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ISP209s9 Lecture 18 -1-
Today
• HW 7 and Exam 2 due Thurs. 8pm
• 10 min recap from last lecture on QM
• Finish QM odds and ends from ch.14
• The Standard Model
– 4 forces of Nature
– Fundamental particles of Nature
– Feynman diagrams
ISP209s9 Lecture 18 -2-
Wave-Matter Duality
• EM waves are waves in
EM fields
• EM waves interfere
• EM waves are quantized
Efield = 0,1hf, 2hf, 3hf,…
• “quanta” are photons
Ephoton = hf
• Quantum non-locality
• Matter waves are waves in
matter fields
• Matter waves interfere
• Matter waves are quantized
Efield = 0, mc2, 2mc2, …
• “quanta” are the particles
(e.g., electrons)
• Quantum non-locality
ISP209s9 Lecture 18 -3-
Quantum Non-Locality
Spread out EM field instantaneously “knows” it has lost 1hf of
energy when the photon impacts the screen at a distant point.
Einstein was
troubled!
“Spooky action
at a distance”
ISP209s9 Lecture 18 -4-
What is “waving” for matter waves?
• Probability – all particles described by a “wave
function” !. The square of ! gives the probability
density of finding a particle per unit volume.
• The ! extends over all space, which gives weird
consequences.
= prob. of finding particle in a small
volume V centered at the point r.
ISP209s9 Lecture 18 -5-
Observation can alter the outcome in QM
Electrons show an interference pattern in the double slit experiment.
ISP209s9 Lecture 18 -6-
Now try to watch which path the e- took
A watched electron doesn’t show interference!
If you try to find out
Which slit the electron
Goes thru, the wave features
Go away
An electron
Detector
Many more weird examples…
ISP209s9 Lecture 18 -7-
Quantum Tunneling
Particle bouncing
around in a box
Classically: A low energy particle does not
Escape the box. It is always inside.
Quantum Theory: The ! function extends
over all space, even outside the box. There
Is a finite probability the particle will
“tunnel” thru the box and found outside.
This is why some nuclei can radioactively
decay.
ISP209s9 Lecture 18 -8-
Quantization of Energy Levels in Atoms
Electrons in atoms can only assume discrete,
quantized values of Energy.
Ground state
1st excited state
2nd excited state
ISP209s9 Lecture 18 -9-
Lasers
E1
E2
Etc…
• Say you have many identical atoms that are all in the excited
state.
• You can set off a “chain reaction” where many of them
de-excite together, and the emitted photons stimulate the
de-excitation in the other atoms that releases still more photons.
Light Amplified Stimulated Emission
ISP209s9 Lecture 18 -10-
Bosons and Fermions
• Particles come in two types
• Bosons have the property that they canoverlap. Examples are photons and certainatoms (helium). They are social.
• Fermions can not exist in the same state. Theyare anti-social. Examples – electrons, protons.
• The fermion nature of electrons explainsatomic structure (periodic table and all that)
ISP209s9 Lecture 18 -11-
Heisenberg’s Uncertainty Principle
• Uncertainty Principle: It is not possible to know
exactly the position and momentum of a particle at
the same time.
• There is no absolute knowledge. The Newtonian
view of the world (if everything were known,
everything could be predicted) in not attainable.
ISP209s9 Lecture 18 -12-
Uncertainty depends on mass
electron
velocity
position
proton
baseball, highly
exaggerated (by
1025)
ISP209s9 Lecture 18 -13-
Sample Problem
!4
hpx "##
!4
htE "##
There are two versions
If the position of a proton, mass 1.67E-27 kg, is known to 1E-9 m the
momentum and velocity could have a range of
smkg
m
Js
x
hp
!!=
!
!=
"#"
$
$
$26
9
34
1027.51000.14
10625.6
4 %%
sm
kg
smkg
smkg
mp
6.311067.1
1027.5
v
1027.5v
27
26
26
=!
!!
="
!!="="
#
#
#
ISP209s9 Lecture 18 -14-
Quantum Nonlocality
1
2
1
2
After interaction the wave functions are
entangled.
If we measure 1 and 2 at the same time the
difference in position forms an interference
pattern.
If we measure 2 before 1, the measurement
of 2 defines where 1 must hit. This
information travels faster than the speed of
light.
This has been confirmed experimentally.
Interaction
ISP209s9 Lecture 18 -15-
From large to small
AtomsAtomic
NucleusA proton (uud)
Made of nuclei and
electrons. Size: 10-9m
Made of neutrons and
proton. Size 10-14 m
Made of quarks:
Size 10-15 m
A neutron has
dduISP209s9 Lecture 18 -16-
There are two more forces in nature – Strong Force
Strong force
– A force that exists between quarks, which have a property called colorcharge.
– The carrier of the force is the gluon (the gluon also has color charge)
– No isolated quarks are found in nature
– The force between protons-proton, protons-neutrons, and neutrons-neutrons is the result of the exchange of pairs of quarks. Pairs of quarksare called mesons (the pion is the lightest meson)
– The Strong force is responsible for binding atomic nuclei.
ISP209s9 Lecture 18 -17-
The Weak Force
Weak force
• A force between electrons, neutrinos and
protons (or neutrons), due to a property of
matter called weak charge.
• The carrier of the force are called weak vector
bosons W+ or W-, Z. The + or – tells the
electric charge of the boson.
• This force allows a neutron to change into a
proton and is responsible for most radioactive
decays.
ISP209s9 Lecture 18 -18-
Weak Potential
2 4 6 8 10DistanceHamL1
2
3
4
5
6
7
Weak Potential
The weak force falls off faster than 1/r2 .
Remember, the slope gives the magnitude of
the field (force).
distancequark quark
Electric potential shape - 1/r
Weak potential
ISP209s9 Lecture 18 -19-
A big picture
• Forces come about because of some
property of matter (charge, mass, weak
charge, color charge)
• The force is due to the exchange of “force
carrier” particles (photon, graviton, vector
boson, gluon)
ISP209s9 Lecture 18 -20-
The particles of nature
T. Kondo
-1
-1/3
+2/3
0
-1
Charge
(e)
00W-
1/30d
1/30u
01"
01e
Baryon
number
Lepton
number
Type
Quantum Numbers
ISP209s9 Lecture 18 -21-
Antiparticles
Every particle has a corresponding antiparticle. When a particle and an
anti particle meet they annihilate giving off energy. The fraction of
mass converted to energy in a matter anti-matter annihilation is 1, that
is, all the mass is converted to energy.
• A particle and its antiparticle have opposite values for all quantum
numbers except spin and mass.
• Example: The antiparticle of an electron is a positron. In all other
cases, the name of the antiparticle is anti- in front of the name of the
particle, such as proton and anti-proton.
• Antiparticles are written with a line over the top: p vs p (the
antiproton)
ISP209s9 Lecture 18 -22-
Antimatter
• Antimatter (matter made of anti-particles) is very difficult to
make. It can artificially be produced only at large particle
accelerators (“atom smashers”).
• Matter and anti-matter are created naturally in pairs
• So far the total amount of antimatter ever produced by
humankind is a few grams, and that almost immediately
annihilated with matter.
• The total energy in 1 g of anti-matter is:
E=mc2 = 0.001kg (3E8)2=9E14 J = 9E5 GJ
enough to run a normal power plant for 1 day.
ISP209s9 Lecture 18 -23-
Neutrinos
• Subatomic particles that do not have charge, but interactvia the weak force.
• These are very unusual particles and we still don’t knowmuch about their properties. They have a mass, but it is sosmall we have not been able to measure it.
• They come in three types, but the types mix.
• They account for about 2% of the universe but interactweakly. One light-year of lead would have only a 50%chance of stopping one.
ISP209s9 Lecture 18 -24-
Observatories for neutrinos
Sudbury solar neutrino
detector
ISP209s9 Lecture 18 -25-
A way to picture forces – Feynman Diagrams
quarkquark
g
ISP209s9 Lecture 18 -26-
Alternative version of the uncertainty principle
Time and energy also also related.
!4
htE "##
!4
hpx "##
It is possible for a short time to get something for nothing. But, it
has to be paid back.
On the very small scale, empty space is alive with “fluctuations”.
Particles can pop into and out of existence.
ISP209s9 Lecture 18 -27-
Quantum Chromo Dynamics - QCD
Feynman Diagram for the Strong force
Looks
like
This is called an exchange
force. The probability of an
interaction decreases
exponentially with the mass
of the exchanges particle.
Exponentially means, twice
the mass is e2=7.3 times less
space
tim
e
The more massive the particle exchanged, the shorter the range
of the force.ISP209s9 Lecture 18 -28-
The problem with QCD
Gluons themselves have color charge!
“normal” This is also possible.
ISP209s9 Lecture 18 -29-
Equations – sort of
Rules for Feynman Diagrams:
1). The number of leptons and baryons must be conserved.
2). Charge must be conserved.
Not
allowed
since lepton
number not
conserved
allowed
ISP209s9 Lecture 18 -30-
A summary of the forces of nature
infiniteGraviton (?)6x10-39Gravity
10-18
Only 0.001 width
of proton
Vector Bosons W+, W-, Z010-6Weak
infinitephoton1/137Electromagnetic
10-15 size of a
proton
Gluon, g, between quarks
Mesons-protons/neutrons
1Strong
Range (m)CarrierStrengthForce
ISP209s9 Lecture 18 -31-
Back to the weak and electromagnetic forces
Transformation of a neutron into a
proton by an interaction with a neutrino
via the Weak force.
(udd)
neutron
proton
(udu)
W-
e
electron
"
neutrino
e e
e e
photon
In the process: Energy (including mass); momentum,
charge, baryon number, lepton number, are conserved.
Repulsive force between two
electrons.
ISP209s9 Lecture 18 -32-
Quantum Electrodynamics - QED
• The description of the forces on the previous page is based on atheory called quantum electrodynamics.
• Most successful theory every devised – it has at the moment noknown problems and describes all electric, magnetic and weakinteractions.
• Strength of the EM force:
• Unification of EM and Weak Forces is called Electroweak theory
• Theory of the strong force is called Quantum Chromodynamics
experiment)32(03599979.137
1
theory)56(03599941.137
1
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=
!
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