3,675,299 research outputs found
General form of the deformation of Poisson superbracket on (2,2)-dimensional superspace
Continuous formal deformations of the Poisson superbracket defined on
compactly supported smooth functions on n-dimensional space taking values in a
Grassmann algebra with m generating elements are described up to an equivalence
transformation for the case n=m=2. It is shown that in this case the Poisson
superalgebra has an additional deformation comparing with other superdimensions
(n,m).Comment: LaTex, 13 page
Low mass variable stars in the globular cluster NGC 6397
We have conducted a photometric survey of the globular cluster NGC 6397 in a
search for variable stars. We obtained ~11h of time-resolved photometric images
with one ne European Southern Observatory-Very Large Telescope using the FOcal
Reducer and low dispersion Spectrograph imager distributed over two consecutive
nights. We analyzed 8391 light curves of stars brighter than magnitude 23 with
the 465 nm-filter, and we identified 412 variable stars, reaching ~ 4.8 +- 0.2
per cent of variability with timescales between 0.004 and 2d, with amplitudes
variation greater than +- 0.2 mag.Comment: 9 figures, complementary dat
Galactic longitude dependent Galactic model parameters
We present the Galactic model parameters for thin disc estimated by Sloan
Digital Sky Survey (SDSS) data of 14 940 stars with apparent magnitudes
in six intermediate latitude fields in the first Galactic
quadrant. Star/galaxy separation was performed by using the photometric
pipeline and the isodensity contours in the two colour
diagram. The separation of thin disc stars is carried out by the bimodal
distribution of stars in the histogram, and the absolute magnitudes
were evaluated by a procedure presented in the literature Bilir et al. (2005).
Exponential density law fits better to the derived density functions for the
absolute magnitude intervals and , whereas
sech/sech laws are more appropriate for absolute magnitude intervals
and . We showed that the scaleheight and
scalelength are Galactic longitude dependent. The average values and ranges of
the scaleheight and the scalelength are pc ( pc)
and pc ( pc) respectively. This result would
be useful to explain different numerical values claimed for those parameters
obtained by different authors for the fields in different directions of the
Galaxy.Comment: 28 pages, including 12 figures and 7 tables, accepted for publication
in New Astronom
A cluster algorithm for resistively shunted Josephson junctions
We present a cluster algorithm for resistively shunted Josephson junctions
and similar physical systems, which dramatically improves sampling efficiency.
The algorithm combines local updates in Fourier space with rejection-free
cluster updates which exploit the symmetries of the Josephson coupling energy.
As an application, we consider the localization transition of a single junction
at intermediate Josephson coupling and determine the temperature dependence of
the zero bias resistance as a function of dissipation strength.Comment: 4 page
Measurement of charm production in deep inelastic scattering with the ZEUS detector
We present measurements of charm production in DIS using the ZEUS detector.
Data with an integrated luminosity of 83 pb have been analysed. For the
channel a
cross section has been extracted, differential in the kinematical variables
and Bjorken . In addition the decay has been studied in a data sample of an integrated
luminosity of 34 pb. This results in a cross section, differential in
, and of the event and in and of the decay electron.
The structure function f2-charm has also been determined for this channel. All
measured cross sections show good agreement with NLO pQCD predictions from
HVQDIS.Comment: 4 pages, 4 figures. As presented at DIS01 Bologna, Ital
Integrated p-channel MOS gyrator
Several circuits can be integrated into one chip for applications which require more than one gyrator. They can also be integrated with other p-channel MOS circuits to eliminate need for external connections. Devices can operate at economical low-power levels, because they use FET amplifiers that do not degrade with decreases in supply
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