19.2 PHYSICAL EXAMPLES OF OPERATORS
quantum-mechanical operators are those corresponding to positionrand mo-
mentump. One prescription for making the transition from classical to quantum
mechanics is to express classical quantities in terms of these two variables in
Cartesian coordinates and then make the component by component substitutions
r→multiplicative operatorr and p→differential operator−i∇.
(19.22)
This generates the quantum operators corresponding to the classical quantities.
For the sake of completeness, we should add that if the classical quantity contains
a product of factors whose corresponding operatorsAandBdo not commute,
then the operator^12 (AB+BA) is to be substituted for the product.
The substitutions (19.22) invoke operators that are closely connected with the
two that we considered at the start of the previous subsection, namelyxand
∂/∂x.One,x, corresponds exactly to thex-component of the prescribed quantum
position operator; the other, however, has been multiplied by the imaginary
constant−i,whereis the Planck constant divided by 2π. This has the (subtle)
effect of converting the differential operator into thex-component of anHermitian
operator; this is easily verified using integration by parts to show that it satisfies
equation (17.16). Without the extra imaginary factor (which changes sign under
complex conjugation) the two sides of the equation differ by a minus sign.
Making the differential operator Hermitian does not change in any essential
way its commutation properties, and the commutation relation of the two basic
quantum operators reads
[px,x]=
[
−i
∂
∂x
,x
]
=−i. (19.23)
Corresponding results hold whenxis replaced, in both operators, byyorz.
However, it should be noted that if different Cartesian coordinates appear in the
two operators then the operators commute, i.e.
[px,y]=[px,z]=
[
py,x
]
=
[
py,z
]
=[pz,x]=[pz,y]=0.
(19.24)
As an illustration of the substitution rules, we now construct the Hamiltonian
(the quantum-mechanical energy operator)Hfor a particle of massmmoving
in a potentialV(x, y, z) when it has one of its allowed energy values, i.e its
energy isEn,whereH|ψn〉=En|ψn〉. This latter equation when expressed in a
particular coordinate system is the Schr ̈odinger equation for the particle. In terms
of position and momentum, the total classical energy of the particle is given by
E=
p^2
2 m
+V(x, y, z)=
p^2 x+p^2 y+p^2 z
2 m
+V(x, y, z).
Substituting−i∂/∂xforpx(and similarly forpyandpz) in the first term on the