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86                   General principles of quantum theory

                             State function
                             According to the ®rst postulate, the state of a physical system is completely
                             described by a state function Ø(q, t) or ket jØi, which depends on spatial
                             coordinates q and the time t. This function is sometimes also called a state
                             vector or a wave function. The coordinate vector q has components q 1 , q 2 , ... ,
                             so that the state function may also be written as Ø(q 1 , q 2 , ... , t). For a particle
                             or system that moves in only one dimension (say along the x-axis), the vector q
                             has only one component and the state vector Ø is a function of x and
                             t: Ø(x, t). For a particle or system in three dimensions, the components of q
                             are x, y, z and Ø is a function of the position vector r and t: Ø(r, t). The state
                             function is single-valued, a continuous function of each of its variables, and
                             square or quadratically integrable.

                               For a one-dimensional system, the quantity Ø (x, t)Ø(x, t) is the probabil-
                             ity density for ®nding the system at position x at time t. In three dimensions,

                             the quantity Ø (r, t)Ø(r, t) is the probability density for ®nding the system at

                             point r at time t. For a multi-variable system, the product Ø (q 1 , q 2 ,
                             ... , t)Ø(q 1 , q 2 , ... , t) is the probability density that the system has coordi-
                             nates q 1 , q 2 , ... at time t. We show below that this interpretation of Ø Ø

                             follows from postulate 3. We usually assume that the state function is normal-
                             ized
                                   …

                                    Ø (q 1 , q 2 , ... , t)Ø(q 1 , q 2 , ... , t)w(q 1 , q 2 , ...)dq 1 dq 2 ... ˆ 1
                             or in Dirac notation
                                                            hØjØiˆ 1
                             where the limits of integration are over all allowed values of q 1 , q 2 , ...



                             Physical quantities or observables
                             The second postulate states that a physical quantity or observable is represented
                             in quantum mechanics by a hermitian operator. To every classically de®ned
                             function A(r, p) of position and momentum there corresponds a quantum-
                                                                 ^
                             mechanical linear hermitian operator A(r,("=i)=). Thus, to obtain the quan-
                             tum-mechanical operator, the momentum p in the classical function is replaced
                             by the operator ^ p
                                                                 "
                                                             ^ p ˆ =                           (3:44)
                                                                  i
                             or, in terms of components
                                                    " @           " @          " @
                                               ^ p x ˆ   ,  ^ p y ˆ   ,   ^ p z ˆ
                                                     i @x         i @ y        i @z
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