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General features of spontaneous baryogenesis. / Arbuzova, Elena.

In: EPJ Web of Conferences, Vol. 142, 01003, 12.04.2017.

Research output: Contribution to journal › Conference article › peer-review

Harvard

Arbuzova, E 2017, 'General features of spontaneous baryogenesis', EPJ Web of Conferences, vol. 142, 01003. https://doi.org/10.1051/epjconf/201714201003

APA

Arbuzova, E. (2017). General features of spontaneous baryogenesis. EPJ Web of Conferences, 142, [01003]. https://doi.org/10.1051/epjconf/201714201003

Vancouver

Arbuzova E. General features of spontaneous baryogenesis. EPJ Web of Conferences. 2017 Apr 12;142:01003. doi: 10.1051/epjconf/201714201003

Author

Arbuzova, Elena. / General features of spontaneous baryogenesis. In: EPJ Web of Conferences. 2017 ; Vol. 142.

BibTeX

@article{cb570199f8664b4b8a87be9f50bb432a,
title = "General features of spontaneous baryogenesis",
abstract = "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.",
author = "Elena Arbuzova",
year = "2017",
month = apr,
day = "12",
doi = "10.1051/epjconf/201714201003",
language = "English",
volume = "142",
journal = "EPJ Web of Conferences",
issn = "2101-6275",
publisher = "EDP Sciences",

}

RIS

TY - JOUR

T1 - General features of spontaneous baryogenesis

AU - Arbuzova, Elena

PY - 2017/4/12

Y1 - 2017/4/12

N2 - 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.

AB - 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.

UR - http://www.scopus.com/inward/record.url?scp=85018821410&partnerID=8YFLogxK

U2 - 10.1051/epjconf/201714201003

DO - 10.1051/epjconf/201714201003

M3 - Conference article

AN - SCOPUS:85018821410

VL - 142

JO - EPJ Web of Conferences

JF - EPJ Web of Conferences

SN - 2101-6275

M1 - 01003

ER -

ID: 10041109