Particle Interactions
|
Key Words Feynman Diagram, Interaction |
In the exam, you are expected
to know about:
Simple Feynman diagrams to represent the above reactions or interactions in terms of particles going in and out and exchange particles. |
Annihilation
When particles and antiparticles meet, they annihilate each other, releasing their combined mass as energy in the form of photons:

Because momentum and energy
have to be conserved, two or three photons are created.
If there is sufficient energy, other particles may be created as well.
For example, the collision between an electron and a positron may give
rise to two muons:
e- +
e+ ---->
m+
+ m-
The reverse process can apply
as well. Electrons and positrons
can be formed when a gamma ray passes through matter.
This pair production is a good
illustration of the interchangeability of mass and energy.
We can see this by applying a magnetic field. The opposite charges make
circular paths in opposite directions.
Lepton Interactions
There are six
particle-antiparticle pairs known. Leptons
(Greek – “light thing” or “small coins”) are the smallest of the
fundamental particles. They have
the following properties:
fundamental
particles without structure
they interact by the weak interaction. If
they are charged, they interact by the electromagnetic interaction, but NOT
the strong interaction.
charge and lepton number are conserved in all allowed
lepton processes.
There are three categories of lepton
number, Le, Lm,
and Lt.
Each lepton has a lepton number, 0 or 1, in
each category, and each antilepton has a number 0 or -1 in each category.
You need to know the lepton numbers.
The names of the leptons are:
|
Lepton |
Symbol
|
Charge
|
Lepton Number |
|
electron
|
e- |
-1e |
Le =
1, Lm,
& Lt
= 0 |
|
electron neutrino |
ne |
0 |
Le =
1, Lm,
& Lt
= 0 |
|
muon
|
m- |
-1e |
Lm =
1, Le,
& Lt
= 0 |
|
neutrino |
nm |
0 |
Lm =
1, Le,
& Lt
= 0 |
|
tau |
t- |
-1e |
Lt =
1, Lm,
& Le
= 0 |
|
tau neutrino |
nt |
0 |
Lt =
1, Lm,
& Le
= 0 |
Each particle has an antiparticle; for the electron, it is the positron, the muon the antimuon, and the tau, the antitau. We show the anti-particle either by an opposite charge (e+) or by putting a bar across the symbol.
| What is the symbol, the charge, and the lepton number of the particle antitau? |
Consider this decay:

Notice how the lepton number and charge are conserved. This means that the decay can proceed. If leptons interact with hadrons, the hadrons are considered to have a lepton number of 0.
| Question 2 |
Will this reaction work?
|
Hadrons
There are a very large number
of particles that are classified as hadrons,
which are subdivided into two further classifications, the mesons, and the baryons.
Hadrons interact by the strong, weak, and electromagnetic
force.
They are not fundamental particles but have a structure.
They have non-zero rest masses, about 1 GeV/c2
They have an associated value of charge, Q,and baryon
number B.
Hadrons with zero baryon number
are called mesons; those with baryon
number of 1 are called baryons.
Mesons
These particles have a smaller
rest mass than the baryons (and a lower rest mass than the tau lepton). They have:
Zero baryon number.
Short lifetimes.
Antiparticles
Here are a few mesons:
|
Name |
Symbol
|
Q
B
|
Lifetime
(s) |
Antiparticle |
|
Pion |
p0 |
0
0
|
0.8 x 10-16
|
Itself |
|
|
p+ |
1
0
|
2.6 x 10-8 |
p- |
|
Kaon |
K+ |
1
0
|
1.2 x 10-8 |
K- |
|
|
K0 |
0
0
|
8.9 x 10-11
5.2 x 10-8
|
|
Notice how short the lifetimes are of these mesons.
| Why does the neutral pion seem to have a particularly short lifetime? |
We should note the following:
Mesons
have TWO quantum numbers that must be conserved in interactions.
The charge is denoted by Q,
the baryon number by B.
Mesons have a baryon number of 0.
Here is a typical decay:

Notice the conservation of charge and baryon number.
Here are some more:

| Question 4 |
Show that this interaction can
proceed:
p+ ---> m+ + nm |
These are the heavyweights of
particle physics, and include the familiar proton and neutron.
They are made up of three quarks
They have quantum numbers such as charge and baryon
number, which must be conserved in interactions.
|
Name
|
Symbol |
Q
B
|
Lifetime (s) |
Antiparticle |
|
Proton
|
p |
1
1 |
stable |
p |
|
Neutron |
n |
0
1 |
898 |
n |
|
Lambda |
L0 |
0
1 |
2.6 x 10-10 |
L0 |
|
Sigma
|
S+ |
1 1 |
0.8 x 10-10 |
S+ |
|
|
S0 |
0 1 |
7.4 x 10-20
|
S0 |
|
|
S- |
-1 1 |
1.5 x 10-10 |
S- |
|
Omega
|
W- |
-1
1 |
0.8 x 10-10 |
W+ |
Typical Decay

The proton is the only stable baryon. All the others spontaneously decay, although the neutron within a nucleus is stable, apart from beta decay. The decay times are incredibly short, except the isolated neutron which takes about 8 to 10 minutes. Baryons decay to protons, either directly (S+ --> p + p0) or indirectly (W- --> L0 + K, then L0 --> p + p-). Mesons decay to photons or leptons.
| Question 5 |
Show that this decay is possible: L0 -----> p+ + p- |
As in radioactivity, the decay of particles is random. The values quoted are the mean lifetimes, not half-lives.
It
is believed that gluons are shuttled
backward and forward between the quarks like rugby footballs.

Mesons bind the baryons together with the strong force.
The proton is the only baryon that is stable in isolation. The neutron on its own decays to a proton by beta minus decay after about 14 minutes. The decay is as a result of the weak interaction that occurs within nucleons.

Beta
decay
Beta emission is completely different to alpha.
Beta particles can be negative (b-), which is more common, or b+ in which a positively
charged particle is given off.
For beta b-
emission we know the following:
b- particles are given off by
neutron-rich nuclei
b- particles are electrons
b- emission is accompanied by
the simultaneous emission of an antineutrino,
<ne>.
It is worth noting that the
electron and antineutrino are NOT present in the nucleus before the beta decay. We can write the same for a b+
decay. A
neutron decays to give a b+ with a
neutrino.
The b+
particle is called a
positron,
which is the same size as an electron but has a charge of +1.
We can write general equations to describe beta decay.
|
b-
AX
---->
AY
+
0e- +
0n-bar
Z
Z + 1
-1
0
electron
electron antineutrino |
|
b+
AX
---->
AY
+
0e+ +
0n
Z
Z - 1
+1
0
|

| Show that this interaction is possible. |
Feynman Diagrams
We can show this using a Feynman diagram, which we will use as a pictorial representation of what is going on. They were first devised by Richard Philips Feynman (1918 – 1988) who was an American particle physicist. At the nucleon level we see:

At the quark level we see:

| What would the Feynman Diagram look like for beta plus decay? |
Beta
plus decay is mediated by the W+ particle, to release a positron and an electron
neutrino.
There are many other interactions that can be
summed up with Feynman diagrams, for example:
electron
capture
neutrino-neutron
collisions
antineutrino-proton
collisions
electron
proton collisions.
When we attempt these, we need to know what the interaction is in terms
of the four fundamental forces.
Photons
The forces between electrically charged particles are
thought to be transmitted by photons,
which are emitted and absorbed by the particles. We normally associate photons with the particle properties of
electromagnetic waves.
Gluons
As
separate particles, gluons have never
been directly identified. They are
however the mediators of the strong
nuclear force and there is compelling indirect evidence for them. They are thought to be fundamental particles.
There are eight gluons that have been identified theoretically from quantum
chromodynamics, each having a different “colour”, although all have zero
rest mass and zero charge. The
nucleons in the nucleus are thought to be held together by mesons such as the
pi-meson.
W+,
W-, and Z
These
are thought to mediate the weak force.
W+ mediates beta plus decay, W-
beta minus. The weak force is
little understood, but is thought to be responsible for fusion in stars.
The role of the Z boson is
unclear.
|
Suggested websites |
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| http://www.cyberphysics.pwp.blueyonder.co.uk/index.html | Excellent site |
| http://www.pparc.ac.uk | for the Particle Physics and Astronomy Research Council |

| Presentation |
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Now try
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