18,102 research outputs found
GRB000301C with peculiar afterglow emission
The CCD magnitudes in Johnson V and Cousins R and I photometric passbands are
determined for GRB 000301C afterglow starting ~ 1.5 day after the gamma-ray
burst. In fact we provide the earliest optical observations for this burst.
Light curves of the afterglow emissions in U, B, V, R, I, J and K' passbands
are obtained by combining the present measurements with the published data.
Flux decay shows a very uncommon variation relative to other well observed
GRBs. Overall, there is a steepening of the optical and near-infrared flux
decay caused by a geometric and sideways expanding jet. This is superimposed by
a short term variability especially during early time (Delta t < 8 days). The
cause of variability is not well understood, though it has occurred
simultaneously with similar amplitude in all the filters. We derive the early
and late time flux decay constants using jet model. The late time flux decay is
the steepest amongst the GRB OTs observed so far with alpha ~ 3. Steepening in
the flux decay seems to have started simultaneously around Delta t ~ 7.6 day in
all passbands. The value of spectral index in the optical-near IR region is ~
-1.0. Redshift determination with z=2.0335 indicates cosmological origin of the
GRB having a luminosity distance of 16.6 Gpc. Thus it becomes the second
farthest amongst the GRBs with known distances. An indirect estimate of the
fluence > 20 keV indicates, if isotropic,> =10^53 ergs of release of energy.
The enormous amount of released energy will be reduced, if the radiation is
beamed which is the case for this event. Using a jet break time of 7.6 days, we
infer a jet opening angle of ~ 0.15 radian. This means the energy released is
reduced by a factor of ~ 90 relative to the isotropic value.Comment: LaTeX file, 11 pages including 4 figures, uses psfig.sty, Bull.
Astron. Society of India(accepted, Sept, 2000 issue
Shallow Deep Transitions of Neutral and Charged Donor States in Semiconductor Quantum Dots
We carry out a detailed investigation of neutral () and charged ()
impurity states of hydrogen-like donors in spherical semiconductor quantum
dots. The investigation is carried out within the effective mass theory (EMT).
We take recourse to local density approximation (LDA) and the Harbola-Sahni
(HS) schemes for treating many-body effects. We experiment with a variety of
confining potentials: square, harmonic and triangular. We observe that the
donor level undergoes shallow to deep transition as the dot radius () is
reduced. On further reduction of the dot radius it becomes shallow again. We
term this non-monotonic behaviour \textbf{SHADES}. This suggests the
possibility of carrier {\textbf{\textit{``freeze out''}}} for both and
. Further, our study of the optical gaps also reveals a {\textbf{SHADES}}
transition.Comment: 19 pages, 8 figures, Revised Versio
BVRI CCD photometric standards in the field of GRB 990123
The CCD magnitudes in Johnson and Cousins photometric passbands are
determined for 18 stars in the field of GRB 990123. These measurements can be
used in carrying out precise CCD photometry of the optical transient of GRB
990123 using differential photometric techniques during non--photometric sky
conditions. A comparison with previous photometry indicates that the present
photmetry is more precise.Comment: Tex file, 5 pages with 1 figure. Bull. Astron. Society India, Vol. 27
(accepted
The effect of asymmetric disorder on the diffusion in arbitrary networks
Considering diffusion in the presence of asymmetric disorder, an exact
relationship between the strength of weak disorder and the electric resistance
of the corresponding resistor network is revealed, which is valid in arbitrary
networks. This implies that the dynamics are stable against weak asymmetric
disorder if the resistance exponent of the network is negative. In the
case of , numerical analyses of the mean first-passage time on
various fractal lattices show that the logarithmic scaling of with the
distance , , is a general rule, characterized by a new
dynamical exponent of the underlying lattice.Comment: 5 pages, 4 figure
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