2005/05/31 by Sanjib Kumar Agarwalla, Amitava Raychaudhuri, Abhijit Samanta · 2 citations
Physics and Astronomy · #Astronomy #Astrophysics and Cosmic Phenomena #BETA (programming language) #Baseline (sea) #Beam (structure) #Calorimeter (particle physics) #Computer science #Detector #Large Hadron Collider #Neutrino #Neutrino Physics Research #Neutrino oscillation #Nuclear physics #Observatory #Optics #Particle physics #Particle physics theoretical and experimental studies #Physics #hep-ph
paper · pdf · doi:10.1016/j.physletb.2005.09.053
published as Phys.Lett.B629:33-40,2005 · 11 pages, 6 figures, Latex, more discussions added, version accepted in Phys. Lett. B
openalex publication_date 2005/10/03 · arxiv created 2005/10/07 · arxiv updated 2014/11/17 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
A high intensity source of a single neutrino flavour with known spectrum is most desirable for precision measurements, the consensus direction for the future. The beta beam is an especially suitable option for this. We discuss the prospects of a very long baseline beta beam experiment with a magnetized iron calorimeter detector. In particular, with the source at CERN and the detector at the proposed India-based Neutrino Observatory (INO) the baseline is near the ‘magic’ value where the effect of the CP phase is small. We observe that this experiment will be well suited to determine the sign of m32−m22 and will be capable of probing θ13 down to about 1°.