Postulates of quantum mechanics 377=xp〈x|p〉+i ̄h〈x|p〉−xpˆ〈x|p〉=i ̄h〈x|p〉, (9.2.45)where the penultimate line follows from eqns. (9.2.40) and (9.2.44). Since|x〉and|p〉
are not null vectors, eqn. (9.2.45) implies that the operator
ˆxpˆ−ˆpˆx= [ˆx,pˆ] =i ̄hI.ˆ (9.2.46)Next, consider a classical particle of massmmoving in one dimension with a
Hamiltonian
H(x,p) =
p^2
2 m+U(x). (9.2.47)The quantum Hamiltonian operatorHˆ is obtained by promoting both ˆpand ˆxto
operator, which yields
Hˆ(ˆx,pˆ) = pˆ2
2 m+U(ˆx). (9.2.48)The promotion of a classical phase space function to a quantum operator via the
substitutionx→xˆandp→pˆis known as thequantum-classical correspondence
principle. Using eqn. (9.2.44), we can now project the Schr ̈odinger equation onto the
basis of position eigenvectors:
〈x|Hˆ(ˆx,pˆ)|Ψ(t)〉=i ̄h∂
∂t〈x|Ψ(t)〉−
̄h^2
2 m∂^2
∂x^2Ψ(x,t) +U(x)Ψ(x,t) =i ̄h∂
∂tΨ(x,t), (9.2.49)where Ψ(x,t)≡ 〈x|Ψ(t)〉. Eqn. (9.2.49) is a partial differential equation that is often
referred to as theSchr ̈odinger wave equation, and the function Ψ(x,t) is referred to
as thewave function. Despite the nomenclature, eqn. (9.2.49) differs from a classical
wave equation in that it is complex and only first-order in time, and it includes a
multiplicative potential energy termU(x)Ψ(x,t). A solution Ψ(x,t) is then used to
compute expectation values at timetof any operator. In general, the promotion of
classical phase space functionsa(x) orb(p), which depend only on position or momen-
tum, to quantum operators follows by simply replacingxby the operator ˆxandpby
the operator ˆp. In this case, the expectation valuesAˆ(ˆx) orBˆ(ˆp) are defined by
〈Aˆ〉t=〈Ψ(t)|Aˆ(ˆx)|Ψ(t)〉=∫
dxΨ∗(x,t)Ψ(x,t)a(x)〈Bˆ〉t=〈Ψ(t)|Bˆ(ˆp)|Ψ(t)〉=∫
dxΨ∗(x,t)b(
̄h
i∂
∂x)
Ψ(x,t). (9.2.50)For phase space functionsa(x,p) that depend on both position and momentum, pro-
motion to a quantum operator is less straightforward for the reason that in a classical
function, how the variablesxandpare arranged is irrelevant, but the order matters