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PUBLIC UNDERSTANDING OF SCIENCE W. G. SCOTT RAL/PPD 28 Nov 2007 We are encouraged to spend 1% of our research grant funding on “outreach” activities, promoting.

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Presentation on theme: "PUBLIC UNDERSTANDING OF SCIENCE W. G. SCOTT RAL/PPD 28 Nov 2007 We are encouraged to spend 1% of our research grant funding on “outreach” activities, promoting."— Presentation transcript:

1 PUBLIC UNDERSTANDING OF SCIENCE W. G. SCOTT RAL/PPD 28 Nov 2007 We are encouraged to spend 1% of our research grant funding on “outreach” activities, promoting understanding, appreciation and awareness of our science to the general public: Targeting 11-16 yr olds in schools etc. can help attract more young people into a scientific career. (e.g. RAL MasterClass 12-14 Mar 2008). Helps ensure that the UKs front line contribution in this science is recognised by opinion formers, decision-takers/politicians. Taxpayers can have an appreciation and awareness of the research being funded on their behalf. Helps produce highly qualified researchers with advanced skills needed by academia, industry and commerce.

2 THE STANDARD MODEL: “higgs potential” fermion kinetic term gauge “kinetic” term yukawa term higgs kinetic term where: “covariant derivative” field-strength tensor vector potential (schematic)

3 THE HIGGS FIELD: gives masses to the pointlike particles : quarks leptons W,Z etc. refraction?.

4 u=“UP” (+2/3) PROTON NEUTRON d=“DOWN” (-1/3) QUARKS …but not to the neutron/proton!

5 PARTICLE PHYSICS http://www.net.rl.ac.uk/ramfiles/ppd2001-01.ram

6 THE ATOM neutron NUCLEUS electrons (-) proton (+)

7 u=“UP” (+2/3) PROTON NEUTRON d=“DOWN” (-1/3) QUARKS

8 ELECTRICAL FORCES e-e- e-e- Photon QUANTUM FIELD THEORY

9 QED e- γ

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13 d d γ QED

14 QUARK CONFINEMENT The “Strong” Force Quark Antiquark

15 “CHROMOSTATICS”

16 THE “COLOUR” FORCE

17 QCD gluons 8 colours quarks 3 colours

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19 THE WEAK FORCE Beta Decay np Antineutrino Electron

20 BETA DECAY (at the quark level) du Antineutrino Electron

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22 u e- d W+ WEAK INTERACTION

23 THE WEAK FORCE u e- W+ Due to W-boson exchange

24 The Discovery of the W +/- and Z 0 UAI (1983) MASSES: W +/- ≈ 80GeV Z 0 ≈ 91GeV

25 NEUTRAL CURRENTS (1973)

26 ELECTRO-WEAK

27 THE “FORCE” PARTICLES g 1 g 2 g 3 g 4 g 5 g 6 g 7 g 8 W - Z 0 W + γ

28 CERN

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34 THE “MATTER” PARTICLES Q -1 0-1/3 +2/3

35 THE DISCOVERY OF TOP (Fermilab USA 1994) top ≈ 180 GeV

36 ELECTROWEAK e-e- e+e+ z0z0 w+w+ w-w-

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38 GAUGE THEORIES

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42 MATTER PARTICLES (Fermions) FORCE PARTICLES (Bosons) 1 + 1 = 0 (Pauli exclusion principle) 1 + 1 = 4 (Stimulated emission, lasers etc)

43 PLANCK SCALE 10 GeV 19 GUT SCALE 10 GeV 16 GRAND UNIFICATION: strong weak hyper. INVERSE COUPLING ENERGY GeV

44 INTERACTION WITH THE HIGGS FIELD gives masses to the “point-like” particles, quarks, leptons, W, Z etc.

45 PROF HIGGS UNIV EDINBURGH

46 HIGGS AT LEP

47 TO DISCOVER THE HIGGS WE NEED: THE LHC

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52 V THE NEUTRINO A VERY FRIENDLY PARTICLE

53 ATMOSPHERIC NEUTRINOS

54 SUPER-KAMIOKANDE

55 MINOS CHICAGOMINESSOTA (750 Km)

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57 CP-VIOLATION

58 THE FUNDAMENTAL FORCES WEAK STRONGGRAVITY ELECTRO- MAGNETIC UNIFIED FORCE?

59 1973“Neutral currents” 1983w+/-, z 1996z* → ww RECENT DEVELOPMENTS IN PARTICLE PHYSICS

60 NEUTRINO MASSES ?? 1)Solar 2)Atmospheric →v 3 ≈ 85 MeV ?

61 THE DISCOVERY OF TOP (1994) t → b w ev top ≈ 180 GeV

62 ATMOSPHERIC NEUTRINOS EARTH Cosmic ray (protons) Neutrino Detector


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