COMPLEMENTARITY > Origins
The formal tool allowing one to account for both the corpuscular and wavelike aspects of quantum phenomena is the
wave function (introduced by
Erwin Schrödinger in 1926, together with the famous equation governing its evolution in time). It associates a complex number

, called a
probability amplitude, with any point

in space and time.

contains part of the information encoded in the system's
quantum state,
and allows one to compute the probability of the
possible outcomes of measurements involving kinematical variables such
as position and momentum. The square modulus of the
wave function,

, gives for example the probability of finding the system in

at time
t (this important result can be derived from the
Born rule). According to
de Broglie's relations, the
wave function associated with a beam of particles of equal momentum
p and energy E, is a monochromatic wave of wavelength λ =
h/p and frequency ν =
E/h . For instance, a spherical wave provides a good approximation of the
wave function associated with a particle propagating from a point-like source:
(

being the position of the source,

being the
wave vector governing the propagation of the wave, whose modulus is 2π/λ). Notice that, in this example,

differs significantly from zero over a large region of space. This means that the distribution which describes the
probability to detect the particle at a given location is not localized
. Well-localized systems (i.e.
corpuscular objects) are not associated with a monochromatic wave, but
rather with a
wave packet. Wave packets can be regarded as superpositions of an infinite number of monochromatic waves of different wavelengths,
interfering destructively anywhere but in a small region where they add up
constructively giving rise to a signal. The spectral and spatial
extensions of a
wave packet have to obey the
uncertainty relations.
The
interference pattern observed in the
double-slit experiment is easily understood in terms of
wave function. The two slits split the wave associated with the incoming atom beam into two secondary spherical waves

and

(like in
figure 3). The atom's
wave function 
after the double-slit filter is given by a weighted sum of these two
secondary waves. This is why an ensemble of atoms produces
interference fringes on the detection plate: the maxima and minima of
probability reflect the different phase relations existing between the two waves

and

at different points of the detection screen (see
figure 1 and the related discussion).
In analogy with the optical case, the spacing between the fringes is proportional to the wavelength λ of the atoms. This explains why
interference cannot be observed in a
double-slit experiment with macroscopic bodies. Indeed, according to the
de Broglie relations,
the inter-fringes spacing turns out to be extremely small for large
mass objects. So tiny, in fact, that no physical detector has enough
resolution to distinguish the
interference between maxima and minima.
In general, however, whether an ensemble of systems does or does not display
interference is not a matter of size. Rather, it depends on the amount of
information in principle available to the observer. To make this point
clear, let's go back to the
double-slit experiment and compute the probability
p(
x) of detecting an atom at a point of coordinate
x along the axis perpendicular to the atom beam. Following an approach due to Richard Feynman, we consider the two possible ‘
paths’ connecting the atom source to each point of the detection screen (see figure 6). We will call the
paths coming from slit 1: ‘↑’
paths, and the
paths coming from slit 2: ‘↓’
paths.
Figure 6. For each point of the detection screen one can imagine two converging paths for the atom, each one coming from one of the slits.
We can also associate a
state vector
to the atoms following a ‘↑
path’:

is the
state vector that predicts for the atoms' position on the screen the
distribution observed in an apparatus
where only slit 1 is open (red curve of
figure 4). Conversely, we call

the
state vector that predicts the
distribution observed in an apparatus
where only slit 2 is open (blue curve of
figure 4). Having stated these definitions, we can discern two cases.
•
Case 1 – INDISTINGUISHABLE PATHS
Suppose that there is no way to say whether the atom has followed a ‘↑’
path or a ‘↓’
path (the
paths are said in this case to be
indistinguishable). The
state vector representing this situation is the following:
Applying
Born’s rule to state (2), one can formally derive the spatial
distribution p(
x) expected in this case. Our previous discussion on
wave functions provides us with the recipe necessary to carry out this simple calculation. We get:

and

correspond to the red and blue
distributions in
figure 4 respectively. Besides the weighed sum of these two terms (green curve A in
figure 4), the probability associated with state (2) contains ‘cross’ terms. It is easily seen using eq. (1) that cross terms oscillate as a function of
x. When added to the first and second term, this oscillating function give rise to the typical
interference pattern (green curve B in
figure 4).
•
Case 2 – DISTINGUISHABLE PATHS
Let's consider now the case in which it is possible to discriminate the
paths (without disturbing the motion of the atoms). Suppose for example that the atoms are excited and decay emitting a
photon exactly while passing through the slit (
figure 5). Detecting the emitted
photon would bring the ‘which slit’ information to our knowledge. Therefore, ‘↑’
paths and ‘↓’
paths are now
distinguishable (in the sense that they can – in principle – be distinguished). Let
W be the
photon observable carrying the ‘which slit’ information, and let's conventionally call ‘

’ the outcome of
W that indicates slit 1 and ‘

’ the outcome of
W that indicates slit 2. The
state vector corresponding to the new experimental configuration is the following
entangled state, involving the atom and the emitted
photon:
According to the definition of
entangled state, if the
photon indicates

, then the atom will follow the
probability distributions predicted by
state 
, whereas if the photon indicates

, then the atom will follow the
probability distributions predicted by

. Since each photon indicates either

or

, it's clear that each atom is compelled to follow
either the spatial distribution associated to
or the one associated to

. Therefore, if we look at the detected atoms
disregarding the information supplied by the photon, we will see a spatial distribution that is simply the weighted sum of the
probability distributions predicted by

and

respectively. The weights of the sum are the probabilities for the outcomes

and

to occur, namely ½ and ½.
Cross terms, and hence
interference fringes, are absent in this case (compare to the discussion on the
entangled states of
spin ½ particle).
The disappearance of
interference when the ‘which slit’ information becomes in principle available should not appear too surprising. The atom
state vectors 
and

can be expressed as
superpositions of either position
eigenstates or momentum
eigenstates. Therefore, they assign probabilities not only to different positions, but also to different momenta. In particular,
state 
assigns probability 0 to momenta indicating that ‘the atom is coming from slit 2’, whereas the opposite is true for

.
Thus , making the ‘which slit’ information available amounts to
(partially) measuring the atoms' momentum. Position and momentum being
incompatible observables, a measurement of momentum unavoidably modifies the spatial
distribution of the atoms in any subsequent measurement of position.
Interference, in particular, is washed out (see the discussion of
quantum states for more details).
Feynman's rules are a powerful tool that can be used in several contexts, once a set of ‘
paths’ and the corresponding
probability amplitudes have been recognized.
Interference itself is a general feature of quantum phenomena, not limited to
position measurements. Regardless of the way a system is
prepared, one can find an observable such that the
probability distribution associated with its outcomes displays
interference (meaning that some outcomes are found with high probability, while others are
never found). In general, if the
state of the system can be written as a superposition of the
eigenstates of an observable
A,
interference fringes are observed when measuring an observable
B incompatible with
A. The condition for
interference to be observed is that there be no ‘which
path’ information available (neither in principle), i.e. that there is no observable
C whose outcomes are correlated with those of the ‘
path observable’
A (see the example of
spin observables).
Interference effects illustrate the deep connection between the
principle of superposition,
incompatible observables and
complementarity.
This link shows in turn to what extent the mathematical core of quantum
theory is determined by the relations existing among the observables we
use to ‘structure’ physical phenomena (see
implications).