Radiochemical neutrino detection viaI(,Xe
- 29 February 1988
- journal article
- research article
- Published by American Physical Society (APS) in Physical Review Letters
- Vol. 60 (9) , 768-771
- https://doi.org/10.1103/physrevlett.60.768
Abstract
Solar or supernova neutrinos incident on an iodine-bearing liquid will produce the noble gas (=36.4 d), which can be recovered and counted as in the present experiment. The rate of neutrino reactions per unit volume of detector could be more than an order of magnitude greater than in perchloroethylene. I discuss the new physics that might be learned from such an experiment.
Keywords
This publication has 8 references indexed in Scilit:
- The (p, n) reaction as a probe of beta decay strengthNuclear Physics A, 1987
- Gamow-Teller Strength Function invia the () Reaction at Medium EnergiesPhysical Review Letters, 1985
- Solar-Neutrino Detection: Experimental Determination of Gamow-Teller Strengths via theand() ReactionsPhysical Review Letters, 1985
- Nuclear data sheets for A = 127Nuclear Data Sheets, 1982
- Empirical Evaluation of Gamow-Teller Strength Function for→and its Implication in the Cross Section for Solar Neutrino Absorption byPhysical Review Letters, 1981
- The decay of127CsJournal of Physics G: Nuclear Physics, 1976
- High-spin states in odd Xe nucleiNuclear Physics A, 1970
- The decay of127CsThe European Physical Journal A, 1967