O ct 1 99 7 Multichannel Approach to Clustering Matter

0 v 1 9 O ct 1 99 7 Confronting cold dark matter cosmologies with strong clustering of Lyman break galaxies at z ∼ 3

We perform a detailed analysis of the statistical significance of a concentration of Lyman break galaxies at z ∼ 3 recently discovered by Steidel et al. (1997), using a series of N-body simulations with N = 256 particles in a (100hMpc) comoving box. While the observed number density of Lyman break galaxies at z ∼ 3 implies that they correspond to systems with dark matter halos of < ∼ 10 12M⊙, t...

ar X iv : h ep - p h / 98 10 33 5 v 1 1 3 O ct 1 99 8 Gamma - Ray Bursts and Dark Matter - a joint origin ?

x / 99 10 05 8 v 1 2 7 O ct 1 99 9 Rare Φ Decays and Exotic Hadrons

ar X iv : g r - qc / 9 71 01 37 v 1 3 1 O ct 1 99 7 METRIC FLUCTUATIONS IN SEMICLASSICAL GRAVITY ∗

The Einstein-Langevin equation is a perturbative correction to the semiclassical Ein-stein equation which takes into account the lowest order quantum fluctuations of the matter stress-energy tensor. It predicts classical stochastic fluctuations in the metric field which may describe some of the remnant gravitational fluctuations after the process of environment induced decoherence driving the q...

ar X iv : h ep - l at / 9 71 00 36 v 1 9 O ct 1 99 7 1 Heavy Meson Spectroscopy at β = 6 . 0

Charm physics continues to pose difficulties for lattice QCD simulations. The systems are significantly relativistic [1,2] causing problems for the NRQCD approach, and have amQ ≃ O(1) causing significant discretisation effects in the heavy Wilson quark approach. We present the results of a simulation using the tadpole improved clover action and perform the analysis using the Fermilab [3] interp...