| dc.contributor.author | Salvado, J | en_US |
| dc.contributor.author | Argüelles, C | en_US |
| dc.contributor.author | Katori, T | en_US |
| dc.date.accessioned | 2016-11-29T15:40:01Z | |
| dc.date.submitted | 2016-11-23T09:56:45.705Z | |
| dc.identifier.uri | http://qmro.qmul.ac.uk/xmlui/handle/123456789/18004 | |
| dc.description | 6 pages, 4 figures, proceedings | |
| dc.description | 6 pages, 4 figures, proceedings | en_US |
| dc.description | 6 pages, 4 figures, proceedings | en_US |
| dc.description | 6 pages, 4 figures, proceedings | en_US |
| dc.description | 6 pages, 4 figures, proceedings | en_US |
| dc.description.abstract | Astrophysical neutrinos are powerful tools to study fundamental properties of particle physics. We perform a general new physics study on ultra high energy neutrino flavor content by introducing effective operators. We find that at the current limits on these operators, new physics terms cause maximal effects on the flavor content, however, the flavor content at Earth is confined to a region related to the initial flavor content. | en_US |
| dc.subject | hep-ph | en_US |
| dc.subject | hep-ph | en_US |
| dc.title | New Physics in Astrophysical Neutrino Flavor (NuFact 2016) | en_US |
| dc.type | Article | |
| pubs.author-url | http://arxiv.org/abs/1611.05710v1 | en_US |
| pubs.notes | Not known | en_US |
