496 research outputs found

    Noble Gas Clusters and Nanoplasmas in High Harmonic Generation

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    We report a study of high harmonic generation from noble gas clusters of xenon atoms in a gas jet. Harmonic spectra were investigated as a function of backing pressure, showing spectral shifts due to the nanoplasma electrons in the clusters. At certain value of laser intensity this process may oppose the effect of the well-known ionization-induced blueshift. In addition, these cluster-induced harmonic redshifts may give the possibility to estimate cluster density and cluster size in the laser-gas jet interaction range.Comment: 5 pages, 4 figure

    Space-time extensions II

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    The global extendibility of smooth causal geodesically incomplete spacetimes is investigated. Denote by γ\gamma one of the incomplete non-extendible causal geodesics of a causal geodesically incomplete spacetime (M,gab)(M,g_{ab}). First, it is shown that it is always possible to select a synchronised family of causal geodesics Γ\Gamma and an open neighbourhood U\mathcal{U} of a final segment of γ\gamma in MM such that U\mathcal{U} is comprised by members of Γ\Gamma, and suitable local coordinates can be defined everywhere on U\mathcal{U} provided that γ\gamma does not terminate either on a tidal force tensor singularity or on a topological singularity. It is also shown that if, in addition, the spacetime, (M,gab)(M,g_{ab}), is globally hyperbolic, and the components of the curvature tensor, and its covariant derivatives up to order k1k-1 are bounded on U\mathcal{U}, and also the line integrals of the components of the kthk^{th}-order covariant derivatives are finite along the members of Γ\Gamma---where all the components are meant to be registered with respect to a synchronised frame field on U\mathcal{U}---then there exists a CkC^{k-} extension Φ:(M,gab)(M^,g^ab)\Phi: (M,g_{ab}) \rightarrow (\widehat{M},\widehat{g}_{ab}) so that for each γˉΓ\bar\gamma\in\Gamma, which is inextendible in (M,gab)(M,g_{ab}), the image, Φγˉ\Phi\circ\bar\gamma, is extendible in (M^,g^ab)(\widehat{M},\widehat{g}_{ab}). Finally, it is also proved that whenever γ\gamma does terminate on a topological singularity (M,gab)(M,g_{ab}) cannot be generic.Comment: 42 pages, no figures, small changes to match the published versio

    What does a strongly excited 't Hooft-Polyakov magnetic monopole do?

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    The time evolution of strongly exited SU(2) Bogomolny-Prasad-Sommerfield (BPS) magnetic monopoles in Minkowski spacetime is investigated by means of numerical simulations based on the technique of conformal compactification and on the use of hyperboloidal initial value problem. It is found that an initially static monopole does not radiate the entire energy of the exciting pulse toward future null infinity. Rather, a long-lasting quasi-stable `breathing state' develops in the central region and certain expanding shell structures -- built up by very high frequency oscillations -- are formed in the far away region.Comment: 4 pages, 6 figure

    Derivation of the Matalon-Packter law for Liesegang patterns

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    Theoretical models of the Liesegang phenomena are studied and simple expressions for the spacing coefficients characterizing the patterns are derived. The emphasis is on displaying the explicit dependences on the concentrations of the inner- and the outer-electrolytes. Competing theories (ion-product supersaturation, nucleation and droplet growth, induced sol- coagulation) are treated with the aim of finding the distinguishing features of the theories. The predictions are compared with experiments and the results suggest that the induced sol-coagulation theory is the best candidate for describing the experimental observations embodied in the Matalon-Packter law.Comment: 9 pages, 7 figures, RevTe

    A Note on Hartle-Hawking Vacua

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    The purpose of this note is to establish the basic properties--- regularity at the horizon, time independence, and thermality--- of the generalized Hartle-Hawking vacua defined in static spacetimes with bifurcate Killing horizon admitting a regular Euclidean section. These states, for free or interacting fields, are defined by a path integral on half the Euclidean section. The emphasis is on generality and the arguments are simple but formal.Comment: 5 pages, LaTe
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