The primordial nucleosynthesis as a probe of possible deviations of fundamental physical constants

A.V. Ivanchik, A.V. Orlov, D.A. Varshalovich
Department of Theoretical Astrophysics, Ioffe Physical Technical Institute RAS, St. Petersburg, Russia

We have studied an effect of possible deviation of fundamental physical constants on the yields of light nuclei 2D, 3He, 4He, 7Li, etc. during the primordial nucleosynthesis. The deviation of fundamental constants from their present values has been considered in the framework of the low-energy approach of string theories. These theories predict the existence of a scalar field which is supposed to be a partner of tensor gravity field and defines the spatial geometry as well. In the frames of such approach we have elaborated two-parameter ({eta},{delta}) model of the primordial nucleosynthesis. Parameter {eta}=nB/n{gamma} characterizes the baryon-to-photon ratio by number. Parameter {delta} characterizes the deviation of values of fundamental physical constants at the primordial nucleosynthesis epoch from the present ones. In the framework of the model a functional relation between {eta} and {delta} is obtained under condition that primordial helium abundance is Yp=f({eta},{delta})=Const, where Const corresponds to the observational data available. Thus it is shown that the relative baryon density {eta} (as well as {Omega}B) determined from the observational data may satisfy the experimental constraints in essentially wider range of values than it was allowed by the standard nucleosynthesis model.


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