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by Pravegaa Education
Chapter 15

Scattering Theory

15.1  Classical Scattering in a Central Field

  • The force vanishes at large distances; energy and angular momentum are conserved.

  • Incident beam: intensity (flux) \(I\) = particles crossing unit area normal to the beam per unit time.

  • Near the centre the orbit bends (attraction or repulsion) and then again becomes a straight line.

Figure
  • Differential cross section: \(D(\Omega)\,d\Omega=\dfrac{N(\Omega)}{I}\), \(N\) = particles scattered into \(d\Omega\) per unit time; dimensions of area.

  • Impact parameter \(b\): perpendicular distance between the centre and the incident line. \(E=\frac12mv_0^2\), \(l=mv_0b=b\sqrt{2mE}\).

  • \(E\) and \(b\) fix the scattering angle \(\Theta\); particles through the ring \(2\pi b\,db\) go into \(2\pi\sin\Theta\,d\Theta\): \[D(\Theta)=\frac{b}{\sin\Theta}\Big|\frac{db}{d\Theta}\Big|,\qquad \sigma=\int D\,d\Omega.\]

  • Orbit symmetric about periapsis: \(\Theta=\pi-2\psi\) and \[\Theta(b)=\pi-2\int_0^{u_m}\frac{b\,du}{\sqrt{1-\dfrac{V(u)}{E}-b^2u^2}},\qquad u=\frac1r.\]

Rutherford scattering

  • Coulomb force \(F=\dfrac{zz'e^2}{r^2}\): hyperbolic orbit, eccentricity \(\varepsilon=\sqrt{1+\big(\frac{2Eb}{zz'e^2}\big)^2}\), and \(\sin\frac\Theta2=\frac1\varepsilon\): \[b=\frac{zz'e^2}{2E}\cot\frac\Theta2,\qquad D(\Theta)=\Big(\frac{zz'e^2}{4E}\Big)^2\frac{1}{\sin^4(\Theta/2)}.\]

  • Total \(\sigma\) diverges (long-range force).

Example 15.1   Hard sphere

Classical scattering off a hard sphere of radius \(R\).

Solution

  • Reflection law: \(2\alpha+\Theta=\pi\), \(b=R\sin\alpha=R\cos\frac\Theta2\).

  • \(D=\dfrac{R\cos(\Theta/2)}{\sin\Theta}\cdot\dfrac R2\sin\dfrac\Theta2=\dfrac{R^2}{4}\) (isotropic).

  • \(\sigma=\dfrac{R^2}{4}\cdot4\pi=\pi R^2\) — the geometric cross section.

Figure

Example 15.2   Distance of closest approach

A particle with speed \(v_0\) and impact parameter \(b\) approaches a repulsive centre \(F=k/r^2\). Find the closest distance \(R\).

Solution

  • Energy: \(\frac12mv_0^2=\frac kR+\frac12mv^2\); angular momentum: \(v_0b=vR\).

  • \(R^2-\dfrac{2k}{mv_0^2}R-b^2=0\Rightarrow R=\dfrac{k}{mv_0^2}+\sqrt{\Big(\dfrac{k}{mv_0^2}\Big)^2+b^2}\).

Example 15.3   Pion capture cross section

A pion of kinetic energy \(T\) hits a nucleus (charge \(Ze\), radius \(R\)) if it reaches \(r\le R\). Show \(\sigma=\pi R^2\big(1-\frac VT\big)\) for \(\pi^+\) and \(\pi R^2\big(1+\frac VT\big)\) for \(\pi^-\), \(V=\frac{Ze^2}{R}\).

Solution

  • Grazing orbit: \(\sqrt{2mT}\,b=mR\,v_R\) and \(T=\pm V+\frac12mv_R^2\).

  • \(b^2=R^2\,\dfrac{T\mp V}{T}\) \(\Rightarrow\sigma=\pi b^2=\pi R^2\Big(1\mp\dfrac VT\Big)\) (upper sign \(\pi^+\)).

Example 15.4   Counting scattered particles

\(\dfrac{d\sigma}{d\Omega}=a^2+b^2\cos^2\theta\), incident flux \(N\). Particles scattered per unit time?

Solution

  • \(\sigma=2\pi\displaystyle\int_0^\pi(a^2+b^2\cos^2\theta)\sin\theta\,d\theta=4\pi\Big(a^2+\frac{b^2}{3}\Big)\) \(\Rightarrow N\sigma=4\pi N\Big(a^2+\dfrac{b^2}{3}\Big)\).

15.2  Quantum-Mechanical Scattering

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