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Lecture PowerPoint
Chapter 32
Physics: Principles with
Applications, 6th edition
Giancoli
Chapter 32
Elementary Particles
Units of Chapter 32
• High-Energy Particles and Accelerators
• Beginnings of Elementary Particle Physics –
Particle Exchange
• Particles and Antiparticles
• Particle Interactions and Conservation Laws
• Neutrinos – Recent Results
• Particle Classification
Units of Chapter 32
• Particle Stability and Resonances
• Strange Particles? Charm? Maybe a New
Model Is Needed!
• Quarks
• The “Standard Model”: Quantum
Chromodynamics (QCD) and the Electroweak
Theory
• Grand Unified Theories
• Strings and Supersymmetry
32.1 High Energy Particles and
Accelerators
If an incoming particle in a nuclear reaction has
enough energy, new particles can be produced.
This effect was first observed in cosmic rays;
later particle accelerators were built to provide
the necessary energy.
32.1 High Energy Particles and
Accelerators
As the momentum of a particle increases, its
wavelength decreases, providing details of
smaller and smaller structures:
(32-1)
In addition, with additional kinetic energy
more massive particles can be produced.
32.1 High Energy Particles and
Accelerators
One early particle
accelerator was the
cyclotron. Charged
particles are maintained
in near-circular paths by
magnets, while an electric
field accelerates them
repeatedly. The voltage is
alternated so that the
particles are accelerated
each time they traverse
the gap.
32.1 High Energy Particles and
Accelerators
The frequency of the applied voltage must
equal that of the circulating particles, and is
given by:
(32-2)
This is called the cyclotron frequency.
32.1 High Energy Particles and
Accelerators
Larger accelerators are of a type called
synchrotrons. Here, the magnetic field is
increased as the particles accelerate, so that the
radius of the path stays constant. This allows
the construction of a narrow circular tunnel to
house a ring of magnets.
Synchrotrons can be very large, up to several
miles in diameter.
32.1 High Energy Particles and
Accelerators
Accelerating particles radiate; this causes them to lose
energy. This is called synchrotron radiation for particles
in a circular path. For protons this is usually not a
problem, but the much lighter electrons can lose
substantial amounts. One solution is to construct a linear
accelerator for electrons; the largest is about 3 km long.
32.2 Beginnings of Elementary Particle
Physics – Particle Exchange
The electromagnetic force acts over a
distance – direct contact is not necessary.
How does that work?
Because of wave-particle duality, we can
regard the electromagnetic force between
charged particles as due to:
1. an electromagnetic field, or
2. an exchange of photons
32.2 Beginnings of Elementary Particle
Physics – Particle Exchange
This is a crude analogy
for how particle
exchange would work to
transfer energy and
momentum. The force
can either be attractive
or repulsive.
32.2 Beginnings of Elementary Particle
Physics – Particle Exchange
Physicists visualize interactions using
Feynman diagrams, which are a kind of x-t
graph.
Here is a Feynman diagram for photon
exchange by electrons:
32.2 Beginnings of Elementary Particle
Physics – Particle Exchange
The photon is emitted by one electron and
absorbed by the other; it is never visible and is
called a virtual photon. The photon carries the
electromagnetic force.
32.2 Beginnings of Elementary Particle
Physics – Particle Exchange
Originally, the strong force was thought to be
carried by mesons. The mesons have nonzero
mass, which is what limits the range of the
force, as conservation of energy can only be
violated for a short time.
32.2 Beginnings of Elementary Particle
Physics – Particle Exchange
The mass of the meson
can be calculated,
assuming the range, d,
is limited by the
uncertainty principle:
(32-3)
For d = 1.5 x 10-15 m,
this gives 130 MeV.
32.2 Beginnings of Elementary Particle
Physics – Particle Exchange
This meson was soon discovered, and is called
the pi meson, or pion, symbol π.
Pions are created in interactions in particle
accelerators; here are two examples:
(32-4)
32.2 Beginnings of Elementary Particle
Physics – Particle Exchange
The weak nuclear force is also carried by
particles; they are called the W+, W-, and Z0.
They have been directly observed in
interactions.
32.2 Beginnings of Elementary Particle
Physics – Particle Exchange
A carrier for the gravitational force, called the
graviton, has been proposed, but there is as yet
no theory that will accommodate it.
32.2 Beginnings of Elementary Particle
Physics – Particle Exchange
This table details the four known forces, their
relative strength for two protons in a nucleus,
and their field particle.
32.3 Particles and Antiparticles
The positron is the same as the electron, except
for having opposite charge (and lepton number).
We call the positron the antiparticle of the
electron.
32.3 Particles and Antiparticles
Every type of particle has its own antiparticle,
with the same mass but most quantum numbers
being opposite.
A few particles, such as the photon and the π0,
are their own antiparticles, as all the relevant
quantum numbers are zero for them.
32.3 Particles and Antiparticles
This is a drawing of an
interaction between an
incoming antiproton and a
proton (not seen) that
results in the creation of
several different particles
and antiparticles.
32.4 Particle Interactions and
Conservation Laws
In the study of particle interactions, it was found
that certain interactions did not occur, even
though they conserve energy and charge, such
as:
A new conservation law was proposed, the
conservation of baryon number. Baryon
number is a generalization of nucleon
number to include more exotic particles.
32.4 Particle Interactions and
Conservation Laws
Particles such as the proton and neutron have
baryon number B = +1; antiprotons,
antineutrons, and the like have B = -1; all other
particles (electrons, photons, etc.) have B = 0.
32.4 Particle Interactions and
Conservation Laws
There are three types of leptons – the electron,
the muon (about 200 times more massive), and
the tau (about 3000 electron masses). Each
type of lepton is conserved separately.
32.4 Particle Interactions and
Conservation Laws
This accounts for the following decays:
Decays that have an unequal mix of e-type
and μ-type leptons are not allowed.
32.5 Neutrinos – Recent Results
Neutrinos are currently a subject of active
research. Evidence has shown that a neutrino
of one type may change into a neutrino of
another type; this is called flavor oscillation.
32.5 Neutrinos – Recent Results
This suggests that the individual lepton
numbers are sometimes not strictly conserved,
although there is no evidence that the total
lepton number is no.
In addition, these oscillations cannot take place
unless at least one neutrino type has a nonzero
mass.
32.6 Particle Classification
As work continued, more and more particles of
all kinds were discovered. They have now been
classified into different categories.
• Gauge bosons are the particles that mediate
the forces
• Leptons interact weakly and (if charged)
electromagnetically, but not strongly
• Hadrons interact strongly; there are two types
of hadrons, baryons (B = 1) and mesons (B = 0).
32.7 Particle Stability and Resonances
Almost all of the particles that have been
discovered are unstable. If they decay weakly,
their lifetimes are around 10-13 s; if
electromagnetically, around 10-16 s; and if
strongly, around 10-23 s.
32.7 Particle Stability and Resonances
Strongly decaying particles do not travel far
enough to be observed; their existence is
inferred from their decay products.
32.7 Particle Stability and Resonances
The lifetime of strongly decaying particles is
calculated from the variation in their effective
mass using the uncertainty principle. These
particles are often called resonances.
32.8 Strange Particles? Charm? Maybe a
New Model Is Needed!
When the K, Λ, and Σ particles were first
discovered in the early 1950s, there were
mysteries associated with them:
• They are always produced in pairs
• They are created in a strong interaction, decay
to strongly interacting particles, but have
lifetimes characteristic of the weak interaction
To explain this, a new quantum number, called
strangeness, S, was introduced.
32.8 Strange Particles? Charm? Maybe a
New Model Is Needed!
Particles such as the K, Λ, and Σ have S = 1
(and their antiparticles S = -1); other particles
have S = 0.
32.8 Strange Particles? Charm? Maybe a
New Model Is Needed!
The strangeness number is conserved in
strong interactions but not in weak ones;
therefore these particles are produced in
particle-antiparticle pairs, and decay weakly.
More recently, another new quantum number
called charm was discovered to behave in the
same way.
32.9 Quarks
Due to the regularities seen in the particle
tables, as well as electron scattering results that
showed internal structure in the proton and
neutron, a theory of quarks was developed.
32.9 Quarks
There are six different “flavors” of quarks; each
has baryon number B = ⅓.
Hadrons are made of three quarks; mesons are a
quark-antiquark pair.
32.9 Quarks
Here are the quark compositions for some
baryons and mesons:
32.9 Quarks
This table gives the properties of the six known
quarks.
32.9 Quarks
This is a list of some of the hadrons that have
been discovered that contain c, t, or b quarks.
32.9 Quarks
The particles that we now consider to be truly
elementary – having no internal structure – are
the quarks, the gauge bosons, and the leptons.
The quarks and leptons are arranged in three
“generations”; each has the same pattern of
electric charge, but the masses increase from
generation to generation.
32.10 The “Standard Model”: Quantum
Chromodynamics (QCD) and the
Electroweak Theory
Soon after the quark theory was proposed, it
was suggested that quarks have another
property, called color, or color charge.
32.10 The “Standard Model”: Quantum
Chromodynamics (QCD) and the
Electroweak Theory
Unlike other quantum numbers, color takes on
three values. Real particles must be colorless;
this explains why only 3-quark and quark-
antiquark configurations are seen. Color also
ensures that the exclusion principle is still
valid.
32.10 The “Standard Model”: Quantum
Chromodynamics (QCD) and the
Electroweak Theory
Each quark carries a color charge, and the
force between them is called the color force –
hence the name Quantum Chromodynamics.
The particles that transmit the color force are
called gluons; there are eight different ones,
with all possible color-anticolor
combinations.
32.10 The “Standard Model”: Quantum
Chromodynamics (QCD) and the
Electroweak Theory
The color force becomes much larger as quarks
separate; quarks are therefore never seen as
individual particles, as the energy to separate
them is less than the energy to create a new
quark-antiquark pair.
Conversely, when the quarks are very close
together, the force is very small.
32.10 The “Standard Model”: Quantum
Chromodynamics (QCD) and the
Electroweak Theory
These Feynman diagrams show a quark-quark
interaction mediated by a gluon; a baryon-
baryon interaction mediated by a meson; and the
baryon-baryon interaction as mediated on the
quark level by gluons.
32.10 The “Standard Model”: Quantum
Chromodynamics (QCD) and the
Electroweak Theory
Beta decay is the result of a
weak interaction, and is
mediated by a W± particle.
Here is a Feynman diagram
of beta decay:
32.11 Grand Unified Theories
A Grand Unified Theory (GUT) would unite the
strong, electromagnetic, and weak forces into
one. There would be (rare) transitions that
would transform quarks into leptons and vice
versa.
This unification would occur at extremely high
energies; at lower energies the forces would
“freeze out” into the ones we are familiar with.
This is called “symmetry breaking.”
32.11 Grand Unified Theories
GUTs predict that the proton will eventually
decay; in fact, the simplest GUT predicts a
lifetime for the proton that is shorter than the
measured limit, so a more complex GUT must
be the correct theory.
32.12 Strings and Supersymmetry
Finally, there are theories that attempt to include
the gravitational force as well.
String theory models the fundamental particles as
different resonances on tiny loops of “string.”
Supersymmetry postulates a fermion partner for
each boson, and vice versa.
Neither of these theories has any experimental
evidence either favoring or disfavoring it at the
moment.
Summary of Chapter 32
• Particle accelerators accelerate particles to
very high energy, to probe the detailed structure
of matter and to produce new massive particles
• Every particle has an antiparticle, with the same
mass and opposite charge (and some other
quantum numbers)
• Other quantum numbers: baryon number;
lepton number; strangeness; charm; topness;
bottomness
• Strong force is mediated by gluons
Summary of Chapter 32
• Fundamental force carriers are called gauge
bosons
• Leptons interact weakly and
electromagnetically
• Hadrons are made of quarks, and interact
strongly
• Most particles decay quickly, either weakly,
electromagnetically, or strongly
• There are six quarks and six leptons
Summary of Chapter 32
• The quarks also carry color charge
• Quantum chromodynamics is the theory of
the strong interaction
• Electroweak theory unites the
electromagnetic and weak forces
• Grand unified theories attempt to unite all
three forces