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Professor Peter Kalmus

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Particles and the Universe. Professor Peter Kalmus. Physics Department. 170,000 light years. 10,000,000,000,000,000,000,000,000,000,000,000,000,000,000,000,000,000,000,000. Supernova 1987A. Neutrino numbers Emitted ~ 10 58 Hit Earth ~ 10 29 Hit tank ~ 10 17 Interact ~ 10. - PowerPoint PPT Presentation
34
s School Peter Kalmus March 2006 Professor Peter Kalmus articles and the Universe Physics Department
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Page 1: Professor  Peter Kalmus

Charters School Peter Kalmus March 2006

Professor Peter Kalmus

Particles and the Universe

Physics Department

Page 2: Professor  Peter Kalmus

Charters School Peter Kalmus March 2006

Supernova 1987A Neutrino numbers

Emitted ~ 1058

Hit Earth ~ 1029

Hit tank ~ 1017

Interact ~ 10SN

1987A Earth

170,000light years

Energy release ~ 1046 J

SN~ 1046 J

10,000,000,000,000,000,000,000,000,000,000,000,000,000,000,000,000,000,000,000

Page 3: Professor  Peter Kalmus

8 arc min

Large Magellanic Cloud

Sanduleak - 69o 202

Page 4: Professor  Peter Kalmus
Page 5: Professor  Peter Kalmus

Charters School Peter Kalmus March 2006

Page 6: Professor  Peter Kalmus

1016 1 TeV

1013 1 GeV

1010 1 MeV

107 1 keV

104 1 eV

10 1 meV

T/K Energy

ParticleEra

NuclearEra

AtomicEra

PrimordialSoup

Sun forms

Todayps ns s ms s

1 day

1 year

Time

Era ofAstronomy

TevatronLEP

History of theUniverse

10-12 10-6 100 1013 1018Time sinceBig Bang / s

LHC

Hot as Hell445oC = Boiling point of Brimstone

Page 7: Professor  Peter Kalmus

Charters School Peter Kalmus March 2006

Primordial Soup CERN style 100 GeV / particle

Ingredients56% quarks16% gluons 9% charged leptons 9% W & Z particles 5% neutrinos 2% photons 2% gravitons 1% Higgs bosonsRecipe by Rocky Kolb

Hot 3 x 1015KCondensed

Missingingredients

Dark matterDark energy

Page 8: Professor  Peter Kalmus

Charters School Peter Kalmus March 2006

Sun

Inverse square law

a

Rotation in spiral galaxiesStars move too fast(measured by Doppler shift)

96 % of universe is undetected~4% Baryonic; ~24% “Dark Matter”~72% “Dark Energy”

Kepler, Newton

T2 = 4 2 a3 /G Mo

v2 = G Mo/a (circular orbit)

Mo

v

Page 9: Professor  Peter Kalmus

Charters School Peter Kalmus March 2006

Expect from detected stars etc.

Measured velocities from Doppler shifts

Galaxy rotation curve

Hence there is more gravitationally attractive material than has been detected Dark matter

Distance from centre

velo

city

Page 10: Professor  Peter Kalmus

Dark energy

Slowest v

2 v

3 v

Fastest 4 v

After some time the fastest particles will be furthest away

Explosion in empty space (forget about gravity)

Page 11: Professor  Peter Kalmus

Charters School Peter Kalmus March 2006

Recession velocity (Doppler Redshift z)

Dis

tanc

e (

Mag

nitu

de)

Hubble Diagram

Plot distance againstrecession velocity for many galaxies Get straight line Big Bang

nearest galaxy

furthest galaxyhighest recession velocity

The Universe is like this !

Page 12: Professor  Peter Kalmus

Charters School Peter Kalmus March 2006

Recession velocity (Doppler Redshift z)

Dis

tanc

e (

Mag

nitu

de)

Hubble Diagram But cannot ignore gravity which slows down the flow

Expect this line to curve downwards for very distant galaxies. Expansion would decelerate

Page 13: Professor  Peter Kalmus

Charters School Peter Kalmus March 2006

Recession velocity (Doppler Redshift z)

Dis

tanc

e (

Mag

nitu

de)

Hubble Diagram (simplified)

Recent results show that expansion is accelerating !

Cosmic repulsion !“Dark energy”

Page 14: Professor  Peter Kalmus

Charters School Peter Kalmus March 2006

Structure of the Atom

Atom

~ 10-10m

Nucleus

Early 20th Century electron, nucleus

electric forceelectromagnetism

1930s

bunch ofgrapes

Proton +Neutron

strongforcetown

~ 10-15m

Page 15: Professor  Peter Kalmus

Charters School Peter Kalmus March 2006

Neutrinos

Antiparticles

1950s, 1960s

> 200 new “elementary” (?) particles

Feel weak force“predicted” later discovered 100,000,000,000,000 per second pass through each person from the Sun

Equal and opposite properties “predicted” later discoveredAnnihilate with normal particlesNow used in PET scans

Many new particles created in high energy collisions

Convert energy to mass. Einstein E = mc2

Page 16: Professor  Peter Kalmus

Charters School Peter Kalmus March 2006

Today’s building blocks

Leptons(do not feel strong force)

electron e- -1e-neutrino e 0

Quarks(feel strong force)

up u +2/3down d -1/3

proton = u u d+2/3 +2/3 -1/3 = +1

neutron = u d d+2/3 -1/3 -1/3 = 0

4 particles very simple

multiply by 3 (generations)multiply by 2 (antiparticles)

First generation

Page 17: Professor  Peter Kalmus

Charters School Peter Kalmus March 2006

Today’s building blocks

Leptons(do not feel strong force)

electron e- -1e-neutrino e 0

Quarks(feel strong force)

up u +2/3down d -1/3

muon -1

-neutrino 0

tau -1

-neutrino 0

charm c +2/3strange s -1/3

top t +2/3bottom b -1/3

Also antileptonsantiquarks

6 leptons6 antileptons

6 quarks6 antiquarks

baryons q q q

antibary. q q q

mesons q q

Recent news:pentaquarks

Page 18: Professor  Peter Kalmus

Charters School Peter Kalmus March 2006

Earth, Moon, X Solar system XAntistars in our Galaxy ?Other (anti-) galaxies ?

Telescopes XCosmic rays ?AMS (Space station)

AntimatterAnti-hydrogen : made in labBulk antimatter ? Where ?Difficult to detect

Annihilation ofAntigalaxy ?

Signal ?

e+ + e - + 0.511 MeV -ray “line” Alfven hypothesis

Radiation pressure

Page 19: Professor  Peter Kalmus

Charters School Peter Kalmus March 2006

Constituents How can we find internal structure?

Insect 1 lens2 lenses3 lenses

: Magnifying glass: Microscope : No improvement

Resolution limited by wavelength of light =

Visible light wavelength ~ 5 x 10-7 mThis is 5,000 times size of atom500 million times size of nucleus

To “probe” elementary particles need wavelengths lower by factor more than a billion !

Page 20: Professor  Peter Kalmus

Charters School Peter Kalmus March 2006

Quantum physics to the rescue

hp

Planckconstant

momentumwavelength

Particles have wave properties

“See” small objects small wavelength high momentum high energy large accelerator

Non-relativistic p = m vmass x velocity

Relativistic p = m v = 1/ (1 - v2/c2)1/2

To observe the smallest objects we need the largest machines !

Page 21: Professor  Peter Kalmus

Charters School Peter Kalmus March 2006

AcceleratorExtractbeam

Injector

Vacuum ring

RF cavitieselectric kick

~Bendingelectro-magnet

Focusingelectro-magnet

Page 22: Professor  Peter Kalmus
Page 23: Professor  Peter Kalmus

Charters School Peter Kalmus March 2006

Forces

Gravity

falling objectsplanet orbitsstarsgalaxies

inversesquare law

graviton

inversesquare law

photon

shortrange

W±, Z0

Electro-magnetic

atomsmoleculesopticselectronicstelecom.

Weak

betadecay

solarfusion

Strong

nuclei

particles

shortrange

gluon

Page 24: Professor  Peter Kalmus

Charters School Peter Kalmus March 2006

Forces by exchange

Analogy onlyUseful mental picture ?

Page 25: Professor  Peter Kalmus

Charters School Peter Kalmus March 2006

Attraction

Page 26: Professor  Peter Kalmus

Charters School Peter Kalmus March 2006

Unification of the fundamentalforces of nature

Electricity Magnetism Apples Planets

Electro-magnetic

Gravity

Faraday, Maxwell Newton

Page 27: Professor  Peter Kalmus

Charters School Peter Kalmus March 2006

Unification of the fundamentalforces of nature

Electricity Magnetism Apples Planets

Electro-magnetic

Weak Strong Gravity

Faraday, Maxwell Newton

Electroweakunified force

Salam, Weinberg, Glashow

, W +, W -, Z 0 0 80 80 90 GeV

Do the W and Z particles really exist ?

Page 28: Professor  Peter Kalmus

Charters School Peter Kalmus March 2006

Collider Injectanti-protons

Injectprotons

Collide 2 beamsInside vacuum

RF cavitieselectric kick

~Bendingelectro-magnet

Focusingelectro-magnet

Carlo RubbiaAntiprotons

Simon van der MeerStochastic cooling

Page 29: Professor  Peter Kalmus

Charters School Peter Kalmus March 2006

UA1 Experiment Muon

Neutrino

Electromagcalorimeter

Hadron calorim.and magnet

Proton Antiproton

Hadron

Electron

Wire

chamber

Vacuumpipe

Muon chambers

Page 30: Professor  Peter Kalmus

Charters School Peter Kalmus March 2006

Page 31: Professor  Peter Kalmus

Charters School Peter Kalmus March 2006

Carriers of Weak ForceFound at CERNThe W boson the hypo

carries the weak force whichcontrols the production ofenergy in the Sun and some

The Discovery of the W Boson

The observation of the W intermediate vector boson, the particle that

carries the weak nuclear force, is the most outstanding achievement

of the CERN laboratory in Geneva and one of the most important

advances in physics of this century. It is the successful conclusion of

The Role of UK ScientistsTwenty-five British scientists played an important part inthe remarkable discovery of the W boson. They were ledby Professor J D Dowell of Birmingham University,Professor P I P Kalmus of Queen Mary College and Dr AAstbury of Rutherford Appleton Laboratory. The W boson

Page 32: Professor  Peter Kalmus

Charters School Peter Kalmus March 2006

FromTHE PRIME MINISTER10 Downing StreetToProfessor P. I. P. Kalmus

It is very encouraging that so many British scientists were in the team that discovered the “W boson”, and I would like to congratulate you and your colleagues from Queen Mary College on your success. I am sure that British physicists will be among the first to unify all the four basic forces

Page 33: Professor  Peter Kalmus

Charters School Peter Kalmus March 2006

W and Z particles discoveredUA1 Collaboration at CERNIncluded following members of Queen MaryPeter KalmusAlan Honma

Eric EisenhandlerRichard Keeler

Reg GibsonGiordi Salvi

Graham ThompsonThemis Bowcock

Results confirmed by another CERN collaboration,and few years later at Fermilab USA

Electroweak unification confirmedNature’s fundamental forcesreduced from 4 to 3Nobel Prizes

Page 34: Professor  Peter Kalmus

Charters School Peter Kalmus March 2006

[email protected]://www.ph.qmul.ac.uk

THE END


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