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Physical Review A

Hydrogen atom in the momentum representation

John R. Lombardi

Published Sep 1, 1980• 33 citations
Publisher

Abstract

The wave functions for the hydrogen atom are determined in the momentum representation, using momentum variables ${p}_{r}$, ${p}_{\ensuremath{\theta}}$, ${p}_{\ensuremath{\varphi}}$ which are associated with the spherical polar variables $r$, $t(={e}^{i\ensuremath{\pi}cos\ensuremath{\theta}})$ and $v({e}^{i\ensuremath{\varphi}})$. The functions may be written as ${{\ensuremath{\varphi}}_{n,l,m}({p}_{r},{p}_{\ensuremath{\theta}},{p}_{\ensuremath{\varphi}})={\ensuremath{\alpha}}_{n,l}({p}_{r}){\ensuremath{\beta}}_{l}^{m}({p}_{\ensuremath{\theta}})\ensuremath{\delta}({p}_{\ensuremath{\varphi}}+m),}{{\ensuremath{\alpha}}_{n,l}({p}_{r})={\left(\frac{n}{i{p}_{0}}\right)}^{3l+z}\ensuremath{\Sigma}\stackrel{n\ensuremath{-}l\ensuremath{-}1}{k=0}\left({n\ensuremath{-}l\ensuremath{-}1}{k}\right)\frac{{2}^{k\ensuremath{-}l+1}}{(2l+k+1)(2l+k)\ensuremath{\cdots}(l+k+2)}{\left(\frac{\frac{i{p}_{0}}{n}}{{p}_{r}\ensuremath{-}\frac{i{p}_{0}}{n}}\right)}^{l+k+2},}{{\ensuremath{\beta}}_{l}^{m}({p}_{\ensuremath{\theta}})=\ensuremath{\Sigma}\stackrel{E(\frac{l}{2})}{j=E(\frac{m}{2})}{{a}_{j}{p}_{\ensuremath{\theta}}}^{\ensuremath{-}\frac{(m+1)}{2}}{J}_{\frac{j\ensuremath{-}(m\ensuremath{-}1)}{2}}({p}_{\ensuremath{\theta}}),}$ where $\ensuremath{\delta}$ is the Dirac delta function and ${p}_{0}=Z{a}_{0}^{\ensuremath{-}1}$ (${a}_{0}$ is the Bohr radius). ${J}_{\ensuremath{\nu}}({p}_{0})$ are Bessel functions of integer or half-integer order. The radial functions are shown to have poles up to order $n+1$ at ${p}_{r}=i\frac{{p}_{0}}{n}$.

DOI
10.1103/physreva.22.797

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The wave functions for the hydrogen atom are determined in the momentum representation, using momentum variables pr{p}_{r}pr​, p\ensuremathθ{p}_{\ensuremath{\theta}}p\ensuremathθ​, p\ensuremathφ{p}_{\ensuremath{\varphi}}p\ensuremathφ​ which are associated with the spherical polar variables rrr, t(=ei\ensuremathπcos\ensuremathθ)t(={e}^{i\ensuremath{\pi}cos\ensuremath{\theta}})t(=ei\ensuremathπcos\ensuremathθ) and v(ei\ensuremathφ)v({e}^{i\ensuremath{\varphi}})v(ei\ensuremathφ). The functions may be written as \ensuremathφn,l,m(pr,p\ensuremathθ,p\ensuremathφ)=\ensuremathαn,l(pr)\ensuremathβlm(p\ensuremathθ)\ensuremathδ(p\ensuremathφ+m),\ensuremathαn,l(pr)=(nip0)3l+z\ensuremathΣk=0n\ensuremath−l\ensuremath−1(n\ensuremath−l\ensuremath−1k)2k\ensuremath−l+1(2l+k+1)(2l+k)\ensuremath⋯(l+k+2)(ip0npr\ensuremath−ip0n)l+k+2,\ensuremathβlm(p\ensuremathθ)=\ensuremathΣj=E(m2)E(l2)ajp\ensuremathθ\ensuremath−(m+1)2Jj\ensuremath−(m\ensuremath−1)2(p\ensuremathθ),{{\ensuremath{\varphi}}_{n,l,m}({p}_{r},{p}_{\ensuremath{\theta}},{p}_{\ensuremath{\varphi}})={\ensuremath{\alpha}}_{n,l}({p}_{r}){\ensuremath{\beta}}_{l}^{m}({p}_{\ensuremath{\theta}})\ensuremath{\delta}({p}_{\ensuremath{\varphi}}+m),}{{\ensuremath{\alpha}}_{n,l}({p}_{r})={\left(\frac{n}{i{p}_{0}}\right)}^{3l+z}\ensuremath{\Sigma}\stackrel{n\ensuremath{-}l\ensuremath{-}1}{k=0}\left({n\ensuremath{-}l\ensuremath{-}1}{k}\right)\frac{{2}^{k\ensuremath{-}l+1}}{(2l+k+1)(2l+k)\ensuremath{\cdots}(l+k+2)}{\left(\frac{\frac{i{p}_{0}}{n}}{{p}_{r}\ensuremath{-}\frac{i{p}_{0}}{n}}\right)}^{l+k+2},}{{\ensuremath{\beta}}_{l}^{m}({p}_{\ensuremath{\theta}})=\ensuremath{\Sigma}\stackrel{E(\frac{l}{2})}{j=E(\frac{m}{2})}{{a}_{j}{p}_{\ensuremath{\theta}}}^{\ensuremath{-}\frac{(m+1)}{2}}{J}_{\frac{j\ensuremath{-}(m\ensuremath{-}1)}{2}}({p}_{\ensuremath{\theta}}),}\ensuremathφn,l,m​(pr​,p\ensuremathθ​,p\ensuremathφ​)=\ensuremathαn,l​(pr​)\ensuremathβlm​(p\ensuremathθ​)\ensuremathδ(p\ensuremathφ​+m),\ensuremathαn,l​(pr​)=(ip0​n​)3l+z\ensuremathΣk=0n\ensuremath−l\ensuremath−1(n\ensuremath−l\ensuremath−1k)(2l+k+1)(2l+k)\ensuremath⋯(l+k+2)2k\ensuremath−l+1​(pr​\ensuremath−nip0​​nip0​​​)l+k+2,\ensuremathβlm​(p\ensuremathθ​)=\ensuremathΣj=E(2m​)E(2l​)​aj​p\ensuremathθ​\ensuremath−2(m+1)​J2j\ensuremath−(m\ensuremath−1)​​(p\ensuremathθ​), where \ensuremathδ\ensuremath{\delta}\ensuremathδ is the Dirac delta function and p0=Za0\ensuremath−1{p}_{0}=Z{a}_{0}^{\ensuremath{-}1}p0​=Za0\ensuremath−1​ (a0{a}_{0}a0​ is the Bohr radius). J\ensuremathν(p0){J}_{\ensuremath{\nu}}({p}_{0})J\ensuremathν​(p0​) are Bessel functions of integer or half-integer order. The radial functions are shown to have poles up to order n+1n+1n+1 at pr=ip0n{p}_{r}=i\frac{{p}_{0}}{n}pr​=inp0​​.
The probability density that an electron have certain momenta is given by the square of the absolute magnitude of a momentum eigenfunction ${\ensuremath{\Upsilon}}_{\mathrm{nlm}}(P, \ensuremath{\Theta}, \ensuremath{\Phi})$, in which PPP, $\ensuremath{\Theta}$, and $\ensuremath{\Phi}$ are spatial polar coordinates of the total momentum vector referred to the same axes as the coordinates rrr, $\ensuremath{\theta}$, and $\ensuremath{\varphi}$ of the electron. The following general expression for these functions for a hydrogen-like atom is obtained: ${\ensuremath{\Upsilon}}_{\mathrm{nlm}}(P, \ensuremath{\Theta}, \ensuremath{\Phi})=\left\{\frac{1}{{(2\ensuremath{\pi})}^{\frac{1}{2}}}{e}^{\ifmmode\pm\else\textpm\fi{}\mathrm{im}\ensuremath{\Phi}}\right\} \left\{{\left(\frac{(2l+1)(l\ensuremath{-}m)!}{2(l+m)!}\right)}^{\frac{1}{2}}{{P}_{l}}^{m}(cos\ensuremath{\Theta})\right\}$ $\left\{\frac{\ensuremath{\pi}{2}^{2l+4}l!}{{(\ensuremath{\gamma}h)}^{\frac{3}{2}}}{\left(\frac{n(n\ensuremath{-}l\ensuremath{-}1)!}{(n+l)!}\right)}^{\frac{1}{2}}\frac{{\ensuremath{\zeta}}^{l}}{{({\ensuremath{\zeta}}^{2}+1)}^{l+2}}{C}_{n\ensuremath{-}l\ensuremath{-}1}^{l+1}\left(\frac{{\ensuremath{\zeta}}^{2}\ensuremath{-}1}{{\ensuremath{\zeta}}^{2}+1}\right)\right\}$ in which $\ensuremath{\zeta}=(\frac{2\ensuremath{\pi}}{\ensuremath{\gamma}h})P$, with $\ensuremath{\gamma}=(\frac{4{\ensuremath{\pi}}^{2}\ensuremath{\mu}{e}^{2}Z}{n{h}^{2}})=(\frac{Z}{n{a}_{0}})$. The probability ${\ensuremath{\Xi}}_{\mathrm{nl}}(P)\mathrm{dP}$ that the electron have a total momentum lying within the limits PPP and P+dPP+dPP+dP is also evaluated, and it is shown that the root mean square of the total momentum is equal to the momentum of the electron in a circular Bohr orbit with the same total quantum number.
A novel realization of the classical SU(2) algebra is introduced for the Dirac relativistic hydrogen atom defining a set of operators that allow the factorization of the problem. An extra phase is needed as a new variable in order to define the algebra. We take advantage of the operators to solve the Dirac equation using algebraic methods. A similar path to the one used in the angular momentum case is used; hence, the radial eigenfunctions so calculated comprise nonunitary representations of the algebra. One of the interesting properties of such nonunitary representations is that they are not labeled by integer nor by half-integer numbers, as occurs in the usual angular momentum representation.
The radial form of Hylleraas’ equation for the hydrogen atom, Λl‖El〉=4ℏ4a−2‖El〉 (a=Bohr radius), is considered and it is shown that the operator Λl can be factorized. Hence ladder operators P±l are derived that are linear in the position operator r and are nonlinear functions of the momentum operator p. It is proven that P±l‖El〉 =2ℏ2a−1[1+(l+ (1)/(2) ± (1)/(2) )2 ×(2Mℏ−2a2E)]1/2‖E,l±1〉. In the momentum representation of wave mechanics the solutions to these equations are the radial momentum-space wavefunctions for the hydrogen atom. Thus a simple method of calculating these wavefunctions is obtained. The results complement the familiar operator solution for the hydrogen atom that is based on factorization of the radial Hamiltonian and yields operators that are linear in p and are nonlinear functions of r.