37,413 research outputs found

    Non-dopplerian cosmological redshift parameters in a model of graviton-dusty universe

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    Possible effects are considered which would be caused by a hypothetical superstrong interaction of photons or massive bodies with single gravitons of the graviton background. If full cosmological redshift magnitudes are caused by the interaction, then the luminosity distance in a flat non-expanding universe as a function of redshift is very similar to the specific function which fits supernova cosmology data by Riess et al. From another side, in this case every massive body, slowly moving relatively to the background, would experience a constant acceleration, proportional to the Hubble constant, of the same order as a small additional acceleration of Pioneer 10, 11.Comment: 5 pages. It was presented: at SIGRAV'2000 Congress, Italy (this version); in Proc. of the Int. Symp. "FFP 4" (9-13 Dec 2000, Hyderabad, India), Sidharth& Altaisky, Eds., Kluwer Academic/Plenum, 2001;in Proc. of the 4th Edoardo Amaldi Conference on GW (Perth, W. Australia, 8-13 July 2001

    Allowed charge transfers between coherent conductors driven by a time-dependent scatterer

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    We derive constraints on the statistics of the charge transfer between two conductors in the model of arbitrary time-dependent instant scattering of non-interacting fermions at zero temperature. The constraints are formulated in terms of analytic properties of the generating function: its zeroes must lie on the negative real axis. This result generalizes existing studies for scattering by a time-independent scatterer under time-dependent bias voltage.Comment: 5 pages, no figures, corrected misprints and minor changes in version

    A model of gravitation with global U(1)-symmetry

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    It is shown that an embedding of the general relativity 44-space into a flat 1212-space gives a model of gravitation with the global U(1)U(1)-symmetry and the discrete D1D_{1}-one. The last one may be transformed into the SU(2)SU(2)-symmetry of the unified model, and the demand of independence of U(1)U(1)- and SU(2)SU(2)-transformations leads to the estimate sin2θmin=0,20\sin^{2}\theta_{min}=0,20 where θmin\theta_{min} is an analog of the Weinberg angle of the standard model.Comment: 7 page
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