Neutrinos. Invisible particles all around us. Amol Dighe. Department of Theoretical Physics Tata Institute of Fundamental Research, Mumbai
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1 Neutrinos Invisible particles all around us Amol Dighe Department of Theoretical Physics Tata Institute of Fundamental Research, Mumbai DTP Presentation, VSRP 2013, TIFR, May 29, 2013
2 Why care about invisible neutrinos? 1 (Pragmatist:) They are needed for the Sun to shine 2 (Philosopher:) They are responsible for our existence 3 (Fatalist:) They are everywhere: we can t escape them 4 (Quizmaster:) They set up interesting puzzles 5 (Adventurer:) Detecting them is a challenge!
3 Why care about invisible neutrinos? 1 (Pragmatist:) They are needed for the Sun to shine 2 (Philosopher:) They are responsible for our existence 3 (Fatalist:) They are everywhere: we can t escape them 4 (Quizmaster:) They set up interesting puzzles 5 (Adventurer:) Detecting them is a challenge!
4 How does the sun shine? Nuclear fusion reactions: mainly H + 2e 4 2 He + light +2ν e Neutrinos needed to conserve energy, momentum, angular momentum Neutrinos essential for the Sun to shine!! Davis-Koshiba Nobel prize 2002
5 How does the sun shine? Nuclear fusion reactions: mainly H + 2e 4 2 He + light +2ν e Neutrinos needed to conserve energy, momentum, angular momentum Neutrinos essential for the Sun to shine!! Davis-Koshiba Nobel prize 2002
6 How does the sun shine? Nuclear fusion reactions: mainly H + 2e 4 2 He + light +2ν e Neutrinos needed to conserve energy, momentum, angular momentum Neutrinos essential for the Sun to shine!! Davis-Koshiba Nobel prize 2002
7 Neutrinos from the Sun A very very large number of neutrinos About hundred trillion through our body per second Hundred trillion = Even during night! Neutrinos during night = Neutrinos during day Reach us directly from the core of the Sun Light from the Sun s core cannot reach us directly Why do we not notice them?
8 Neutrinos from the Sun A very very large number of neutrinos About hundred trillion through our body per second Hundred trillion = Even during night! Neutrinos during night = Neutrinos during day Reach us directly from the core of the Sun Light from the Sun s core cannot reach us directly Why do we not notice them?
9 Neutrinos from the Sun A very very large number of neutrinos About hundred trillion through our body per second Hundred trillion = Even during night! Neutrinos during night = Neutrinos during day Reach us directly from the core of the Sun Light from the Sun s core cannot reach us directly Why do we not notice them?
10 Neutrinos from the Sun A very very large number of neutrinos About hundred trillion through our body per second Hundred trillion = Even during night! Neutrinos during night = Neutrinos during day Reach us directly from the core of the Sun Light from the Sun s core cannot reach us directly Why do we not notice them?
11 Neutrinos from the Sun A very very large number of neutrinos About hundred trillion through our body per second Hundred trillion = Even during night! Neutrinos during night = Neutrinos during day Reach us directly from the core of the Sun Light from the Sun s core cannot reach us directly Why do we not notice them?
12 Three questions, the same answer Why did the roti char? Why did the betel leaves (paan) rot? Why could the horse not run? Because they were not moved!
13 Three questions, the same answer Why did the roti char? Why did the betel leaves (paan) rot? Why could the horse not run? Because they were not moved!
14 Three questions about neutrinos Why do we not notice neutrinos passing through us? Why do neutrinos from the Sun reach us during night? Why can we see inside the sun with neutrinos? Pauli Dirac Because neutrinos interact extremely weakly!
15 Three questions about neutrinos Why do we not notice neutrinos passing through us? Why do neutrinos from the Sun reach us during night? Why can we see inside the sun with neutrinos? Pauli Dirac Because neutrinos interact extremely weakly!
16 The most weakly interacting particles Stopping radiation with lead shielding Stopping α, β, γ radiation: 50 cm Stopping neutrinos from the Sun: light years of lead! Answers to the three questions Why do we not notice neutrinos passing through us? Neutrinos pass through our bodies without interacting Why do neutrinos from the Sun reach us during night? Neutrinos pass through the Earth without interacting Why can we see inside the sun with neutrinos? Neutrinos pass through the Sun without interacting How do we see the neutrinos then?
17 The most weakly interacting particles Stopping radiation with lead shielding Stopping α, β, γ radiation: 50 cm Stopping neutrinos from the Sun: light years of lead! Answers to the three questions Why do we not notice neutrinos passing through us? Neutrinos pass through our bodies without interacting Why do neutrinos from the Sun reach us during night? Neutrinos pass through the Earth without interacting Why can we see inside the sun with neutrinos? Neutrinos pass through the Sun without interacting How do we see the neutrinos then?
18 The most weakly interacting particles Stopping radiation with lead shielding Stopping α, β, γ radiation: 50 cm Stopping neutrinos from the Sun: light years of lead! Answers to the three questions Why do we not notice neutrinos passing through us? Neutrinos pass through our bodies without interacting Why do neutrinos from the Sun reach us during night? Neutrinos pass through the Earth without interacting Why can we see inside the sun with neutrinos? Neutrinos pass through the Sun without interacting How do we see the neutrinos then?
19 The most weakly interacting particles Stopping radiation with lead shielding Stopping α, β, γ radiation: 50 cm Stopping neutrinos from the Sun: light years of lead! Answers to the three questions Why do we not notice neutrinos passing through us? Neutrinos pass through our bodies without interacting Why do neutrinos from the Sun reach us during night? Neutrinos pass through the Earth without interacting Why can we see inside the sun with neutrinos? Neutrinos pass through the Sun without interacting How do we see the neutrinos then?
20 The most weakly interacting particles Stopping radiation with lead shielding Stopping α, β, γ radiation: 50 cm Stopping neutrinos from the Sun: light years of lead! Answers to the three questions Why do we not notice neutrinos passing through us? Neutrinos pass through our bodies without interacting Why do neutrinos from the Sun reach us during night? Neutrinos pass through the Earth without interacting Why can we see inside the sun with neutrinos? Neutrinos pass through the Sun without interacting How do we see the neutrinos then?
21 The most weakly interacting particles Stopping radiation with lead shielding Stopping α, β, γ radiation: 50 cm Stopping neutrinos from the Sun: light years of lead! Answers to the three questions Why do we not notice neutrinos passing through us? Neutrinos pass through our bodies without interacting Why do neutrinos from the Sun reach us during night? Neutrinos pass through the Earth without interacting Why can we see inside the sun with neutrinos? Neutrinos pass through the Sun without interacting How do we see the neutrinos then?
22 SuperKamiokande: litres of water Recipe for observing neutrinos Build very large detectors Wait for a very long time SuperKamiokande observes about 5-10 neutrinos per day
23 SuperKamiokande: litres of water Recipe for observing neutrinos Build very large detectors Wait for a very long time SuperKamiokande observes about 5-10 neutrinos per day
24 Why care about invisible neutrinos? 1 (Pragmatist:) They are needed for the Sun to shine 2 (Philosopher:) They are responsible for our existence 3 (Fatalist:) They are everywhere: we can t escape them 4 (Quizmaster:) They set up interesting puzzles 5 (Adventurer:) Detecting them is a challenge!
25 A view from the Hubble telescope
26 The world without neutrinos
27 The world without neutrinos Role of neutrinos in creating atoms Neutrinos helped create the matter-antimatter asymmetry, without which, no atoms, no stars, no planets, no galaxies
28 Role of neutrinos in creating the Earth Earth has elements heavier than iron, which can be created only inside an exploding star (supernova) A supernova must have exploded bilions of years ago whose fragments formed the solar system Supernovae explode by neutrinos pushing the shock wave
29 Why care about invisible neutrinos? 1 (Pragmatist:) They are needed for the Sun to shine 2 (Philosopher:) They are responsible for our existence 3 (Fatalist:) They are everywhere: we can t escape them 4 (Quizmaster:) They set up interesting puzzles 5 (Adventurer:) Detecting them is a challenge!
30 The second-most abundant particles in the universe Cosmic microwave background: 400 photons/ cm 3 Temperature: 3 K Cosmic neutrino background: 300 neutrinos / cm 3 Temperature: 2 K Even empty space between galaxies is full of neutrinos!
31 Neutrinos everywhere
32 Three kinds of neutrinos: νe νµ ντ
33 The Standard Model of Particle Physics 3 neutrinos: ν e, ν µ, ν τ Zero charge spin 1/2 almost massless: at least a million times lighter than electron + Higgs
34 Why care about invisible neutrinos? 1 (Pragmatist:) They are needed for the Sun to shine 2 (Philosopher:) They are responsible for our existence 3 (Fatalist:) They are everywhere: we can t escape them 4 (Quizmaster:) They set up interesting puzzles 5 (Adventurer:) Detecting them is a challenge!
35 Neutrinos setting long-term puzzles Solar neutrino puzzle: 1960s 2002 Only about half the expected ν e observed! Possible solution: ν e change to ν µ /ν τ Atmospheric neutrino puzzle: 1980s 1998 Half the ν µ lost in the Earth! Possible solution: ν µ change to ν τ Reactor neutrino experiments Breaking news of 2012: 10% of reactor ν e are lost! Possible solution: ν e change to ν τ / ν τ
36 Neutrinos setting long-term puzzles Solar neutrino puzzle: 1960s 2002 Only about half the expected ν e observed! Possible solution: ν e change to ν µ /ν τ Atmospheric neutrino puzzle: 1980s 1998 Half the ν µ lost in the Earth! Possible solution: ν µ change to ν τ Reactor neutrino experiments Breaking news of 2012: 10% of reactor ν e are lost! Possible solution: ν e change to ν τ / ν τ
37 Three questions, the same answer ν conference participants Why did half the ν e from the sun become ν µ /ν τ? Why did half the ν µ from the atmosphere become ν τ? Why did 10% ν e from the reactors become ν µ /ν τ? Because neutrinos have different masses and they mix! Quantum Mechanics
38 Three questions, the same answer ν conference participants Why did half the ν e from the sun become ν µ /ν τ? Why did half the ν µ from the atmosphere become ν τ? Why did 10% ν e from the reactors become ν µ /ν τ? Because neutrinos have different masses and they mix! Quantum Mechanics
39 A short-lived puzzle ( ) Superluminal neutrinos? The neutrinos do not travel faster than light Relativity
40 Why care about invisible neutrinos? 1 (Pragmatist:) They are needed for the Sun to shine 2 (Philosopher:) They are responsible for our existence 3 (Fatalist:) They are everywhere: we can t escape them 4 (Quizmaster:) They set up interesting puzzles 5 (Adventurer:) Detecting them is a challenge!
41 Bigger and better detectors needed Superkamiokande: 50 kiloton 50 kiloton water = litres Observes about 5-10 neutrinos per day
42 Bigger and better: Megaton detectors 1 Megaton water = litres R&D continues... Have to locate deep underground to remove cosmic ray background
43 Below the antarctic ice: Gigaton IceCube 1 gigaton water = litres Only look at upward-going neutrinos to remove cosmic ray background
44 Coming soon inside a mountain near you: INO India-based Neutrino Observatory Under a mountain, inside a tunnel (Bodi Hills, TN) 1 km rock coverage from all sides 50 kiloton of magnetized iron ( kg) 25 years: a lifelong project
45 What do I take back from this talk? Neutrinos are everywhere, a wide energy range They are essential for our existence They tend to pose interesting puzzles Their detection needs LARGE detectors and a LOT of patience They may provide clues to many fundamental questions: What are we made of? Where do we come from? The actual nature of neutrinos is still unknown A very active field of research
46 What do I take back from this talk? Neutrinos are everywhere, a wide energy range They are essential for our existence They tend to pose interesting puzzles Their detection needs LARGE detectors and a LOT of patience They may provide clues to many fundamental questions: What are we made of? Where do we come from? The actual nature of neutrinos is still unknown A very active field of research
47 What do I take back from this talk? Neutrinos are everywhere, a wide energy range They are essential for our existence They tend to pose interesting puzzles Their detection needs LARGE detectors and a LOT of patience They may provide clues to many fundamental questions: What are we made of? Where do we come from? The actual nature of neutrinos is still unknown A very active field of research
48 What do I take back from this talk? Neutrinos are everywhere, a wide energy range They are essential for our existence They tend to pose interesting puzzles Their detection needs LARGE detectors and a LOT of patience They may provide clues to many fundamental questions: What are we made of? Where do we come from? The actual nature of neutrinos is still unknown A very active field of research
49 What do I take back from this talk? Neutrinos are everywhere, a wide energy range They are essential for our existence They tend to pose interesting puzzles Their detection needs LARGE detectors and a LOT of patience They may provide clues to many fundamental questions: What are we made of? Where do we come from? The actual nature of neutrinos is still unknown A very active field of research
50 What do I take back from this talk? Neutrinos are everywhere, a wide energy range They are essential for our existence They tend to pose interesting puzzles Their detection needs LARGE detectors and a LOT of patience They may provide clues to many fundamental questions: What are we made of? Where do we come from? The actual nature of neutrinos is still unknown A very active field of research
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