2,816,939 research outputs found
Density Matrix Renormalization Group Method for the Random Quantum One-Dimensional Systems - Application to the Random Spin-1/2 Antiferromagnetic Heisenberg Chain -
The density matrix renormalization group method is generalized to one
dimensional random systems. Using this method, the energy gap distribution of
the spin-1/2 random antiferromagnetic Heisenberg chain is calculated. The
results are consistent with the predictions of the renormalization group theory
demonstrating the effectiveness of the present method in random systems. The
possible application of the present method to other random systems is
discussed.Comment: 13 pages, 3 figures upon reques
Quantum Fourier transform, Heisenberg groups and quasiprobability distributions
This paper aims to explore the inherent connection among Heisenberg groups,
quantum Fourier transform and (quasiprobability) distribution functions.
Distribution functions for continuous and finite quantum systems are examined
first as a semiclassical approach to quantum probability distribution. This
leads to studying certain functionals of a pair of "conjugate" observables,
connected via the quantum Fourier transform. The Heisenberg groups emerge
naturally from this study and we take a rapid look at their representations.
The quantum Fourier transform appears as the intertwining operator of two
equivalent representation arising out of an automorphism of the group.
Distribution functions correspond to certain distinguished sets in the group
algebra. The marginal properties of a particular class of distribution
functions (Wigner distributions) arise from a class of automorphisms of the
group algebra of the Heisenberg group. We then study the reconstruction of
Wigner function from the marginal distributions via inverse Radon transform
giving explicit formulas. We consider applications of our approach to quantum
information processing and quantum process tomography.Comment: 39 page
On the nature of the z=0 X-ray absorbers: I. Clues from an external group
Absorption lines of OVII at redshift zero are observed in high quality
Chandra spectra of extragalactic sightlines. The location of the absorber
producing these lines, whether from the corona of the Galaxy or from the Local
Group or even larger scale structure, has been a matter of debate. Here we
study another poor group like our Local Group to understand the distribution of
column density from galaxy to group scales. We show that we cannot yet rule out
the group origin of z=0 systems. We further argue that the debate over Galactic
vs. extragalactic origin of z=0 systems is premature as they likely contain
both components and predict that future higher resolution observations will
resolve the z=0 systems into multiple components.Comment: Submitted to ApJ
The Elliptical Galaxy formerly known as the Local Group: Merging the Globular Cluster Systems
Prompted by a new catalogue of M31 globular clusters, we have collected
together individual metallicity values for globular clusters in the Local
Group. Although we briefly describe the globular cluster systems of the
individual Local Group galaxies, the main thrust of our paper is to examine the
collective properties. In this way we are simulating the dissipationless merger
of the Local Group, into presumably an elliptical galaxy. Such a merger is
dominated by the Milky Way and M31, which appear to be fairly typical examples
of globular cluster systems of spiral galaxies.
The Local Group `Elliptical' has about 700 +/- 125 globular clusters, with a
luminosity function resembling the `universal' one. The metallicity
distribution has peaks at [Fe/H] ~ -1.55 and -0.64 with a metal-poor to
metal-rich ratio of 2.5:1. The specific frequency of the Local Group Elliptical
is initially about 1 but rises to about 3, when the young stellar populations
fade and the galaxy resembles an old elliptical. The metallicity distribution
and stellar population corrected specific frequency are similar to that of some
known early type galaxies. Based on our results, we briefly speculate on the
origin of globular cluster systems in galaxies.Comment: 22 pages, Latex, 4 figures, 5 tables, submitted to A &
A statistical analysis of the Two Dimensional XMM-Newton Group Survey: The impact of feedback on group properties
(abridged) We present a statistical analysis of 28 nearby galaxy groups from
the Two-Dimensional XMM-Newton Group Survey (2dXGS). We focus on entropy and
the role of feedback, dividing the sample into cool core (CC) and non cool core
(NCC) systems, the first time the latter have been studied in detail in the
group regime. The coolest groups have steeper entropy profiles than the warmest
systems, and NCC groups have higher central entropy and exhibit more scatter
than their CC counterparts. We compare the entropy distribution of the gas in
each system to the expected theoretical distribution ignoring non-gravitational
processes. In all cases, the observed maximum entropy far exceeds that expected
theoretically, and simple models for modifications of the theoretical entropy
distribution perform poorly. Applying initial pre-heating, followed by
radiative cooling, generally fails to match the low entropy behaviour, and only
performs well when the difference between the maximum entropy of the observed
and theoretical distributions is small. Successful feedback models need to work
differentially to increase the entropy range in the gas, and we suggest two
basic possibilities. We analyse the effects of feedback on the entropy
distribution, finding systems with a high measure of `feedback impact' to reach
higher entropy than their low feedback counterparts and also to show
significantly lower central metallicities. If low entropy, metal-rich gas has
been boosted to large entropy in the high feedback systems, it must now reside
outside 0.5r_500, to remain undetected. We find similar levels of enrichment in
both high and low feedback systems, and argue that the lack of extra metals in
the highest feedback systems points to an AGN origin for the bulk of the
feedback, probably acting within precursor structures.Comment: 24 pages, 21 figures; accepted for publication in MNRA
Kinetic description of avalanching systems
Avalanching systems are treated analytically using the renormalization group
(in the self-organized-criticality regime) or mean-field approximation,
respectively. The latter describes the state in terms of the mean number of
active and passive sites, without addressing the inhomogeneity in their
distribution. This paper goes one step further by proposing a kinetic
description of avalanching systems making use of the distribution function for
clusters of active sites. We illustrate application of the kinetic formalism to
a model proposed for the description of the avalanching processes in the
reconnecting current sheet of the Earth magnetosphere.Comment: 9 page
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