We will now define a concept which will be of great importance both for
the solution of the mathematical problems of the theory and in relation
to its physical interpretation, even when it is not possible to find
exact solutions. This is the concept of momentum space. The fields,
as defined so far, are written as functions of the sites and hence of
their integer coordinates
. As we saw before, we refer to the
space of all possible fields as the space of field configurations. We
will call this representation of the fields, as functions of the sites,
by the name position space. Another representation of the fields
exists in momentum space, which is obtained by means of a linear
transformation that effects a change of basis in the space of
configurations. The integer coordinates
of the sites will be
mapped on a new set of integer coordinates
that index what we
will call the modes of the lattice, in a way similar to the
indexing of the sites by
. The name originates from the
classical concept of normal modes of oscillation.
We will begin by showing a simple property of exponentials with discrete
arguments involving integers. Let be an integer and
consider the exponential function
for the set of possible values of the argument. We have here complex
phases, which means that this function assumes values along the unit
circle of the complex plane. As
varies from
to
the function
goes around the circle, defining along it
equally spaced points. In
figure 2.5.1 we have an example with
, with
the
values of
marked for each phase.
Note that, since the sum of the complex numbers is equivalent to the sum of the two-dimensional vectors shown in the figure, its symmetry implies that
Note that this argument does not depend on the parity of , but only on
the fact that the vectors are equally spaced along the circle. In
figure 2.5.2 we show an example with
.
We will now consider the slightly more complicated case in which we
multiply the argument of the exponential by another integer
, obtaining the function
In this case, as varies from
to
the function goes around the
circle exactly
times. In the case
we will still be defining
in this way sets of points equally spaced along it. For example, for
we have, for the two values of
used before, the phases shown in
figures 2.5.3
and 2.5.4.
As one can see, in the case all the possible phases end up occupied
a single time, as before, but in a different order. In the case
only one half of the possible phases ends up occupied, each one of them
twice. Hence, in this latter case, in which
is divisible by
, the
set of phases ends up reduced to the set of the case
, repeated
times. From the symmetry of the resulting sets of phases in either
case, we see that it is still true that the sum of all these phases is
zero,
The same is valid for any other values of in the interval under
consideration, except for
. In this case we always have, very
simply,
times the positive real phase
, so that we may
write for our sum of phases
where is the Kronecker delta, equal to
if
, equal
to
if
. In order to convince oneself of the truth of this
fundamental relation, which will give rise to the relations of orthogonality and completeness that we will frequently use, one
may try out a certain number of particular cases, until one acquires a
practical understanding of how the sum of phases works. We may also
verify it in a simple and elegant way using the formula for the sum of a
geometrical progression2.1, although the numbers involved are complex
rather than real. The extension of this formula to the complex domain is
a simple process of analytical extension and its validity can be verified
algebraically (problem 2.5.1). If we have as the
initial element of the progression
and as
the ratio
, with
, we will also
have
for any
, and the sum is given by
For the case and
the formula cannot be used due to the zero
in denominator, but in this case the result is obvious because all the
elements of the sum are equal. In the problems a different approach to
this question is proposed, equally rigorous and more complicated and
detailed (problems 2.5.5,
2.5.6 and 2.5.7).
Observe that we may use integer coordinates for the sites with values in
the interval , or any other interval containing
consecutive
integers, as well as in the interval
, as we have been doing. In
addition to this, the exponential that appears in the sum above is
symmetrical by the exchange of
e
, so that it is equally true that
One can also see that the modes e
are in reality the same
mode, in fact
and
always represent the same mode
(problem 2.5.2). Thus, in the case of the
coordinates we may also choose the extremes of the interval of variation
arbitrarily, so long as we always take
consecutive values. For
reasons associated to the physical interpretation of these modes, it will
be convenient that we take the intervals of variation of
in a way as
symmetrical as possible around
. For this reason we will adopt the
following standard intervals, one for odd
,
and another for even ,
We may now write the relations above in a slightly different form, that we will name relation of orthogonality,
and relation of completeness,
where and
are the minimum and maximum limits of the
interval of values of
in each case. Once these relations are
established for the one-dimensional case as we have done here, their
extensions to higher dimensions is immediate, achieved by means of the
use of the properties of the exponential function
(problem 2.5.3). Hence in
dimensions we
have the relations
The first relation establishes a definition of scalar product between
modes, according to which they are all orthogonal to one another. The
exponential functions
are called
the mode functions of these Fourier modes. This scalar product is
defined as a sum over position space of products of two mode functions,
which are characterized by
and
. The second relations
involves a sum over momentum space and establishes that any function of
the sites on the lattice can be written as a linear superposition of
these mode functions, which therefore constitute a complete set of
functions on the lattice (problem 2.5.4).
is contained within the set of phases given by
where the integer is given in terms of
by
where is some integer. We say that
is equal to
module
. In
this way we succeed to map the phases generated by any given
back to
the interval described by an integer from
to
.