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The Standard Model The Standard Model and and Beyond Beyond Harrison B. Prosper 6 July, 2010 Fermilab Summer Lecture Series

The Standard Model and Beyond

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The Standard Model and Beyond. Harrison B. Prosper 6 July, 2010 Fermilab Summer Lecture Series. Where Do We Come From? What Are We? Where Are We Going? Paul Gauguin (1897) Museum of Fine Arts, Boston. The Standard Model. What is the Standard Model?. - PowerPoint PPT Presentation

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Page 1: The Standard Model and  Beyond

The Standard ModelThe Standard Modeland and

BeyondBeyondHarrison B. Prosper

6 July, 2010Fermilab Summer Lecture Series

Page 2: The Standard Model and  Beyond

2

Where Do We Come From? What Are We?

Where Are We Going? Paul Gauguin

(1897) Museum of Fine Arts, Boston

Page 3: The Standard Model and  Beyond

The Standard ModelThe Standard Model

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4

What is the Standard Model?What is the Standard Model?

The Standard Model (SM) is a quantum field theoryquantum field theory

that describes the excitationsexcitations of quantum fields quantum fields in spacetime

We interpret these excitations as particlesparticles

Page 5: The Standard Model and  Beyond

Matter

Up quark Down quark

e

Electron Antielectron Neutrino

νe

u d

Page 6: The Standard Model and  Beyond

ForcesForcesStrong Force 11 (Gluons)(Gluons)

Binds protons and neutrons to form nuclei

Electromagnetic Force 1010-2-2 (Photon)(Photon)Binds electrons and nuclei to form atoms

Weak Force 1010-5-5 (W & Z Bosons)(W & Z Bosons)Causes radioactivity

Gravitational Force 1010-39-39 (Graviton)(Graviton)Binds matter on large scales

Page 7: The Standard Model and  Beyond

Discovery, Electron – 18971897

J.J Thomson

Discovery, Top Quark – 19951995 CDF & DØ

A Century of High Energy PhysicsA Century of High Energy Physics

Page 8: The Standard Model and  Beyond

1897 – ELECTRON discovery Thomson1909 – PROTON discovery Rutherford

1928 – ANTIMATTER theory Dirac1930 – NEUTRINO theory Pauli1932 – NEUTRON discovery Chadwick1932 – POSITRON discovery Anderson1935 – EXCHANGE theory Yukawa

1948 – QED theory Feynman,…1961 - ELECTROWEAK theory Glashow 1964 – QUARK theory Gell-Man, Zweig1964 – HIGGS theory Higgs, Englert,…1967 – ELECTROWEAK theory Weinberg, Salam,…

A Century of Particle PhysicsA Century of Particle Physics

Page 9: The Standard Model and  Beyond

1971 – 73 QCD theory ‘t Hooft, Veltman, Gell-Man, Frisch,

Gross, Wilzcek, Politzer

1974 – CHARM discovery Ting, Richter1977 – BOTTOM discovery Lederman1979 – GLUON1979 – GLUON discovery TASSO, JADEJADE,

MARK-J, PLUTO1983 – W & Z discovery Rubbia/UA1, UA2

1995 – TOP1995 – TOP discovery DDØØ & CDF

A Century of Particle PhysicsA Century of Particle Physics

Page 10: The Standard Model and  Beyond

N

Neutron

Proton

P

e

Electron νe

Anti-electron neutrino

Fermi’s 1934 theory of beta-decay

Enrico Fermi 1901 - 1954

1934 – Theory of Beta Decay1934 – Theory of Beta Decay

Page 11: The Standard Model and  Beyond

11

1935 – Particle Exchange Theory1935 – Particle Exchange Theory

Hideki Yukawa (1935) showed that the potential energypotential energy between two particles has the form

mm is the mass of the particleparticle exchanged between the them

RR = = hc hc / mcmc2 is the range of the force

U (r) =−

g2

4πrexπ −

rR

⎛⎝⎜

⎞⎠⎟

Hideki Yukawa 1907 - 1981

Page 12: The Standard Model and  Beyond

12

1948 – Quantum Electrodynamics1948 – Quantum Electrodynamics

Feynman invented a systematic way to calculate the force between electrically charged particles, based on Yukawa’s idea of particle exchange

g g

y y

f

Richard P. Feynman 1918 - 1988

Feynman Diagram

Page 13: The Standard Model and  Beyond

N

Neutron

Proton

P

e

Electron

The Weak ForceThe Weak ForceGiven the success of QED it was natural to try to create an analogous theory of the weak force

νe

Anti-electron neutrino

Page 14: The Standard Model and  Beyond

N

Neutron

Proton

P

e

Electron

The Weak ForceThe Weak ForceGiven the success of QED it was natural to try to create an analogous theory of the weak force

νe

Anti-electron neutrino

W-

Page 15: The Standard Model and  Beyond

15

1961 – The Electroweak Theory1961 – The Electroweak Theory

Glashow Theory + Higgs Theory Electroweak Theory

(1967)

Steven Weinberg Abdus Salam

Sheldon Glashow (1961)

Page 16: The Standard Model and  Beyond

u d e

s μ

νe

νμ

Quarks Leptons+2/3 -1/3 -1 0

1964 – The Quark Model1964 – The Quark Model

Gell-Man and Zweig

Page 17: The Standard Model and  Beyond

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The Quark ModelThe Quark Model

u ud

d du

Proton Neutron

uuu

Delta++

The Delta++ puzzle

+1 0 +2

Page 18: The Standard Model and  Beyond

u

s

d e νe

Quarks Leptons+2/3 -1/3 -1 0

The Quark ModelThe Quark Model

u u u d d d

s s s

One possible solution: color charge color charge

(Greenberg, Frizsch, Gell-Man, Leutwyler)

μ νμ

Page 19: The Standard Model and  Beyond

u uu

d ud

u du

19

The Quark ModelThe Quark Model

Proton Neutron Delta++

Problem solved !

+1 0 +2

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1971 – The Theories Make Sense!1971 – The Theories Make Sense!

Martinus Veltman Gerard 't Hooft

1971 - Proved that theories of the sort created by Glashow, Weinberg and Salam are consistent

Page 21: The Standard Model and  Beyond

The Strong ForceThe Strong ForceProton

u

u d

u

u d

u

u d

gg

g

u

u d

u

u d

u

u d

1972-73 Quantum Chromodynamics (QCD)

Gross

Politzer

Wilczek

Page 22: The Standard Model and  Beyond

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Discovery of the GluonDiscovery of the Gluongqqee

1979 TASSOMARK-JJADEJADEPLUTO

DESYHamburg,Germany

Page 23: The Standard Model and  Beyond

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Discovery of Top the QuarkDiscovery of Top the Quark

1995CDFDØDØ

Fermilab

p π→ t→ e νe b

t → q ′q b

Page 24: The Standard Model and  Beyond

u u u d d d e

b b b t

c c c s s s μ

g g g g g g g g

g Z W+

νe

νt

νμ

Quarks Leptons+2/3 -1/3 -1 0

I

II

III

Bos

ons

Ferm

ions

The Standard ModelThe Standard Model

H

t t t

W-

Page 25: The Standard Model and  Beyond

……And BeyondAnd Beyond

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SupersymmetrySupersymmetry

CompositenessCompositeness

StringsStrings

MultiverseMultiverse

TechnicolorTechnicolor

Extra DimensionsExtra Dimensions

Brane WorldsBrane Worlds

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PuzzlesPuzzlesThe Identity Puzzle

What makes a top quark a top quark, an electron an electron, and a neutrino a neutrino? (Chris Quigg, 2007)

The Mass PuzzleWhat is the origin of the mass of fundamental

particles?

The Matter PuzzleWhy is there overwhelmingly more matter than

antimatter?

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The Just-So PuzzleWhat determines the values of the Standard Model

parameters? Or, are we special?

The Gravity PuzzleWhy strongstrong: emem: weakweak: gravitygravity = 11: : 1010-2-2: : 1010-5-5: 10: 10-39-39 ?

The Dark Matter PuzzleWhat is dark matter?

The Dark Energy PuzzleWhy is dark energy?

PuzzlesPuzzles

Page 29: The Standard Model and  Beyond

The Mass Puzzle

u d

u

Total mass 9.6 MeV

Total mass 938 MeV !!

m =Ec2

The Proton BasketThe Proton Basket2.3 MeV 5 MeV

2.3 MeV

Page 30: The Standard Model and  Beyond

The Mass Puzzle – A Solution?

B. Robson, “The Generation Model and the Origin of Mass”,Int. J. Mod. Phys. E18 (2009)

T T

VT T

T

T

V

V

e

V

V

VV

V

V

T

V

V T

T

V T

T

T

u d

ν ν

d u e−

Page 31: The Standard Model and  Beyond

The Just-So Puzzle

d u

d

NeutronProton

u d

u

2.3 MeV2.3 MeV5.0 MeV_______9.6 MeV

5.0 MeV5.0 MeV2.3 MeV_______12.3 MeV

938.3 MeV – 9.6 MeV928.7 MeV928.7 MeV

939.6 MeV–12.3 MeV927.3 MeV927.3 MeV

Are we special?

Page 32: The Standard Model and  Beyond

Life in the Multiverse

Alejandro JenkinsFlorida State University

Scientific AmericanJanuary 2010

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33

The Gravity PuzzleThe Gravity Puzzle

1010-39-39

Page 34: The Standard Model and  Beyond

Gravity on the BraneGravity on the Brane

34

Isaac Newton(1687)

F =GμMr2

rg ⋅d

rA=4πGM—∫

Gauss’ Law

Our 3-D brane

Page 35: The Standard Model and  Beyond

Gravity in 3 + n DimensionsGravity in 3 + n Dimensions

35

F ~ GnmMrn2

Arkani-Hamed, Dimopoulos, Dvali

(1998)

rg ⋅d

rA=4πGM—∫

Gauss’ Law

Our 3-D brane

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R

Gravity in 3 + n DimensionsGravity in 3 + n Dimensions

F ~ GnmMrn2

Suppose that gravity can propagate a distance R away from our 3-D brane world

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When r >> R, the gravity force should look like Newton’s law of gravity

RThis yieldsthe relationGG = = GGn n / / RRnn

F ~Gn

Rn⎛⎝⎜

⎞⎠⎟μMr2

Gravity in 3 + n DimensionsGravity in 3 + n Dimensions

Page 38: The Standard Model and  Beyond

Searching for Branes at Fermilab!Searching for Branes at Fermilab!

38

G

p p

g

One way: look for photon + unexplained amounts of missing momentum

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39

The Era of the Large Hadron ColliderThe Era of the Large Hadron Collider

CERN

Geneva

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The EndThe EndCERN