'Cosmic neutrino background' diaporamas de présentation

Neutrinos Theory

Neutrinos Theory. ~. Carlos Pena Garay IAS, Princeton. References. Neutrino Unbound http://www.nu.to.infn.it/. Massive Neutrinos : Dirac. n (p,h). n (p,-h). CPT. Boost, if m ? 0. Boost, if m ? 0. n (p,-h). n (p,h). CPT. Standard Model + right handed.

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How Powerful is the Sun?

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Search for the Cosmic Neutrino Background and the Nuclear Beta Decay .

Search for the Cosmic Neutrino Background and the Nuclear Beta Decay . Amand Faessler University of Tuebingen Germany. Publication : Amand F aessler, Rastislav Hodak , Sergey Kovalenko , Fedor Simkovic: arXiv : 1304.5632 [ nucl-th ] 20. April 2013. .

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Cosmic Neutrino Background

Cosmic Neutrino Background. Zong-Kuan Guo NCU, Taiwan, March 30, 2013. particles:. h istory of the relic neutrinos. ~0.3MeV. ~0.1MeV. ~1eV. ~1MeV. n eutrino decoupling. e ? e ? annihilation. photon decoupling. structure formation. BBN. the weak reaction rate:.

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Search for Neutrino D ecay

Search for Neutrino D ecay. Univ. of Tsukuba, JAXA/ISAS, Okayama Univ., Fukui Univ., Kinki Univ., KEK, Seoul National Univ., Fermilab. Expected spectrum for. Search for in cosmic neutrino background (CNB) Direct detection of CNB Direct m easurement of neutrino mass

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