✦ LIBER ✦

Neutrino physics from SNO

✍ Scribed by A.L. Hallin

Publisher: Elsevier Science
Year: 2010
Tongue: English
Weight: 265 KB
Volume: 64
Category: Article
ISSN: 0146-6410
DOI: 10.1016/j.ppnp.2009.12.009

No coin nor oath required. For personal study only.

📜 SIMILAR VOLUMES

SNO & Solar Neutrino Results

✍ J. Maneira 📂 Article 📅 2007 🏛 Elsevier Science 🌐 English ⚖ 398 KB

Results from SNO and Other Solar Neutrin

Results from SNO and Other Solar Neutrino Experiments

✍ R.G.H. Robertson 📂 Article 📅 2005 🏛 Elsevier Science 🌐 English ⚖ 292 KB

Neutrino physics from cosmological obser

Neutrino physics from cosmological observations

✍ Steen Hannestada 📂 Article 📅 2003 🏛 Elsevier Science 🌐 English ⚖ 943 KB

The rich neutrino programme of the SNO+

The rich neutrino programme of the SNO+ experiment

✍ Christine Kraus; Simon J.M. Peeters 📂 Article 📅 2010 🏛 Elsevier Science 🌐 English ⚖ 513 KB

The SNO+ experiment is a multi-faceted neutrino experiment re-using the existing infrastructure and detector hardware of the Sudbury Neutrino Observatory located in Vale Inco's Creighton mine, Sudbury (ON), Canada. The main aim of this, now fully-funded, experiment is the search for neutrinoless dou

Physics Results from the Baikal Neutrino

Physics Results from the Baikal Neutrino Telescope

✍ K. Antipin; V. Aynutdinov; V. Balkanov; I. Belolaptikov; N. Budnev; I. Danilchen 📂 Article 📅 2007 🏛 Elsevier Science 🌐 English ⚖ 397 KB

UHE neutrinos: From conventional to new

UHE neutrinos: From conventional to new physics

✍ V. Berezinsky 📂 Article 📅 2009 🏛 Elsevier Science 🌐 English ⚖ 463 KB

UHE neutrinos with E410 17 eV are produced by ultra-high energy cosmic rays (UHECR) interacting with CMB photons (cosmogenic neutrinos) and by top-down sources, such as topological defects (TDs) and superheavy dark matter (SHDM). Cosmogenic neutrinos are reliably predicted and their fluxes can be nu