Hashim, I. H. and Ejiri, H. and Shima, T. and Takahisa, K. and Sato, A. and Kuno, Y. and Ninomiya, K. and Kawamura, N. and Miyake, Y. (2018) Muon capture reaction on Mo-100 to study the nuclear response for double-beta decay and neutrinos of astrophysics origin. Physical Review C, 97 (1). 014617-014617. ISSN 2469-9985
Full text not available from this repository.
Official URL: http://dx.doi.org/10.1103/PhysRevC.97.014617
Abstract
Ordinary muon capture (OMC) on enriched Mo100 isotopes was studied for the first time to investigate neutrino nuclear responses for neutrinoless double-β decays and supernova neutrino nuclear interactions. Muon capture on Mo100 proceeds mainly as Mo100(μ,xn)Nb100-x with x being the number of neutrons emitted from negative muon capture. The Nb isotope mass distribution was obtained by measuring delayed γ rays from radioactive Nb100-x. By using the neutron emission model after the muon capture, the neutrino response (the strength distribution) for OMC was derived. The OMC strength distribution shows a giant resonance (GR) at the peak energy around 11-14 MeV, suggesting the concentration of the OMC strength at the muon GR region.
| Item Type: | Article |
|---|---|
| Uncontrolled Keywords: | Mo10, neutrino nuclear |
| Subjects: | Q Science > QC Physics |
| Divisions: | Science |
| ID Code: | 86256 |
| Deposited By: | Widya Wahid |
| Deposited On: | 31 Aug 2020 13:54 |
| Last Modified: | 31 Aug 2020 13:54 |
Repository Staff Only: item control page
