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Meulders, JP; Slypen, I; Benck, S; Raeymackers, E; Cabrera, J; Dufauquez, Ch; Keutgen, T; Roberfroid, V; Tilquin, I; Masri, Y; Corcalciuc, V; Nica, N
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1 Citations
The experimental setup of LouvainlaNeuve (UCLBelgium) used to perform lightcharged particle production experiment in fast neutroninduced reactions is presented. A short description of the neutron modular detector DEMON is also given. DEMON is a detector array for neutrons emitted in heavy ion induced reactions at low to intermediate energies.
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Gaspard, Pierre; Jain, Sudhir R
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6 Citations
We present a treatment of manybody fermionic systems that facilitates an expression of wellknown quantities in a series expansion inħ. The ensuing semiclassical result contains, to a leading order of the response function, the classical time correlation function of the observable followed by the WeylWigner series; on top of these terms are the periodicorbit correction terms. The treatment given here starts from linear response assumption of the manybody theory and in its connection with semiclassical theory, it assumes that the onebody quantal system has a classically chaotic dynamics. Applications of the framework are also discussed.
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Pandey, B. P.; Vranješ, J.; Parhi, S.
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9 Citations
In the present work, the radiative condensation instability is investigated in the presence of dust charge fluctuations. We find that the charge variability of the grain reduces the growth rate of radiative mode only for fluctuation wavelength smaller or of the order of the Debye length and this reduction is not very large. Far from the Debye sphere, radiative mode can damp due to thermal conduction of electrons and ions
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Borghini, N.; Dinh, P. M.; Ollitrault, J. Y.
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3 Citations
First observations of elliptic flow in AuAu collisions at RHIC have been interpreted as evidence that the colliding system reaches thermal equilibrium. We discuss some of the arguments leading to this conclusion and show that a more accurate analysis is needed, which the standard flow analysis may not provide. We then present a new method of flow analysis, based on a systematic study of multiparticle azimuthal correlations. This method allows one to test quantitatively the collective behaviour of the interacting system. It has recently been applied by the STAR Collaboration at RHIC.
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Heinrichs, J
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We recall some basic aspects of the pinning of flux lines in a superconducting cylindrical shell subjected to a depinning magnetic field, as well as its description by the quantum mechanics of a disordered ring with an imaginary vector potential proportional to the depinning field (N Hatano and D R Nelson, Phys. Rev.B56, 8651 (1997)). We then discuss our recent analysis of the pinningdepinning transition in terms of an explicit solution for the inverse localization length of the eigenstates of the nonhermitian quantum system for weak disorder. Our results as to the nature of the non hermitian quantum states, differ qualitatively from earlier studies which did not examine the detailed properties of the localization length. Nevertheless we obtain a welldefined simple picture for the pinningdepinning transition of flux lines. We discuss furthermore a new exact calculation of localized state eigenenergies for weak disorder, which we compare with previous analytic and numerical results.
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Dubey, Govind; Holst, Bart; Poedts, Stefaan
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3 Citations
The initiation of solar Coronal Mass Ejections (CMEs) is studied in the framework of numerical magnetohydrodynamics (MHD). The initial CME model includes a magnetic flux rope in spherical, axisymmetric geometry. The initial configuration consists of a magnetic flux rope embedded in a gravitationally stratified solar atmosphere with a background dipole magnetic field. The flux rope is in equilibrium due to an image current below the photosphere. An emerging flux triggering mechanism is used to make this equilibrium system unstable. When the magnetic flux emerges within the filament below the flux rope, this results in a catastrophic behavior similar to previous models. As a result, the flux rope rises and a current sheet forms below it. It is shown that the magnetic reconnection in the current sheet below the flux rope in combination with the outward curvature forces results in a fast ejection of the flux rope as observed for solar CMEs. We have done a parametric study of the emerging flux rate.
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Pandey, B. P.; Holst, B.; Vranješ, J.; Poedts, S.
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The dynamics of a selfgravitating unmagnetized, inhomogeneous, streaming dusty plasma is studied in the present work. The presence of the shear flow causes the coupling between gravitational and electrostatic forces. In the absence of selfgravity, the fluctuations in the plasma may grow at the expense of the density inhomogeneity and for certain wavelengths, such an unstable mode may dominate the usual streaming instability. However, in the presence of selfgravity, the plasma inhomogeneity causes an overlap between Jeans and streaming modes and collapse of the grain will continue at all wavelengths.
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Verma, Mahendra K.; Ayyer, Arvind; Debliquy, Olivier; Kumar, Shishir; Chandra, Amar V.
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In this paper we analytically compute the strength of nonlinear interactions in a triad, and the energy exchanges between wavenumber shells in incompressible fluid turbulence. The computation has been done using firstorder perturbative field theory. In three dimensions, magnitude of triad interactions is large for nonlocal triads, and small for local triads. However, the shelltoshell energy transfer rate is found to be local and forward. This result is due to the fact that the nonlocal triads occupy much less Fourier space volume than the local ones. The analytical results on threedimensional shelltoshell energy transfer match with their numerical counterparts. In twodimensional turbulence, the energy transfer rates to the nearby shells are forward, but to the distant shells are backward; the cumulative effect is an inverse cascade of energy.
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Rao, N. Kameswara; Houziaux, L.; Giridhar, Sunetra
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The new spectroscopic observation of MV Sgr obtained at ESO in 1987 July shows enhanced emission lines of He I λ3889, [SII] λ4068 relative to the observations discussed by Jeffreyet al. (1988). The presence of [SII] λ4068 indicates the presence of planetarynebulaelike envelope around the star. Although the radial velocity of the absorption lines and Fe II emission lines do agree with the velocity given by Jeffreyet al., the [SII] λ4068 and probably He I emission lines appear to behave differently.
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Balakrishnan, V; Nicolis, G; Nicolis, C
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2 Citations
The invariant density of onedimensional maps in the regime of fullydeveloped chaos with uncorrelated additive noise is considered. Boundary conditions are shown to play a significant role in determining the precise form of the invariant density, via the manner in which they handle the spillover, caused by the noise, of orbits beyond the interval. The known case of periodic boundary conditions is briefly recapitulated. Analytic solutions for the invariant density that are possible under certain conditions are presented with applications to specific wellknown maps. The case of ‘sticky’ boundaries is generalized to ‘reinjection at the nearest boundary’, and the exact functional equations determining the invariant density are derived. Interesting boundary layer effects are shown to occur, that lead to significant modifications of the invariant density corresponding to the unperturbed (noisefree) case, even when the latter is a constant — as illustrated by an application of the formalism to the noisy tent map. All our results are nonperturbative, and hold good for any noise amplitude in the interval.
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