In situ determination of Earth matter density in a neutrino factory
Creators
- 1. Department of Physics, Tokyo Metropolitan University, 1-1 Minami-Osawa, Hachioji, Tokyo 192-0397 (Japan)
Description
We point out that an accurate in situ determination of the earth matter density ρ is possible in neutrino factory by placing a detector at the magic baseline, L=√(2)π/GFNe where Ne denotes electron number density. The accuracy of matter density determination is excellent in a region of relatively large θ13 with fractional uncertainty δρ/ρ of about 0.43%, 1.3%, and < or approx. 3% at 1σ CL at sin22θ13=0.1, 10-2, and 3x10-3, respectively. At smaller θ13 the uncertainty depends upon the CP phase δ, but it remains small, 3%-7% in more than 3/4 of the entire region of δ at sin22θ13=10-4. The results would allow us to solve the problem of obscured CP violation due to the uncertainty of earth matter density in a wide range of θ13 and δ. It may provide a test for the geophysical model of the earth, or it may serve as a method for a stringent test of the Mikheyev-Smirnov-Wolfenstein theory of neutrino propagation in matter once an accurate geophysical estimation of the matter density is available
Additional details
Identifiers
- DOI
- 10.1103/PhysRevD.75.073013;
- arXiv
- arXiv:hep-ph/0612002v3;
Publishing Information
- Journal Title
- Physical Review. D, Particles Fields
- Journal Volume
- 75
- Journal Issue
- 7
- Journal Page Range
- p. 073013-073013.12
- ISSN
- 0556-2821
- CODEN
- PRVDAQ
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 39042049
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; S58: GEOSCIENCES;
- Descriptors DEI
- ACCURACY; CP INVARIANCE; ELECTRON DENSITY; ELECTRONS; NEUTRINO DETECTION; NEUTRINO REACTIONS; NEUTRINOS
- Descriptors DEC
- DETECTION; ELEMENTARY PARTICLES; FERMIONS; INVARIANCE PRINCIPLES; LEPTON REACTIONS; LEPTONS; MASSLESS PARTICLES; NUCLEAR REACTIONS; RADIATION DETECTION
Optional Information
- Notes
- (c) 2007 The American Physical Society