Tau Particle
14th April 2008Fergus Wilson, RAL1 Fergus Wilson, Email: F.F.Wilson at rl.ac.uk Experimental Particle Physics PHYS6011 Southampton University 2008 Lecture.
The Sun and the Particle Physics
5.3 Nuclear physics G485 Fields, Particles, Frontiers of Physics 5.3 Nuclear physics G485 Fields, Particles, Frontiers of Physics Mr Powell 2012 Index.
By Miriam Aczel. What are neutrinos? They are almost massless— hardly feel the force of gravity They have no electric charge— don’t feel the electromagnetic.
FLAVOURS 50 Years After SU(3) Discovery Djordje Šijački.
Amand Faessler, Tuebingen Double Beta Decay and Neutrino Masses Amand Faessler Tuebingen 1. Solution of the Solar Neutrino Problem by SNO. 2. Neutrino.
Modern Physics: A Conclusion Michael Dine May, 2003.
F.Sanchez (UAB/IFAE)ISS Meeting, Detector Parallel Meeting. Jan 2006 Low Energy Neutrino Interactions & Near Detectors F.Sánchez Universitat Autònoma de.
The Role of Neutrinos in Galaxy Formation Katherine Cook and Natalie Johnson .
Great Observatories Fermi Gamma ray Space Telescope (2008) Large Area Telescope Gammas hit thin metal sheets, converting to electron-positron pairs via.
5.3.2 Fundamental Particles. (a) explain that since protons and neutrons contain charged constituents called quarks they are, therefore, not fundamental.