A search for solar axions and axion-like particles produced in the p+d→3He+A(5.5MeV) reaction was performed using the complete dataset of the Borexino detector (3995 days of measurement live-time). The following interaction processes have been considered: axion decay into two photons (A→2γ), inverse Primakoff conversion on nuclei (A+Z→γ+Z), the Compton conversion of axions to photons (A+e→e+γ) and the axio-electric effect (A+e+Z→e+Z). Model-independent limits on product of axion–photon (gAγ), axion–electron (gAe), and isovector axion–nucleon (g3AN) couplings are obtained: |gAγ×g3AN|≤2.3×10-11GeV-1 and |gAe×g3AN|≤1.9×10-13 at mA< 1 MeV (90% c.l.). The Borexino results exclude new large regions of gAγ, and gAe coupling constants and axion masses mA, and leads to constraints on the products |gAγ×mA| and |gAe×mA| for the KSVZ- and the DFSZ-axion models.
Zuzel, G., Zuber, K., Zavatarelli, S., Wurm, M., Wojcik, M., Von Feilitzsch, F., et al. (2025). Search for high energy 5.5 MeV solar axions with the complete Borexino dataset. THE EUROPEAN PHYSICAL JOURNAL. C, PARTICLES AND FIELDS, 85(10) [10.1140/epjc/s10052-025-14811-9].
Search for high energy 5.5 MeV solar axions with the complete Borexino dataset
Guffanti D.;
2025
Abstract
A search for solar axions and axion-like particles produced in the p+d→3He+A(5.5MeV) reaction was performed using the complete dataset of the Borexino detector (3995 days of measurement live-time). The following interaction processes have been considered: axion decay into two photons (A→2γ), inverse Primakoff conversion on nuclei (A+Z→γ+Z), the Compton conversion of axions to photons (A+e→e+γ) and the axio-electric effect (A+e+Z→e+Z). Model-independent limits on product of axion–photon (gAγ), axion–electron (gAe), and isovector axion–nucleon (g3AN) couplings are obtained: |gAγ×g3AN|≤2.3×10-11GeV-1 and |gAe×g3AN|≤1.9×10-13 at mA< 1 MeV (90% c.l.). The Borexino results exclude new large regions of gAγ, and gAe coupling constants and axion masses mA, and leads to constraints on the products |gAγ×mA| and |gAe×mA| for the KSVZ- and the DFSZ-axion models.| File | Dimensione | Formato | |
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