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Einstein, String Theory, and the Future Jonathan Feng University of California, Irvine Einstein: A Century of Relativity Skirball Cultural Center, Los Angeles 29 January 2005
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Einstein, String Theory, and the Future

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Einstein, String Theory, and the Future. Jonathan Feng University of California, Irvine Einstein: A Century of Relativity Skirball Cultural Center, Los Angeles 29 January 2005. Relativity in a Nutshell. 60 mph. 90 mph. 30 mph. Common Sense Physics. v new = v old + v train. v light. - PowerPoint PPT Presentation
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Page 1: Einstein, String Theory, and the Future

Einstein, String Theory,and the Future

Jonathan FengUniversity of California, Irvine

Einstein: A Century of RelativitySkirball Cultural Center, Los Angeles

29 January 2005

Page 2: Einstein, String Theory, and the Future

29 January 2005 Einstein: A Century of Relativity Feng 2

Relativity in a Nutshell

Page 3: Einstein, String Theory, and the Future

29 January 2005 Einstein: A Century of Relativity Feng 3

60 mph

30 mph

90 mph

vnew = vold + vtrain

Common Sense Physics

Page 4: Einstein, String Theory, and the Future

29 January 2005 Einstein: A Century of Relativity Feng 4

vlight

30 mph

vlight

vnew = voldvnew =

vold + vtrain_____________1 + voldvtrain/vlight2

Weird Physics

Page 5: Einstein, String Theory, and the Future

29 January 2005 Einstein: A Century of Relativity Feng 5

Classical Physics (1687)

Special Relativity (1905)

fast

Quantum Mechanics (1905)

small

General Relativity (1915)

heavy

Quantum Field Theory (1940’s)

String Theory ??

Page 6: Einstein, String Theory, and the Future

29 January 2005 Einstein: A Century of Relativity Feng 6

What is String Theory?

Page 7: Einstein, String Theory, and the Future

29 January 2005 Einstein: A Century of Relativity Feng 7

Standard Model of Particle Physics:The Modern Theory of Matter

Page 8: Einstein, String Theory, and the Future

29 January 2005 Einstein: A Century of Relativity Feng 8

Elementary Particles and Interactions

Page 9: Einstein, String Theory, and the Future

29 January 2005 Einstein: A Century of Relativity Feng 9

In String Theory, Particles are Strings

String Combinations Particle Interactions

Different Vibrations Different Particles

upquark

downquark electron

String theory realizes Einstein’s dream of a unified theory

Page 10: Einstein, String Theory, and the Future

29 January 2005 Einstein: A Century of Relativity Feng 10

Is String Theory Right ?

Page 11: Einstein, String Theory, and the Future

29 January 2005 Einstein: A Century of Relativity Feng 11

Is String Theory Testable?

• It depends.

• Is it falsifiable?

No – not yet, anyway.

• Does it predict anything that could have observable consequences?

Yes – string theory extra dimensions!

Page 12: Einstein, String Theory, and the Future

29 January 2005 Einstein: A Century of Relativity Feng 12

Extra Dimensions

• (x, y, z, t) + w, v,…? Science fiction?

• No – a major topic in science today:

What is our world made of?How does gravity work?

• How did this happen?

Page 13: Einstein, String Theory, and the Future

29 January 2005 Einstein: A Century of Relativity Feng 13

Isaac Newton

1687: Space and time are the static stageon which physical processes act

Page 14: Einstein, String Theory, and the Future

29 January 2005 Einstein: A Century of Relativity Feng 14

Albert Einsten

1915: Spacetime is an active player:curves, expands, shrinks, …

Page 15: Einstein, String Theory, and the Future

29 January 2005 Einstein: A Century of Relativity Feng 15

Edwin Hubble

1929: The universe is expanding

Page 16: Einstein, String Theory, and the Future

29 January 2005 Einstein: A Century of Relativity Feng 16

The Big Bang

• The universe does not expand into space – space itself expands

• Extrapolating back, space was small – the Big Bang

• Other dimensions could exist but still be small. String theory requires 6 extra dimensions.

• How can we test this possibility?

Page 17: Einstein, String Theory, and the Future

29 January 2005 Einstein: A Century of Relativity Feng 17

Dark Matter

Page 18: Einstein, String Theory, and the Future

29 January 2005 Einstein: A Century of Relativity Feng 18

Small Dimensions

• Suppose all particles propagate in extra dimensions, but these are curled up in circles.

• We will not notice them if the circles are very small.

Garden hose

Page 19: Einstein, String Theory, and the Future

29 January 2005 Einstein: A Century of Relativity Feng 19

Extra Dimensional Matter• However, particles can move in the

extra directions.

• From our viewpoint, we will see this as new particles with masses

m ~ 0, 1/R, 2/R, 3/R, 4/R, …

Each known particle has an infinite “tower” of copies.

• Extra dimensions many new particles – what good are these?

mas

s

1/R

2/R

3/R

4/R

0

Page 20: Einstein, String Theory, and the Future

29 January 2005 Einstein: A Century of Relativity Feng 20

Standard Model of Cosmology

Page 21: Einstein, String Theory, and the Future

29 January 2005 Einstein: A Century of Relativity Feng 21

Dark Matter

disk ends here

data

expected

Dark matter is required to hold galaxies together

Page 22: Einstein, String Theory, and the Future

29 January 2005 Einstein: A Century of Relativity Feng 22

• A lot of dark matter is required to hold galaxies together

• It cannot all be made of known particles

• It must be some new form of matter – maybe a sign of extra dimensions!

Page 23: Einstein, String Theory, and the Future

29 January 2005 Einstein: A Century of Relativity Feng 23

Dark Matter Detection

DDMM

CDMS in the Soudan mine ½ mile underground in Minnesota

Page 24: Einstein, String Theory, and the Future

29 January 2005 Einstein: A Century of Relativity Feng 24

Dark Matter at CollidersLarge Hadron Collider at CERN, Geneva

Page 25: Einstein, String Theory, and the Future

29 January 2005 Einstein: A Century of Relativity Feng 25

Strong Gravity and Black Holes

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29 January 2005 Einstein: A Century of Relativity Feng 26

Gravity

• Gravity is the least understood force.• Many deep problems, but one obvious one:

Gravity is extraordinarily weak. It is important in everyday life only because it is always attractive.

Page 27: Einstein, String Theory, and the Future

29 January 2005 Einstein: A Century of Relativity Feng 27

• More quantitatively, for separation distance r ,

For two protons, Fgravity ~ 10-36 FEM

• Very likely, we are missing something important. Why is gravity so weak?

• Maybe it isn’t…

Page 28: Einstein, String Theory, and the Future

29 January 2005 Einstein: A Century of Relativity Feng 28

Extra Dimensions• Suppose our world is only a slice of the whole universe

Page 29: Einstein, String Theory, and the Future

29 January 2005 Einstein: A Century of Relativity Feng 29

Strong Gravity

• In this case, gravity may be strong but appear weak only because its strength is diluted by extra dimensions.

• Fgravity ~ 1/r 2+n for small lengths, where n is

the number of extra dimensions. Can this be true?

Page 30: Einstein, String Theory, and the Future

29 January 2005 Einstein: A Century of Relativity Feng 30

1Feng, S

cience (2003)

10-60

10-40

10-20

Yes!

Page 31: Einstein, String Theory, and the Future

29 January 2005 Einstein: A Century of Relativity Feng 31

• If two particles pass close enough with enough energy, they will form a tiny black hole.

Black Holes

• For 3 spatial dimensions, gravity is too weak for this to happen. But with extra dimensions, gravity becomes strong, micro black holes can be created in particle collisions!

Page 32: Einstein, String Theory, and the Future

29 January 2005 Einstein: A Century of Relativity Feng 32

Micro Black Holes

• Where can we find them?

• What will they look like?

S. Harris

Page 33: Einstein, String Theory, and the Future

29 January 2005 Einstein: A Century of Relativity Feng 33

Black Holes

• But quantum mechanically, black holes Hawking radiate: black holes emit light!

• Classically, light and other particles do not escape: black holes are black.

Page 34: Einstein, String Theory, and the Future

29 January 2005 Einstein: A Century of Relativity Feng 34

Black Hole Evaporation• “Normal” black holes:

Mass: MBH ~ Msun

Size: kilometerTemperature: 0.01 KLifetime: ~ forever

• Micro black holes:Mass: MBH ~ 1000 Mproton

Size: 10-18 mTemperature: 1016 KLifetime: 10-27 s

They explode!

Page 35: Einstein, String Theory, and the Future

29 January 2005 Einstein: A Century of Relativity Feng 35

Black Holes at CollidersLarge Hadron Collider at CERN, Geneva

p p

Page 36: Einstein, String Theory, and the Future

29 January 2005 Einstein: A Century of Relativity Feng 36

Black Holes from Cosmic Rays

The Auger Observatory in Argentina

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COLLISION COURSE CREATES MICROSCOPIC ‘BLACK HOLES’, 16 January 2002:

“…Dozens of tiny ‘black holes’ may be forming right over our heads… A new observatory might start spotting signs of the tiny terrors, say physicists Feng and Shapere… They’re harmless and pose no threat to humans.”

Page 38: Einstein, String Theory, and the Future

29 January 2005 Einstein: A Century of Relativity Feng 38

Summary• A century later, Einstein’s remarkable papers still

are the foundation of physics, and we are still trying to realize his dream of a unified theory.

• String theory is our best attempt so far.

• Diverse experimental searches are underway. Will they be successful?

“It's tough to make predictions, especially about the future.” – Yogi Berra