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

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手榴弹

https://doi.org/10.1007/978-3-211-74420-8tion with an account taken of the expansion of the universe and the backreaction of created particles, including the effects of their rescattering. A detailed account of our results can be found in [4, 5]; here I will concentrate on the main picture, emphasizing qualitative rather than quantitative aspects of the theory.

infringe

Gegenüberstellung mit der Vorausgabeical magnetic fields this translates into a present-day bound of . Gauss. We explain why the limits obtained from primordial nucleosynthesis are generally weaker than those imposed by the microwave background isotropy. The effect of inflation on all these stresses is also calculated.

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Commentary

Covariant Analysis of Dynamics and of CBR Anisotropythe expression for CBR anisotropies due to adiabatic perturbations, that appears to imply a zero in the CBR anisotropy spectrum in an interesting angular region, irrespective of the detailed matter model.

和谐

Reheating in Inflationary Cosmologytion with an account taken of the expansion of the universe and the backreaction of created particles, including the effects of their rescattering. A detailed account of our results can be found in [4, 5]; here I will concentrate on the main picture, emphasizing qualitative rather than quantitative aspects of the theory.

arsenal

Limits on Cosmological Magnetic Fields and Other Anisotropic Stressesical magnetic fields this translates into a present-day bound of . Gauss. We explain why the limits obtained from primordial nucleosynthesis are generally weaker than those imposed by the microwave background isotropy. The effect of inflation on all these stresses is also calculated.