| Issue |
EPJ Web Conf.
Volume 142, 2017
International Symposium Advances in Dark Matter and Particle Physics
|
|
|---|---|---|
| Article Number | 01003 | |
| Number of page(s) | 11 | |
| DOI | https://doi.org/10.1051/epjconf/201714201003 | |
| Published online | 12 April 2017 | |
https://doi.org/10.1051/epjconf/201714201003
General features of spontaneous baryogenesis
1 Department of Higher Mathematics, Dubna State University, 141980 Dubna, Russia,
2 Novosibirsk State University, 630090 Novosibirsk, Russia
* e-mail: arbuzova@uni-dubna.ru
Published online: 12 April 2017
The classical version of spontaneous baryogenesis is studied in details. It is shown that the relation between the time derivative of the (pseudo)goldstone field and the baryonic chemical potential essentially depends upon the representation chosen for the fermionic fields with non-zero baryonic number (quarks). The kinetic equation, used for the calculations of the cosmological baryon asymmetry, is generalized to the case of non-stationary background. The effects of the finite interval of the integration over time are also included into consideration.
© The Authors, published by EDP Sciences, 2017
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