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Kamiokande II Results
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Neutrino Oscillations and the Solar Neutrino Puzzle by Professor G Srinivasan
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- 1 Summer course 2018 - A Random walk in astro-physics
- 2 Neutrino Oscillation and the Solar Neutrino Puzzle Lecture-09Lecture - 09
- 3 The case of the Missing Neutrinos
- 4 Radioactivity and B-decay
- 5 The Neutrino 1930
- 6 Fermi's theory of B - Decay
- 7 The Neutrino family
- 8 Mean free path of the neutrinos
- 9 The fusion of hydrogen into helium
- 10 The proton - proton chain reaction
- 11 Branch 1 85 percent:
- 12 How do we know that all this is true?
- 13 The brave warriors!
- 14 Raymond Davis Experiment
- 15 Davis' Experiment: First results, 1968
- 16 What was wrong?
- 17 The Neutrino family
- 18 Something happened on the way to the earth?
- 19 Neutrino Oscillations
- 20 The Solar Neutrino Puzzle
- 21 The experiment was refined and refined!
- 22 New experiments were planned
- 23 The Gallium Experiments
- 24 Neutrino-electron scattering experiments
- 25 Kamiokande II Experiment
- 26 Kamiokande II Results
- 27 The Super-Kamiokande Detector
- 28 Three men in a boat!
- 29 The Super-Kamiokande Results
- 30 Amount of electron neutrinos expected
- 31 The missing solar neutrinos
- 32 Could the standard model of the Sun be wrong?
- 33 Helioseismology
- 34 The atmospheric neutrinos
- 35 Atmospheric Neutrinos
- 36 Super Kamiokande experiment to detect the atmospheric neutrinos
- 37 The atmospheric neutrinos
- 38 Atmospheric neutrino data from Super Kamikande expt.
- 39 Expected number without oscillation
- 40 Atmospheric neutrino experiment had proved neutrino oscillations.
- 41 Expected Ve from the Sun
- 42 To find the 'smoking gun'
- 43 The Sudbury Neutrino Observatory
- 44 Neutrino Absorption in Heavy water
- 45 Neutrino - Electron scattering:
- 46 Deuteron break up: v + d =n+ +v
- 47 Actual data of a candidate neutrind event
- 48 Background events
- 49 The Sudbury Results
- 50 The Sensational Sudbury Results
- 51 Nobel Prize 1995
- 52 Nobel Prize, 2002
- 53 Nobel Prize for Physics - 2015
- 54 Neutrino Oscillation
- 55 Circularly Polarized Light
- 56 The time evolution of an electron neutrino state may now be expressed as
- 57 Oscillation probabilities between two neutrino flavors
- 58 The mystery is solved!
- 59 Epilogue
- 60 Next Lecture: Quantum Stars
- 61 Q&A
