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Documents LRP2010 - WG5 Fundamental Interactions Nathal Severijns ( K.U.Leuven) for WG5 Town Meeting Madrid,.....

Slide 1LRP2010 - WG5 Fundamental Interactions Nathal Severijns ( K.U.Leuven) for WG5 Town Meeting Madrid, June 1 - 3, 2010 2/10/20141WG5 - N. Severijns - Town Meeting, Madrid,…

Documents Are we sure it isn’t ordinary matter/baryons? Not in compact objects (brown dwarfs, etc.) Baryons....

Slide 1Are we sure it isn’t ordinary matter/baryons? Not in compact objects (brown dwarfs, etc.) Baryons should also contribute to nucleosynthesis But we got it to work…

Documents Status of LHC, CMS & India in CMS A. Gurtu Tata Institute of Fundamental Research, Mumbai.

Slide 1Status of LHC, CMS & India in CMS A. Gurtu Tata Institute of Fundamental Research, Mumbai Slide 2114 GeV from LEP)"> A. Gurtu: Talk at "Workshop on…

Documents Characterization of an Antenna for the Search of Neutrino Mass. By: John Ndungu Advisor: Dr. Leslie....

Slide 1 Characterization of an Antenna for the Search of Neutrino Mass. By: John Ndungu Advisor: Dr. Leslie Rosenberg Post Doc Advisor: Dr. Gray Rybka Philander Smith College…

Documents Two of the essential gradients of lepto-genesis CP violation D( B-L) 0 Majorana

Future Prospect of Accelerator-based Neutrino Oscillation Experiments and other next generation experiments Two of the essential gradients of lepto-genesis CP violation D(B-L)…

Documents SNOLAB @ GeoNeutrino 2008 Sudbury Sept 18 th, 2008 SNOLAB: A New International Facility for...

SNOLAB: A New International Facility for Underground Astroparticle Physics T. Noble Queenâs University 3 Our model of how the Sun burns is very accurate. 2 Neutrinos must…

Documents DARK MATTER IN THE UNIVERSE? PRESENTED BY L. KULL AT THE R.H.FLEET SCIENCE CENTER December 14,2005.

DARK MATTER IN THE UNIVERSE? PRESENTED BY L. KULL AT THE R.H.FLEET SCIENCE CENTER December 14,2005 Why be concerned about the amount of matter in the universe? Start with…

Documents Recent Neutrino Oscillation Results and Future

Sever@IHEP Recent Neutrino Oscillation Results and Future Jun Cao Institute of High Energy Physics ‹#› 1 There are 3 famailes of massless Neutrinos in the SM. There are…