299 research outputs found

    MAXIMUM MISSILE RANGES FROM CASED EXPLOSIVE CHARGES

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    Curves are calculated and plotted to show maximum missile ranges from TNT changes cased with aluminum or steel of various thicknesses. The maxfmum initial missile velocity is assumed to be 10,000 fps. General trajectory formulas are derived from which the range may be calculated for any initial missile velocity, as determined from the ratio of the case weight to the explosive weight. (auth

    Magnetic order in spin-1 and spin-3/2 interpolating square-triangle Heisenberg antiferromagnets

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    Using the coupled cluster method we investigate spin-ss J1J_{1}-J2J_{2}' Heisenberg antiferromagnets (HAFs) on an infinite, anisotropic, triangular lattice when the spin quantum number s=1s=1 or s=3/2s=3/2. With respect to a square-lattice geometry the model has antiferromagnetic (J1>0J_{1} > 0) bonds between nearest neighbours and competing (J2>0J_{2}' > 0) bonds between next-nearest neighbours across only one of the diagonals of each square plaquette, the same one in each square. In a topologically equivalent triangular-lattice geometry, we have two types of nearest-neighbour bonds: namely the J2κJ1J_{2}' \equiv \kappa J_{1} bonds along parallel chains and the J1J_{1} bonds producing an interchain coupling. The model thus interpolates between an isotropic HAF on the square lattice at κ=0\kappa = 0 and a set of decoupled chains at κ\kappa \rightarrow \infty, with the isotropic HAF on the triangular lattice in between at κ=1\kappa = 1. For both the s=1s=1 and the s=3/2s=3/2 models we find a second-order quantum phase transition at κc=0.615±0.010\kappa_{c}=0.615 \pm 0.010 and κc=0.575±0.005\kappa_{c}=0.575 \pm 0.005 respectively, between a N\'{e}el antiferromagnetic state and a helical state. In both cases the ground-state energy EE and its first derivative dE/dκdE/d\kappa are continuous at κ=κc\kappa=\kappa_{c}, while the order parameter for the transition (viz., the average on-site magnetization) does not go to zero on either side of the transition. The transition at κ=κc\kappa = \kappa_{c} for both the s=1s=1 and s=3/2s=3/2 cases is analogous to that observed in our previous work for the s=1/2s=1/2 case at a value κc=0.80±0.01\kappa_{c}=0.80 \pm 0.01. However, for the higher spin values the transition is of continuous (second-order) type, as in the classical case, whereas for the s=1/2s=1/2 case it appears to be weakly first-order in nature (although a second-order transition could not be excluded).Comment: 17 pages, 8 figues (Figs. 2-7 have subfigs. (a)-(d)

    Foliations of Isonergy Surfaces and Singularities of Curves

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    It is well known that changes in the Liouville foliations of the isoenergy surfaces of an integrable system imply that the bifurcation set has singularities at the corresponding energy level. We formulate certain genericity assumptions for two degrees of freedom integrable systems and we prove the opposite statement: the essential critical points of the bifurcation set appear only if the Liouville foliations of the isoenergy surfaces change at the corresponding energy levels. Along the proof, we give full classification of the structure of the isoenergy surfaces near the critical set under our genericity assumptions and we give their complete list using Fomenko graphs. This may be viewed as a step towards completing the Smale program for relating the energy surfaces foliation structure to singularities of the momentum mappings for non-degenerate integrable two degrees of freedom systems.Comment: 30 pages, 19 figure

    The imposition of Cauchy data to the Teukolsky equation I: The nonrotating case

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    Gravitational perturbations about a Kerr black hole in the Newman-Penrose formalism are concisely described by the Teukolsky equation. New numerical methods for studying the evolution of such perturbations require not only the construction of appropriate initial data to describe the collision of two orbiting black holes, but also to know how such new data must be imposed into the Teukolsky equation. In this paper we show how Cauchy data can be incorporated explicitly into the Teukolsky equation for non-rotating black holes. The Teukolsky function % \Psi and its first time derivative tΨ\partial_t \Psi can be written in terms of only the 3-geometry and the extrinsic curvature in a gauge invariant way. Taking a Laplace transform of the Teukolsky equation incorporates initial data as a source term. We show that for astrophysical data the straightforward Green function method leads to divergent integrals that can be regularized like for the case of a source generated by a particle coming from infinity.Comment: 9 pages, REVTEX. Misprints corrected in formulas (2.4)-(2.7). Final version to appear in PR

    Second order gauge invariant gravitational perturbations of a Kerr black hole

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    We investigate higher than the first order gravitational perturbations in the Newman-Penrose formalism. Equations for the Weyl scalar ψ4,\psi_4, representing outgoing gravitational radiation, can be uncoupled into a single wave equation to any perturbative order. For second order perturbations about a Kerr black hole, we prove the existence of a first and second order gauge (coordinates) and tetrad invariant waveform, ψI\psi_I, by explicit construction. This waveform is formed by the second order piece of ψ4\psi_4 plus a term, quadratic in first order perturbations, chosen to make ψI\psi_I totally invariant and to have the appropriate behavior in an asymptotically flat gauge. ψI\psi_I fulfills a single wave equation of the form TψI=S,{\cal T}\psi_I=S, where T{\cal T} is the same wave operator as for first order perturbations and SS is a source term build up out of (known to this level) first order perturbations. We discuss the issues of imposition of initial data to this equation, computation of the energy and momentum radiated and wave extraction for direct comparison with full numerical approaches to solve Einstein equations.Comment: 19 pages, REVTEX. Some misprints corrected and changes to improve presentation. Version to appear in PR

    Onset of Superfluidity in 4He Films Adsorbed on Disordered Substrates

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    We have studied 4He films adsorbed in two porous glasses, aerogel and Vycor, using high precision torsional oscillator and DC calorimetry techniques. Our investigation focused on the onset of superfluidity at low temperatures as the 4He coverage is increased. Torsional oscillator measurements of the 4He-aerogel system were used to determine the superfluid density of films with transition temperatures as low as 20 mK. Heat capacity measurements of the 4He-Vycor system probed the excitation spectrum of both non-superfluid and superfluid films for temperatures down to 10 mK. Both sets of measurements suggest that the critical coverage for the onset of superfluidity corresponds to a mobility edge in the chemical potential, so that the onset transition is the bosonic analog of a superconductor-insulator transition. The superfluid density measurements, however, are not in agreement with the scaling theory of an onset transition from a gapless, Bose glass phase to a superfluid. The heat capacity measurements show that the non-superfluid phase is better characterized as an insulator with a gap.Comment: 15 pages (RevTex), 21 figures (postscript

    Chaos and the Quantum Phase Transition in the Dicke Model

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    We investigate the quantum chaotic properties of the Dicke Hamiltonian; a quantum-optical model which describes a single-mode bosonic field interacting with an ensemble of NN two-level atoms. This model exhibits a zero-temperature quantum phase transition in the N \go \infty limit, which we describe exactly in an effective Hamiltonian approach. We then numerically investigate the system at finite NN and, by analysing the level statistics, we demonstrate that the system undergoes a transition from quasi-integrability to quantum chaotic, and that this transition is caused by the precursors of the quantum phase-transition. Our considerations of the wavefunction indicate that this is connected with a delocalisation of the system and the emergence of macroscopic coherence. We also derive a semi-classical Dicke model, which exhibits analogues of all the important features of the quantum model, such as the phase transition and the concurrent onset of chaos.Comment: 51 pages, 15 figures, late

    In situ simultaneous photovoltaic and structural evolution of perovskite solar cells during film formation

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    Metal-halide perovskites show remarkably clean semiconductor behaviour, as evidenced by their excellent solar cell performance, in spite of the presence of many structural and chemical defects. Here, we show how this clean semiconductor performance sets in during the earliest phase of conversion from the metal salts and organic-based precursors and solvent, using simultaneous in situ synchrotron X-ray and in operando current–voltage measurements on films prepared on interdigitated back-contact substrates. These structures function as working solar cells as soon as sufficient semiconductor material is present across the electrodes. We find that at the first stages of conversion from the precursor phase, at the percolation threshold for bulk conductance, high photovoltages are observed, even though the bulk of the material is still present as precursors. This indicates that at the earliest stages of perovskite structure formation, the semiconductor gap is already well-defined and free of sub-gap trap states. The short circuit current, in contrast, continues to grow until the perovskite phase is fully formed, when there are bulk pathways for charge diffusion and collection. This work reveals important relationships between the precursors conversion and device performance and highlights the remarkable defect tolerance of perovskite materials
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