5,612 research outputs found
Biochemical Aspects of Genetics
It would be impossible, in the time and space available, to cover all of the noteworthy advances that have been made in biochemical genetics during the past year. We have, therefore, selected for review a number of topics that are especially active at the moment and that promise to yield important new results in the near future. At the same time, we have tried to avoid duplicating the material of other chapters in this volume which are germane to biochemical genetics. We refer, in particular, to the chapters on Metabolism of Nucleic Acids (Macromolecular DNA and RNA); Nucleic Acids and Protein Biosynthesis; The Basic Proteins of Cell Nuclei; and Chemistry of Differentiation in Lower Organisms. The reader should consult these reviews, as well as the present one, for a fuller view of current activities in this field
Unitarity, quasi-normal modes and the AdS_3/CFT_2 correspondence
In general, black-hole perturbations are governed by a discrete spectrum of
complex eigen-frequencies (quasi-normal modes). This signals the breakdown of
unitarity. In asymptotically AdS spaces, this is puzzling because the
corresponding CFT is unitary. To address this issue in three dimensions, we
replace the BTZ black hole by a wormhole, following a suggestion by Solodukhin
[hep-th/0406130]. We solve the wave equation for a massive scalar field and
find an equation for the poles of the propagator. This equation yields a rich
spectrum of {\em real} eigen-frequencies. We show that the throat of the
wormhole is , where is Newton's constant. Thus, the quantum
effects which might produce the wormhole are non-perturbative.Comment: 9 page
Poincare recurrences of Schwarzschild black holes
We discuss massive scalar perturbations of a Schwarzschild black hole. We
argue that quantum effects alter the effective potential near the horizon
resulting in Poincare recurrences in Green functions. Results at the
semi-classical level are independent of the details of the modification of the
potential provided its minimum near the horizon is inversely proportional to
the square of the Poincare time. This modification may be viewed as a change in
the near-horizon geometry. We consider explicitly the examples of a brick wall,
a smooth cutoff and a wormhole-like modification showing that they all lead to
the same results at leading order.Comment: 15 page
Nonequilibrium Detailed Fluctuation Theorem for Repeated Discrete Feedback
We extend the framework of forward and reverse processes commonly utilized in
the derivation and analysis of the nonequilibrium work relations to
thermodynamic processes with repeated discrete feedback. Within this framework,
we derive a generalization of the detailed fluctuation theorem, which is
modified by the addition of a term that quantifies the change in uncertainty
about the microscopic state of the system upon making measurements of physical
observables during feedback. As an application, we extend two nonequilibrium
work relations: the nonequilibrium work fluctuation theorem and the
relative-entropy work relation.Comment: 7 pages, 3 figure
Viking on Mars: The carbon assimilation experiments
A fixation of atmospheric carbon, presumably into organic form, occurs in Martian surface material under conditions approximating the actual Martian ones. The reaction showed the following characteristics: The amount of carbon fixed is small by terrestrial standards; highest yields were observed in the light, but some dark activity was also detected; and heating the surface material to 90°C for nearly 2 hours had no effect on the reaction, but heating to 175°C for 3 hours reduced it by nearly 90%. New data from Mars do not support an earlier suggestion that the reaction is inhibited by traces of water. There is evidence of considerable heterogeneity among different samples, but different aliquots from the same sample are remarkably uniform in their carbon-fixing capacity. In view of its thermostability it is unlikely that the reaction is biological
Comments on Black Holes in Matrix Theory
The recent suggestion that the entropy of Schwarzschild black holes can be
computed in matrix theory using near-extremal D-brane thermodynamics is
examined. It is found that the regime in which this approach is valid actually
describes black strings stretched across the longitudinal direction, near the
transition where black strings become unstable to the formation of black holes.
It is argued that the appropriate dynamics on the other (black hole) side of
the transition is that of the zero modes of the corresponding super Yang-Mills
theory. A suggestive mean field theory argument is given for the entropy of
black holes in all dimensions. Consequences of the analysis for matrix theory
and the holographic principle are discussed.Comment: 15 pages, harvmac, minor errors correcte
Designing optimal discrete-feedback thermodynamic engines
Feedback can be utilized to convert information into useful work, making it
an effective tool for increasing the performance of thermodynamic engines.
Using feedback reversibility as a guiding principle, we devise a method for
designing optimal feedback protocols for thermodynamic engines that extract all
the information gained during feedback as work. Our method is based on the
observation that in a feedback-reversible process the measurement and the
time-reversal of the ensuing protocol both prepare the system in the same
probabilistic state. We illustrate the utility of our method with two examples
of the multi-particle Szilard engine.Comment: 15 pages, 5 figures, submitted to New J. Phy
Neutrino Trapping in a Supernova and Ion Screening
Neutrino-nucleus elastic scattering is reduced in dense matter because of
correlations between ions. The static structure factor for a plasma of
electrons and ions is calculated from Monte Carlo simulations and parameterized
with a least squares fit. Our results imply a large increase in the neutrino
mean free path. This strongly limits the trapping of neutrinos in a supernova
by coherent neutral current interactions.Comment: 9 pages, 1 postscript figure using epsf.st
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