Interpretation of the atmospheric muon charge ratio in MINOS
| dc.creator | Schreiner, Philip | |
| dc.creator | Goodman, Maury | |
| dc.date | 2007-06-04 | |
| dc.date.accessioned | 2026-07-07T08:04:18Z | |
| dc.date.available | 2026-07-07T08:04:18Z | |
| dc.description | MINOS is the first large magnetic detector deep underground and is the first to measure the muon charge ratio with high statistics in the region near 1 TeV.\cite{bib:adamson} An approximate formula for the muon charge ratio can be expressed in terms of $ε_π$ = 115 GeV, $ε_K$ = 850 GeV and $\ec$. The implications for K production in the atmosphere will be discussed. | |
| dc.description | Contribution to the 30th International Cosmic Ray Conference, Merida Mexico 2007 | |
| dc.identifier | https://arxiv.org/abs/0706.0538 | |
| dc.identifier | http://arxiv.org/abs/0706.0538 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/129903 | |
| dc.subject | High Energy Physics - Experiment | |
| dc.subject | Astrophysics | |
| dc.title | Interpretation of the atmospheric muon charge ratio in MINOS | |
| dc.type | text |