3,662 research outputs found
Quantization on a torus without position operators
We formulate quantum mechanics in the two-dimensional torus without using
position operators. We define an algebra with only momentum operators and shift
operators and construct irreducible representation of the algebra. We show that
it realizes quantum mechanics of a charged particle in a uniform magnetic
field. We prove that any irreducible representation of the algebra is unitary
equivalent to each other. This work provides a firm foundation for the
noncommutative torus theory.Comment: 12 pages, LaTeX2e, the title is changed, minor corrections are made,
references are added. To be published in Modern Physics Letters
The effect of stellar-mass black holes on the structural evolution of massive star clusters
We present the results of realistic N-body modelling of massive star clusters
in the Magellanic Clouds, aimed at investigating a dynamical origin for the
radius-age trend observed in these systems. We find that stellar-mass black
holes, formed in the supernova explosions of the most massive cluster stars,
can constitute a dynamically important population. If a significant number of
black holes are retained (here we assume complete retention), these objects
rapidly form a dense core where interactions are common, resulting in the
scattering of black holes into the cluster halo, and the ejection of black
holes from the cluster. These two processes heat the stellar component,
resulting in prolonged core expansion of a magnitude matching the observations.
Significant core evolution is also observed in Magellanic Cloud clusters at
early times. We find that this does not result from the action of black holes,
but can be reproduced by the effects of mass-loss due to rapid stellar
evolution in a primordially mass segregated cluster.Comment: Accepted for publication in MNRAS Letters; 2 figures, 1 tabl
Surface Brightness Profiles and Structural Parameters for 53 Rich Stellar Clusters in the Large Magellanic Cloud
We have compiled a pseudo-snapshot data set of two-colour observations from
the Hubble Space Telescope archive for a sample of 53 rich LMC clusters with
ages 10^6-10^10 yr. We present surface brightness profiles for the entire
sample, and derive structural parameters for each cluster, including core
radii, and luminosity and mass estimates. Because we expect the results
presented here to form the basis for several further projects, we describe in
detail the data reduction and surface brightness profile construction
processes, and compare our results with those of previous ground-based studies.
The surface brightness profiles show a large amount of detail, including
irregularities in the profiles of young clusters (such as bumps, dips, and
sharp shoulders), and evidence for both double clusters and post core-collapse
(PCC) clusters. In particular we find power-law profiles in the inner regions
of several candidate PCC clusters, with slopes of approximately -0.7, but
showing considerable variation. We estimate that 20 +/- 7 % of the old cluster
population of the LMC has entered PCC evolution, a similar fraction to that for
the Galactic globular cluster system. In addition, we examine the profile of
R136 in detail and show that it is probably not a PCC cluster. We also observe
a trend in core radius with age that has been discovered and discussed in
several previous publications by different authors. Our diagram has better
resolution however, and appears to show a bifurcation at several hundred Myr.
We argue that this observed relationship reflects true physical evolution in
LMC clusters, with some experiencing small scale core expansion due to mass
loss, and others large scale expansion due to some unidentified characteristic
or physical process.Comment: Accepted for publication in MNRAS. 24 pages plus 16 figures and 9
pages of profiles. We strongly recommend that the interested reader visit
http://www.ast.cam.ac.uk/STELLARPOPS/LMC_clusters/ for on-line data and the
full resolution pape
Models of the circumstellar medium of evolving, massive runaway stars moving through the Galactic plane
At least 5 per cent of the massive stars are moving supersonically through
the interstellar medium (ISM) and are expected to produce a stellar wind bow
shock. We explore how the mass loss and space velocity of massive runaway stars
affect the morphology of their bow shocks. We run two-dimensional axisymmetric
hydrodynamical simulations following the evolution of the circumstellar medium
of these stars in the Galactic plane from the main sequence to the red
supergiant phase. We find that thermal conduction is an important process
governing the shape, size and structure of the bow shocks around hot stars, and
that they have an optical luminosity mainly produced by forbidden lines, e.g.
[OIII]. The Ha emission of the bow shocks around hot stars originates from near
their contact discontinuity. The H emission of bow shocks around cool
stars originates from their forward shock, and is too faint to be observed for
the bow shocks that we simulate. The emission of optically-thin radiation
mainly comes from the shocked ISM material. All bow shock models are brighter
in the infrared, i.e. the infrared is the most appropriate waveband to search
for bow shocks. Our study suggests that the infrared emission comes from near
the contact discontinuity for bow shocks of hot stars and from the inner region
of shocked wind for bow shocks around cool stars. We predict that, in the
Galactic plane, the brightest, i.e. the most easily detectable bow shocks are
produced by high-mass stars moving with small space velocities.Comment: 22 pages, 24 figure
What measurable zero point fluctuations can(not) tell us about dark energy
We show that laboratory experiments cannot measure the absolute value of dark
energy. All known experiments rely on electromagnetic interactions. They are
thus insensitive to particles and fields that interact only weakly with
ordinary matter. In addition, Josephson junction experiments only measure
differences in vacuum energy similar to Casimir force measurements. Gravity,
however, couples to the absolute value. Finally we note that Casimir force
measurements have tested zero point fluctuations up to energies of ~10 eV, well
above the dark energy scale of ~0.01 eV. Hence, the proposed cut-off in the
fluctuation spectrum is ruled out experimentally.Comment: 4 page
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