Titlebook: Current Topics in Astrofundamental Physics; Primordial Cosmology N. Sánchez,A. Zichichi Book 1998 Springer Science+Business Media Dordrecht

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娴熟

Large-Scale Anisotropy of the Cosmic Microwave Backgroundge-scale structure forms as the result of gravitational amplification of initially small perturbations in the primordial density distribution. The COBE-DMR maps of the cosmic microwave background anisotropy measure the primordial density distribution on super-horizon scales and offer a unique probe

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instill

”Dark Ages” of the Universe estimate the possible space density of the active galaxies at very early epoch, and demonstrated, that there are no observational constrains on the existence on very HZ objects, . 》 1, up to recombination epoch and at least some classes of the Early Universe population may are in the range of prese

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dapper

The Direct Detection of Dark Matterications of the recent evidence for the presence of Massive Compact Halo Objects (MACHOS) in the halo of our galaxy. Within the current observational uncertainties, the fraction of MACHOs can be as high as 100% of the halo or as low as 10%. We argue that the “natural” conclusion that they form the t

令人作呕

Kinetic Theory of Hot Gauge Theories: Overview, Details & Extensionstic theory may arise at one loop order. Using the wordline representation of the one loop effective action, I follow D’Hoker and Gagné to replace the Wilson line by an integral over worldline fermions. A bilinear of these worldline fermions naturally defines a nonabelian charge, whose equation of motion is Wong’s equation.

VOC

Nerve-Block

Varying G and Other Constantsonstants and show how we can incorporate the simultaneous variations of several ‘constants’ exactly by using higher-dimensional unified theories. Finally, we describe some new observational limits on possible space or time variations of the fine structure constant.

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