1. The Ghostly Neutrino Steve Boyd, University of Warwick

2. “If we are to understand “why we are here” and the basic properties of the universe we live in, we must understand the neutrino.” American Physical Society Report - 2004

3. A little bit of history What are they? Where do they come from? Why study them? A recent surprise The T2K Project

4. CRISIS

5. Energy(Ra) ≠ Energy(Ac)+Energy(e)

6. “At the present stage of atomic theory we have no arguments for upholding the concept of energy balance in the case of b-ray disintegrations.” Neils Bohr

7. Wolfgang Pauli “Desperate remedy.....” “I do not dare publish this idea....” “I admit my way out may look improbable....” “Weigh it and pass sentence....” “You tell them. I'm off to a party”

8. Energy(Ra) ≠ Energy(Ac)+Energy(e)

9. Energy(Ra) = Energy(Ac)+Energy(e) + Energy(Neutrino)

10. What are neutrinos?

11. Electron, e Tiny mass ( 1 ) -

12. Electron Neutrino, n e 0 Very tiny mass (<0.0000001) Electron, e Tiny mass ( 1 ) -

16. x 500

17. Very tiny mass (<0.0000001) e nene e nene Electron Neutrino, n e 0 Very tiny mass (<0.0000001) Electron, e Tiny mass ( 1 ) -

18. In experiments neutrinos are NEVER seen. We can only detect them through the byproducts of their interactions with matter. Type of the charged particle detected used to infer the type of incoming neutrino. e e

19. Electron Neutrino, n e Electron, e mass ( 1 ) - Muon Neutrino, n m Muon, m mass ( 200 ) - Tau Neutrino, n t Tau, t mass ( 3500 ) - 3 Lepton Types

20. m nene t nene

21. Electron Antineutrino, n e Positron, e + mass ( 1 ) + 3 Antiparticles Muon Antineutrino, n m Muon, m + mass ( 200 ) + Tau Antineutrino, n m Tau, t + mass ( 3500 ) +

22. Where do they come from?

23. Everywhere

25. From the Big Bang Artist's conception

26. From the Big Bang Artist's conception One cubic foot of space contains about 10,000,000 neutrinos left over from the Big Bang.

27. From Astrophysical Objects Supernovae created the heavy elements (us) and neutrinos appear to be important to the explosion dynamics.

28. From the Sun ≈ 70 million per cm 2 per second at the Earth

29. From Cosmic Rays.

31. Geoneutrinos

32. From Us.

33. So why don't we notice? n are almost ghosts. They interact extremely weakly with matter. To a neutrino a planet is mostly empty space.

34. "The chances of a neutrino actually hitting something as it travels through all this howling emptiness are roughly comparable to that of dropping a ball bearing at random from a cruising 747 and hitting, say, an egg sandwich." Douglas Adams

35. 500,000,000,000,000 solar n just went through you

36. enpnenpn enpnenpn enpnenpn enpnenpn enpnenpn enpnenpn enpnenpn

37. Why do we study them?

38. Probes of environments that we otherwise cannot see Probes of objects too far away for anything else Cosmological and astrophysical implications Matter/Antimatter imbalance

39. Probes of environments that we otherwise cannot see Probes of objects too far away for anything else Cosmological and astrophysical implications Matter/Antimatter imbalance NEUTRINO ASTROPHYSICS

41. Probes of environments that we otherwise cannot see Probes of objects too far away for anything else Cosmological and astrophysical implications Matter/Antimatter imbalance

42. Universal Structure m  eVm  eV m  eVm  eV

43. Probes of environments that we otherwise cannot see Probes of objects too far away for anything else Cosmological and astrophysical implications Matter/Antimatter imbalance

44. Why is there more matter than antimatter? =

46. Sub-Atomic Talk Show Disasters

47. CP Violation Q. Is there a difference between the physics of matter and antimatter? A.Yes there is. We study this here with an experiment called BaBar “B 0 / B 0 mixing”

48. Q. Is there a difference between the physics of matter and antimatter? A.Yes there is. We've never seen it in neutrinos, though. Matter-Antimatter Asymmetry n n n n n n n n n n n n “Leptogenesis”

49. How to study this?

50. Neutrino Oscillations THE discovery in neutrinos of the last 20 years l nlnl l nlnl A typical neutrino experiment

51. The Sun is Broken!!! Ray Davis – Early 1970s

52. An atom a day 1 Ar atom every two days Only

53. Less than expected Expected Measured Number n observed

54. Neutrino Oscillations THE discovery in neutrinos of the last 20 years e nene m nmnm Neutrinos were changing flavour between sun and detector!

55. Distance Travelled Prob. It is n e 0 1 e nene m nmnm

56. Eh? Q. How can a n e spontaneously turn into a n m ?

57. Eh? Q. How can a n e spontaneously turn into a n m ? A. The n e isn't a particle. It's three! n e ≡ “that thing which was always produced/detected with an electron” e nene

58. Quantum Stuff e nene e n1n1 e n2n2 e n3n3 = or 60% 30% 10%

59. e nene m nmnm Original n 1,n 2,n 3 mixture Different n 1,n 2,n 3 mixture n 1,n 2,n 3 travels at different speeds This can only happen if n 1,n 2,n 3 have different masses Only gives us differences in masses Long journey

60. Why so important? The Standard Model of Particle Physics has no explanation for a non-zero, but tiny, neutrino mass – so we are in “unknown physics” territory. Neutrino masses link to GUT theories. Has cosmological implications (mass balance, structure)

61. The T2K Experiment

62. University of Warwick University of Sheffield Imperial College, University of London Oxford University University of Liverpool University of Lancaster Queen Mary College, University of London Rutherford-Appleton Laboratories

63. 295 km

68. JPARC Facility

69. TARGET nmnm

70. 295 km

71. Super-Kamiokande nmnm nene

74. Water Cerenkov

75. Electron-like : has a fuzzy ring Muon-like : has a sharp edged ring and particle stopped in detector.

76. Open Questions How much do n 1,n 2 and n 3 weigh? Why are they so much lighter than all the other massive particles? Are neutrinos the same as antineutrinos? Are neutrinos the reason we are here at all?

77. ‘‘...these kind of findings have implications that are not limited to the laboratory. They affect the whole of society — not only our economy, but our very view of life, our understanding of our relations with others, and our place in time.’’ Bill Clinton

79. L sin 2 (2q) Dm 2 = m 1 2 -m 2 2

80. Why do blue sky research? 5% of jobs in UK are in physics-based sectors Gross added value from physics sectors was estimated to be 70 billion pounds in 2005 Synergy between PP projects and industry – industry acquires added skills base for other applications Training - 50% of PP PhDs go into other sectors Radioisotope production Sensors for medical applications High level computing for biological modelling Spin off tools for other science (e.g. DIAMOND) Nuclear fusion research Muon tomography in border security Airport scanners Rock Imaging Cancer treatment using next gen cyclotrons