Gauge five-brane moduli in four-dimensional heterotic models

Physical Review D - Particles, Fields, Gravitation and Cosmology 70:8 (2004)

Authors:

J Gray, A Lukas

Abstract:

We present a Kähler potential for four-dimensional heterotic M-theory which includes moduli describing a gauge five-brane living on one of the orbifold fixed planes. This result can also be thought of as describing compactifications of either of the weakly coupled heterotic strings in the presence of a gauge five-brane. This is the first example of a Kähler potential in these theories which includes moduli describing background gauge field configurations. Our results are valid when the solitons width is much smaller than the size scale of the Calabi-Yau threefold and can be used to provide a more complete description of some moving brane scenarios. We point out that, in general, it is not consistent to truncate away the gauge five-brane moduli in a simple manner. © 2004 The American Physical Society.

Kink-boundary collisions in a two-dimensional scalar field theory

Physical Review D - Particles, Fields, Gravitation and Cosmology 69:6 (2004) 11

Authors:

ND Antunes, EJ Copeland, M Hindmarsh, A Lukas

Abstract:

In a two-dimensional toy model, motivated from five-dimensional heterotic M theory, we study the collision of scalar field kinks with boundaries. By numerical simulation of the full two-dimensional theory, we find that the kink is always inelastically reflected with a model-independent fraction of its kinetic energy converted into radiation. We show that the reflection can be analytically understood as a fluctuation around the scalar field vacuum. This picture suggests the possibility of spontaneous emission of kinks from the boundary due to small perturbations in the bulk. We verify this picture numerically by showing that the radiation emitted from the collision of an initial single kink eventually leads to a bulk populated by many kinks. Consequently, processes changing the boundary charges are practically unavoidable in this system. We speculate that the system has a universal final state consisting of a stack of kinks, their number being determined by the initial energy. © 2004 The American Physical Society.

Moduli Kähler potential for M theory on a [Formula Presented] manifold

Physical Review D - Particles, Fields, Gravitation and Cosmology 69:6 (2004) 17

Authors:

A Lukas, S Morris

Abstract:

We compute the moduli Kähler potential for M theory on a compact manifold of [Formula Presented] holonomy in a large radius approximation. Our method relies on an explicit [Formula Presented] structure with small torsion, its periods and the calculation of the approximate volume of the manifold. As a verification of our result, some of the components of the Kähler metric are computed directly by integration over harmonic forms. We also discuss the modification of our result in the presence of codimension-four singularities and derive the gauge-kinetic functions for the massless gauge fields that arise in this case. © 2004 The American Physical Society.

Reply to “Comment on ‘Clustering of ultrahigh energy cosmic rays and their sources’ ”

Physical Review D - Particles, Fields, Gravitation and Cosmology 69:12 (2004)

Authors:

NW Evans, F Ferrer, S Sarkar

Abstract:

We reiterate that there is no evidence that BL Lacs are sources of ultrahigh energy cosmic rays. © 2004 The American Physical Society.

Rolling G2 moduli

Journal of High Energy Physics 8:1 (2004) 1169-1184

Authors:

A Lukas, S Morris

Abstract:

We study the time evolution of freely rolling moduli in the context of M-theory on a G2 manifold. This free evolution approximates the correct dynamics of the system at sufficiently large values of the moduli when effects from non-perturbative potentials and flux are negligible. Moduli fall into two classes, namely bulk moduli and blow-up moduli. We obtain a number of non-trivial solutions for the time-evolution of these moduli. As a generic feature, we find the blow-up moduli always expand asymptotically at early and late time. © SISSA/ISAS 2004.