Phys
557 – Lecture 2
Units
and Sizes –
Recall
from freshman physics that one of the most confusing issues in the introductory
course is the question of units. For
quantities with units (which I will call “dimensionfull” quantities) the
specific size will depend on the choice of units. For example, in (old) English units I am
nearly six feet tall, while in by now standard (except in the
Further,
since particle physics is “naturally” relativistic and quantum mechanical, we
would like to choose units so that the speed of light c, which is large in MKS
units, and h,
which is small in MKS units, are both of order 1. It turns out we can address all of the above
issues by defining a new set of “particle physics units” such that both c and h
are exactly to 1!!!! In the process we
have reduced the number of types of dimensionfull quantities to 1. We have

Thus time now has the same units as
distance. Likewise mass and energy have
the same units and both go like 1/distance or 1/time. In these new units the mass of the proton is
essentially 1 GeV (0.938 GeV/c2).
We also have one fm equal to 1/(197 MeV) ~
1/(200 MeV) = 1/(0.2 GeV). It is
typical in particle physics to express nearly all dimensionfull quantities in
terms of the “natural particle” unit of GeV.
A list of useful relationships is provided in the following table (and
also on the web).
Units

Sizes (Ignore factors of 2)

As suggested by the table the areas of the particles (the cross
sections for scattering) are typically measured in millibarnes
(mb).
You will not be surprised to learn that
with only one fundamental type of dimensionfull unit it is easy to define
dimensionless ratios. In many instances
these are the simplest quantities to understand in particle physics. As we will see, the gauge field theories that
underlie the Standard Model contain, in fact, no dimensionfull parameters in
the classical (and symmetric) limit.
Consider, for example, the case of QED. In MKS units the electric charge of an
electron has size e ~ 1.6 x 10-19 C.
Thus one often sees the fine structure constant as (e0
is the electric permittivity of the vacuum with value 8.85 x 10-12
fm)

We
will use Heavyside-Lorentz units where m0 (the magnetic permeability
of the vacuum) and e0
are both 1. In our units charges are
pure (dimensionless) quantities

In
our efforts to understand the fundamental interactions of particle physics the
really interesting (and difficult to explain) quantities are the small number
of dimensionfull quantities. Examples
include LQCD, the fundamental
dimensionfull parameter characterizing the strong interaction (and induced by
the radiative corrections), GF (the Fermi constant) or MW
(the mass of the W boson), the dimensionfull parameters that characterize the
weak interactions and GN,
Vocabulary of the Standard Model (and beyond):
(see also the PDG webpage http://pdg.lbl.gov/2002/contents_sports.html#
stanmodeletc)
The big picture: First the interactions -
|
Interaction |
Observed |
Strength |
Range |
Carrier |
|
|
Strong QCD |
nuclear forces |
~1 |
~10-15 m |
Gluon
|
Standard Model |
|
EM |
Atomic systems |
~10-2 |
1/r2 |
Photon
|
Standard Model |
|
Weak |
Decays |
~10-5 |
~10-18 m |
W±, Z |
Standard Model |
|
Gravity |
Astronomy |
~10-39 |
1/r2 |
Graviton
|
“SUSY Strings” |
+ the Higgs sector that is (presumably) responsible for the generation of masses but that has not yet been directly detected.
·
Matter particles (fields) - The basic building blocks of matter are spin ½ fermions. As
we learn from relativistic quantum mechanics (see chapter 4 in Rolnick) spin ½
particles (and antiparticles) satisfy a matrix form, linear equation of motion.
leptons – electron (e), muon (m), tau (t) and their corresponding
neutrinos (i.e., the ones they are coupled to by the weak interaction, ne , nm , nt) Þ 6
total plus antiparticles (recall that the existence of antiparticles is another
result of requiring a relativistic theory of spinor
particles). Leptons interact via EM,
weak interactions and gravity. Since the
neutrinos are electrically neutral and the weak coupling is only to the
left-handed component (right handed for the anti-neutrino), the simplest
version of the SM has massless neutrinos only in the left-handed chiral state.
There is now evidence that at least two of the neutrinos have nonzero masses.
quarks –
up, down, charm, strange, top, bottom Þ 6 “flavor” types. All come in 3 “colors” Þ 18 total plus antiparticles. Quarks interact via strong interactions, EM,
weak interactions and gravity. All
quarks have nonzero masses and the top quark is VERY heavy (~ 175 times the
mass of a proton). The quarks bind
together to form the directly observed strongly interacting particles – the hadrons. These fall into two classes: ½ integer spin baryons, integer spin mesons. The baryons are composed of quark triplets (
), while the mesons contain quark-antiquark pairs (
). These multi-quark
bound states are color singlets, i.e., zero total color charge.
The quarks and leptons seem to aggregate naturally into three families or
generations – (u, d, e, ne), (c, s, m, nm), (t, b, t, nt), which seem to be
identical reproductions of each other except for their masses. But why 3 generations? This seems to be a deep question, perhaps
related to our very existence (in the sense that it seems to be related to CP
violation and thus the abundance of baryons over anti-baryons).
·
Gauge particles (fields) – as we will learn (see chapters 7 & 8 in
Rolnick), the existence of a local gauge
invariance requires the theory to have an associated massless
vector (spin 1) field that couples to the charge associated with the
symmetry. These particles mediate the
interactions and are the “glue” that holds the matter fields together in the
universe.
Photon (g) – the gauge boson that couples to the electric
charge of electromagnetism. The
corresponding U(1) symmetry is unbroken and so the
photon is massless. All charged
particles correspond to 1-D fundamental (singlet) representations of U(1). U(1) is an Abelian symmetry
group and the photon itself is electrically neutral.
Weak bosons (W±, Z0) – the 3
gauge bosons that couple to the weak charge (responsible for radioactive
decays). The corresponding symmetry is a
spontaneously broken SU(2)
and the observed weak bosons all have masses of order 100 GeV. Pair-wise the quarks and leptons are members
of 2-D fundamental (doublet) representations of SU(2), e.g.,

The weak bosons are in the 3-D adjoint
representation (modulo issues of mixing with the U(1)
of EM). SU(2)
is a non-Abelian symmetry group and the weak
bosons have weak charge (they couple to each other). Strictly, the W bosons couple only to the
left handed components of the quarks and leptons, with the right handed
components appearing as SU(2) singlets.
Gluons (the
Quantum ChromoDynamics bosons – g) – the 8 gauge
bosons that couple to the “color” charge of the QCD strong interaction. The corresponding SU(3)
symmetry is unbroken and so the gluons are massless. The three colors of each flavor quark form
3-D fundamental (triplet) representations of SU(3),
while the gluons are in the 8-D adjoint (octet) representation. SU(3) is also a
non-Abelian symmetry group so that the gluons carry color charge and couple to
each other.

|
Particle |
Spin |
QEM |
SU(2)L
Weak* |
SU(3)QCD |
Mass |
|
Electron,
e |
½
|
-1 |
LH- |
|
0.510998902
±0.000000021 MeV |
|
ne |
½
|
0 |
LH- |
|
<
2.8 eV |
|
Muon,
m |
½
|
-1 |
LH- |
|
105.6583568±0.0000052 MeV |
|
nm |
½
|
0 |
LH- |
|
<
0.17 MeV |
|
Tau,
t |
½
|
-1 |
LH- |
|
|
|
nt |
½
|
0 |
LH- |
|
<
18.2 MeV |
|
u quark |
½ |
2/3 |
LH- |
|
1.5
to 4.5 MeV |
|
d quark |
½ |
-1/3 |
LH- |
|
5
to 8.5 MeV |
|
c quark |
½ |
2/3 |
LH- |
|
1.0
to 1.4 GeV |
|
s quark |
½ |
-1/3 |
LH- |
|
80
to 155 MeV |
|
t quark |
½ |
2/3 |
LH- |
|
174.3
± 3.2 ± 4.0 GeV |
|
b
quark |
½ |
-1/3 |
LH- |
|
4.0
to 4.5 GeV |
|
Photon,
g |
1 |
0 |
|
|
0
(< 2x10-16 eV) |
|
Z0 |
1 |
0 |
|
|
91.1876
± 0.0021 GeV |
|
W± |
1 |
±1 |
|
|
80.451
± 0.033 GeV |
|
Gluon,
g |
1 |
0 |
|
|
0 |
|
Higgs,
h |
0 |
0 |
|
|
>
107 GeV |
* To understand the
multiplets of the SU(2) of the weak interactions we
should discuss the concept of “mixing”. If we have two basis sets, e.g., one
defined by the mass eigenstates and one defined by the SU(2)
interactions, we can define mixing between the two. This is just what happens for the weak
interactions. The lower member of the SU(2) doublet, in which the u quark is the upper member, is
not the d quark mass eigenstate but rather a mixture of the d and s quarks (
, in terms of the Cabibbo angle qC). This allows the strange quark to decay into
the u quark by emitting a virtual W-. The full mixing structure is described by the
3x3 CKM (Cabibbo-Kobayashi-Maskawa) quark mixing
matrix. Current experiments indicate that
neutrinos exhibit oscillations (e.g., nm® nt). Thus there must be similar mixing for the
neutrinos and at least two of the neutrinos (and probably all) must have nonzero
masses (in order to define the second basis set).
**
If the neutrinos are ordinary massive Dirac fermions, but with extremely small
masses, then they will have RH components like the charged leptons that do not
participate in the Weak interactions.
The neutrinos could also be Majorana fermions, i.e., the neutrinos are their own antiparticles. In that case there is no extra Weak singlet
component. There are
just the LH neutrino and the RH “antineutrino”, both of which are
members of weak doublets.
***
Strictly speaking the physical Z0 and photon are mixtures of the
neutral gauge bosons of the underlying unbroken U(1)
and SU(2) symmetries.
To
understand several features of the structure of the Standard Model, especially
the strong interactions, we must understand at least qualitatively the ideas of
renormalization, running couplings, dimensional
transmutation, infrared slavery and asymptotic
freedom. As suggested in chapter
4 of Rolnick (see especially Fig. 4.3) the way we evaluate the various
contributions that arise in relativistic quantum mechanics and relativistic
quantum field theory essentially guarantees that individual contributions,
defined by a specific Feynman diagram, will often be infinite. However, the sum over all contributions
(Feynman diagrams) will be finite if we consider a real physical
quantity. We view the (finite) physical
quantities as being calculated as the result of subtracting two infinite quantities, or multiplying infinity times zero, finding a
finite answer in both cases. The formal
structure of this remarkable procedure is typically codified by the
“renormalization group”. The resulting
behavior of quantities like coupling constants, i.e., the effective
charge of a particle for a specific interaction is somewhat surprising and it
is essential that we establish some understanding of this issue. We will come back to this in more detail
later but for now we need some of the results.
Running
Couplings –
we know from relativistic quantum field theory that what we think of as the
vacuum is not really empty but filled with virtual particle – antiparticle
pairs that are constantly forming and then annihilating. In the presence of a real charge these pairs
will be polarized and influence the effective charge that we observe. (Recall classical screening effects in EM and
the permittivity of the vacuum, e0,
mentioned
above.) Thus when we talk about the
charge of a particle, or better, the strength of its coupling to the
appropriate gauge field, we must be careful to specify the “size” of the
particle we are talking about (i.e., the effective volume inside of
which we are measuring the net charge).
This size will be determined by the

With the picture to the left in mind, it is reasonable that the short distance (large m) EM coupling is larger (less screened) than the coupling observed at long distance. In fact, the coupling is so weak at long distances that it essentially stops changing. The “infrared fixed point” result is the usual 1/137.035999…. we are accustomed to in classical EM. Less well known is the result that the EM coupling becomes arbitrarily strong at short distances.

This
remarkable behavior is actually observed in the data. The linear relationship between 1/a and ln(m) suggested in the figure is
correct for small coupling.
For
the case of the strong interactions, QCD, there is a similar renormalization
effect complicated by the facts that there are 3 colors (and 3 anti-colors)
carried by the quarks (and anti-quarks) and that the gluons themselves carry
color charge. The vacuum polarization
due to the virtual quarks-antiquark pairs again serves to screen color charges,
just like in the U(1) case, but the effect of the virtual gluons is to
anti-screen
(i.e., to enhance the
charge inside the volume rather than hide it)!!
(I don’t know any slick way to draw a picture illustrating this.) As long as there are not too many kinds of
quarks (and 6 flavors is small enough) the gluons determine the sign of the
renormalization effect and the strong coupling decreases as the scale m increases (asymptotic freedom) and increases
as m decreases (infrared slavery). Note also that the latter point means that
there is no saturation effect at long distances and the strong interactions are
confining in the soft limit momentum, long distance limit – the quarks never
get out of hadrons! The particles
separated by long distances must be color singlets (i.e., no net color
charges). As we will learn, we can make
a color singlet from a quark and antiquark or 3 quarks, which explains the observed mesons and baryons, respectively. The fact that aQCD reaches the value 1 around
a scale of 250 MeV connects nicely to the observation that hadrons are of size
1 fermi.
The concept of running
coupling constants suggests the related concept of Grand
Unification (see chapters 22.2 in Peskin and Schroeder or 17.2 in
Rolnick). Maybe
at large scales (short distances) an even larger symmetry group obtains that
includes the observed U(1), SU(2) and SU(3) symmetries, e.g., SU(5) or
SO(10). Thus, as suggested by the
figure, the 3 couplings will converge to a single value at this large
scale. (As we will discuss later, we
know that something like this does happen in the unification of the
electro-weak theories. Note that the
physical EM coupling is a linear combination of the couplings 1 and 2 in the
figure.) In the Grand Unified Theory
(GUT) the leptons and quarks are in the same representation of the underlying
symmetry group. Thus there must be a
symmetry generator that transforms quarks into leptons and allow protons to
decay (into mesons and leptons). This
effect has not yet been observed (hence the lower limit on the GUT scale) but
the idea of Grand Unification remains extremely attractive. It also serves to illustrate the very
important idea that the physics can (will?) change as we reach larger energies
with our accelerators. We should view
the Standard Model as an effective field theory that is only known to be valid
up to 1 TeV.
New degrees of freedom are likely to be relevant at larger energies.
The
Standard Model does not explain the value of ~ 1 TeV for the vacuum expectation
value of the Higgs (i.e., the
quadratic divergences in the scalar sector suggest that the appropriate scale
should be the Grand Unification scale or above) nor the role of gravity (i.e.,
how does it work quantum mechanically).
The fact that gravity seems to have a natural scale (unlike the U(1),
SU(2) and SU(3) gauge theories of the EM, weak and strong interactions, which
exhibit no intrinsic scale – although renormalization introduces one), the
Planck scale at 1016 TeV that is very much larger than the Higgs
scale is referred to as the “hierarchy problem”.
·
Gravitons & SUSY – the expected quanta of quantum gravity are
spin 2 particles (and will be hunted at LIGO in eastern
·
Strings – since there are so many “fundamental” particles it
would be more elegant if the many particles we see are excitations of the same
fundamental object – the string. Just
like a violin string the fundamental string can become excited and correspond
to a state with greater mass and different quantum numbers, the various
fundamental particles of the Standard Model.
Since the fundamental objects in string theory are extended objects (in
1-D), the short distance (UV) properties of string theory are much less
singular than usual field theory (of point particles). Also, since we want both fermionic and bosonic
excitations, it is not surprising that the desired string theory (SuperString theory) exhibits supersymmetry. Even though it is not yet known how to
calculate scattering amplitudes, masses, etc. in the context of string
theory, string theory does tell us some things (assuming that it is the correct
underlying theory). For example, we know
that supersymmetry must be relevant at some scale for string theories to work
and that there are more than 3 spatial dimensions.
·
Extra dimensions – If string theories are correct, the universe
really has 1 time and 10 (or 9) spatial dimensions (depending on some details
of interpretation). The extra dimensions
are thought to be currently unobserved either because they are compact (curled
up) on a tiny scale (e.g., 10-35
m) and our microscopes cannot see into them, or because our usual probes do not
propagate in the extra dimensions, even if they are extended. This second remarkable scenario can be
motivated by the following observation.
The usual matter fields and gauge fields are open strings (i.e.,
with ends), while the gravitons are closed strings (loops). String theory suggests that the ends of the
open strings (where the usual charges are located) are confined to regions of
lower dimensional – called branes (from membranes) or more carefully D-branes
(for Dirichlet-branes). So maybe the matter and interactions of the
Standard Model are confined to the 4-D brane (a 3-brane) we know and love and
only gravity probes the rest of space.
Recently interest (see the August 2000 Scientific
American, page 62) has focused on the possibility that there might exist n
extra compact (size R), but not truly tiny (perhaps as large as R
~ 1 mm) dimensions in which only gravity propagates. The usual gravitational potential would then
take the form

Thus it might be that the usual
, appears to define a very large scale (the Planck scale ~ 1019
GeV) while the true gravitational constant,
, defines a scale as small as 1 TeV for the correct values of
R and n. This would
eliminate the hierarchy problem! Our
experimental colleagues, Adelberger, Heckel and Gundlach are avidly
pursuing this possibility (see the September 2000 Physics Today, page 22).
Question: Since the gravitational potential defined
above is more singular at short distances than the usual potential, is it
possible that such gravitational interactions would be evident in atomic or
particle interactions? To truly analyze
the situation at short distances requires a quantum theory of gravity. However, we can check semi-classically to see
at what interaction distance gravity of this form becomes numerically relevant. To proceed we will compare the short distance
form above with the usual electrical potential applied to the system of a
proton and an electron (a hydrogen atom).
Thus we want to find r0 such that

Solving this in the case n = 2, R = 1 mm (take mp ~ 1 GeV, me ~ 0.5 x 10-3 GeV), yields

I interpret this to suggest that gravity will still
not be significant in existing atomic or particle physics measurements, which
are not sensitive to physics at this scale.
However as we heard from Scott Thomas at the