1 back to class 10/22/04 ian shipsey quarks and the cosmos ian shipsey(*) (*) one of 15...
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Back to class 10/22/04 Ian Shipsey 1
Quarks and the Cosmos
Ian Shipsey(*) (*) one of 15 astrophysicists
& particle physicists at Purdue University
A lecture to thePresident’s CouncilPurdue University
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Atomic Nucleus
electron1
radius of nucleus1.000
one billionth of a nanometer
0.1 nanometer
1 meter10000.000.000.
The size of atoms, quarks and electrons
Quarks aresimilar insize to electrons
Most of an atom is empty space
1 atomic radius
100,000
one millionth of a nanometer
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Question for the class
Proton electric charge = +1
Neutron electric charge = 0
u
u
d d
u
d
What are the charges of up and down quarks?
up = +2/3 down = +1/3
up = +2/3 down = -1/3
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Inner space: The four forces
Lets quarkschange identity(d u)
(Nobel prize2004)
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The periodic table of the elementary particles
+ anti-matter(antiparticles for each quark & lepton)
1897-2002
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Patterns (symmetry) predict missing particles
Missing particlethe 6th quark
Moremissing particles:GravitonHiggsSUSY
Top quarkfound in 1995
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Unification of the Forces
Electricity
MagnetismElectromagnetism 1864
Electromagnetism
WeakElectroweak 1979
-1982
Electromagnetism
Weak
Strong
Grand unified force?
Requires Higgs
Requires photon
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Grand Unified Force Reqiures SUSY
Supersymmetry=SUSYSUSY normal+ SUSYDecay chain ends in lightest SUSY particlewhich is stable
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Dis
tanc
e
Velocity
AB
Question for the class
Graph shows distance compared to velocity for dots on a rubberband. The white solid line is from two slides ago. What do lines A and B correspond to?
B faster stretchingA slower stretching
B slower stretchingA faster stretching
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Dis
tanc
e
Velocity
Fast
er s
tretc
hingSlo
wer
stre
tchi
ng
Dis
tanc
e
Amount of Stretch
Deceleratingexpansion
Acceleratingexpansion
Longago
Now
Con
stan
tex
pans
ion
What would a change in the expansion rate look like?
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0.10.01 1
1
0.1
0.01
0.001
0.0001
0.00001
Rel
ativ
e In
tens
ity o
f Li
ght
Rel
ativ
e D
ista
nce
Fa
r
Amount of stretchRedshift (z)
Ne
ar
Lo
wH
igh
Acceleratingexpansion
Deceleratingexpansion
Expansion of the Universe is accelerating
Discovery of the year1998
Confirmation & refinements 1999-2004.Major new satellite JDEM planned
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Quantum Uncertainity & “empty” space
Nothing is something!
TIM
E
SPACE
Disappearance
Appearance
Particle
Antiparticle
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INNER SPACE- THE QUANTUM
PARTICLE ACCELERATOR =TIME MACHINE= TELESCOPE
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Particle Physics
Primordial Soup0.000 000 000 004 seconds AB3,000,000,000,000,000°
CONDENSED in 50 Earth masses in matter one 50 Earth masses in antimatter can + extra mountain of matterHOT per 10 billion years of total serving energy output of the sunINGREDIENTSIn every spoonful every type of elementary particle
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Particle Physics
Primordial SoupKNOWN INGREDIENTS:56% QUARKS 16% GLUONS16% ELECTRON-LIKE PARTICLES9% W’s AND Z’s 5% NEUTRINOS2% PHOTONSPROBABLE INGREDIENTS:2% GRAVITONS 1% HIGGS
SECRET INGREDIENTS: DARK MATTER, DARK ENERGY, EXTRA DIMENSIONS
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How do we see the soup particles?The Eyes of a Insect:
1 billion collisions/second1,000 particles every 25 nanoseconds
Need highly granular detectors thattake pictures quickly, and canmanipulate the resulting data on board and store it before shipping to a farm of CPUs
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The Eyes of a Piece of Silicon:
The length of each side of the square is about the thickness of a piece of paper. Each eye is called a pixel
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The largest Silicon camera ever built at a
University was built at Purdue in 1999.
We are building a more advanced version of this detector for the LHC
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CMS at LHC
21 m
16m36 Nations159 Institutions1940 scientists(including7 Purdue Professors)
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Summary
The LHC is under construction and will take data in 2008
Many other particle physics and astronomy scientific instruments on Earth, deep below ground and in outer space are coming online soon
Particle physicists & astrophysicists are poised to taste the primordial soup , to answer some of the great questions of the 21st CenturyWhat is dark matter? What is dark energy? Is there only one force?Our notion of space and time may be radically altered.We may understand how the universe was born and how it will end
Reading assignment: Scientific American September 2004 issueMany research opportunities for undergraduates: Learn more about our exciting research programs at: http://www.physics.purdue.edu
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Acknowledgements
This talk has drawn heavily on images obtained from CERN, NASA and Scientific American, and excellent talks given by Rocky Kolb, Lawrence Krauss, Gerard `t Hooft, Michael Turner and Jim Virdee.
Original artwork was preparedby Steven Lichti (Purdue).Daniela Bortoletto and Francesca Shipsey are thanked for their love and support.