The primordial helium abundance from updated emissivities
Observations of metal-poor extragalactic H II regions allow the determination of the primordial helium abundance, Y_p. The He I emissivities are the foundation of the model of t...
Observations of metal-poor extragalactic H II regions allow the determination of the primordial helium abundance, Y_p. The He I emissivities are the foundation of the model of t...
The time evolution of the baryon asymmetry ($\frac{k{n}_{B}}{s}$) due to the interactions of a superheavy gauge boson (mass ${M}_{X}\ensuremath{\sim}{10}^{15}$ GeV, coupling str...
The time evolution of the baryon asymmetry of the universe due to superheavy Higgs bosons is obtained by integrating the Boltzmann equations. The interactions included are decay...
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