12,337 research outputs found
Numerical estimate of finite size corrections to the free energy of the SK model using Guerra--Toninelli interpolation
I use an interpolating formula introduced by Guerra and Toninelli to
investigate numerically the finite size corrections to the free energy of the
Sherrington--Kirkpatrick model. The results are compatible with a behavior at , as predicted by Parisi, Ritort and Slanina, and
a behavior below
Narrow-band noise due to the moving vortex lattice in superconducting niobium
We report measurements of voltage noise due to vortex motion in Niobium, a
conventional low-Tc superconductor. A coherent oscillation leading to narrow
band noise (NBN) is evidenced. Its characteristic frequency is a linear
function of the overcritical transport current in the flux-flow regime, and
hence scales as the main velocity of the vortex flow. The associated length
scale is not the intervortex distance but the width of the sample, indicating
temporal coherence at a large scale. NBN is also observed in the non linear
part of the V(I) at the onset of depinning, in apparent disagreement with a
stochastic creep motion of flux bundles. NBN exists in the peak effect region,
showing that long range temporal correlations are preserved in this regime.Comment: accepted for publication in Phys Rev
An analyst's take on the BPHZ theorem
We provide a self-contained formulation of the BPHZ theorem in the Euclidean
context, which yields a systematic procedure to "renormalise" otherwise
divergent integrals appearing in generalised convolutions of functions with a
singularity of prescribed order at their origin. We hope that the formulation
given in this article will appeal to an analytically minded audience and that
it will help to clarify to what extent such renormalisations are arbitrary (or
not). In particular, we do not assume any background whatsoever in quantum
field theory and we stay away from any discussion of the physical context in
which such problems typically arise.Comment: Accepted versio
Cosmic microwave background multipole alignments in slab topologies
Several analyses of the microwave sky maps from the Wilkinson Microwave
Anisotropy Probe (WMAP) have drawn attention to alignments amongst the
low-order multipoles. Amongst the various possible explanations, an effect of
cosmic topology has been invoked by several authors. We focus on an alignment
of the first four multipoles (\ell = 2 to 5) found by Land and Magueijo (2005),
and investigate the distribution of their alignment statistic for a set of
simulated cosmic microwave background maps for cosmologies with slab-like
topology. We find that this topology does offer a modest increase in the
probability of the observed value, but that even for the smallest topology
considered the probability of the observed value remains below one percent.Comment: 6 pages RevTex with 6 figures included. Minor changes to match
version accepted as Physical Review D Rapid Communicatio
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