1. POURQUOI LE CERN? C. Vander Velde ULB 19 avril 2002 Le CERN Contenu: Matin: • Introduction: qu’est-ce que le CERN? • Qu’est-ce que la physique des particules?…

Slide 1 Neutrinos as probes of ultra-high energy astrophysical phenomena Jenni Adams, University of Canterbury, New Zealand Slide 2 up to 10 MeV 10-40 MeV GeV – 10sTeV…

Slide 1 1 Neutrino: a spy of the innermost solar interior Nuclear reactions in the Sun and solar neutrinos Slide 2 2 The spy of nuclear reactions in the Sun The real proof…

Slide 1 1 Some key problems and key reactions in Nuclear Astrophysics Main issues: BBN: was the universe always the same? What’s in the core of Sun and other MS stars?…

Slide 1 Pierre Descouvemont Université Libre de Bruxelles, Brussels, Belgium The 12 C(  ) 16 O reaction: dreams and nightmares theoretical introduction Slide 2…

Slide 1 Bonding Slide 2 Bonds Atoms of different elements may join together in a number of ways. Slide 3 Colors First, take two primary colors, like elements of color instead…

Slide 1 Chapter 8 Periodic Table of Properties Slide 2 Review: Mendeleev’s Periodic Table Slide 3 Periodic Law Recall from C7…Elements in the same group (vertical column)…

Forbidden & Exotic decays in NA62 Gianluca Lamanna 11.12.2009 NA62 Physics Handbook Meeting “Forbiddens” and “exotics” * Only K+ modes (for the moment) Direct…

JP Mendiburu- LAPP - Les Houches June 2001 JPM- LAPP-Les Houches-2001, slide# Discovery : V. Hess (1911) Ballon flight (5000m) Electrometers Non solar origin (eclipse) Understanding…