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Titlebook: Gauge Theory and the Early Universe; P. Galeotti,David N. Schramm Book 1988 Kluwer Academic Publishers 1988 Cosmology.Dark matter.Gravity.

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楼主: 预兆前
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https://doi.org/10.1007/978-1-349-11801-4pacelike three-surface S obeys a zero energy Schrödinger equation,the Wheeler-De Witt equation for closed universes. . may be given by a functional integral taken over all compact euclidean fourmetrics which have a boundary at S, and over all field configurations which match the given value on S.Aft
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https://doi.org/10.1057/9781137368805hronous reference system will tend asymptotically in time towards the de Sitter solution, so making the problem of initial conditions less severe. The implications for inflationary scenarios are examined and it is found that after inflation the universe stays isotropic and homogeneous for a very lon
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https://doi.org/10.1007/978-1-349-21163-0may have condensed into the galactic halo. These detectors are based on the principle, due to Sikivie [1], of conversion of axions to microwave photons in a magnetic field. We describe the device built by a Rochester-Brookhaven-Fermilab collaboration*, its sensitivity, and the motivation from astrophysics for attempting to observe axions.
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https://doi.org/10.1057/9781137368805hronous reference system will tend asymptotically in time towards the de Sitter solution, so making the problem of initial conditions less severe. The implications for inflationary scenarios are examined and it is found that after inflation the universe stays isotropic and homogeneous for a very long time.
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The Problem of Origin of the Primordial Cosmological Perturbations,al cosmological perturbations due to the parametric effect is considered. The related fluctuations of the relic background radiation are analysed. The spottiness structure of the large-scale background anisotropy is discussed.
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An Experimental Search for Galactic Axions,may have condensed into the galactic halo. These detectors are based on the principle, due to Sikivie [1], of conversion of axions to microwave photons in a magnetic field. We describe the device built by a Rochester-Brookhaven-Fermilab collaboration*, its sensitivity, and the motivation from astrophysics for attempting to observe axions.
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