Levinson's theorem

Levinson's theorem is an important theorem of scattering theory. In non-relativistic quantum mechanics, it relates the number of bound states in channels with a definite orbital momentum to the difference in phase of a scattered wave at infinite and zero momenta. It was published by Norman Levinson in 1949.

{{cite journal |last1 = Levinson |first1=N. |year=1949 |title= On the uniqueness of the potential in a Schrödinger equation for a given asymptotic phase

|journal= Danske Vid. Selsk., Mat.-Fys. Medd. |volume=25 |issue=9|

page= 29 |zbl=0032.20702 |url=https://zbmath.org/?q=an:0032.20702 }}

The theorem applies to a wide range of potentials that increase limitedly at zero distance and decrease sufficiently fast as the distance grows.

Statement of theorem

The difference in the \ell-wave phase shift of a scattered wave at infinite momentum, \varphi(+\infty), and zero momentum, \varphi(0), for a spherically symmetric potential V(r) is related to the number of bound states n_b by:

: \varphi(+\infty) - \varphi(0) = - \pi \left( \frac{1}{2}n_{0} + n_{b} \right) ,

where n_{0} = 0 or 1.

The scenario n_{0} = 1 is uncommon and can only occur in s-wave scattering, if a bound state with zero energy exists. The following conditions are sufficient to guarantee the theorem:A. Galindo and P. Pascual, Quantum Mechanics II (Springer-Verlag, Berlin, Germany, 1990).

: V(r) continuous in (0,+\infty) except for a finite number of finite discontinuities,

: V(r) = O(r^{ -3/2 + \varepsilon}) ~\text{ as } ~r\rightarrow 0, ~~\varepsilon>0,

: V(r) = O(r^{ -3 - \varepsilon}) ~\text{ as } ~r \rightarrow \infty, ~~\varepsilon>0.

Generalizations of Levinson's theorem include tensor forces, nonlocal potentials, and relativistic effects.

In relativistic scattering theory, essential information about the system is contained in the Jost function, whose analytical properties are well defined and can be used to prove and generalize Levinson's theorem. The presence of Castillejo, Dalitz and Dyson (CDD) poles

{{cite journal | first1 = L. | last1 = Castillejo| first2 = R. H. | last2 = Dalitz| first3 = F. J. | last3 = Dyson| year = 1956 |

title= Low's Scattering Equation for the Charged and Neutral Scalar Theories | journal = Phys. Rev. | volume = 101 | pages = 453–458 | issue = 1

| doi = 10.1103/physrev.101.453| bibcode = 1956PhRv..101..453C}}

and Jaffe and Low primitives

{{cite journal |last1=Jaffe |first1=R. L. |author1-link=Robert Jaffe (physicist) |author2-link=Francis E. Low |last2=Low |first2=F. E. |year=1979 |title=Connection between quark-model eigenstates and low-energy scattering |journal=Phys. Rev. D |volume=19 |issue=7| page=2105 |doi=10.1103/PhysRevD.19.2105 |bibcode=1979PhRvD..19.2105J }}

which correspond to zeros of the Jost function at the unitary cut modifies the theorem. In general case, the phase difference at infinite and zero particle momenta is determined by the number of bound states, n_{b} ,

the number of primitives, n_{p} , and the number of CDD poles, n_{\text{CDD}} :

{{cite journal |last1=Krivoruchenko |first1=M. I. |last2=Tyrin |first2=K. S. |year=2021 |title= Generalization of the Levinson Theorem on the Asymptotic Value of the Scattering-Amplitude Phase Shift |journal=Physics of Atomic Nuclei |volume=84 |issue=1| pages=29–33 |doi=10.1134/S1063778821010130|arxiv=2006.09366 |bibcode=2021PAN....84...29K }}

: \varphi(+\infty) - \varphi(0) = - \pi \left( \frac{1}{2}n_{0} + n_{b} + n_{p} - n_{\text{CDD}}\right) .

The bound states and primitives give a negative contribution to the phase asymptotics, while the CDD poles give a positive contribution. In the context of potential scattering, a decrease (increase) in the scattering phase shift due to greater particle momentum is interpreted as the action of a repulsive (attractive) potential. The following universal properties of the Jost function, \omega_J (s) , are essential to guarantee the generalized theorem:

: \omega_J(s) an analytic function of the square of energy, s , in the center-of-mass frame of the scattered particles with a cut from threshold to infinity, n_b simple zeros below the threshold, n_p simple zeros above the threshold, and n_{\text{CDD}} simple poles on the real axis. The zeros correspond to bound states and primitives in a fixed channel with total angular momentum J .

References

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