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Transcript
Probing the Structure of Matter
A History of Fundamental Particle Physics
Steve Schnetzer
Rutgers University
1
Fundamental Particle Physics
2
Fundamental Particle Physics
ä What are the fundamental constituents of the universe?
2
Fundamental Particle Physics
ä What are the fundamental constituents of the universe?
ä How do they interact with each other?
2
How to Judge How We’re Doing
Constituents
• Number: economical
• Properties: few and simple
• Point-like? (no structure)
Theory
• Mathematically consistent
• Explains all observations
• Able to make predictions
3
Ancient Greece
Plato
Aristotle
4
Ancient Greece
All is mathematical form
Plato
Aristotle
4
Ancient Greece
All is mathematical form
I can figure
out the universe
by pure thought
Plato
Aristotle
4
Fundamental Physics
Circa 500 B.C.
The universe is built on the five Platonic solids
Democritus
5
Fundamental Physics
Circa 500 B.C.
PSST! The universe is made up
of atoms
The universe is built on the five Platonic solids
Democritus
5
The Classical Period
1687 − 1897
6
Newton
7
Newton
The world is made of point particles
7
Newton
8
Newton
The world is I made
have of
no point
idea
what
they are
particles
8
Chemists Discover Evidence for Atoms
1802
John Dalton
•
•
•
•
Gay-Lussac’s Law
Boyle’s Law
Charles’s Law
Law of Multiple Proportions
9
World’s First Particle Physicist
1827
Discovered Brownian Motion
Robert Brown
Botanist
movie
10
Periodic Table
1869
a classification scheme
Mendeleev
11
Periodic Table
1869
a classification scheme
Mendeleev
11
Fundamental Particle Physics
End of 19th century
92 Atoms
12
The Romantic Period
1897 − 1932
NJAAPT Banquet
March 14, 2008
13
The Cavendish
World’s premier physics
laboratory late 19th century
The Cavendish
Cambridge University
Bunsen Cell
A Typical Lab
14
Discovery of the Electron
J. J. Thomson
A new particle
Thomson’s CRT
electrically charged
15
The Plum Pudding Model
can knock electrons out of atoms (photoelectric effect)
⇒ electrons are a part of atoms
How to make a stable
electrically neutral atom?
negatively charged electrons distributed like raisins in a positively charged “pudding”
16
Lord Rutherford
World’s first high energy physicist
1910
Use high energy (5 MeV) alpha particles from radium decay to study structure of the atom.
Ernest Rutherford
very light electrons should
have no effect on the alpha’s
scattering of the alpha’s will
indicate structure of the “pudding”
17
Rutherford Scattering
A surprise
some of the alpha’s
scattered at large angles
Data is described by
assuming alpha’s scattered
of a massive point charge
18
Rutherford Scattering
A surprise
some of the alpha’s
scattered at large angles
Data is described by
assuming alpha’s scattered
of a massive point charge
18
The Nuclear Atom
Nearly all of the mass of the atom concentrated in a very
small positively charged nucleus.
How small is the nucleus?
19
Heisenberg Uncertainty Principle
precision of measurement
Why we need large, expensive
high energy accelerators
if you want to probe
something at small distances, you have
to kick it hard
momentum transferred
Rutherford couldn’t
resolve the nucleus.
It looked like a point.
20
Discovery of the Neutron
1932
James Chadwick
Alpha particles interacting in air found to knock out neutral particles.
Rutherford had earlier discovered the proton (the nucleus of the hydrogen atom)
Atoms made out of:
protons, neutrons, electrons
21
The Neutrino
A free neutron decays
to a proton and electron in about 15 minutes
• not a 2-body decay
• must be a third unseen particle
Ghost-like neutrino
Predicted in 1930 by Pauli
Discovered in 1956 by Cowan and Reines
Pauli
22
Fundamental Particle Physics
1932
neutrino
electron
photon
proton
neutron
23
The Modern Period
1932 − 1974
24
Cosmic Rays
The cosmic accelerator
much higher energies
than available in the lab
with higher energies can
produce more massive particles
cloud chamber
25
26
Antimatter
1932
Carl Anderson discovers anti-electrons (positrons)
positron track
27
Discovery of the Muon
1937: the muon a heavy electron
discovered by Anderson
Just like electron
except about 200 times more mass
I.I. Rabi
28
Discovery of the Muon
1937: the muon a heavy electron
discovered by Anderson
Who ordered that?
Just like electron
except about 200 times more mass
I.I. Rabi
28
Particle Discoveries
29
Particle Discoveries
1947: pions discovered using photographic emulsions at high altitudes
.jpg (JPEG Image, 600 × 400 pixels)
http://static01.nyt.com/images/2012/08/07/science/07HESS_SPAN/07HESS-articleLarge.jpg
30
Structure of the Nucleus
1953
Scattered 125 MeV
electrons off of nuclei
Hofstadter
nuclear size:
cm
31
Structure of the Proton
Scattered 550 MeV
1956
electrons off of nuclei
Hofstadter’s spectrometer
Mark 3 electron linac
at Stanford University
The proton has a size
it is not a point-like object
32
The Bevatron
6 GeV proton synchrotron
in the hills of Berkeley
Designed to discover
the anti-proton
33
“Seeing” Particles
The bubble chamber
Donald Glaser
Luis Alvarez
34
The Particle Zoo
Hundreds of new particles discovered 1955 - 1965.
What does it all mean?
35
Quarks
1964
Three quarks
up
down
strange
mesons:
baryons:
Murray Gell-Mann
d
d d
u
proton
neutron
u
u
36
Classification Again
meson octet
baryon octet
prediction:
bound state of
3 strange quarks
baryon decaplet
37
Brookhaven
The AGS
33 GeV proton synchrotron
38
Discovery of the Omega Minus
1964
Nick Samios
80 - inch bubble chamber
39
Discovery of the Omega Minus
40
Stanford Linear Accelerator Center
SLAC
30 GeV electrons
2-mile long linear accelerator
41
Inside the Proton
1968
SLAC - MIT Group
Kendall
Friedman
deep inelastic scattering
Taylor
proton
42
Inside the Proton
1968
SLAC - MIT Group
Kendall
Friedman
deep inelastic scattering
Taylor
Rutherford scattering off
of point objects again
43
Fundamental Particle Physics
1974
leptons
gauge boson
quarks
44
The Golden Period
1974 − 1982
45
Discovery of a New Quark
1974
resonance
SPEAR
Electron-positron collider
Burt Richter
bound state of charm
and anti-charm quarks
Charmonium
46
Simultaneous Discovery
AGS Experiment
Sam Ting
Double-arm spectrometer
47
Discovery of a New Heavy Electron
1975
The tau lepton
Just like electron except about 2000 times more mass
Marty Perl
48
Fermilab
400 GeV Proton Synchrotron
2 km diameter ring
Robert Wilson
49
Discovery of Another New Quark
1976
bound state of bottom
and anti-bottom quarks
Leon Lederman
50
Discovery of Another New Quark
1976
bound state of bottom
and anti-bottom quarks
Leon Lederman
50
Discovery of the Gluon
1979
30 GeV e+e- Collider
Sau Lan Wu
PETRA
carrier of the strong force
Quantum Chromo Dynamics
binds quarks together to make proton
51
The Standard Model
Quantum Electrodynamics
charged particles interacting by photon exchange
atomic physics
Quantum Chromodynamics
quarks interacting by gluon exchange
binding of quarks
Weak Force
particles interacting by W and Z exchange
heavy lepton decay
heavy quark decay
neutrino interactions
52
CERN
Off to the French Alps
proton − antiproton
collisions at 450 GeV
53
Discovery of the W and Z
1982
Rubbia
UA 1 Detector
54
Fundamental Particle Physics
1982
leptons
gauge bosons
quarks
55
The Recent Period
1982 − 2008
56
LEP
1989 - 2000
100 GeV electron - positron
collisions at CERN
27 kilometer tunnel
57
Z Factory
Over 10 million Z’s produced
and decays studied by four
large detectors
Aleph Detector
58
Precision Tests of Standard Model
• Standard Model tested to 0.1% level
in agreement with all measurements
down to 10-16 cm
• Only three light neutrinos
• Higgs still missing
59
Discovery of the Top Quark
1995
2 TeV Proton - Antiproton collisions
Fermilab Tevatron Collider
Production top anti-top
D0 Collaboration
60
Fundamental Particle Physics
2008
leptons
quarks
gauge bosons
Higgs
missing
NJAAPT Banquet
March 14, 2008
61
SM Summary
Complete, consistent theory of fundamental physics
✹ Fundamental constituents:
6 quarks and 6 leptons
plus antiparticles
✹ Three fundamental forces:
Electromagnetic
mediated by
photons
Strong
mediated by
gluons
Weak
mediated by
W+ W- Z0
✹ Agrees with all experiments to 10-16 cm
✹ Needs Higgs particle to be complete
62
The Large Hadron Collider
14 TeV proton antiproton collisions in the LEP tunnel
2008
probing matter at
the 10-17 cm scale
Atlas Detector
CMS Detector
63
The Current Period
2009 − 2015
NJAAPT Banquet
March 14, 2008
64
The Large Hadron Collider
65
Big Detectors, Big Collaborations
The CMS Collaboration
The CMS Collaboration
~ 1/4 of the people who made CMS possible
3170 scientists and engineers (including ~800
66
Higgs Decay Fractions
H ! bb
58%
H ! W +W
22%
H ! gg
8.6%
H ! ⌧ +⌧
6.3%
H ! cc
2.9%
H ! ZZ
2.6%
H!
0.2%
67
The Higgs Discovery
CMS
ATLAS
1 of 1
68
Problems with the Standard Model
• “Natural” mass of the Higgs is 1019 GeV/c2.
Why is it 17 orders of magnitude smaller?
• The Standard Model does not include gravity.
• Why does matter dominate over antimatter?
• Why are there three generations of matter particles?
• What explains the values of the masses?
• Too many parameters (27).
• Higgs mechanism seems ad hoc.
• Doesn’t account for Dark Matter
• Doesn’t account for Dark Energy
69
LHC Physics
Discovery of the Higgs Boson
• Missing ingredient of the Standard Model (SM)
• Now have complete mathematically consistent theory
• Agrees with all experiments down to 10-18 m scale
What lies beyond the SM at smaller
distance (higher energy) scales?
• Measure decay fractions of Higgs to 1% precision
• Search for Supersymmetry (SUSY)
- Might explain why Higgs is unnaturally light
- Lightest SUSY particle provides Dark Matter
candidate
• Search for other exotics
- Vector
- Like quarks, . . .
• Find the unexpected
70
Future Circular Collider
A 100 TeV collider under discussion at CERN / China
No guarantee of new physics
de-image-2.jpg (PNG Image, 517 × 272 pixels)
http://tlep.web.cern.ch/sites/tlep.web.cern.ch/themes/profe
Design report in 2018
Turn on in the 2050?