Chemistry Reference
In-Depth Information
1.2.9 Eigenvalue Equation
The equation
A x Þ¼ A x Þ
ð 1
:
19 Þ
is called the eigenvalue equation for the linear operator A. When (1.19) is
satisfied, the constant A is called the
the
eigenfunction of the operator A. Often, A is a differential operator, and
there may be a whole spectrum of eigenvalues, each one with its corre-
sponding eigenfunction. The spectrum of the eigenvalues can be either
discrete or continuous. An eigenvalue is said to be n-fold degenerate when
n different independent eigenfunctions belong to it. We shall see later that
the Schroedinger equation for the amplitude
eigenvalue, the function
c
(x) is a typical eigenvalue
equation, where A ¼ H ¼ T þ V is the total energy operator (the
Hamiltonian), T being the kinetic energy operator and V the potential
energy characterizing the system (a scalar quantity).
c
1.2.10 Hermitian Operators
A Hermitian operator is a linear operator satisfying the so-called 'turn-
over rule':
<
hcj A wi¼h A cjwi
ð dx c
ð dx ð A x ÞÞ
ð 1
:
20 Þ
ð x Þð A x ÞÞ ¼
:
x Þ
The Hermitian operators have the following properties:
(i)
real eigenvalues;
(ii)
orthogonal (or anyway orthogonalizable) eigenfunctions;
(iii)
their eigenfunctions form a complete set.
Completeness also includes the eigenfunctions belonging to the contin-
uous part of the eigenvalue spectrum.
Hermitian operators are i
2 , T ¼ð h 2
2
2
=@ x 2 , r
@=@ x, i r ,
@
=
2m Þr
H ¼ T þ V, where
(i 2
and
i
is
the
imaginary
unit
¼ 1),
i ð@=@ x Þþ j ð@=@ y Þþ k ð@=@ z Þ
is
the gradient vector operator,
2
=@ z 2 is the Laplacian operator
(in Cartesian coordinates), T is the kinetic energy operator for a particle
of mass m with
2
=@ x 2
2
=@ y 2
2
r
¼rr¼@
þ@
þ@
H is the
h ¼ h =
2
p
the reduced Planck constant and
Hamiltonian operator.
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