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    Two-dimensional melting far from equilibrium in a granular monolayer

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    We report an experimental investigation of the transition from a hexagonally ordered solid phase to a disordered liquid in a monolayer of vibrated spheres. The transition occurs as the intensity of the vibration amplitude is increased. Measurements of the density of dislocations and the positional and orientational correlation functions show evidence for a dislocation-mediated continuous transition from a solid phase with long-range order to a liquid with only short-range order. The results show a strong similarity to simulations of melting of hard disks in equilibrium, despite the fact that the granular monolayer is far from equilibrium due to the effects of interparticle dissipation and the vibrational forcing.Comment: 4 pages, 4 figure

    Functional determinants on certain domains

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    Functional determinants on various domains of the sphere and flat space are presented for scalar and spinor fields.Comment: 14p, plain TeX, talk presented at the 6th Moscow Quantum Gravity Seminar, Moscow, June 12-19, 1995.(Minor errors corrected.

    Deflationary cosmology: constraints from angular size and ages of globular clusters

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    Observational constraints to a large class of decaying vacuum cosmologies are derived using the angular size data of compact radio sources and the latest age estimates of globular clusters. For this class of deflationary Λ(t)\Lambda(t) models, the present value of the vacuum energy density is quantified by a positive β\beta parameter smaller than unity. In the case of milliarcsecond compact radio-sources, we find that the allowed intervals for β\beta and the matter density parameter Ωm\Omega_m are heavily dependent on the value of the mean projected linear size ll. For l≃20h−1−30h−1l \simeq 20h^{-1} - 30h^{-1} pc, the best fit occurs for β∼0.58\beta \sim 0.58, Ωm∼0.58\Omega_{\rm{m}} \sim 0.58, and β∼0.76\beta \sim 0.76, Ωm∼0.28\Omega_{\rm{m}} \sim 0.28, respectively. This analysis shows that if one minimizes χ2\chi^{2} for the free parameters ll, Ωm\Omega_{\rm{m}} and β\beta, the best fit for these angular size data corresponds to a decaying Λ(t)\Lambda(t) with Ωm=0.54\Omega_{\rm{m}} = 0.54 β=0.6\beta=0.6 and l=22.64h−1l = 22.64h^{-1} pc. Constraints from age estimates of globular clusters and old high redshift galaxies are not so restrictive, thereby suggesting that there is no age crisis for this kind of Λ(t)\Lambda(t) cosmologies.Comment: 6 pages, 3 figures, revised version to appear in Phys. Rev.

    Heat kernels on curved cones

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    A functorial derivation is presented of a heat-kernel expansion coefficient on a manifold with a singular fixed point set of codimension two. The existence of an extrinsic curvature term is pointed out.Comment: 4p.,sign errors corrected and a small addition,uses JyTeX,MUTP/94/0
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