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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Fred Cahir,Sara Weuffen,Jo Caminitial 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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Rosemary Berreen,Michael Wearingcrowave background (CMB), and the agreement between the predictions of the primordial nucleosynthesis theories and the observed abundance of light elements. The cosmological Friedmann models are parametrized by the density parameter Ω.. This measures the present cosmological density in units of the

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https://doi.org/10.1007/978-981-15-6145-0the universe seem to be placing severe constraints on cosmological models. In addition, it is shown that the bulk of the baryonic matter is also dark and must be accounted for as well. The nucleosynthesis arguments are now strongly supported by high energy collider experiments as well as astronomica

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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 astrop

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oncologist