Effect of the neutron lifetime on processes in the early universe


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The influence of the neutron lifetime on the abundance of light elements produced during the primordial nucleosynthesis early in the birth of the Universe is considered. Among light elements, namely, D, 3He, 4He, and 7Li, 4He proves to be most sensitive to neutron lifetime τn. Astronomic data on the light element abundance also provide the best accuracy for 4He. The solution of a number of problems discussed in this paper requires improving the accuracy of observations for the 4He abundance and refining the value of τn.

Sobre autores

A. Chechkin

Peter the Great St. Petersburg Polytechnic University; Petersburg Nuclear Physics Institute

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Email: a.4ech89@gmail.com
Rússia, Politekhnicheskaya ul. 29, St. Petersburg, 195251; Gatchina, Leningrad oblast, St. Petersburg, 188300

A. Ivanchik

Peter the Great St. Petersburg Polytechnic University; Ioffe Physical-Technical Institute

Email: a.4ech89@gmail.com
Rússia, Politekhnicheskaya ul. 29, St. Petersburg, 195251; Politekhnicheskaya ul. 26, St. Petersburg, 194021

A. Serebrov

Petersburg Nuclear Physics Institute

Email: a.4ech89@gmail.com
Rússia, Gatchina, Leningrad oblast, St. Petersburg, 188300

S. Bobashev

Peter the Great St. Petersburg Polytechnic University; Ioffe Physical-Technical Institute

Email: a.4ech89@gmail.com
Rússia, Politekhnicheskaya ul. 29, St. Petersburg, 195251; Politekhnicheskaya ul. 26, St. Petersburg, 194021

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