170 likes | 244 Views
Big World of Small Neutrinos. Roman Shcherbakov 21, March, 2007. 3 Nobel prizes. 1988 LEDERMAN, SCHWARTZ and JACK STEIN BERG ER – detected muon neutrinos 1995 REINES – detected reactor neutrinos in 1956 2002 RAYMOND and KOSHIBA – detected solar neutrinos. NS. Neutrino optics.
E N D
Big World of Small Neutrinos Roman Shcherbakov 21, March, 2007
3 Nobel prizes • 1988 LEDERMAN,SCHWARTZ and JACKSTEINBERGER – detected muon neutrinos • 1995 REINES – detected reactor neutrinos in 1956 • 2002 RAYMOND andKOSHIBA – detected solar neutrinos
NS Neutrino optics in the Neutron Star in the Sun in the Earth
Mixing matrix =>different neutrino & antineutrino For E=10MeV L12~300km L13~10km Neutrino oscillations Hierarchy is not yet known Only 1/3 of born electron neutrino stay electron neutrino
Solar neutrinos > 50 trillion solar neutrinos pass through the human body every second but it would take approximately one light year of lead to block half of them 400kEv 10MEv
In the nucleus Atom recoil
8 B-decay energy spectrum
MSW effect Oscillations enforced by scattering • Not important for the Sun • Considered in detailed calculations of supernova explosions
Supernova 1987a 51kpc away 24 neutrinos
Cosmic neutrino background (CNB) Similar to CMB Undetectable by any means Bad dark matter candidate – relativistic in the time of recombination Cold dark matter is favorable for structure formation
Cuspy halos are not cuspy 2 solutions • Large annihilation cross-section of • cold dark matter (KKT model) • Warm dark matter
Cold dark matter annihilation Doesn’t work Only decay to sterile particles Is possible
☻ ☺ ☺ ☻ Conclusions Neutrinos provide a new great tool for: • probing the interior of the Sun • observing the early stages of supernovae • proving particle theories