For partial waves in three dimensions, Levinson's theorem asserts that delta (0)= pi n b , where delta (p) is the phase shift at wavenumber p, and n b the number of bound states ( delta ( infinity )=0 by convention). The corresponding theorem in one dimension calls first for a systematic parametrisation of the transmission amplitude T(p)=cos theta e i tau , and of the left (right)-incidence reflection amplitudes R L,R (p)=i sin theta exp(i tau +or-i rho ), where the phase angles tau , theta , rho are functions of p. If the potential is not everywhere zero, and excluding throughout the exceptional case where it has a zero-energy bound state, heuristic arguments show that R L,R (0)=-1, that theta (0)= 1 / 2 pi (- 1 / 2 pi ) when n b is odd (even), and that tau (0)= pi (n b - 1 / 2 ); (by convention, tau ( infinity )=0= theta ( infinity )). Thus mod tau (0) mod cannot be less than 1 / 2 pi , no matter how weak the potential; the transition to the limit of zero potential is non-uniform. In the special case of reflection-symmetric potentials, rho =0, one can subdivide n b =n b (e) +n b (o) , and define even- and odd-parity phase shifts E= 1 / 2 ( tau + theta ) and Delta = 1 / 2 ( tau - theta ); then E(0)= pi (n b (e) - 1 / 2 ), Delta (0)= pi n b (o) . The appendix shows how E(0) is obtainable by suitably adapting the familiar s-wave argument which exploits the analyticity properties of the Jost solutions.
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G. Barton (1985) studied this question.
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