Standard

Sensitivity of the gamma-ray method for strong primordial magnetic fields. / Korochkin, A.; Kalashev, O.; Neronov, A. et al.

In: Proceedings of Science, Vol. 395, 919, 18.03.2022.

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

Harvard

Korochkin, A, Kalashev, O, Neronov, A & Semikoz, D 2022, 'Sensitivity of the gamma-ray method for strong primordial magnetic fields', Proceedings of Science, vol. 395, 919. https://doi.org/10.22323/1.395.0919

APA

Korochkin, A., Kalashev, O., Neronov, A., & Semikoz, D. (2022). Sensitivity of the gamma-ray method for strong primordial magnetic fields. Proceedings of Science, 395, [919]. https://doi.org/10.22323/1.395.0919

Vancouver

Korochkin A, Kalashev O, Neronov A, Semikoz D. Sensitivity of the gamma-ray method for strong primordial magnetic fields. Proceedings of Science. 2022 Mar 18;395:919. doi: 10.22323/1.395.0919

Author

Korochkin, A. ; Kalashev, O. ; Neronov, A. et al. / Sensitivity of the gamma-ray method for strong primordial magnetic fields. In: Proceedings of Science. 2022 ; Vol. 395.

BibTeX

@article{b8655c28734b418e9fe88b6b150cdd06,
title = "Sensitivity of the gamma-ray method for strong primordial magnetic fields",
abstract = "We study the sensitivity reach of the gamma-ray method for measurement of relatively strong cosmological magnetic field with strength in the 1-10 pG range using deep exposure of the nearest hard spectrum blazar Mrk 501 with CTA telescopes. We show that the gamma-ray measurement technique can sense the primordial magnetic field with a strength of up to 10-11 G. Combination of the cosmic microwave background and gamma-ray constraints can thus sense the full range of possible cosmological magnetic fields to confirm or rule out their relevance to the problem of the origin of cosmic magnetic fields, as well as their influence on recombination and reionization epochs.",
author = "A. Korochkin and O. Kalashev and A. Neronov and D. Semikoz",
note = "Funding Information: This work has been supported by the French National Research Agency (ANR) grant ANR-19-CE31-0020 and Russian Science Foundation grant 20-42-09010. Publisher Copyright: {\textcopyright} Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License (CC BY-NC-ND 4.0); 37th International Cosmic Ray Conference, ICRC 2021 ; Conference date: 12-07-2021 Through 23-07-2021",
year = "2022",
month = mar,
day = "18",
doi = "10.22323/1.395.0919",
language = "English",
volume = "395",
journal = "Proceedings of Science",
issn = "1824-8039",
publisher = "Sissa Medialab Srl",

}

RIS

TY - JOUR

T1 - Sensitivity of the gamma-ray method for strong primordial magnetic fields

AU - Korochkin, A.

AU - Kalashev, O.

AU - Neronov, A.

AU - Semikoz, D.

N1 - Funding Information: This work has been supported by the French National Research Agency (ANR) grant ANR-19-CE31-0020 and Russian Science Foundation grant 20-42-09010. Publisher Copyright: © Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License (CC BY-NC-ND 4.0)

PY - 2022/3/18

Y1 - 2022/3/18

N2 - We study the sensitivity reach of the gamma-ray method for measurement of relatively strong cosmological magnetic field with strength in the 1-10 pG range using deep exposure of the nearest hard spectrum blazar Mrk 501 with CTA telescopes. We show that the gamma-ray measurement technique can sense the primordial magnetic field with a strength of up to 10-11 G. Combination of the cosmic microwave background and gamma-ray constraints can thus sense the full range of possible cosmological magnetic fields to confirm or rule out their relevance to the problem of the origin of cosmic magnetic fields, as well as their influence on recombination and reionization epochs.

AB - We study the sensitivity reach of the gamma-ray method for measurement of relatively strong cosmological magnetic field with strength in the 1-10 pG range using deep exposure of the nearest hard spectrum blazar Mrk 501 with CTA telescopes. We show that the gamma-ray measurement technique can sense the primordial magnetic field with a strength of up to 10-11 G. Combination of the cosmic microwave background and gamma-ray constraints can thus sense the full range of possible cosmological magnetic fields to confirm or rule out their relevance to the problem of the origin of cosmic magnetic fields, as well as their influence on recombination and reionization epochs.

UR - http://www.scopus.com/inward/record.url?scp=85144190218&partnerID=8YFLogxK

U2 - 10.22323/1.395.0919

DO - 10.22323/1.395.0919

M3 - Conference article

AN - SCOPUS:85144190218

VL - 395

JO - Proceedings of Science

JF - Proceedings of Science

SN - 1824-8039

M1 - 919

T2 - 37th International Cosmic Ray Conference, ICRC 2021

Y2 - 12 July 2021 through 23 July 2021

ER -

ID: 41156946