introduction to particle physics (for non physics students) 4. unified universe (no strings...

54
troduction to Particle Physi (for non physics students) 4. UNIFIED UNIVERSE (no strings attached)

Upload: ashlee-harmon

Post on 14-Dec-2015

223 views

Category:

Documents


1 download

TRANSCRIPT

Page 1: Introduction to Particle Physics (for non physics students) 4. UNIFIED UNIVERSE (no strings attached)

Introduction to Particle Physics (for non physics students)

4. UNIFIED UNIVERSE (no strings attached)

Page 2: Introduction to Particle Physics (for non physics students) 4. UNIFIED UNIVERSE (no strings attached)
Page 3: Introduction to Particle Physics (for non physics students) 4. UNIFIED UNIVERSE (no strings attached)

Feynman rules:

If energy E flows throughthe transmitted “virtual”particle (photon; Z)it costs 1/(E^2+M^2)

If E >> M the cost is 1/E^2….like the case of the photon

Only appears weak at low energy. Unified at high energy

Page 4: Introduction to Particle Physics (for non physics students) 4. UNIFIED UNIVERSE (no strings attached)

WEAK

STRONG

Page 5: Introduction to Particle Physics (for non physics students) 4. UNIFIED UNIVERSE (no strings attached)

WEAK

STRONG why sun hasshone for 5 Byr…Intelligent lifedeveloped

Page 6: Introduction to Particle Physics (for non physics students) 4. UNIFIED UNIVERSE (no strings attached)

The weak force is feeble in the Sun…

..because 10,000,000K ~ 1 keV << 80 GeV

The weak force is feeble in the Sun

…this is why the sun has stayed active long enough for us to have evolvedand be having this conversation.

We exist because m(W) is not zero

Mass matters

Page 7: Introduction to Particle Physics (for non physics students) 4. UNIFIED UNIVERSE (no strings attached)
Page 8: Introduction to Particle Physics (for non physics students) 4. UNIFIED UNIVERSE (no strings attached)

Mc^2 >0Gravity PE <0Total E =0 (?!)

Page 9: Introduction to Particle Physics (for non physics students) 4. UNIFIED UNIVERSE (no strings attached)

Mc^2 >0Gravity PE <0Total E =0 (?!)

Page 10: Introduction to Particle Physics (for non physics students) 4. UNIFIED UNIVERSE (no strings attached)

Heisenberg:

E ->0t ->infinity

“Universe erupted as quantum fluctuationout of nothing”

(what/where/how encodedHeisenberg in “nothing”?

Mc^2 >0Gravity PE <0Total E =0 (?!)

Page 11: Introduction to Particle Physics (for non physics students) 4. UNIFIED UNIVERSE (no strings attached)

Heisenberg:

E ->0t ->infinity

“Universe erupted as quantum fluctuationout of nothing”

(what/where/how encodedHeisenberg in “nothing”?

Mc^2 >0Gravity PE <0Total E =0 (?!)

Page 12: Introduction to Particle Physics (for non physics students) 4. UNIFIED UNIVERSE (no strings attached)
Page 13: Introduction to Particle Physics (for non physics students) 4. UNIFIED UNIVERSE (no strings attached)

Quarks “freeze” into protons/neutrons

Page 14: Introduction to Particle Physics (for non physics students) 4. UNIFIED UNIVERSE (no strings attached)
Page 15: Introduction to Particle Physics (for non physics students) 4. UNIFIED UNIVERSE (no strings attached)
Page 16: Introduction to Particle Physics (for non physics students) 4. UNIFIED UNIVERSE (no strings attached)
Page 17: Introduction to Particle Physics (for non physics students) 4. UNIFIED UNIVERSE (no strings attached)
Page 18: Introduction to Particle Physics (for non physics students) 4. UNIFIED UNIVERSE (no strings attached)
Page 19: Introduction to Particle Physics (for non physics students) 4. UNIFIED UNIVERSE (no strings attached)

Nuclear Physics

Page 20: Introduction to Particle Physics (for non physics students) 4. UNIFIED UNIVERSE (no strings attached)
Page 21: Introduction to Particle Physics (for non physics students) 4. UNIFIED UNIVERSE (no strings attached)

symmetry

pattern

symmetry

pattern

Page 22: Introduction to Particle Physics (for non physics students) 4. UNIFIED UNIVERSE (no strings attached)

symmetry

pattern

symmetry

pattern

Page 23: Introduction to Particle Physics (for non physics students) 4. UNIFIED UNIVERSE (no strings attached)

symmetry

pattern

symmetry

pattern

Atoms

Page 24: Introduction to Particle Physics (for non physics students) 4. UNIFIED UNIVERSE (no strings attached)
Page 25: Introduction to Particle Physics (for non physics students) 4. UNIFIED UNIVERSE (no strings attached)

3K microwave bgnd now seen to have structure

COBE 2000

WMAP 2003

Page 26: Introduction to Particle Physics (for non physics students) 4. UNIFIED UNIVERSE (no strings attached)

5byr ago accelerated expansion= Dark Energy. What? Why?......

Page 27: Introduction to Particle Physics (for non physics students) 4. UNIFIED UNIVERSE (no strings attached)

One further symmetry??

Page 28: Introduction to Particle Physics (for non physics students) 4. UNIFIED UNIVERSE (no strings attached)

Whole new families to be found

Page 29: Introduction to Particle Physics (for non physics students) 4. UNIFIED UNIVERSE (no strings attached)
Page 30: Introduction to Particle Physics (for non physics students) 4. UNIFIED UNIVERSE (no strings attached)

Finale: A glimpse of the futurerecall from lecture 1…..

TemperatureEnergy andTime

The Universe

in

Page 31: Introduction to Particle Physics (for non physics students) 4. UNIFIED UNIVERSE (no strings attached)

…and the nature of matter

Page 32: Introduction to Particle Physics (for non physics students) 4. UNIFIED UNIVERSE (no strings attached)

…and patterns (that change)

Page 33: Introduction to Particle Physics (for non physics students) 4. UNIFIED UNIVERSE (no strings attached)

symmetry

pattern

Temperatureand symmetry in the universe

Page 34: Introduction to Particle Physics (for non physics students) 4. UNIFIED UNIVERSE (no strings attached)

The Idea

(I will tell you when to be cautious about inhaling)

Page 35: Introduction to Particle Physics (for non physics students) 4. UNIFIED UNIVERSE (no strings attached)

Symmetrywhen warm(high energy)

patterns and structureswhen cold(low energy)

Page 36: Introduction to Particle Physics (for non physics students) 4. UNIFIED UNIVERSE (no strings attached)

GrandUnifiedForce

ElectromagneticWeakStrong

ElectroWeakStrong (QCD)

FORCES 1955-2005

COLD

WARM

HOT

Page 37: Introduction to Particle Physics (for non physics students) 4. UNIFIED UNIVERSE (no strings attached)

Standard Model of Quarks Leptons and

forces

= pattern based on mass “cold” =“low” energy= below 1 TeV

Page 38: Introduction to Particle Physics (for non physics students) 4. UNIFIED UNIVERSE (no strings attached)

superSymmetrywhen “warm”(= high energy > 1TeV)

Higgs BosonSupersymmetryNature of Reality

Standard Model of Quarks Leptons and

forces

= pattern based on mass “cold” =“low” energy= below 1 TeV

Page 39: Introduction to Particle Physics (for non physics students) 4. UNIFIED UNIVERSE (no strings attached)

symmetry

pattern

symmetry

pattern

Page 40: Introduction to Particle Physics (for non physics students) 4. UNIFIED UNIVERSE (no strings attached)

5. symmetries can disappear or change

Page 41: Introduction to Particle Physics (for non physics students) 4. UNIFIED UNIVERSE (no strings attached)

We like symmetry and when its absent wewant to know why

?

Page 42: Introduction to Particle Physics (for non physics students) 4. UNIFIED UNIVERSE (no strings attached)

Buridan’s Ass

Page 43: Introduction to Particle Physics (for non physics students) 4. UNIFIED UNIVERSE (no strings attached)

The problem ofthe symmetricdinner party

Page 44: Introduction to Particle Physics (for non physics students) 4. UNIFIED UNIVERSE (no strings attached)

symmetry

Broken symmetry

Page 45: Introduction to Particle Physics (for non physics students) 4. UNIFIED UNIVERSE (no strings attached)

Why is this a peak and not a trough?

Broken symmetry

Answer: random chanceBut given it’s a peak hereit dictates where the other peaks are

Page 46: Introduction to Particle Physics (for non physics students) 4. UNIFIED UNIVERSE (no strings attached)
Page 47: Introduction to Particle Physics (for non physics students) 4. UNIFIED UNIVERSE (no strings attached)

Symmetrywhen warm(high energy)

patterns and structureswhen cold(low energy)

Page 48: Introduction to Particle Physics (for non physics students) 4. UNIFIED UNIVERSE (no strings attached)

… “froze” into structures …. And patterns

Such as Atoms ……. Mendeleev’s periodic table,And particles …. Quarks, forces and the Standard Model

As the universe cooled after the hot big bang…..We think that an elegant symmetry……..

… which is a pattern based on MASS

2008: heat up to energies above 1000 GeV = “1 TeV” and discover the origin of MASS (= Higgs?)

Page 49: Introduction to Particle Physics (for non physics students) 4. UNIFIED UNIVERSE (no strings attached)

Next….

Page 50: Introduction to Particle Physics (for non physics students) 4. UNIFIED UNIVERSE (no strings attached)
Page 51: Introduction to Particle Physics (for non physics students) 4. UNIFIED UNIVERSE (no strings attached)

More in Vsi

And particle odyssey

A Very Short Introduction

Page 52: Introduction to Particle Physics (for non physics students) 4. UNIFIED UNIVERSE (no strings attached)

The Particle OdysseyThe Particle Odyssey

A Journey to the Heart of matter

Frank Close, Michael Marten, Christine Sutton

Page 53: Introduction to Particle Physics (for non physics students) 4. UNIFIED UNIVERSE (no strings attached)
Page 54: Introduction to Particle Physics (for non physics students) 4. UNIFIED UNIVERSE (no strings attached)