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Effective Range, Shallow Poles, and Universality Windows

The scattering length is only the first coefficient in the low-energy amplitude. Effective range and shape parameters determine how quickly zero-range universality fails and how a shallow pole’s energy and residue depart from their leading forms. A universality window is therefore a momentum interval, not simply the statement that a|a| is large.

Required background. Short-Range Scattering Data as Many-Body Inputs fixes the amplitude and pole conventions.

Helpful background. Effective Field Theory as a Controlled Expansion explains order-by-order uncertainty.

For elastic ss-wave scattering below the first inelastic threshold,

kcotδ0(k)=1a+12rek2+Pk4+O(k6R5),k\cot\delta_0(k) =-\frac1a+\frac12r_ek^2+P k^4+O(k^6R^5),

and

A(k)=4π/mkcotδ0(k)ik.\mathcal A(k) =\frac{4\pi/m}{k\cot\delta_0(k)-ik}.

Here rer_e is the effective range and PP a shape parameter with dimension length cubed. Analyticity requires kR1kR\ll1, where RR is set by the nearest left-hand singularity or inelastic threshold. A large a|a| does not enlarge this analytic radius.

If the effective-range term is treated perturbatively, its relative size near momentum QQ is approximately QreQ|r_e| at unitarity or reQ2/a1+iQ|r_e|Q^2/|a^{-1}+iQ| more generally. Resumming a truncated effective-range denominator can introduce spurious deep poles; whether to resum is a power-counting decision.

For a bound state put k=iκk=i\kappa, κ>0\kappa>0. Through effective range,

1a12reκ2+κ=0.-\frac1a-\frac12r_e\kappa^2+\kappa=0.

When re/a1|r_e|/a\ll1 and a>0a>0,

κ=1a+re2a2+O ⁣(re2a3,Pa4).\kappa=\frac1a+\frac{r_e}{2a^2} +O\!\left(\frac{r_e^2}{a^3},\frac{P}{a^4}\right).

The derivative of the inverse amplitude fixes the pole residue. In the energy plane it contains the wave-function factor

Zpole11reκ+O(Pκ3).Z_{\mathrm{pole}}\propto\frac{1}{1-r_e\kappa+O(P\kappa^3)}.

Thus matching the pole energy alone does not fix its coupling to external probes. A residue near a singular denominator also warns that higher effective-range terms cannot be neglected.

For a many-body observable characterized by QkFQ\sim k_F, λT1\lambda_T^{-1}, a binding momentum, or a probe momentum, leading zero-range universality requires

QR1,Qre1,Q R\ll1, \qquad Q|r_e|\ll1,

along with any channel-specific conditions. A next-to-leading result retaining rer_e must show that the shape correction PQ3|P|Q^3 is smaller than the required accuracy. Near a narrow resonance re|r_e| can be parametrically larger than the microscopic range, making QreQ|r_e| the limiting parameter.

For finite-range, energy-independent potentials, causality constrains possible effective ranges at a fixed range. Such Wigner-type bounds do not apply unchanged to explicitly energy-dependent or coupled-channel models; the degrees of freedom and regulator must be stated. The analytic and causality restrictions are reviewed in Hammer and Lee 2010, §§II–III.

Suppose the amplitude is used through rer_e. Vary the shape coefficient over a natural range tied to R3R^3, or compare fits with and without the k4k^4 term over the actual energy interval. Propagate the resulting amplitude change through the many-body calculation. Quoting only the experimental error on aa understates the theory error whenever QreQr_e or QRQR is comparable.

Using aR|a|\gg R as the only check. The observable also has a momentum QQ; universality requires QR1QR\ll1.

Resumming a polynomial beyond its domain. A truncated effective-range expression is local information near threshold and can create unphysical remote poles.

Ignoring the residue. Pole energy and pole strength are independent pieces of shallow-state phenomenology once range corrections enter.

Solve the pole equation perturbatively through first order in re/ar_e/a.

Solution

Write κ=a1+δ\kappa=a^{-1}+\delta. Keeping only linear order gives a1(re/2)a2+a1+δ=0-a^{-1}-(r_e/2)a^{-2}+a^{-1}+\delta=0, hence δ=re/(2a2)\delta=r_e/(2a^2).

At unitarity, an observable probes Q=0.1/RQ=0.1/R and re=3Rr_e=3R. Is leading zero range accurate at the ten-percent level?

Solution

QR=0.1QR=0.1, but Qre=0.3Q|r_e|=0.3. Effective-range effects are potentially thirty percent, so leading zero range is not supported at ten-percent accuracy even though the microscopic-range parameter is small.

Two-Channel Resonance Models makes a large effective range dynamical. Efimov Physics and the Three-Body Parameter adds the leading three-body scale. Dimensional Crossover and Confinement-Induced Resonances combines range physics with a geometric spectrum.

  • Hammer, H.-W., and Dean Lee. “Causality and the Effective Range Expansion.” Annals of Physics 325 (2010): 2212–2233. DOI.
  • Bethe, Hans A. “Theory of the Effective Range in Nuclear Scattering.” Physical Review 76 (1949): 38–50. DOI.
  • Braaten, Eric, and Hans-Werner Hammer. “Universality in Few-Body Systems with Large Scattering Length.” Physics Reports 428 (2006): 259–390. DOI.