PDF-October 6, 2011 |year 54Do neutrinos really travel faster than light?

3 Mystery Tour 147We no longer ght conventional wars148 Biweekly magazine of the Eindhoven University of TechnologyFor news wwwtuenlcursor and follow tuecursor on Twitter and Facebook 4 . 10K pace 1520 seconds per mile faster than 12 marathon race pace Marathon Pace 1520 seconds per mile slower than 12 marathon pace 10 11 12 WEEK MON TUE WED THUR FRI SAT SUN REST DAY Cross training or core work EASY RUN 4 miles 4 x 20 second strides From . Dark Matter . Annihilation. Jason Kumar. University of. H. a. w. a. i. i. collaborators. Jin In. Carsten. . Rott. Pearl Sandick. Jennifer Gaskins. David Yaylali. 1502. 02091, 15xx.xxxxx. dark matter and monoenergetic neutrinos. Angela Zhang. 7/11/14. Theory of Relativity. Faster than light?. Lab Spots of CERN. Antonio . Ereditato. The words “errors”, “mistakes” and “flop” were bandied about regarding what in actual fact is standard scientific procedure in experimental work.. 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 . C.W. James, . ECAP, University of Erlangen,. on behalf of the ANTARES collaboration.. Cosmic . rays and neutrinos. What produces this spectrum?. Standard model: acceleration at relativistic astrophysical shocks. Physics Opportunities with. Supernova Neutrinos. Georg Raffelt, Max-Planck-Institut für Physik, München. Sanduleak -69 202. Sanduleak . -. 69 202. Large Magellanic Cloud . Distance 50 kpc . (160.000 light years). 1. John Beacom, The Ohio State University. 2. Plan of the Talk. Introduction to Supernova . N. eutrinos. Focus on . B. urst . D. etection. . What will we know after the next burst?. What . new capabilities do we need?. Angela Zhang. 7/11/14. Theory of Relativity. Faster than light?. Lab Spots of CERN. Antonio . Ereditato. The words “errors”, “mistakes” and “flop” were bandied about regarding what in actual fact is standard scientific procedure in experimental work.. and Earth Structures. 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 force. Have no . Neutrinos. Ghost . Particles . of the . Universe. Georg G. Raffelt. Max-Planck-Institut f. ür Physik, München, Germany. Neutron. Proton. Gravitation (Gravitons?) . Weak . Interaction (W and Z Bosons). Dr Susan Cartwright. Department of Physics and Astronomy. Discovering neutrinos. Routes to scientific discovery:. Accident!. You find something unexpected in your data. For example, gamma-ray bursts (discovered by satellites designed to look for clandestine nuclear tests). Art McDonald, Professor Emeritus. Queen’s University, Kingston, . Ontario, Canada. T. he middle of the sun is so hot that the centers of the atoms (nuclei). f. use together, giving off lots of energy and neutrinos. The neutrinos penetrate easily through the dense material in the Sun and reach the earth.. ?. History in the Making?. 1862: Maxwell found that there should be electromagnetic waves travelling at approximately the (known) speed of light. 1905: Einstein used universal speed of light as foundation of geometric description of physics. When is travel . considered. University . Business. ? . Only qualified travel is eligible for . reimbursements.. Travel will be considered to have a University business purpose if the travel:. Is an integral part of the student's degree work, e.g. attend a conference; visit a field site or laboratory facility, or.