Helium and deuterium abundances as a test for the time variation of the fine structure constant and the Higgs vacuum expectation value

We use the semi-analytic method of Esmailzadeh et al (1991 Astrophys. J. 378 504-18) to calculate the abundances of helium and deuterium produced during Big Bang nucleosynthesis assuming the fine structure constant and the Higgs vacuum expectation value may vary in time. We analyse the dependence on...

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Detalles Bibliográficos
Autores principales: Chamoun, N., Landau, S.J., Mosquera, M.E., Vucetich, H.
Formato: JOUR
Acceso en línea:http://hdl.handle.net/20.500.12110/paper_09543899_v34_n2_p_Chamoun
Aporte de:
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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