What is the statistical significance of the solar neutrino flux problem?
| dc.creator | Goldberg, Jacques | |
| dc.date | 1994-01-25 | |
| dc.date.accessioned | 2026-07-07T03:56:41Z | |
| dc.date.available | 2026-07-07T03:56:41Z | |
| dc.description | Uniform random numbers, not Gaussian random numbers, should have been used with Standard Solar Models to estimate the effect on the neutrino flux of uncertainties in input data. The observed discrepancy is therefore probably quite smaller than currently accepted. | |
| dc.description | 8 pages, TECHNION-PH-94-2 | |
| dc.identifier | https://arxiv.org/abs/hep-ph/9401322 | |
| dc.identifier | http://arxiv.org/abs/hep-ph/9401322 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/45086 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | What is the statistical significance of the solar neutrino flux problem? | |
| dc.type | text |