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96                   General principles of quantum theory

                             and is an even function of each q k . If the potential energy V(q) is also an even
                                                                    ^
                                                            ^
                             function of each q k , then we have H(q) ˆ H(ÿq) and
                                                ^
                              ^ ^
                                            ^
                                                                       ^
                                                                                    ^
                                                         ^ ^
                             [H, Ð]f (q) ˆ H(q)Ðf (q) ÿ ÐH(q) f (q) ˆ H(q) f (ÿq) ÿ H(ÿq) f (ÿq) ˆ 0
                                                                                   ^
                                                                                          ^
                             Since the function f (q) is arbitrary, the commutator of H and Ð vanishes.
                             Thus, these operators have simultaneous eigenfunctions for systems with
                             V(q) ˆ V(ÿq).
                               If the potential energy of a system is an even function of the coordinates and
                             if ø(q) is a solution of the time-independent Schrodinger equation, then the
                                                                            È
                             function ø(ÿq) is also a solution. When the eigenvalues of the Hamiltonian
                             operator are non-degenerate, these two solutions are not independent of each
                             other, but are proportional
                                                          ø(ÿq) ˆ cø(q)
                             These eigenfunctions are also eigenfunctions of the parity operator, leading to
                             the conclusion that c ˆÐ 1. Consequently, some eigenfunctions will be of even
                             parity while all the others will be of odd parity.
                               For a degenerate energy eigenvalue, the several corresponding eigenfunc-
                                     ^
                             tions of H may not initially have a de®nite parity. However, each eigenfunction
                             may be written as the sum of an even part ø e (q) and an odd part ø o (q)
                                                       ø(q) ˆ ø e (q) ‡ ø o (q)

                             where
                                                       1
                                               ø e (q) ˆ [ø(q) ‡ ø(ÿq)] ˆ ø e (ÿq)
                                                       2
                                                       1
                                               ø o (q) ˆ [ø(q) ÿ ø(ÿq)] ˆÿø o (ÿq)
                                                       2
                                                                                       È
                             Since any linear combination of ø(q) and ø(ÿq) satis®es Schrodinger's equa-
                                                                                  ^
                             tion, the functions ø e (q) and ø o (q) are eigenfunctions of H. Furthermore, the
                                                                                               ^
                             functions ø e (q) and ø o (q) are also eigenfunctions of the parity operator Ð, the
                             ®rst with eigenvalue ‡1 and the second with eigenvalue ÿ1.



                                                 3.9 Hellmann±Feynman theorem
                             A useful expression for evaluating expectation values is known as the Hell-
                             mann±Feynman theorem. This theorem is based on the observation that the
                             Hamiltonian operator for a system depends on at least one parameter ë, which
                             can be considered for mathematical purposes to be a continuous variable. For
                             example, depending on the particular system, this parameter ë may be the mass
                             of an electron or a nucleus, the electronic charge, the nuclear charge parameter
                             Z, a constant in the potential energy, a quantum number, or even Planck's
                                                                            ^
                             constant. The eigenfunctions and eigenvalues of H(ë) also depend on this
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