Precise 8B solar neutrino spectrum for neutrino oscillation analysis
| Project/Area Number |
21740189
|
|---|
| Research Category |
Grant-in-Aid for Young Scientists (B)
|
| Allocation Type | Single-year Grants |
|---|
| Research Field |
Particle/Nuclear/Cosmic ray/Astro physics
|
|---|
| Research Institution | Tokyo University of Science |
|---|
Principal Investigator |
SUMIKAMA Toshiyuki Tokyo University of Science, 理工学部 (20392003)
|
|---|
| Project Period (FY) |
2009 – 2010
|
| Project Status |
Completed (Fiscal Year 2010)
|
| Budget Amount *help |
¥3,510,000 (Direct Cost: ¥2,700,000、Indirect Cost: ¥810,000)
Fiscal Year 2010: ¥1,560,000 (Direct Cost: ¥1,200,000、Indirect Cost: ¥360,000)
Fiscal Year 2009: ¥1,950,000 (Direct Cost: ¥1,500,000、Indirect Cost: ¥450,000)
|
|---|
| Keywords | 太陽ニュートリノ / β線角度分布 |
|---|
| Research Abstract |
Solar neutrino spectrum from 8B is one of the most precise observables to investigate the neutrino oscillation beyond the standard model. One of the largest uncertainties of neutrino spectrum observed at Super-Kamiokande is the spectral shape factor just after the neutrino emission from 8B. In this study, the weak magnetism and axial charge matrix elements, which are the terms in shape factor, were determined directly from experimental results of beta decay. Uncertainties in the shape factor were determined based on experimental uncertainties for the first time.
|
Report
(3 results)
Research Products
(5 results)
