cern, 31 january, 2001 egil lillestøl, cern & univ. of bergen this lecture is being recorded...
TRANSCRIPT
CERN, 31 January, CERN, 31 January, 20012001CERN, 31 January, CERN, 31 January, 20012001Egil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of Bergen
This lecture is being recorded and will be viewable on the
Web from Friday 2nd February at –
http://wlap.web.cern.ch/
CERN, 31 January, CERN, 31 January, 20012001CERN, 31 January, CERN, 31 January, 20012001Egil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of Bergen
CERN, 31 January, CERN, 31 January, 20012001CERN, 31 January, CERN, 31 January, 20012001Egil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of Bergen
10 7 m
Large structures and Orders of Magnitude
CERN, 31 January, CERN, 31 January, 20012001CERN, 31 January, CERN, 31 January, 20012001Egil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of Bergen
Sun (Eclipse)
corona
10 9 m
Sun ≈ 2x1030 kg ≈ 1057 (protons + neutrons)
nucleons
CERN, 31 January, CERN, 31 January, 20012001CERN, 31 January, CERN, 31 January, 20012001Egil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of Bergen
10 11 m
Earth Orbit
CERN, 31 January, CERN, 31 January, 20012001CERN, 31 January, CERN, 31 January, 20012001Egil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of Bergen
Milky Way
CERN, 31 January, CERN, 31 January, 20012001CERN, 31 January, CERN, 31 January, 20012001Egil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of Bergen
Spiral Galaxy
100 000 light years = 10 21 m
10 11 stars
CERN, 31 January, CERN, 31 January, 20012001CERN, 31 January, CERN, 31 January, 20012001Egil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of Bergen
Galaxy Cluster (Hercules)
10 23 m
Thousands of Galaxies
CERN, 31 January, CERN, 31 January, 20012001CERN, 31 January, CERN, 31 January, 20012001Egil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of Bergen
Hubble Deep Field
CERN, 31 January, CERN, 31 January, 20012001CERN, 31 January, CERN, 31 January, 20012001Egil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of Bergen
A Foamy Universe (bubbles 200 Mly across)
CERN, 31 January, CERN, 31 January, 20012001CERN, 31 January, CERN, 31 January, 20012001Egil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of Bergen
10 21 m 10 22 m 10 23 m
10 24 m 10 25 m 10 26 m
10 11
galaxies
10 22
stars
Summary of the largest structures
1080
nucleons
CERN, 31 January, CERN, 31 January, 20012001CERN, 31 January, CERN, 31 January, 20012001Egil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of Bergen
Dominated by Matter and Gravity **(1011 galaxies, 1022 stars)
Described by General Relativity
(or Newtonian Mechanics)
** This is far from the whole truth !!
CERN, 31 January, CERN, 31 January, 20012001CERN, 31 January, CERN, 31 January, 20012001Egil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of Bergen
Where it all came from
15 billions = 1.5 x 10 12
years ago
and since thenever expanding
CERN, 31 January, CERN, 31 January, 20012001CERN, 31 January, CERN, 31 January, 20012001Egil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of Bergen
Will the Expansion ever stop ?
Inflation predicts a flat universe.
This means that the Density of Matter and Energyequals the so called critical density
Ordinary Matter can account for only up to5% of the critical density
Dark Matter Problems
CERN, 31 January, CERN, 31 January, 20012001CERN, 31 January, CERN, 31 January, 20012001Egil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of Bergen
The First Dark Matter problem:these Galaxies should simply not exist !
Need a spherical halo of matter around the galaxy
So:is there
invisible (dark) matteraround the
galaxy ?
CERN, 31 January, CERN, 31 January, 20012001CERN, 31 January, CERN, 31 January, 20012001Egil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of Bergen
speed
200km/s
distance from center
predicted
measured
CERN, 31 January, CERN, 31 January, 20012001CERN, 31 January, CERN, 31 January, 20012001Egil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of Bergen
Gravitational lensing
Distant galaxy
Foreground cluster
Observer
109 light years
2x 109 light years
CERN, 31 January, CERN, 31 January, 20012001CERN, 31 January, CERN, 31 January, 20012001Egil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of Bergen
Reconstruction of Mass Distribution(250 times more matter than expected from light output)
CERN, 31 January, CERN, 31 January, 20012001CERN, 31 January, CERN, 31 January, 20012001Egil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of Bergen
Large amounts of invisible (dark) matter
Can NOT be ordinary matter :- does not interact with light- does not interact with ordinary matter- does concentrate around galaxies and in galaxy clusters.
What is it ???
If the answer is Super Symmetric Particles,
LHC will find it !!
CERN, 31 January, CERN, 31 January, 20012001CERN, 31 January, CERN, 31 January, 20012001Egil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of Bergen
The Second Dark Matter problem:The dark matter seems to make uponly 30-50% of the critical density
This may be linked with observations ofa possible accelerating expansion ofthe universe at large distances.
Study of type 1a Supernovae
(1a Supernovae ≈ standard light sources)
CERN, 31 January, CERN, 31 January, 20012001CERN, 31 January, CERN, 31 January, 20012001Egil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of Bergen
1a Supernova:
white dwarfaccompanying star
CERN, 31 January, CERN, 31 January, 20012001CERN, 31 January, CERN, 31 January, 20012001Egil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of Bergen
Far away* supernovae seem to be too far away !
Very difficult observations, but if true could mean:
Resurrection of Einstein’s Cosmological Constant,or “Qintessence” - one more possibility of
Exotic Matter ????Need more astronomical data
Need the LHC for a better understanding ofdark matter
* for specialists - red shifts z ≈ 1
CERN, 31 January, CERN, 31 January, 20012001CERN, 31 January, CERN, 31 January, 20012001Egil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of Bergen
The Smallest Structures
where Quantum Mechanics reigns, andwhere particles are waves, and waves are particles
Heisenberg’s Uncertainty Relation:
(x)(p) ≈ h/(2) or (t)(E) ≈ h/(2)
h is Planck’s constant - a very small number, (6.6x10-34Js)x is position, p is momentum,t is time, and E is energy.(x) means uncertainty in position, etc
CERN, 31 January, CERN, 31 January, 20012001CERN, 31 January, CERN, 31 January, 20012001Egil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of Bergen
Electrons (10-18 m )
Atom nucleus nucleon quark
10-10 m 10-14 m 10-15 m 10-18 m
Constituents of matter
see
CERN, 31 January, CERN, 31 January, 20012001CERN, 31 January, CERN, 31 January, 20012001Egil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of Bergen
Stable (ordinary) matter:
one up quark (charge +2/3)
one down quark (charge -1/3)
one electron (charge -1)
one neutrino (no charge, “no” mass)
proton
neutron
But for what do we need the neutrino??
leptons
compositeparticles
nucleons
CERN, 31 January, CERN, 31 January, 20012001CERN, 31 January, CERN, 31 January, 20012001Egil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of Bergen
The Forces of Nature(what is a force?)
Newton and Gravity
Faraday and Fields
Forces as “Exchange” Particles
An important difference between Matter Particles and Force Particles:M.P. obey Pauli’s Principle, i.e. only one particle for each quantum state.F.P. does not have this constraint and can clump together.
This is why Matter appears to be Solid
CERN, 31 January, CERN, 31 January, 20012001CERN, 31 January, CERN, 31 January, 20012001Egil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of Bergen
CERN, 31 January, CERN, 31 January, 20012001CERN, 31 January, CERN, 31 January, 20012001Egil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of Bergen
Is the Quantum World a Fuzzy World?
The answer is a clearNO !
QM means that all thequalities of the subatomicworld and by extension ofeverything can be exactly quantified !
Photon, E = h
CERN, 31 January, CERN, 31 January, 20012001CERN, 31 January, CERN, 31 January, 20012001Egil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of Bergen
Can not use light microscopes to study atoms !!!
Quantum mechanics tells us thatparticles behave like waves and visa versa:
h/p
Use electron microscopes
LEP the world’s biggestelectron microscope
electron
CERN, 31 January, CERN, 31 January, 20012001CERN, 31 January, CERN, 31 January, 20012001Egil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of Bergen
electron
quark
New Stuff from E = Mc2
New, unstable particles, can NOT be explainedas made up of up and down quarks only.
High Energy electron-proton scattering
CERN, 31 January, CERN, 31 January, 20012001CERN, 31 January, CERN, 31 January, 20012001Egil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of Bergen
Creating New Matter with LEP
Need two more generations of quarks
CERN, 31 January, CERN, 31 January, 20012001CERN, 31 January, CERN, 31 January, 20012001Egil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of Bergen
How does a point in empty space know exactlythe variety of particles it can produceand all their properties and their forces .... ???
Back to Heisenberg and Faraday:Particles and Forces are Quantum Fields fillingevery point of “Empty” Space (or the “Vacuum”).
The Fields materialize as Particles whenEnergy is fed into this Vacuum.
Structures are temporary, the Pattern lasts for ever !
CERN, 31 January, CERN, 31 January, 20012001CERN, 31 January, CERN, 31 January, 20012001Egil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of Bergen
electron(energy U)
U= 1 eV= 1.6x10-19J(speed at positive plate18 000 km/s)
1 keV = 103 eV1 MeV = 106 eV1 GeV = 109 eV1 TeV = 1012 eV
LEP = 209 GeVLHC = 14 TeV
Practical Units
- +
1 Volt
CERN, 31 January, CERN, 31 January, 20012001CERN, 31 January, CERN, 31 January, 20012001Egil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of BergenEgil Lillestøl, CERN & Univ. of Bergen
Einstein: E = Mc2
pc
use units such that c =1 E (GeV or MeV)p (GeV/c or MeV/c)M (GeV/c2 or MeV/c2)
M0c2Mproton = 0.931 GeV/c2 ≈ 1 GeV/c2 Melectron = 0.5 MeV/c2
( Mtop = 170 GeV/c2 )
proton diameter = length scale:10-15 m = 1 fermi (femtometer)
E
Special Relativity:( E2= (pc)2 + (M0c2)2 )