'Solar neutrinos' diaporamas de présentation

Recent Results from KamLAND

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HE2: Muons and Neutrinos

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Neutrino Ocillations and Astroparticle Physics (2)

Neutrino Ocillations and Astroparticle Physics (2). John Carr Centre de Physique des Particules de Marseille (IN2P3/CNRS). Pisa, 7 May 2002. ? Neutrino Oscillations - Solar Neutrinos - Atmospheric Neutrinos

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Mrs. Coronado Modern Physics Notes

Mrs. Coronado Modern Physics Notes. TMHS. The Atom. Nucleus contains p rotons and neutrons. Electrons orbit nucleus i n energy levels. Atomic Mass. Combination of protons and neutrons (nucleus). What atom is this?. Atomic Number.

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Exam 2: Wednesday, March 30 Review Session to be scheduled.

Exam 2: Wednesday, March 30 Review Session to be scheduled. Homework 5 Due Wednesday Multiple choice by 6:00 pm Extra credit by 2:30 pm. THE SUN. The source of light, heat and (nearly all) energy on the earth. Diameter: 1,390,000 km (4.6 light seconds)

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Experimental Neutrino Physics

Experimental Neutrino Physics. Susan Cartwright University of Sheffield. Introduction: Massive neutrinos in the Standard Model. Dirac and Majorana masses The mixing matrix and neutrino oscillations . Massive neutrinos in the Standard Model.

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The Unbearable Lightness of Neutrinos

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Neutrino Oscillations, Proton Decay and Grand Unified Theories

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Physics Potential of the LENA Detector

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Nuclear reactions and solar neutrinos

Trieste 23-25 Sept. 2002. Episode III. Nuclear reactions and solar neutrinos. Nuclear reactions and solar neutrinos. The basis of Nuclear Astrophysics The spies of nuclear reactions in the Sun The luminosity constraint The pp chain -pp neutrinos -Be neutrinos -B neutrinos

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Chapter 15

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Chapter 15

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Solar Neutrino Analysis of S uper- K amiokande ICRC2013 @Rio de J aneiro 8 July 2013

Solar Neutrino Analysis of S uper- K amiokande ICRC2013 @Rio de J aneiro 8 July 2013 . Hiroyuki Sekiya ICRR, University of Tokyo for the Super-K Collaboration. 1. Super- Kamiokande. Physics targets of Super- Kamiokande. Proton decay. Relic SN ?. WIMPs. Atmospheric ?. Solar ?.

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The Borexino Solar Neutrino Experiment

1. The Borexino Solar Neutrino Experiment. Frank Calaprice for the Borexino Collaboration. Milano. Perugia. Borexino Collaboration. Princeton University. Genova. APC Paris. Virginia Tech. University. Univ. Massachusetts. Kurchatov Institute. Jagiellonian U. Cracow.

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Small Scale Facilities in EUROPE ( not included in the Large Scale Facilitity Network)

Small Scale Facilities in EUROPE ( not included in the Large Scale Facilitity Network). Belgium: 1 IKS KU Leuven Czech Republic: 2 Nucl. Phys. Inst. Acad. Sci. Rez Greece: 1 Demokritos Athens France: 2 IPN Orsay and CEN Bordeaux Hungary: 2 Inst. Nucl. Research Debrecen

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Neutrino oscillations/mixing

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T . It is true! The Sun is about 74% hydrogen, 25% helium and 1% everything else (by mass).

IQ. The sun is made of hydrogen (~74%) and helium (~25%), making it similar in composition to the theoretical mix of the universe at the time of the Big Bang. T F. IQ. T . It is true! The Sun is about 74% hydrogen, 25% helium and 1% everything else (by mass).

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Best values and uncertainties of the nuclear reaction cross sections important to solar burning

PHYSUN 2010 THE PHYSICS OF THE SUN AND THE SOLAR NEUTRINOS. Best values and uncertainties of the nuclear reaction cross sections important to solar burning (SOLAR FUSION II) A. Formicola for LUNA collaboration. Reaction rate in the laboratory. ?. Extrapolation is needed !!.

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