In physics, a coupling constant, usually denoted g, is a number that determines the strength of an interaction. Usually the Lagrangian or the Hamiltonian of a system can be separated into a kinetic part and an interaction part. The coupling constant determines the strength of the interaction part with respect to the kinetic part, or between two sectors of the interaction part. For example, the electric charge of a particle is a coupling constant.
A coupling constant plays an important role in dynamics. For example, one often sets up hierarchies of approximation based on the importance of various coupling constants. In the motion of a large lump of magnetized iron, the gravitational forces are more important than the magnetic forces because of the relative coupling constants. However, in classical mechanics one usually makes these decisions directly by comparing forces.
Fine structure constant
The coupling constant comes into its own in a
quantum field theory. A special role is played in relativistic quantum theories by coupling constants which are dimensionless, ie, are pure numbers. For example, the
fine-structure constant,
-
(where
e is the
charge of an electron,
ε0 is the
permittivity of free space,
is the
reduced Planck constant and
c is the
speed of light) is such a dimensionless coupling constant that determines the strength of the
electromagnetic force on an electron.
Gauge coupling
In a non-Abelian gauge theory, the
gauge coupling parameter,
g, appears in the
Lagrangian as
-
(where
G is the gauge
field tensor) in some conventions. In another widely used convention,
G is rescaled so that the coefficient of the kinetic term is 1/4 and g appears in the
covariant derivative. This should be understood to be similar to a dimensionless version of the electric charge defined as
-
Weak and strong coupling
In a
quantum field theory with a dimensionless coupling constant,
g, if it is (much) smaller than one, then one says that the theory is
weakly coupled. In this case it is well described by an expansion in powers of
g, called
perturbation theory. If the coupling constant is of order one or larger, the theory is said to be
strongly coupled. An example of the latter is the
hadronic theory of
strong interactions (which is why it is called strong in the first place). In such a case non-perturbative methods have to be used to investigate the theory.
Running coupling
One can probe a
quantum field theory at short times or distances by changing the wavelength or momentum,
k of the probe one uses. With a high frequency, ie, short time probe, one sees
virtual particles taking part in every process. The reason this can happen, seemingly violating the
conservation of energy is the
uncertainty relation
-
which allows such violations at short times. The previous remark only applies to some formulations of QFT, in particular,
canonical quantization in the
interaction picture. In other formulations, the same event is described by "virtual" particles going off the
mass shell. Such processes
renormalize the coupling and make it dependent on the scale,
k at which one observes the coupling. The phenomenon of scale dependence of the coupling,
g(k) is called
running coupling in a
quantum field theory.
Beta-function
The
beta function β(
g) of a
quantum field theory measures the running of a coupling parameter. It is defined by the relation:
-
For most theories the beta function is positive, so that the coupling is increasing in
k (equivalently, the coupling rises as the scale at which the theory is observed becomes shorter). This is also the case in
quantum electrodynamics (QED). At low energy, i.e. long distances, α ≈ 1/137. At the scale of the
Z boson, about 90
GeV, α ≈ 1/127.
In a classical field theory in which a scale change is an invariance (symmetry) of the theory, the beta function breaks this scale invariance. Since this is a quantum effect arising directly from the uncertainty principle, a non-zero beta function implies a scale anomaly in such a quantum field theory.
Landau pole and asymptotic freedom
We noted that QED is
weakly coupled at long distances, but the coupling increases at short distances. This increase was first noticed by
Lev Landau who showed that QED becomes
strongly coupled at high energy, and in fact the coupling becomes infinite at asympototically high energy. This phenomenon is called the
Landau pole.
In non-Abelian gauge theories, the beta function is negative, as first found by Frank Wilczek, David Politzer and David Gross. As a result the coupling decreases at short distances. Furthermore, the coupling decreases logarithmically, a phenomenon known as asymptotic freedom. The coupling decreases approximately as
-
where β
0 is a constant computed by Wilczek, Gross and Politzer.
QCD scale
In
quantum chromodynamics (QCD), the quantity Λ is called the
QCD scale. The value is
-
This value is to be used at a scale above the bottom
quark mass of about 5
GeV. The meaning of Λ
MS is given in the article on
dimensional regularization.
Charge, colour charge, etc
In
quantum field theory, since the
size of the interaction term is absorbed into the notion of the coupling constant (more correctly
coupling parameter, since it runs), the word
charge is freed up for another use. One says, for example, that the electrical charge of an
electron is -1 and that of any observable
particle is an integer multiple of this. The notion of charge is now exactly the same as the representation of the gauge group to which the particle belongs. Thus the
colour charge of a
quark is fixed at 4/3 since it belongs to the
fundamental representation of
SU(3), and the colour charge of a
gluon is 8 since it belongs to the
adjoint representation.
This difference in the notion of charge in classical and quantum field theory is alluded to in a shorthand phrase that is sometimes used: "charge in units of the positron charge".
String theory
A remarkably different situation exists in
string theory. Each perturbative description of string theory depends on a string coupling constant. However, in the case of string theory, these coupling constants are not pre-determined, adjustable, or universal parameters; rather they are dynamical
scalar fields that can depend on the position in space and time and whose values are determined dynamically.
See also
References and external links
Interaction | Quantum field theory | Quantum mechanics | Statistical mechanics | Renormalization group
Constante de couplage