar field will in general not be in thermal equilibrium but have a distribution of values determined by the inflationary Hubble parameter. If such a field subsequently undergoes discrete symmetry breaking, then the different degenerate vacua may not be equally populated so the domain walls which form will be "biased" and the wall network will subsequently collapse. Thus the cosmological domain wall problem may be solved for sufficiently weakly coupled fields in a post inflationary universe. We quantify the criteria for determining whether this does happen, using a Higgs-like potential, with a spontaneously broken ZQuasinormal modes of near extremal black branes
Physical Review D Particles Fields Gravitation and Cosmology 66:12 (2002)