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advanced · Physics · Advanced QM: Scattering & Relativistic QM

Phase Shifts

We now turn the partial-wave machinery into an actual number. The cleanest example is the hard sphere: an impenetrable ball of radius aa. It has no free parameters beyond aa, its phase shifts are exact, and it exhibits the famous low-energy result σ=4πa2\sigma = 4\pi a^2.

The radial equation

For a central potential, write ψ=R(r)P(cosθ)\psi = R_\ell(r)\,P_\ell(\cos\theta) and substitute u(r)=rR(r)u_\ell(r) = r R_\ell(r). The radial Schrödinger equation becomes a 1D problem with a centrifugal barrier:

22mu+[V(r)+2(+1)2mr2]u=Eu,u(0)=0.-\frac{\hbar^2}{2m}u_\ell'' + \Big[V(r) + \frac{\hbar^2\,\ell(\ell+1)}{2m r^2}\Big]u_\ell = E\,u_\ell , \qquad u_\ell(0) = 0 .

The phase shift δ\delta_\ell is fixed entirely by how this uu_\ell joins onto the free asymptotic form sin(krπ/2+δ)\sin(kr - \ell\pi/2 + \delta_\ell) at large rr.

Hard sphere, s-wave

Take =0\ell = 0, where the centrifugal term drops out. Outside the sphere (r>ar > a) the potential vanishes, so u0=k2u0u_0'' = -k^2 u_0 and the general solution is

u0(r)=Csin(kr+δ0).u_0(r) = C\,\sin(kr + \delta_0).

The sphere is impenetrable, so the wavefunction must vanish on its surface: u0(a)=0u_0(a) = 0. That single condition gives

sin(ka+δ0)=0  δ0=ka  \sin(ka + \delta_0) = 0 \quad\Longrightarrow\quad \boxed{\;\delta_0 = -ka\;}

(choosing the branch continuous with δ00\delta_0\to 0 as a0a\to 0). The phase shift is negative — the hard core pushes the wave out, a repulsive signature. This result is exact at all energies, not an approximation.

The low-energy cross-section

The s-wave contribution to the total cross-section is

σ0=4πk2sin2δ0=4πk2sin2(ka).\sigma_0 = \frac{4\pi}{k^2}\sin^2\delta_0 = \frac{4\pi}{k^2}\sin^2(ka).

In the low-energy limit ka1ka \ll 1, sin(ka)ka\sin(ka)\approx ka, so

σ0  ka0  4πk2(ka)2=4πa2.\sigma_0 \;\xrightarrow{\,ka\to 0\,}\; \frac{4\pi}{k^2}(ka)^2 = 4\pi a^2 .

This is four times the classical geometric cross-section πa2\pi a^2. The factor of four is purely quantum: at low energy the wave diffracts around the entire sphere, "seeing" its full surface area 4πa24\pi a^2 rather than just its silhouette.

The high-energy crossover

When ka1ka \gg 1, many partial waves contribute and a careful sum gives σ2πa2\sigma \to 2\pi a^2 — twice the geometric cross-section. (The "extra" πa2\pi a^2 beyond classical is a forward diffraction shadow, an unavoidable wave-optics effect.) The hard sphere thus interpolates from 4πa24\pi a^2 at low energy to 2πa22\pi a^2 at high energy, never reaching the naive classical πa2\pi a^2 — a clean illustration that quantum cross-sections are not simple geometric areas.

Try it

For a hard sphere of radius a=1 fma = 1\ \text{fm} probed at k=0.2 fm1k = 0.2\ \text{fm}^{-1}, compute the s-wave phase shift δ0=ka\delta_0 = -ka and the s-wave cross-section σ0=(4π/k2)sin2δ0\sigma_0 = (4\pi/k^2)\sin^2\delta_0. Confirm it is close to 4πa24\pi a^2.

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