A Time Varying Strong Coupling Constant as a Model of Inflationary Universe

2); Argentina; (2) H.I.A.S.T.; Damascus; H.Vucetich (1)((1)U.N.L.P.; La Plata; N.Chamoun (1; S.J.Landau (1); Syria)

arxiv: astro-ph/0009204 · v4 · submitted 2000-09-13 · 🌌 astro-ph · gr-qc

A Time Varying Strong Coupling Constant as a Model of Inflationary Universe

N.Chamoun (1 , 2) , S.J.Landau (1) , H.Vucetich (1)((1)U.N.L.P. , La Plata , Argentina; (2) H.I.A.S.T. , Damascus , Syria) This is my paper

classification 🌌 astro-ph gr-qc

keywords constantcouplinginflationmodelstronguniverseapproachattribute

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We consider a scenario where the strong coupling constant was changing in the early universe. We attribute this change to a variation in the colour charge within a Bekenstein-like model. Treating the vacuum gluon condensate $<G^2>$ as a free paramete r, we could generate inflation with the required properties to solve the fluctuation and other standard cosmology problems. A possible approach to end the inflation is suggested.

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A Time Varying Strong Coupling Constant as a Model of Inflationary Universe

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