Agarwalla, Sanjib Kumar ; Choubey, Sandhya ; Raychaudhuri, Amitava (2008) Exceptional sensitivity to neutrino parameters with a two-baseline Beta-beam set-up Nuclear Physics B, 805 (1-2). pp. 305-325. ISSN 0550-3213
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Official URL: http://linkinghub.elsevier.com/retrieve/pii/S05503...
Related URL: http://dx.doi.org/10.1016/j.nuclphysb.2008.07.026
Abstract
We examine the reach of a Beta-beam experiment with two detectors at carefully chosen baselines for exploring neutrino mass parameters. Locating the source at CERN, the two detectors and baselines are: (a) a 50 kton iron calorimeter (ICAL) at a baseline of around 7150 km which is roughly the magic baseline, e.g., ICAL@INO, and (b) a 50 kton Totally Active Scintillator Detector at a distance of 730 km, e.g., at Gran Sasso. We choose 8B and 8Li source ions with a boost factor γ of 650 for the magic baseline while for the closer detector we consider 18Ne and 6He ions with a range of Lorentz boosts. We find that the locations of the two detectors complement each other leading to an exceptional high sensitivity. With γ=650 for 8B/8Li and γ=575 for 18Ne/6He and total luminosity corresponding to 5×(1.1×1018) and 5×(2.9×1018) useful ion decays in neutrino and antineutrino modes respectively, we find that the two-detector set-up can probe maximal CP violation and establish the neutrino mass ordering if sin22θ13 is 1.4×10−4 and 2.7×10−4, respectively, or more. The sensitivity reach for sin22θ13 itself is 5.5×10−4. With a factor of 10 higher luminosity, the corresponding sin22θ13 reach of this set-up would be 1.8×10−5, 4.6×10−5 and 5.3×10−5 respectively for the above three performance indicators. CP violation can be discovered for 64% of the possible δCP values for sin22θ13≥10−3 (≥8×10−5), for the standard luminosity (10 times enhanced luminosity). Comparable physics performance can be achieved in a set-up where data from CERN to INO@ICAL is combined with that from CERN to the Boulby mine in United Kingdom, a baseline of 1050 km.
Item Type: | Article |
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Source: | Copyright of this article belongs to Elsevier Science. |
ID Code: | 43239 |
Deposited On: | 10 Jun 2011 13:15 |
Last Modified: | 18 May 2016 00:18 |
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