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Fundamentals of Particle Physics
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Transcript of Fundamentals of Particle Physics
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A short journey to the infinitely small
Fundamentals of
Particle Physics
Stefania Ricciardi
RAL, March 2009
Building blocks: particles and forces Current areas of research
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Warning
This journey may change your vision of the Universe.
What you will hear may alter your perception of reality.
We are entering a Quantum World..
Stay awake and keep an open mind!
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We and all things around us aremade of atoms
Human Hair~ 50 m = 50 10-6 m
= 0.000050 m
Atom ~ 10-10 m= 0.0000000001 m
Magritte
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Atoms
Atoms are all similarly made of:- protons and neutrons in the nucleus- electrons orbiting around
electron
proton
neutron
Protons,neutrons are
made up ofquarks
The electron was thefirst elementary
particle to bediscovered(JJ Thomson 1897)
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From the atom to the quark
Atoms and sub-atomic particles are much smaller than visible light wave-lengthTherefore, we cannot really see them (all graphics are artists impressions)To learn about the sub-atomic structure we need particle accelerators
How small are the smallest constituents of matter?
~ 10-10 m~ 10-14 m
~ 10-15 m
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Wave-particle duality of Nature
Central concept of quantum mechanics:all particles present wave-like properties
De Broglie showed that moving particles have anequivalent wavelength l
p
1
lSo high momentum gives usshort wavelengths so we canmake out small details
Example: electron microscope
Not only light has a dual nature
Electron Microscope Image
Gold atoms(0.2 nm apart)
Copyright FEI
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1911Rutherford found a nucleus in theatom by firing alpha particles at gold
and observing them bounce back
Rutherford: atoms are notelementary particles!
Precursor of modern scattering experiments at accelerator
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Quarks detected within protons
Stanford (SLAC), California, late 1960sFire electrons at proton: big deflections seen!
2 miles long accelerator
End Station Aexperimental area
Freeway 280
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Protons and neutronsin the quark model
proton (charge +1) neutron (charge 0)
u d
d
u u
d
Quarks have fractional electric charge!u electric charge + 2/3d electric charge -1/3
13
1
3
2
3
2
-
pduu 0
3
1
3
1
3
2nddu
-
-
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Neutrinos get under your skin!
Within your body at any instant:roughly 30 million neutrinos fromthe Big Bang
No worries!Neutrinos do not harm us.
Our bodies are transparent to neutrinos
14 neutrinosper second from Sun
are zipping through you
n
Every cm2
of Earth surface iscrossed every second by morethan 10 billion (1010) neutrinosproduced in the Sun
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The particles of ordinary matter
ne
e-
u
d-1/3
+2/30
-1
charge
All stable matter around uscan be described using
electrons, neutrinos, u and d quarks
Quarks:u = up
d = down
Leptons:neutrino
e = electron
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3 Families (or Generations)
nm
m-
c
s
nt
t-
t
b
Ordinary matter Cosmic rays Accelerators
1st generation 2nd generation 3rd generation
3 generations in everything similar but the mass
-1/3-1/3
+2/3 +2/3
ne
e-
u
d-1/3
+2/3
We believe these to be the fundamentalbuilding blocks of matter
-1 -1 -1
0 00
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Quark masses
0
20
40
60
80
100
120
140
160180
Mass
(GeV)
Quarks
Up Down Strange Charm Bottom Top
0.003 0.006 0.095 1.2 4.5
Top(discovered 1995)
175 GeV
E= mc2
1 proton mass ~ 1GeV (10-27 Kg)
The mass grows larger in each successive family
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Anti-matter
For every fundamental particle of matter there is an anti-particlewith same mass and properties but opposite charge
ne
e-
u
d
-1/3
+2/3
ne
e+
u
d
+1/3
-2/3
+1
0
-1
0
positron
Correspondent anti-particles exist for all three families Anti-matter can be produced using accelerators
Matter Anti-Matter
Bar on topto indicateanti-particle
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Matter-antimatter pair creation
Electron-positron pair created out ofphotons hitting the bubble-chamberliquid
Example of conversion of photonenergy into matter and anti-matter
Matter and anti-matter spiral in oppositedirections in the magnetic field due tothe opposite charge
Energy and momentum is conserved
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Quarks and colourAll quark flavours come in 3 versions, called colours
u d+2/3 -1/3uu ddup down
Quarks combine together to form colourless particles
-Baryons(three quarks: red+ green + blue = white)
-Mesons(quark-antiquark pair)such as red+anti-red u-ubar state
proton
uu
pion
p
Strong forcesglue quarks
together inbound states
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Building more particles
b b
J/y
c c
Y
b u
B-
u b
B+
b d
B0
d b
B0
B mesons (bq)
Many more mesons and baryons
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The Particle Physicists Bible:
Particle Data Book
https://pdg.lbl.gov
"Young man, if I could rememberthe names of these particles,
I would have been a botanist!
E.Fermi to his student
L. Lederman (both Nobellaureates)
Most particles are not stable and can decay to lighter particles..
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THE WEAK FORCEBeta Decay
n p
Antineutrino
Electron
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Neutron b-decay
A (free) neutron decays after 15 min
u d
d
n u ud
p e-
d u e-
ne
ne
15 min
At quark level:
Long life time (15min is an eternity in particle physics!) weak
without such weak interactions the Sun would shut down!
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The 4 forces of Nature
Weak Beta-decay pp fusion
StrongQuark binding
ElectromagneticTV, PCs Magnets
e- e+ creation
GravityResponsible of
Keeping uswell-planted on earth
Electriccharge
mass
weak
charge
strongcharge
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Electromagnetic force
e- e-
Photon
The repulsive force that two approaching electrons feel
Photon is the particleassociated to the electromagnetic forcesmallest bundle of force
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Weak force: W-,W+,Z0
b-decaynpene
Electric chargeconserved at each
vertex
W-
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Strong force: gluons
Gluons interact with quarks Gluons interact with other gluons
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Quark confinementThere are no free quarks, quarks and antiquarks are confined
in colourless doublet (mesons) or triplets (baryons) by the exchangeof gluons
The new quarks boundto the old quarksand form new mesons
until the gluon connectionsnaps, and other quark-antiquarkpairs are created out of theenergy released
Gluon hold quarkstogether as they movefurther apart
Z0
Decay
S.Ward
Force Particles (summary)
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Force Particles (summary)
Particles interact and/or decay thanks to forcesForces are also responsible of binding particles together
Strong: gluons
Only quarks
(because of their
colour charge)
Weak: W+, W-, Z0
Leptons and quarks (onlyforce for neutrinos)
Electromagnetic:gQuarks and charged leptons(no neutrinos)
Gravity: graviton?Still to be discovered
Negligible effects onparticles
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O ti :
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Open question:
Why is the Universe made of
matter and not equallyof anti-matter?
We have seen that for every fundamental
particle there is a corresponding antiparticle.
Where are these anti-particles?
Large amount of matter but no evidence oflarge amount of antimatter in the Universe..
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Why has all the anti-matter gone?
Anti-matter
The development of the Universe containing
matter and no antimatter requires thatmatter and antimatter behave differently
This phenomenon is due to CP violation..
matter Puff
Good thing for us that there is no antimatter around!
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CP Violation
CP = Charge Conjugation (reverse charge) x Parity (reverse spatialcoordinates as in a mirror)
CP
beauty anti-beauty
B0 B0
Nobody
is perfect
CP-Violation: B0 and B0 do not behave exactly in the same way
(their decay pattern as a function of time is different)
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Discovery of CP violation in theB-meson system at Babar (SLAC, 2001)
A visible difference is detected, but tiny, not enoughto explain the matter-antimatter asymmetry in the Universe
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The CPV quest will go on at LHC
CMS ALICE
CERN
LHCb experiment:700physicists
50institutes15countries
LHCb cavern
LHCb
ATLAS
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Recent view of the LHCb cavern
Its complete!
RICH-1
The experiment is fully installed and ready for first collisions
RICH2 RICH1
Muondetector
Calorimeters OT Magnet
VELO
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Another open question:What is the Dark Matter?
Astronomical observations have shown that observable mass
represent less than 4% of the Universe!
What is dark matter? We dont really know
Perhaps partially composed of neutrinos, or possibly neutralinos particlespredicted by super-symmetric theories beyond the Standard Model?
Dark MatterVisible Matter
False-color imagesThe brightness ofclumpscorresponds to thedensity of mass.
http://imagine.gsfc.nasa.gov/docs/dict_ad.htmlhttp://imagine.gsfc.nasa.gov/docs/dict_ad.html -
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Looking for Dark Matter at theBoulby Underground Laboratory
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Neutrinos do matter to us:If there were no neutrinosthe sun would not shine!
Almost no interactions (only weak)
Can cross light-years of material without being affected Can travel from the most remote corners of the Universebringing information from the origin of space and time
Puzzling neutrinos
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R. Davis: measuring the solar neutrinoflux in a gold mine in South Dakota for
30 years (1969-1999)
and observing only 1/3 of the expected flux!! Why?
R. DavisSolar neutrinospioneer
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Neutrino oscillationsIf you let the neutrino travel enough,
it can change its flavour!nm
nt
ent
a huge neutrino detectorin the right place exists!
A detector heredoes not see any nm
Kamioka Observatory, ICRR (Institute for
Cosmic Ray Research),The University of Tokyo
a huge neutrino detectorexists!
A detector heresees all nm
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in the Kamioka mine in JapanSuperKamiokande is measuring neutrinos born in the atmospherabove the detector..
flux from below only of flux from above!
..and below the detector (on the other side of the Earth!!)
Total neutrino flux from below = total flux from above _
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Discovery of neutrino oscillationSuper-Kamiokande (1998)
Half of the nm are lost!
Oscillated to undetected nt
2002 Nobel PrizeKoshiba
(superK Spokesman)shared with Davis
Up-going Down-going
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What have we learnt?
A number of surprising things:
A limited number of forces and matter particlesdescribe all the Universe we know about;
A theory of the interactions of matter with forcescalled the Standard Model describes successfully thephenomena of the subatomic world;
There are evidences that there is lot more that we donot know about and our research should find: such asthe missing anti-matter, dark matter, puzzling neutrinoproperties, but also the Standard Model key-vault..the Higgs!
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Looking into the future
The Higgs should be found at theLHCplease be patient for a few more
hours.and you will learn about the
Higgs, the LHC, and much more!
NOT