Published November 1, 2004
| Version v1
Journal article
Detector depth dependence of the high energy atmospheric neutrino flux
Creators
- 1. Physics Department, University of Notre Dame, Notre Dame, Indiana 46556 (United States)
Description
We note that detector depth can influence the decay path length available for the primary and secondary particles that are the source of atmospheric neutrinos. As a consequence there is a location dependent modulation to the neutrino flux
Additional details
Identifiers
- DOI
- 10.1103/PhysRevD.70.097301;
- arXiv
- arXiv:hep-ex/0406072v1;
Publishing Information
- Journal Title
- Physical Review. D, Particles Fields
- Journal Volume
- 70
- Journal Issue
- 9
- Journal Page Range
- p. 097301-097301.4
- ISSN
- 0556-2821
- CODEN
- PRVDAQ
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 37020863
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
- Descriptors DEI
- COSMIC RAY DETECTION; DEPTH; MODULATION; NEUTRINO DETECTION; NEUTRINOS; PARTICLE DECAY
- Descriptors DEC
- DECAY; DETECTION; DIMENSIONS; ELEMENTARY PARTICLES; FERMIONS; LEPTONS; MASSLESS PARTICLES; RADIATION DETECTION
Optional Information
- Notes
- (c) 2004 The American Physical Society