127I(nu,e)127Xe reaction for solar neutrino spectrum clarification

Oct 12, 2020, 3:55 PM


Oral report Section 5. Neutrino physics and astrophysics. Section 5. Neutrino physics and astrophysics


Almaz Fazliakhmetov (MIPT, INR RAS)


Solar neutrino spectrum measurement plays a crucial role for solar metallicity determination. 127I(nu,e)127Xe reaction is sensitive to CNO and boron components of the solar neutrino spectrum due to the relatively high threshold (662 KeV).
For neutrinos with energies upper S_n = 7.246 MeV 127I(nu,e) capture produces 126Xe + n. The concentration ratio of 127Xe and 126Xe could clarify parameters of high energy solar neutrino spectrum and neutrino oscillations. We present production rate estimation for of 127Xe and 126Xe based on experimental strength function from 127I(p,n)Xe reaction.

Primary author

Almaz Fazliakhmetov (MIPT, INR RAS)


Grigory Koroteev (Moscow Institute of Physics and Technology) Prof. Yuri Lutostansky (NRC “Kurchatov institute” – Institute for Theoretical and Experimental Physics, Moscow, 11728, Russia) V. N. Tikhonov (National Research Center Kurchatov Institute, Moscow, 123182 Russia) Mr Alexey Osipenko (National Research Center «Kurchatov Institute»)

Presentation materials