Past exam of the particle physics course of the University of Oxford / 2016 / 2

An observable that reverses sign under parity but has a nonzero expectation in a suitably prepared experiment tests parity violation. A polar momentum reverses, whereas an axial spin angular momentum does not. Thus $\mathbf{J}\cdot \mathbf{p}$ and helicity are parity-odd; an apparatus asymmetry must be separated from a physical asymmetry by reversing the preparation or analyser.

In the Wu experiment, polarized cobalt-60 nuclei preferentially emit beta decay electrons in one direction relative to the nuclear spin angular momentum. The distribution contains $A\mathbf{P}\cdot {\mathbf{p}}_e/E_e$; its sign changes under spatial inversion. Reversing the nuclear polarization reverses the observed asymmetry.^[ref]

In the Goldhaber experiment, the sign of the circular polarization of selected gamma rays determines the sign of the neutrino helicity. A preference for negative helicity is parity-odd because spatial inversion would produce the positive-helicity state. This provides a different experimental observable from the electron angular distribution.

The relevant sequence is electron capture followed by nuclear gamma decay:The nuclear spin angular momenta are $0\to 1\to 0$. The captured K-shell electron has total angular momentum $1/2$, so the initial atom-plus-electron system cannot be treated as having zero angular momentum. The atomic vacancy also produces subsequent X-rays or Auger electrons; these are not the selected nuclear transition.

Choose the neutrino momentum along $+z$ and the recoil momentum along $-z$. For a negative-helicity neutrino, $s_{\nu z}=-1/2$. With the two initial electron spin projections, angular momentum conservation allows the daughter to have $m_z=0$ or $+1$. A photon emitted exactly along the recoil direction is transverse, and the $1\to 0$ transition selects the $m_z=+1$ component. Its spin angular momentum points along $+z$, opposite to its momentum.

Thus in the selected collinear geometry the daughter and photon have the same negative helicity as the neutrino, while their spin angular momenta point opposite to the neutrino spin. Reversing all these spin projections gives the positive-helicity alternative. In normalized notation,The actual eigenvalues of $\mathbf{S}\cdot \hat{\mathbf{p}}$ are $\pm 1/2$ for the neutrino and $\pm 1$ for the photon; the equality concerns their normalized signs.

The nuclear gamma ray can be absorbed by ground-state samarium-152, excite the same level and be re-emitted: nuclear nuclear resonance fluorescence. Its energy in the absorber rest frame must overlap the nuclear absorption line within the relevant natural and thermal broadening. Atomic radiation from refilling the K shell does not have the required transition energy.

Let the excitation energy be $E_0$ and the nuclear mass be $M$. A free stationary emitter loses recoil energy while a free stationary absorber requires recoil energy:For $E_0\simeq 0.96\mathrm{MeV}$ the gap is about $6.5\mathrm{eV}$. A photon emitted along the daughter recoil receives a positive Doppler shift of approximately $E_0{p}_{\nu }/(Mc)$, whereas one emitted opposite the recoil is redshifted. Emission before the daughter slows down therefore selects photons roughly opposite to the neutrino. Comparable neutrino and photon energies nearly compensate the recoil mismatch; finite line widths and thermal motion permit overlap. Exact compensation need not hold for every atom, and this is not an assumption of recoil-free emission.

Magnetized iron supplies polarized electrons. Their Compton scattering cross section depends on the relative electron spin and photon helicity, so the iron attenuates the two circular polarizations differently. Reverse the magnetization and measure the resonance-selected count asymmetry $A=(N_{+}-N_{-})/(N_{+}+N_{-})$. With a calibrated analysing power $a$ and background correction, $A=a{P}_{\gamma }$ determines the sign and magnitude of the circular polarization. A scintillation counter such as NaI(Tl), coupled to a photomultiplier, determines the gamma ray energy from calibrated pulse height; a semiconductor detector could perform the same spectroscopic function.

The functional arrangement below separates the polarization analysis from the resonance selection. The shield prevents the direct source beam from overwhelming the detector; the off-axis detector accepts gamma rays re-emitted by the samarium scatterer.

The europium source emits into magnetized iron, whose magnetization is alternated. A samarium scatterer selects nuclear nuclear resonance fluorescence, favouring photons emitted along the daughter recoil. A shielded NaI(Tl) scintillation counter records the scattered nuclear line. Compare the background-subtracted line rates for the two iron magnetizations, and use the calibrated sign of the analysing power to identify the photon helicity.

The measured circular polarization was negative, compatible after angular acceptance corrections with negative neutrino helicity. By the angular momentum conservation argument, the selected photon helicity and neutrino helicity have the same sign. Thus the experiment concludesfor the emitted relativistic electron neutrino. Finite acceptance dilutes the measured polarization; it does not justify equating the raw count asymmetry to $-1$.^[ref]