Microsoft PowerPoint - resident physics
Moonwalk2014.pdf
Radius of Observable Universe and Expansion Rate vs time, k = 0 = 0 Radiation dominated R = 3 x 10 -33 cm R = 10 cm R. =10 18 c 10 -15 c.
KamLAND Update Lauren Hsu Lawrence Berkeley National Laboratory Fermi National Accelerator Laboratory January 16, 2007.
KamLAND Update Lauren Hsu Lawrence Berkeley National Laboratory June 17, 2005 LEPP Journal Club.
Neutrino Physics & the ISS Peter Dornan Imperial College London.
18 February 2015Modern Physics III Lecture 71Modern Physics III Lecture 8Modern Physics III Lecture 6 Modern Physics for Frommies III A Universe of Leptons,
Neutrino Physics & the ISS
The must fundamental constituents of matter Physics 100 Chapt 26.
