Simple Model with Time–varying Fine structure "Constant"–Part II

Marcelo Samuel Berman

Instituto Albert Einstein, Av. Candido Hartmann, 575, No. 17, 80730–440, Curitiba–PR, Brazil. (msberman@institutoalberteinstein.org).

Received 2009 June 22
Accepted 2009 September 1

RESUMEN

Extendiendo la Hipótesis de los Grandes Números de Dirac para cubrir las "constantes" cosmológica y de estructura fina, y la rotación del Universo, las estudiamos, incluyendo una "demostración", del cálculo de la velocidad angular del Universo actual, y del inflacionario. Se clarifican algunos puntos criticables de este artículo.

ABSTRACT

The extension of Dirac's LNH to cover cosmological and fine–structure time–varying "constants", and the rotation of the universe, is here analysed, including a "derivation" of the angular speed of the present universe, and of the inflationary phase. Controversial points in the present calculation are clarified.

Key Words: cosmological parameters — cosmology: theory — cosmology: miscellaneous — early universe — gravitation.

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