On the Transition from Crystalline to Dynamically Triangulated Surfaces

ArXiv hep-lat/9308005 (1993)

Authors:

Neil Ferguson, JF Wheater

Abstract:

We consider methods of interpolating between the crystalline and dynamically triangulated random surface models. We argue that actions based on the deviation from six of the coordination number at a site are inadequate and propose an alternative based on Alexander moves. Two simplified models, one of which has a phase transition and the other of which does not, are discussed.

On the Transition from Crystalline to Dynamically Triangulated Surfaces

(1993)

Authors:

Neil Ferguson, JF Wheater

The confining string and its tension for SU(2) gauge fields in 2 + 1 dimensions

Physics Letters B 311:1-4 (1993) 223-229

Abstract:

We investigate confinement in D = 3 SU(2) lattice gauge theory. We confirm the approximately linear character of confinement at large distances. The corresponding continuum string tension is found to be √σ/g2 = 0.3340 ± 0.0025. We also find that the flux is located within a tube and that the width of this flux tube is l0{reversed tilde equals} 1.22/Tc where Tc is the deconfining temperature. The dominant fluctuations of the confining flux tube appear to be simple wavelike oscillations. This is remarkably similar to the expected properties of confinement in four dimensions. © 1993.

NJL breaking of supersymmetric GUTs

(1993)

Authors:

EJ Chun, A Lukas

Cosmic neutrinos from unstable relic particles

Nuclear Physics, Section B 392:1 (1993) 111-133

Authors:

P Gondolo, G Gelmini, S Sarkar

Abstract:

We derive constraints on the relic abundance of a generic particle of mass ∼ 1-1014 TeV which decays into neutrinos at cosmological epochs, using data from the Fréjus and IMB nucleon decay detectors and the Fly's Eye air-shower array. The lifetime of such unstable particles which may constitute the dark matter today is bounded to be greater than ∼ 1014-1018 yr, depending on the mass. For lifetimes shorter than the age of the universe, neutrino energy losses due to scattering and the expansion redshift become important and set limits to the ability of neutrino observatories to probe the early universe. © 1993.