15,076 research outputs found

    Neutron Dripline in Odd and Even Mass Calcium and Nickel Nuclei

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    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 72^{72}Ca and 59^{59}Ca, respectively. In Ni isotopes, the corresponding nuclei are 98^{98}Ni and 97^{97}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 YBa2_2Cu3_3O7δ_{7-\delta}

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    The peak effect (PE) has been observed in a twinned crystal of YBa2_2Cu3_3O7δ_{7-\delta} for H\parallelc in the low field range, close to the zero field superconducting transition temperature (Tc_c(0)) . A sharp depinning transition succeeds the peak temperature Tp_p 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 Tp_p(H) values shows a reentrant characteristic with a nose like feature located at Tp_p(H)/Tc_c(0)\approx0.99 and H\approx100 Oe (where the FLL constant a0_0\approxpenetration depth λ\lambda). The upper part of the PE curve (0.5 kOe<<H<<10 kOe) can be fitted to a melting scenario with the Lindemann number cL_L\approx0.25. The vortex phase diagram near Tc_c(0) determined from the characteristic features of the PE in YBa2_2Cu3_3O7δ_{7-\delta}(H\parallelc) bears close resemblance to that in the 2H-NbSe2_2 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

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    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 p11.3p_1 \sim 1.3. The burst appears to be of very low energy (E1048E \sim 10^{48} ergs) confined to a narrow cone of opening angle θ2.3\theta \sim 2.3^{\circ}. 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

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    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

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    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

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    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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