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Journal ArticleDOI

On the origin of the light elements ( Z 6 )

Hubert Reeves
- 01 Jan 1994 - 
- Vol. 66, Iss: 1, pp 193-216
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TLDR
In this article, the status of nucleosynthesis of the light nuclei is reviewed and several astrophysical and cosmological implications are discussed, such as the baryonic density, the possible existence of Baryonic dark matter and of nonbaryonic (exotic) matter, the constraints imposed on new particle physics, the leptonic number of the universe, the increase in cosmic entropy since primordial nucleo-ynthesis, and the constancy of the "constants" of physics.
Abstract
The author reviews the status of our understanding of nucleosynthesis of the light nuclei ($Zl6$). The standard view today is that these elements are, for the most part, generated by two different processes: first, thermonuclear reactions in the early universe (big-bang nucleosynthesis or (BBN), and second, galactic cosmic-ray-induced spallation reactions (GCR) in cold interstellar atoms. A third contribution comes from stellar processes. The arguments in favor of this view are presented. Numerous astrophysical and cosmological implications are discussed, such as the baryonic density, the possible existence of baryonic dark matter and of nonbaryonic (exotic) matter, the constraints imposed on new particle physics, the leptonic number of the universe, the increase in cosmic entropy since primordial nucleosynthesis, and the constancy of the "constants" of physics.

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Journal ArticleDOI

The Confrontation Between General Relativity and Experiment

TL;DR: Tests of general relativity at the post-Newtonian level have reached high precision, including the light deflection, the Shapiro time delay, the perihelion advance of Mercury, the Nordtvedt effect in lunar motion, and frame-dragging.
Journal ArticleDOI

The fundamental constants and their variation: observational and theoretical status

Abstract: This article describes the various experimental bounds on the variation of the fundamental constants of nature. After a discussion of the role of fundamental constants, their definition and link with metrology, it reviews the various constraints on the variation of the fine-structure constant, the gravitational, weak- and strong-interaction couplings and the electron-to-proton mass ratio. The review aims (1) to provide the basics of each measurement, (2) to show as clearly as possible why it constrains a given constant, and (3) to point out the underlying hypotheses. Such an investigation is of importance in comparing the different results and in understanding the recent claims of the detection of a variation of the fine-structure constant and of the electron-to-proton mass ratio in quasar absorption spectra. The theoretical models leading to the prediction of such variation are also reviewed, including Kaluza-Klein theories, string theories, and other alternative theories. Cosmological implications of these results are also discussed. The links with the tests of general relativity are emphasized.
Journal ArticleDOI

The Confrontation between General Relativity and Experiment

TL;DR: Tests of general relativity at the post-Newtonian level have reached high precision, including the light deflection, the Shapiro time delay, the perihelion advance of Mercury, and the Nordtvedt effect in lunar motion.
Journal ArticleDOI

The primordial helium abundance: systematic effects and a new determination

TL;DR: In this paper, the primordial helium abundance was determined for 27 supergiant H II regions in 23 low-metallicity blue compact galaxies (BCGs) with oxygen abundance 12 + log (O/H) between 7.22 and 8.51.
Journal ArticleDOI

The Primordial Abundance of 4He Revisited

TL;DR: In this paper, the primordial helium abundance of 15 blue compact galaxies (BCGs) with oxygen abundance 12 ) log (O/H) between 7.83 and 8.35 was determined using a sample of 45 low-metallicity H II regions.
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