what’s hot in high energy particle physics

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What’s Hot in High Energy Particle Physics the fundamental constituents & interactions of ma the universe made of and by what rules do they pla

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What’s Hot in High Energy Particle Physics. Study of the fundamental constituents & interactions of matter. What is the universe made of and by what rules do they play?. Masses on the subatomic scale. electron proton iron nucleus. 9.1093 10 -31 kg. 0.511 MeV. 938.28 MeV. - PowerPoint PPT Presentation

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Page 1: What’s  Hot  in High Energy Particle Physics

What’s Hot inHigh Energy Particle Physics

Study of the fundamental constituents & interactions of matter.

What is the universe made of and by what rules do they play?

Page 2: What’s  Hot  in High Energy Particle Physics

Masses on the subatomic scale

electron

proton

iron nucleus

9.109310-31 kg 0.511 MeV

1.672110-27 kg 938.28 MeV

9.299010-26 kg 52153.77 MeV

Page 3: What’s  Hot  in High Energy Particle Physics

Henri Becquerel (1852-1908) 1903 Nobel Prize

discovery of natural radioactivity

Wrapped photographic plate showed distinct silhouettes of uranium salt samples stored atop it.

1896 While studying fluorescent & phosphorescent materials, Becquerel finds potassium-uranyl sulfate spontaneously emits radiation that can penetrate

thick opaque black paper aluminum plates copper plates

Page 4: What’s  Hot  in High Energy Particle Physics

fast charged particles leave a trails of Ag grains 1/1000 mm (1/25000 in) diameter

1930s plates coated with thick photographic emulsions (gelatins carrying silver bromide crystals) carried up mountains or in balloons clearly trace cosmic ray tracks through their depth when developed

Page 5: What’s  Hot  in High Energy Particle Physics

C.F.Powell, P.H. Fowler, D.H.PerkinsNature 159, 694 (1947)

Nature 163, 82 (1949)

ee

Page 6: What’s  Hot  in High Energy Particle Physics
Page 7: What’s  Hot  in High Energy Particle Physics

e

HTTP://PDG.LBL.GOV Particle Data Group Created: 10/24/2002

Page 8: What’s  Hot  in High Energy Particle Physics

HTTP://PDG.LBL.GOV Particle Data Group Created: 06/18/2002

0

150 mesons!!

Page 9: What’s  Hot  in High Energy Particle Physics

p

n

HTTP://PDG.LBL.GOV Particle Data Group Created: 06/18/2002

Page 10: What’s  Hot  in High Energy Particle Physics

121 baryons!!

Page 11: What’s  Hot  in High Energy Particle Physics

c

sd u

p n + + 0

Quark Charge up +2/3e down 1/3e charm +2/3estrange 1/3e

Page 12: What’s  Hot  in High Energy Particle Physics

Baryon StatesState Quark content Mass Spin p uud 938.272 MeV 1/2 n udd 939.565 MeV 1/2 uds 1115.683 MeV 1/2 + uus 1189.37 MeV 1/2 0 uds 1192.632 MeV 1/2 - dds 1197.449 MeV 1/2 0 uss 1314.9 MeV 1/2 dss 1321.32 MeV 1/2

uuu 1230. MeV 3/2 uud 1231 MeV 3/2 0 udd 1233 MeV 3/2 - ddd 1234 MeV 3/2 *+ uus 1382.8 MeV 3/2 *0 uds 1383.7 MeV 3/2 * dds 1387.2 MeV 3/2 *0 uss 1531.80 MeV 3/2 * dss 1535.0 MeV 3/2 sss 1672.45 MeV 3/2

can all be explained as combinations of

3 fundamental quarks

Meson Statescan all be explained

2 quarks combinations

+ ud 139.57 MeV + ud 139.57 MeV 0 uu 134.98 MeV 0 dd 546.30 MeV

Page 13: What’s  Hot  in High Energy Particle Physics

To be charged: means the particle is capable of emitting and absorbing photons

e

e

How do 2 (mutually repulsive) electrons sense one another’s presence?

Page 14: What’s  Hot  in High Energy Particle Physics

e e

W

e

e

e

e

electrostatic repulsion

nuclear binding

u

u

d

d

g

“weak” decays

Page 15: What’s  Hot  in High Energy Particle Physics

The Detector in various stages of assembly

Page 16: What’s  Hot  in High Energy Particle Physics

38 foreign institutions3 national labs:BNL, LBL,FNAL

36 U.S. university HEP groups

Page 17: What’s  Hot  in High Energy Particle Physics
Page 18: What’s  Hot  in High Energy Particle Physics
Page 19: What’s  Hot  in High Energy Particle Physics

CERN, Geneva, Switzerland

The CMS Detector

Page 20: What’s  Hot  in High Energy Particle Physics

The Cosmic Questions

Why are there so many particles?

Are there yet any new laws to discover?

What is this Dark Matter?

What are massive neutrinos telling us about the world?

Are there dimensions beyond 4-dimensional space-time?

Do the fundamental forces unify?

How did the universe come to be?

Where did all the antimatter go?

What is the origin of particle masses?

Page 21: What’s  Hot  in High Energy Particle Physics

Astronomers tell us that most of the matter in the universe is invisible

We will look for it

with the LHC

Dark Matter in the Universe

Astronomers saythat most of thematter in theUniverse isinvisible Dark Matter

Supersymmetric particles ?

Something we are actively looking for!

Page 22: What’s  Hot  in High Energy Particle Physics

e

p

e

p

mproton = 1836 melectron

Page 23: What’s  Hot  in High Energy Particle Physics

~

~

~~

~Particle Name Symbol Spartner Name Symbol gluon g gluino g charged Higgs H+ chargino W1,2

charged weak boson light Higgs h neutralino Z1,2,3,4 heavy Higgs Hpseudoscalar Higgs Aneutral weak boson Z photon quark q squark qR,L

lepton l slepton lR,L

SUPERSYMMETRY

Page 24: What’s  Hot  in High Energy Particle Physics

Charginos and NeutralinosCharginos and Neutralinos

Production of 1 0

2 will lead to trilepton final states with ET

perhaps the cleanest signature of supersymmetry.

pp q, g 10

2

+ ET

~ ~ ~ ~

1

02

~

~

01

~

01

~

W*Z*

W*

q

q

q

q

1

02

~

~

1

~ 02

~

~0

1~

*

~

01

~

~ ~

q*~

Page 25: What’s  Hot  in High Energy Particle Physics

q

g

0

1q

0

1

q

q

Squarks and GluinosSquarks and Gluinos can decay directly into the LSP

(01)

or cascade down to the LSP

q

g

q

So that the dominant signature for ppqq, qg, gg + X is jets+ET

q

q

q

q

0

2

q

0

1

q

g q

qq

q

1

q

q

0

1

q

Page 26: What’s  Hot  in High Energy Particle Physics
Page 27: What’s  Hot  in High Energy Particle Physics

Supersymmetry Searches at LHC

`Typical’ supersymmetric

Event at the LHC

LHC reach in

supersymmetric

parameter space

Can cover mostpossibilities forastrophysicaldark matter

Page 28: What’s  Hot  in High Energy Particle Physics

String Theory• Candidate theory of quantum

gravity• Point-like particles →

extended objects• lengths of “string”• Requires extra dimensions

Page 29: What’s  Hot  in High Energy Particle Physics

R

Flat dimension

Page 30: What’s  Hot  in High Energy Particle Physics

221

r

mmGF

gravity 2

21

r

qqkF

ticelectrosta

Picking a fundamental particle for common reference

kgmproton

271067265.1 Cqproton

19106022.1

ticelectrostagravityFF

00000000000000000000000000000001000000000

1

rR

mm

MrR

mm

MrV n

Planck

nn

Dgravity

212

212

11)( for r >> R

If photons traverse our 3-dim space but gravitons spread out over 3+n…

Page 31: What’s  Hot  in High Energy Particle Physics

So far NO distribution of measured particle characteristics or behavior show ANY effect attributable to extra dimensions.

Page 32: What’s  Hot  in High Energy Particle Physics

Hints on the Higgs Mass

Best-fit value: mH = 91+45–32 GeV95% confidence-level upper limit: mH < 219 GeV

Page 33: What’s  Hot  in High Energy Particle Physics

Best-fit value: mH = 91+45–32 GeV

95% confidence-level upper limit: mH < 219 GeV

current limit fixed by direct searchesmH > 114 GeV

I’s expected reach (before CERN’s LHC turns on)

~120 GeV