Big World of Small Neutrinos

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Big World of Small Big World of Small Neutrinos Neutrinos Roman Shcherbakov Roman Shcherbakov 21, March, 2007 21, March, 2007

description

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. - PowerPoint PPT Presentation

Transcript of Big World of Small Neutrinos

Page 1: Big World of Small Neutrinos

Big World of Small NeutrinosBig World of Small Neutrinos

Roman ShcherbakovRoman Shcherbakov21, March, 200721, March, 2007

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3 Nobel prizes3 Nobel prizes

1988 1988 LEDERMAN,LEDERMAN, SCHWARTZ and JACKSCHWARTZ and JACK STEINSTEINBERGBERGERER – – detected muon neutrinosdetected muon neutrinos

1995 REINES – detected reactor neutrinos in 19561995 REINES – detected reactor neutrinos in 1956 2002 2002 RAYMOND andRAYMOND and KOSHIBAKOSHIBA – detected solar neutrinos – detected solar neutrinos

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Neutrino opticsNeutrino optics

NS

in the Neutron Star

in the Earth

in the Sun

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Neutrino oscillationsNeutrino oscillations

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Neutrino oscillationsNeutrino oscillations

Hierarchy is not yet known

Mixing matrix

=>different neutrino & antineutrino

For E=10MeV L12~300km L13~10km

Only 1/3 of born electron neutrino stay electron neutrino

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Solar neutrinosSolar neutrinos> 50 trillion solar neutrinos pass through the human body every second

it would take approximately one light year of lead to block half of them

butbut

400kEv

10MEv

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Qen e p:decayβAtomrecoil

In the nucleus

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B-decay energy spectrumB-decay energy spectrum8

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MSW effectMSW effect

Oscillations enforced by scattering

•Not important for the Sun

•Considered in detailed calculations of supernova explosions

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Supernova 1987aSupernova 1987a

51kpc away

24 neutrinos

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Supernova explosion (type II)Supernova explosion (type II)

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Theoretical neutrino spectrumTheoretical neutrino spectrum

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Total neutrinoTotal neutrinobackground luminositybackground luminosity

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Cosmic neutrino background (CNB)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

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Cuspy halos are not cuspyCuspy halos are not cuspy

2 solutions

• Large annihilation cross-section of cold dark matter (KKT model)

• Warm dark matter

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Cold dark matter annihilationCold dark matter annihilation

Doesn’twork

Only decay tosterile particlesIs possible

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ConclusionsConclusions

Neutrinos provide a new great tool for:Neutrinos provide a new great tool for: probing the interior of the Sunprobing the interior of the Sun observing the early stages of supernovae observing the early stages of supernovae proving particle theoriesproving particle theories

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