460 research outputs found
Broad Band Optical Polarimetric Study of IC 1805
We present the BVR broad band polarimetric observations of 51 stars belonging
to the young open cluster IC 1805. Along with the photometric data from the
literature we have modeled and subtracted the foreground dust contribution from
the maximum polarization (P_{max}) and colour excess (E_{B-V}). The mean value
of the P_max for intracluster medium and the foreground are found to be 5.008
+/-0.005 % and 4.865 +/-0.022 % respectively. Moreover, the mean value of the
wavelength of maximum polarization (lambda_{max}) for intracluster medium is
0.541 +/- 0.003 micro m, which is quite similar as the general interstellar
medium (ISM). The resulting intracluster dust component is found to have
negligible polarization efficiency as compared to interstellar dust. Some of
the observed stars in IC 1805 have shown the indication of intrinsic
polarization in their measurements.Comment: 8 pages, 7 figures, Accepted for publication in MNRA
Coexistence of magnetism and superconductivity in a t-J bilayer
We investigate coexistence of antiferromagnetic and superconducting
correlations in bilayered materials using a two-dimensional t-J model with
couplings across the layers using variational Monte Carlo calculations. It is
found that the underdoped regime supports a coexisting phase, beyond which the
(d-wave) superconducting state becomes stable. Further, the effects of
interplanar coupling parameters on the magnetic and superconducting
correlations as a function of hole doping are studied in details. The magnetic
correlations are found to diminish with increasing interplanar hopping away
from half filling, while the exchange across the layers strengthens interplanar
antiferromagnetic correlations both at and away from half filling. The
superconducting correlations show more interesting features where larger
interplanar hopping considerably reduces planar correlations at optimal doping,
while an opposite behaviour, i.e. stabilisation of the superconducting state is
realised in the overdoped regime, with the interplanar exchange all the while
playing a dormant role.Comment: 8 pages, 9 figures, RevTex4, Submitted to Phys. Rev.
Polarization in young open cluster NGC 6823
We present multiwavelength linear polarimetric observations of 104 stars
towards the region of young open cluster NGC 6823. The polarization towards NGC
6823 is dominated by foreground dust grains and we found the evidence for the
presence of several layers of dust towards the line of sight. The first layer
of dust is located approximately within 200 pc towards the cluster, which is
much closer to the Sun than the cluster (~ 2.1 kpc). The radial distribution of
the position angles for the member stars are found to show a systematic change
while the polarization found to reduce towards the outer parts of the cluster
and the average position angle of coronal region of the cluster is very close
to the inclination of the Galactic parallel (~ 32 degree). The size
distribution of the grains within NGC 6823 is similar to those in general
interstellar medium. The patchy distribution of foreground dust grains are
suggested to be mainly responsible for the both differential reddening and
polarization towards NGC 6823. The majority of the observed stars do not show
the evidence of intrinsic polarization in their light.Comment: 16 pages, 6 tables, 11 figures, Accepted for publication in MNRA
Physical Electronics and Surface Physics
Contains reports on one research project.Joint Services Electronics Program (Contract DAAB07-71-C-0300
The Barrier Method: A Technique for Calculating Very Long Transition Times
In many dynamical systems there is a large separation of time scales between
typical events and "rare" events which can be the cases of interest. Rare-event
rates are quite difficult to compute numerically, but they are of considerable
practical importance in many fields: for example transition times in chemical
physics and extinction times in epidemiology can be very long, but are quite
important. We present a very fast numerical technique that can be used to find
long transition times (very small rates) in low-dimensional systems, even if
they lack detailed balance. We illustrate the method for a bistable
non-equilibrium system introduced by Maier and Stein and a two-dimensional (in
parameter space) epidemiology model.Comment: 20 pages, 8 figure
Computation of nucleation of a non-equilibrium first-order phase transition using a rare-event algorithm
We introduce a new Forward-Flux Sampling in Time (FFST) algorithm to
efficiently measure transition times in rare-event processes in non-equilibrium
systems, and apply it to study the first-order (discontinuous) kinetic
transition in the Ziff-Gulari-Barshad model of catalytic surface reaction. The
average time for the transition to take place, as well as both the spinodal and
transition points, are clearly found by this method.Comment: 12 pages, 10 figure
Multi-wavelength polarimetric study towards the open cluster NGC 1893
We present multi-wavelength linear polarimetric observations for 44 stars of
the NGC 1893 young open cluster region along with V-band polarimetric
observations of stars of other four open clusters located between l ~160 to
~175 degree. We found evidence for the presence of two dust layers located at a
distance of ~170 pc and ~360 pc. The dust layers produce a polarization Pv
~2.2%. It is evident from the clusters studied in the present work that, in the
Galactic longitude range l ~160 to 175 degree and within the Galactic plane
(|b| < 2 degree), the polarization angles remain almost constant, with a mean
~163 degree and a dispersion of 6 degree. The small dispersion in polarization
angle could be due to the presence of uniform dust layer beyond 1 kpc. Present
observations reveal that in case of NGC 1893, the foreground two dust layers,
in addition to the intracluster medium, seems to be responsible for the
polarization effects. It is also found that towards the direction of NGC 1893,
the dust layer that exists between 2-3 kpc has a negligible contribution
towards the total observed polarization. The weighted mean for percentage of
polarization (Pmax) and the wavelength at maximum polarization ({\lambda}max)
are found to be 2.59 \pm 0.02% and 0.55 \pm 0.01 \mum respectively. The
estimated mean value of {\lambda}max indicates that the average size of the
dust grains within the cluster is similar to that in the general interstellar
medium. The spatial variation of the polarization is found to decrease towards
the outer region of the cluster. In the present work, we support the notion, as
already has been shown in previous studies, that polarimetry, in combination
with (U-B)/(B-V) colour-colour diagram, is a useful tool for identifying
non-members in a cluster.Comment: 36 pages, 12 figures, 10 tables, accepted for the publication in
MNRA
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