15,076 research outputs found
Neutron Dripline in Odd and Even Mass Calcium and Nickel Nuclei
Neutron rich Ca and Ni nuclei have been studied in spherical Relativistic
Mean Field formalism in co-ordinate space. A delta interaction has been has
been adopted to treat the pairing correlations for the neutrons. Odd nuclei
have been treated in the blocking approximation. The effect of the positive
energy continuum and the role of pairing in the stability of nuclei have been
investigated using the resonant-BCS (rBCS) approach. In Ca isotopes, N=50 is no
longer a magic number while in Ni nuclei, a new magic number emerges at N=70.
There is a remarkable difference in the relative positions of the drip lines
for odd and even isotopes. In Ca isotopes, the last bound even and odd nuclei
are found to be Ca and Ca, respectively. In Ni isotopes, the
corresponding nuclei are Ni and Ni, respectively. The origin of
this difference in relative positions of the dripline in even and odd isotopes
in the two chain is traced to the difference in the single particle level
structures and consequent modification in the magic numbers in the two
elements. Pairing interaction is seen to play a major role. The effect of the
width of the resonance states on pairing has also been investigated.Comment: To appear in Physical Review
Amorphization of Vortex Matter and Reentrant Peak Effect in YBaCuO
The peak effect (PE) has been observed in a twinned crystal of
YBaCuO for Hc in the low field range, close to
the zero field superconducting transition temperature (T(0)) . A sharp
depinning transition succeeds the peak temperature T of the PE. The PE
phenomenon broadens and its internal structure smoothens out as the field is
increased or decreased beyond the interval between 250 Oe and 1000 Oe.
Moreover, the PE could not be observed above 10 kOe and below 20 Oe. The locus
of the T(H) values shows a reentrant characteristic with a nose like
feature located at T(H)/T(0)0.99 and H100 Oe (where
the FLL constant apenetration depth ). The upper part of
the PE curve (0.5 kOeH10 kOe) can be fitted to a melting scenario with
the Lindemann number c0.25. The vortex phase diagram near T(0)
determined from the characteristic features of the PE in
YBaCuO(Hc) bears close resemblance to that in
the 2H-NbSe system, in which a reentrant PE had been observed earlier.Comment: 15 pages and 7 figure
Optical Observations and Multiband Modelling of the Afterglow of GRB 041006: Evidence of A Hard Electron Energy Spectrum
We present the CCD Cousins R band photometric observations of the afterglow
of GRB 041006. The multiband afterglow evolution is modelled using an
underlying `hard' electron energy spectrum with a . The burst
appears to be of very low energy ( ergs) confined to a narrow
cone of opening angle . The associated supernova is
compared with SN1998bw and is found to be brighter.Comment: Accepted for publication in Bull. Astr. Soc. India (BASI
Correlated particle dynamics in concentrated quasi-two-dimensional suspensions
We investigate theoretically and experimentally how the hydrodynamically
correlated lateral motion of particles in a suspension confined between two
surfaces is affected by the suspension concentration. Despite the long range of
the correlations (decaying as 1/r^2 with the inter-particle distance r), the
concentration effect is present only at short inter-particle distances for
which the static pair correlation is nonuniform. This is in sharp contrast with
the effect of hydrodynamic screening present in unconfined suspensions, where
increasing the concentration changes the prefactor of the large-distance
correlation.Comment: 13 page
A Late-Time Flattening of Afterglow Light Curves
We present a sample of radio afterglow light curves with measured decay
slopes which show evidence for a flattening at late times compared to optical
and X-ray decay indices. The simplest origin for this behavior is that the
change in slope is due to a jet-like outflow making a transition to
sub-relativistic expansion. This can explain the late-time radio light curves
for many but not all of the bursts in the sample. We investigate several
possible modifications to the standard fireball model which can flatten
late-time light curves. Changes to the shock microphysics which govern particle
acceleration, or energy injection to the shock (either radially or azimuthally)
can reproduce the observed behavior. Distinguishing between these different
possibilities will require simultaneous optical/radio monitoring of afterglows
at late times.Comment: ApJ, submitte
Hydrodynamic interactions of spherical particles in Poiseuille flow between two parallel walls
We study hydrodynamic interactions of spherical particles in incident
Poiseuille flow in a channel with infinite planar walls. The particles are
suspended in a Newtonian fluid, and creeping-flow conditions are assumed.
Numerical results, obtained using our highly accurate Cartesian-representation
algorithm [Physica A xxx, {\bf xx}, 2005], are presented for a single sphere,
two spheres, and arrays of many spheres. We consider the motion of freely
suspended particles as well as the forces and torques acting on particles
adsorbed at a wall. We find that the pair hydrodynamic interactions in this
wall-bounded system have a complex dependence on the lateral interparticle
distance due to the combined effects of the dissipation in the gap between the
particle surfaces and the backflow associated with the presence of the walls.
For immobile particle pairs we have examined the crossover between several
far-field asymptotic regimes corresponding to different relations between the
particle separation and the distances of the particles from the walls. We have
also shown that the cumulative effect of the far-field flow substantially
influences the force distribution in arrays of immobile spheres. Therefore, the
far-field contributions must be included in any reliable algorithm for
evaluating many-particle hydrodynamic interactions in the parallel-wall
geometry.Comment: submitted to Physics of Fluid
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