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PARTICLE PHYSICS

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We are encouraged to spend 1% of our research grant funding on 'outreach' ... ev. top 180 GeV. ATMOSPHERIC NEUTRINOS. EARTH. Cosmic ray (protons) Neutrino. Detector ... – PowerPoint PPT presentation

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Title: PARTICLE PHYSICS


1
W. G. SCOTT RAL/PPD 28 Nov 2007
PUBLIC UNDERSTANDING OF SCIENCE
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 produce highly qualified researchers with
advanced skills needed by academia, industry and
commerce.

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.


2
THE STANDARD MODEL
(schematic)
higgs kinetic term
yukawa term
fermion kinetic term
gauge kinetic term
where
higgs potential
field-strength tensor
covariant derivative
vector potential
3
THE HIGGS FIELD
quarks leptons W,Z etc.
gives masses to the pointlike particles
refraction?.
4
but not to the neutron/proton!
PROTON
NEUTRON
uUP (2/3)
QUARKS
dDOWN (-1/3)
5
PARTICLE PHYSICS
  • http//www.net.rl.ac.uk/ramfiles/ppd2001-01.ram

6
THE ATOM
electrons (-)
NUCLEUS
proton()
neutron
7
PROTON
NEUTRON
uUP (2/3)
QUARKS
dDOWN (-1/3)
8
ELECTRICAL FORCES
e-
e-
Photon
QUANTUM FIELD THEORY
9
QED
e-
e-
?
e-
e-
10
(No Transcript)
11
(No Transcript)
12
(No Transcript)
13
QED
d
e-
?
e-
d
14
QUARK CONFINEMENT
The Strong Force
Quark
Antiquark
15
CHROMOSTATICS
16
CHROMOSTATICS
THE COLOUR FORCE
17
QCD
gluons 8 colours
quarks 3 colours
18
(No Transcript)
19
THE WEAK FORCEBeta Decay
n
p
Antineutrino
Electron
20
BETA DECAY(at the quark level)
d
u
Antineutrino
Electron
21
(No Transcript)
22
WEAK INTERACTION
u
e-
W
d
23
THE WEAK FORCE
Due to W-boson exchange
24
The Discovery of the W/- and Z0UAI
(1983)MASSES W/- 80GeVZ0 91GeV
25
NEUTRAL CURRENTS (1973)
26
ELECTRO-WEAK
27
THE FORCE PARTICLES
g1 g2 g3 g4 g5 g6 g7 g8W- Z0 W?
28
CERN
29
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30
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31
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32
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33
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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
w
w-
z0
e
e-
37
(No Transcript)
38
GAUGE THEORIES
39
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40
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41
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42
MATTER PARTICLES(Fermions)
1 1 0(Pauli exclusion principle)
FORCE PARTICLES(Bosons)
1 1 4(Stimulated emission, lasers etc)
43
PLANCK SCALE 10 GeV
GRAND UNIFICATION
19
GUT SCALE 10 GeV
hyper.
16
weak
INVERSE COUPLING
strong
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
48
(No Transcript)
49
(No Transcript)
50
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51
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52
THE NEUTRINO
V
A VERY FRIENDLY PARTICLE
53
ATMOSPHERIC NEUTRINOS
54
SUPER-KAMIOKANDE
55
MINOS
CHICAGO
MINESSOTA (750 Km)
56
(No Transcript)
57
CP-VIOLATION
58
THE FUNDAMENTAL FORCES
ELECTRO- MAGNETIC
UNIFIED FORCE?
STRONG
GRAVITY
WEAK
59
RECENT DEVELOPMENTS IN PARTICLE PHYSICS
1973 Neutral currents 1983 w/-,
z 1996 z ? ww
60
NEUTRINO MASSES ??
1) Solar2) Atmospheric? v3 85 MeV ?
61
THE DISCOVERY OF TOP(1994)
t ? b w evtop 180 GeV
62
ATMOSPHERIC NEUTRINOS
EARTH
Neutrino
Cosmic ray (protons)
Detector
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