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arXiv:1504.03966hep-ph

Detection Prospects of the Cosmic Neutrino Background

Yu-Feng Li

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Abstract

The existence of the cosmic neutrino background (CnuB) is a fundamental prediction of the standard Big Bang cosmology. Although current cosmological probes provide indirect observational evidence, the direct detection of the CnuB in a laboratory experiment is a great challenge to the present experimental techniques. We discuss the future prospects for the direct detection of the CnuB, with the emphasis on the method of captures on beta-decaying nuclei and the PTOLEMY project. Other possibilities using the electron-capture (EC) decaying nuclei, the annihilation of extremely high-energy cosmic neutrinos (EHEC\nus) at the Z-resonance, and the atomic de-excitation method are also discussed in this review.

arXiv comments
10 pages, 5 figures, to be published in the Proceedings of International Conference on Massive Neutrinos, Singapore, February 9-13, 2015
Journal reference
International Journal of Modern Physics A, 30,(2015) 1530031
DOI
doi:10.1142/S0217751X15300318
Subjects
hep-phHigh Energy Physics, Phenomenology astro-ph.COCosmology and Nongalactic Astrophysics hep-exHigh Energy Physics, Experiment

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    • It is something being worked on, though [0]. Extremely difficult does not equate to impossible :) 0: http://arxiv.org/abs/1504.03966

      diceView on HNParent context

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