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The Schroedinger wave function and its dynamics

Operators and expectation values

Consistent with the rules x^iψ=xiψ{\hat x}^i \ket{\psi} = \ket{x^i \psi}, and p^iψ=ixiψ{\hat p}_i \ket{\psi} = \ket{\frac{\hbar}{i}\frac{\del}{\del x^i}\psi}, we simply write

xi:ψxiψpi:ψixiψ\begin{align} & x^i: \psi \to x^i\psi\\ & p_i: \psi \to \frac{\hbar}{i} \frac{\del}{\del x^i} \psi \end{align}

To find inner products, recall that χψ=ddxχ(x)ψ(x)\brket{\chi}{\psi} = \int d^d x \chi^*(x) \psi(x). Thus

χx^iψ=χxiψ=ddxχ(x)xiψ(x)χhatpiψ=ddxχ(x)ixiψ(x)\begin{align} & \bra{\chi}{\hat x}^i \ket{\psi} = \brket{\chi}{x^i\psi} = \int d^d x \chi^*(x) x^i \psi(x)\\ & \bra{\chi}{|hat p}^i \ket{\psi} = \int d^d x \chi^*(x) \frac{\hbar}{i} \frac{\del}{\del x^i} \psi(x) \end{align}

It is easy to show from this representation that x^,p^{\hat x}, {\hat p} are Hermitian. To see this, recall that the adjoint map takes OχχOO\ket{\chi} \to \bra{\chi}O^{\dagger}. We want to show that χOψ=χOψ\bra{\chi}O\ket{\psi} = \bra{\chi}O^{\dagger}\ket{\psi} for all χ,ψ\ket{\chi},\ket{\psi}. for the position operator, xiχ=xiχx^i\ket{\chi} = \ket{x^i\chi} and xiχ=χ(xi)\bra{x^i \chi} = \bra{\chi}(x^i)^{\dagger}. But

xiχψ=χ(xi)ψ=ddx(xiχ)ψ=ddxχxiψ=ddxχ(xiψ)=χxiψ\begin{align} \brket{x^i \chi}{\psi} & = \bra{\chi}(x^i)^{\dagger}\ket{\psi}\\ & = \int d^d x (x^i \chi)^* \psi \\ & = \int d^d x \chi^* x^i \psi \\ & = \int d^d x \chi^*(x^i\psi) = \bra{\chi} x^i \ket{\psi} \end{align}

so that xi=(xi)x^i = (x^i)^{\dagger}.

For p^i{\hat p}_i it is slighly more complicated. Now since

p^iχ=ixiχ{\hat p}_i \ket{\chi} = \ket{\frac{\hbar}{i}\frac{\del}{\del x^i}\chi}

this mwans that

ixiχψ=χp^iψ=ddx(iχxi)ψ=ddxiχxiψ=ddxχixiψ=χp^iψ\begin{align} \brket{\frac{\hbar}{i}\frac{\del}{\del x^i}\chi}{\psi} & = \bra{\chi}{\hat p}_i^{\dagger}\ket{\psi}\\ & = \int d^d x (\frac{\hbar}{i}\frac{\del\chi}{\del x^i})^*\psi\\ & = - \int d^d x \frac{\hbar}{i} \frac{\del \chi^*}{\del x^i} \psi\\ & = \int d^d x \chi^* \frac{\hbar}{i} \frac{\del}{\del x^i} \psi\\ & = \bra{\chi} {\hat p}_i \ket{\psi} \end{align}

where in the second to last line we integrated by parts. Since teh functions must be square integrable, they vanish at infinity, and the bounary term you get from integrating by parts should vanish also.

Wave equation

We have to date discussed quantum mechanics in terms of abstract vector spaces, including the space of functions. In the case of particles moving in space, we have argued that this vector space is the vector space of square-integrable functions. In the case of particles in dd dimensions this is L2(Rd)L^2(\CR^d), that is, complex functions on Rd\CR^d which satisfy

ddxψ(x)2<\int d^d x |\psi({\vec x})|^2 < \infty

In general we expect that we can write the dynamics of the states in terms of the function ψ\psi. First, since any state at any time can be represented by a complex function ψ\psi, we can write it as ψ(x,t)\ket{\psi(x,t)} .For the Hamiltonians such as

H=p^22m+V(x)H = \frac{{\hat{\vec p}}^2}{2m} + V({\vec x})

or (22), the quantum dynamics can be easily written as local partial differential equations for ψ(x,t)\psi(x,t). Using the actions

p^iψ(x,t)=ixiψ(x,t)x^iψ=xiψ(x,t)tψ=tψ\begin{align} {\hat p}_i \ket{\psi({\vec x},t)} & = \ket{\frac{\hbar}{i} \frac{\del}{\del x^i} \psi(x,t)}\\ {\hat x}^i \ket{\psi} & = \ket{x^i \psi({\vec x},t)}\\ \frac{\del}{\del t} \ket{\psi} & = \ket{\frac{\del}{\del t}\psi} \end{align}

This last can be shown via representing the derivative as the limit of a difference between ψ(x,t+ϵ)ψ(t)\psi(x,t+\eps) - \psi(t), and using the linearity of quantum mechanics which means that

ψ(t+ϵ)ψ(t)=ψ(t+ϵ)ψ(t)\ket{\psi(t+\eps)} - \ket{\psi(t)} = \ket{\psi(t+\eps) - \psi(t)}

The upshot of this is that the time-dependent Schrodinger equation can be written as

22m2ψ(x,t)+V(x)ψ(x,t)=itψ(x,t)- \frac{\hbar^2}{2m} {\vec\nabla}^2 \psi({\vec x}, t) + V({\vec x}) \psi({\vec x},t) = i\hbar \frac{\del}{\del t} \psi({\vec x}, t)

Relatedly, the time-independent Schrodinger equation for energy eigenstates becomes

:label3devalue22m2ψ(x,t)+V(x)ψ(x,t)=Eψ(x,t):label 3d_evalue - \frac{\hbar^2}{2m} {\vec\nabla}^2 \psi({\vec x}, t) + V({\vec x}) \psi({\vec x},t) = E \psi({\vec x}, t)

Practically speaking, this is the form we work with for particles moving in space -- for the simple harmonic oscillator, or particles in a magnetic field (eg in the quantum hall systems), the hydrogen atom (ignoring spin), and so on. In the end, though, we should remember we are working with a vector space, and that the Schrodinger equation remains a linear equation.