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Documents Discovery of the Neutrino Mass P1X* Frontiers of Physics Lectures psoler/P1X_neutrino.ppt 21-22...

Slide 1Discovery of the Neutrino Mass P1X* Frontiers of Physics Lectures http://ppewww.ph.gla.ac.uk/~psoler/P1X_neutrino.ppt 21-22 October 2003 Dr Paul Soler University of…

Documents REVISION LECTURE I SOLAR PHYSICS PHAS M314/SPCEG012 April 23, 2012 1.

Slide 1REVISION LECTURE I SOLAR PHYSICS PHAS M314/SPCEG012 April 23, 2012 1 Slide 2 KJHP part of Revision Lecture See http://www.mssl.ucl.ac.uk/~kjhp/http://www.mssl.ucl.ac.uk/~kjhp/…

Documents The Formation and Structure of Stars Chapter 9. The Big Picture Stars exist because of gravity....

Slide 1The Formation and Structure of Stars Chapter 9 Slide 2 The Big Picture Stars exist because of gravity. Gravity causes interstellar material to collapse to form stars.…

Technology 4. electricity and magnetism

1.Book 4 in the Light and Matter series of free introductory physics textbooks www.lightandmatter.com 2. The Light and Matter series of introductory physics textbooks: 1…

Documents Nobuhiro Maekawa (Nagoya Univ. KMI) TexPoint fonts used in EMF. Read the TexPoint manual before you....

Slide 1Nobuhiro Maekawa (Nagoya Univ. KMI) TexPoint fonts used in EMF. Read the TexPoint manual before you delete this box.: AA Slide 2 What I would like to talk today Slide…

Documents Advantage: Neutrinos 2. Neutrino scattering Super Kamiokande located 1000m underground in Kamioka...

Slide 1 Advantage: Neutrinos 2. Neutrino scattering Super Kamiokande located 1000m underground in Kamioka mine in Japan is a water Cherenkov detector made up of 50,000 m…

Documents By Miriam Aczel. What are neutrinos? They are almost massless— hardly feel the force of gravity...

Slide 1 By Miriam Aczel Slide 2 What are neutrinos? They are almost massless— hardly feel the force of gravity They have no electric charge— don’t feel the electromagnetic…

Documents The Sun – Our Star Chapter 8. The preceding chapter described how we can get information from a...

Slide 1 The Sun – Our Star Chapter 8 Slide 2 The preceding chapter described how we can get information from a spectrum. In this chapter, we apply these techniques to the…

Documents KamLAND Update Lauren Hsu Lawrence Berkeley National Laboratory Fermi National Accelerator...

Slide 1KamLAND Update Lauren Hsu Lawrence Berkeley National Laboratory Fermi National Accelerator Laboratory January 16, 2007 Slide 2 I. Reactor Experiments & Neutrino…

Documents It can be powered by NUCLEAR ENERGY! Luminosity ~ 10 billion years Nuclear Potential Energy (core) E...

Slide 1It can be powered by NUCLEAR ENERGY! Luminosity ~ 10 billion years Nuclear Potential Energy (core) E = mc 2 - Einstein, 1905 Slide 2 Gravitational contraction: Provided…