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Pisma v Zhurnal Tekhnicheskoi Fiziki, 2024 Volume 50, Issue 23, Pages 4–6 (Mi pjtf6834)

International Conference Physics.SPb/2024

Serach for 5.5 MeV solar axions with the Borexino detector

A. V. Derbin, I. S. Drachnev, I. S. Lomskaya, V. N. Muratova, N. V. Niyazova, D. A. Semenov, E. V. Unzhakov

The Petersburg Nuclear Physics Institute, The National Research Center "Kurchatov Institute", Gatchina, Russia

Abstract: The sensitivity of the Borexino large scintillation detector was determined for search for axions with an energy of 5.5 MeV produced in the nuclear reaction $p+d\to{}^3\mathrm{He}+A$ in the Sun through the Compton process and the conversion of an axion into a photon in the solar core field . Basing on the measured Borexino spectrum, new upper limits have been established for the product of the coupling constants of the axion with electrons and nucleons $|g_{Ae}g_{AN}^3|\le4.6\cdot10^{13}$ and with a photon and nucleons $|g_{A\gamma}g_{AN}^3|\le3.6\cdot10^{-11}$ GeV$^{-1}$, both limits are given for 90% confidence level.

Keywords: solar axions, dark matter, axion-like particles.

Received: 24.04.2024
Revised: 06.08.2024
Accepted: 30.10.2024

DOI: 10.61011/PJTF.2024.23.59388.6381k



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