Discovery potential of xenon-based neutrinoless double beta decay experiments in light of small angular scale CMB observations
arXiv:1301.2901 · doi:10.1088/1475-7516/2013/03/043
Abstract
The South Pole Telescope (SPT) has probed an expanded angular range of the CMB temperature power spectrum. Their recent analysis of the latest cosmological data prefers nonzero neutrino masses, mnu = 0.32+-0.11 eV. This result, if confirmed by the upcoming Planck data, has deep implications on the discovery of the nature of neutrinos. In particular, the values of the effective neutrino mass involved in neutrinoless double beta decay (bb0nu) are severely constrained for both the direct and inverse hierarchy, making a discovery much more likely. In this paper, we focus in xenon-based bb0nu experiments, on the double grounds of their good performance and the suitability of the technology to large-mass scaling. We show that the current generation, with effective masses in the range of 100 kg and conceivable exposures in the range of 500 kg year, could already have a sizable opportunity to observe bb0nu events, and their combined discovery potential is quite large. The next generation, with an exposure in the range of 10 ton year, would have a much more enhanced sensitivity, in particular due to the very low specific background that all the xenon technologies (liquid xenon, high-pressure xenon and xenon dissolved in liquid scintillator) can achieve. In addition, a high-pressure xenon gas TPC also features superb energy resolution. We show that such detector can fully explore the range of allowed effective Majorana masses, thus making a discovery very likely.
17 pages, 4 figures, submitted to the Journal of Cosmology and Astroparticles
References in corpus (23)
- A 3% Solution: Determination of the Hubble Constant with the Hubble Space Telescope and Wide Field Camera 3
- Leptogenesis
- The WiggleZ Dark Energy Survey: mapping the distance-redshift relation with baryon acoustic oscillations
- Planck Early Results: The Planck mission
- Global fit to three neutrino mixing: critical look at present precision
- Evidence for Neutrinoless Double Beta Decay
- Carnegie Hubble Program: A Mid-Infrared Calibration of the Hubble Constant
- Search for Neutrinoless Double-Beta Decay in Xe with EXO-200
- Limit on Neutrinoless ββ Decay of Xe-136 from the First Phase of KamLAND-Zen and Comparison with the Positive Claim in Ge-76
- Microwave Background Constraints on Cosmological Parameters
- The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: a large sample of mock galaxy catalogues
- Measurement of the double-βdecay half-life of ^{136}Xe with the KamLAND-Zen experiment
- Observation of Two-Neutrino Double-Beta Decay in Xe-136 with EXO-200
- Production of Radioactive Isotopes through Cosmic Muon Spallation in KamLAND
- The EXO-200 detector, part I: Detector design and construction
- Correlated Fluctuations between Luminescence and Ionization in Liquid Xenon
- NEXT-100 Technical Design Report (TDR). Executive Summary
- Robust Cosmological Bounds on Neutrinos and their Combination with Oscillation Results
- Sense and sensitivity of double beta decay experiments
- Radiopurity control in the NEXT-100 double beta decay experiment: procedures and initial measurements
- Neutrinoless Double Beta Decay with SNO+
- The MAJORANA DEMONSTRATOR: A Search for Neutrinoless Double-beta Decay of Germanium-76
- Combining and comparing neutrinoless double beta decay experiments using different nuclei
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- Double Beta Decay Experiments at Canfranc Underground Laboratory
- Improved background rejection in neutrinoless double beta decay experiments using a magnetic field in a high pressure xenon TPC