42
troduction to Particle Physi (for non physics students) 4. UNIFIED UNIVERSE (no strings attached)

Introduction to Particle Physics (for non physics students) 4. UNIFIED UNIVERSE

  • Upload
    rossa

  • View
    38

  • Download
    0

Embed Size (px)

DESCRIPTION

Introduction to Particle Physics (for non physics students) 4. UNIFIED UNIVERSE (no strings attached). Feynman rules: If energy E flows through the 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. - PowerPoint PPT Presentation

Citation preview

Page 1: Introduction to Particle Physics            (for non physics students) 4. UNIFIED UNIVERSE

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
Page 3: Introduction to Particle Physics            (for non physics students) 4. UNIFIED UNIVERSE

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

WEAK

STRONG

Page 5: Introduction to Particle Physics            (for non physics students) 4. UNIFIED UNIVERSE

WEAK

STRONG why sun hasshone for 5 Byr…Intelligent lifedeveloped

Page 6: Introduction to Particle Physics            (for non physics students) 4. UNIFIED UNIVERSE

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
Page 8: Introduction to Particle Physics            (for non physics students) 4. UNIFIED UNIVERSE
Page 9: Introduction to Particle Physics            (for non physics students) 4. UNIFIED UNIVERSE
Page 10: Introduction to Particle Physics            (for non physics students) 4. UNIFIED UNIVERSE
Page 11: Introduction to Particle Physics            (for non physics students) 4. UNIFIED UNIVERSE
Page 12: Introduction to Particle Physics            (for non physics students) 4. UNIFIED UNIVERSE
Page 13: Introduction to Particle Physics            (for non physics students) 4. UNIFIED UNIVERSE
Page 14: Introduction to Particle Physics            (for non physics students) 4. UNIFIED UNIVERSE

3K microwave bgnd now seen to have structure

COBE 2000

WMAP 2003

Page 15: Introduction to Particle Physics            (for non physics students) 4. UNIFIED UNIVERSE

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

Page 16: Introduction to Particle Physics            (for non physics students) 4. UNIFIED UNIVERSE

One further symmetry??

Page 17: Introduction to Particle Physics            (for non physics students) 4. UNIFIED UNIVERSE

Whole new families to be found

Page 18: Introduction to Particle Physics            (for non physics students) 4. UNIFIED UNIVERSE
Page 19: Introduction to Particle Physics            (for non physics students) 4. UNIFIED UNIVERSE

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

TemperatureEnergy andTime

The Universe

in

Page 20: Introduction to Particle Physics            (for non physics students) 4. UNIFIED UNIVERSE

…and the nature of matter

Page 21: Introduction to Particle Physics            (for non physics students) 4. UNIFIED UNIVERSE

…and patterns (that change)

Page 22: Introduction to Particle Physics            (for non physics students) 4. UNIFIED UNIVERSE

symmetry

pattern

Temperatureand symmetry in the universe

Page 23: Introduction to Particle Physics            (for non physics students) 4. UNIFIED UNIVERSE

The Idea

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

Page 24: Introduction to Particle Physics            (for non physics students) 4. UNIFIED UNIVERSE

Symmetrywhen warm(high energy)

patterns and structureswhen cold(low energy)

Page 25: Introduction to Particle Physics            (for non physics students) 4. UNIFIED UNIVERSE

GrandUnifiedForce

ElectromagneticWeakStrong

ElectroWeakStrong (QCD)

FORCES 1955-2005

COLD

WARM

HOT

Page 26: Introduction to Particle Physics            (for non physics students) 4. UNIFIED UNIVERSE

Standard Model of Quarks Leptons and

forces

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

Page 27: Introduction to Particle Physics            (for non physics students) 4. UNIFIED UNIVERSE

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 28: Introduction to Particle Physics            (for non physics students) 4. UNIFIED UNIVERSE

symmetry

pattern

symmetry

pattern

Page 29: Introduction to Particle Physics            (for non physics students) 4. UNIFIED UNIVERSE

5. symmetries can disappear or change

Page 30: Introduction to Particle Physics            (for non physics students) 4. UNIFIED UNIVERSE

We like symmetry and when its absent wewant to know why

?

Page 31: Introduction to Particle Physics            (for non physics students) 4. UNIFIED UNIVERSE

Buridan’s Ass

Page 32: Introduction to Particle Physics            (for non physics students) 4. UNIFIED UNIVERSE

The problem ofthe symmetricdinner party

Page 33: Introduction to Particle Physics            (for non physics students) 4. UNIFIED UNIVERSE

symmetry

Broken symmetry

Page 34: Introduction to Particle Physics            (for non physics students) 4. UNIFIED UNIVERSE

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 35: Introduction to Particle Physics            (for non physics students) 4. UNIFIED UNIVERSE
Page 36: Introduction to Particle Physics            (for non physics students) 4. UNIFIED UNIVERSE

Symmetrywhen warm(high energy)

patterns and structureswhen cold(low energy)

CO2

H2O

Page 37: Introduction to Particle Physics            (for non physics students) 4. UNIFIED UNIVERSE

… “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 38: Introduction to Particle Physics            (for non physics students) 4. UNIFIED UNIVERSE

Nextyear

Page 39: Introduction to Particle Physics            (for non physics students) 4. UNIFIED UNIVERSE

The Particle OdysseyThe Particle Odyssey

A Journey to the Heart of matter

Frank Close, Michael Marten, Christine Sutton

Page 40: Introduction to Particle Physics            (for non physics students) 4. UNIFIED UNIVERSE

More in Vsi

And particle odyssey

NEW

A Very Short Introduction Coming out in December

Page 41: Introduction to Particle Physics            (for non physics students) 4. UNIFIED UNIVERSE
Page 42: Introduction to Particle Physics            (for non physics students) 4. UNIFIED UNIVERSE