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Dr Martin Hendry University of Glasgow. Why are we here?…. The period of inflation in the very early Universe was invoked to explain some apparent fine
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KamLAND Update Lauren Hsu Lawrence Berkeley National Laboratory Fermi National Accelerator Laboratory January 16, 2007
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Post Main Sequence Evolution of “Low-Mass” Stars Chapter 19 (and some of 20) 1
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Evidence of Neutrino Oscillation from SNO Chun Shing Jason Pun Department of Physics The University of Hong Kong Presented at the HKU Neutrino Workshop
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Clicker Question: Earth’s average density is about the same as: A: water B: an iron meteorite C: balsa wood D: a chunk of volcanic rock
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NEW OPPORTUNITIES IN PLASMA-SURFACE INTERACTIONS FOR FUNCTIONALIZATION OF SURFACES* Ananth Bhoj, Natalie Babaeva, Rajesh Dorai and Mark J. Kushner Iowa
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The Sun The Sun in X-rays over several years The Sun is a star: a shining ball of gas powered by nuclear fusion. Luminosity of Sun = 4 x 10 33 erg/s =
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Neutrino Plasma Coupling in Dense Astrophysical Plasmas Robert Bingham CCLRC – Centre for Fundamental Physics (CfFP) Rutherford Appleton Laboratory L O
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Solar Neutrinos Dr Robert Smith Astronomy Centre University of Sussex
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