The experiment monitored the decay of
cobalt-60 (60Co) atoms that were aligned by a uniform magnetic field (the polarizing field) and cooled to near
absolute zero so that thermal motions did not randomize the alignment. Cobalt-60 is an
unstable isotope of cobalt that decays by
beta decay to an
excited state of the isotope
nickel-60 (60Ni). During this decay, one of the
neutrons in the cobalt-60 nucleus decays to a
proton by emitting an
electron (e−) and an
electron antineutrino (e). The resulting excited nickel nucleus promptly decays to its ground state by emitting two
gamma rays (γ) in quick succession. Hence the overall nuclear equation of the reaction is: : {}^{60}_{27}\text{Co} \rightarrow {}^{60}_{28}\text{Ni} + \text{e}^{-} + \bar{\nu}_e + 2{\gamma} Using a magnetic field to orient the cobalt-60 nuclei in one direction and using a reversed field to orient the nuclei in the opposite direction places the detectors in opposite hemispheres with respect to the nuclear spin. If the pattern of electron emission (beta rays) differs in these two conditions, parity is not conserved. . The gamma rays also play a crucial role in the experiment. Gamma rays are photons, and their release from the nickel-60 nucleus is an
electromagnetic process. This is significant because electromagnetism was known to respect parity conservation, and therefore the gamma-ray emission pattern should be independent of changes in parity. The gamma rays are emitted in a distribution peaked around the two directions of the cobalt-60 nuclear spin axis: the degree to which the gamma rays were
not distributed perfectly equally in all directions (the "anisotropy" of their distribution) can be used to determine how well the cobalt-60 nuclear spins had been aligned. Spin alignment is necessary to observe the anisotropy in the electron emission. If the cobalt-60 nuclei were randomly oriented, the experiment would detect equal numbers of electrons emitted in every direction. The experiment then counted the rate of emission of electrons along the magnetic field, and of gamma rays along the magnetic field and perpendicularly to it. These rates were then compared with the polarizing field oriented in the opposite direction. If the electron counting rates differed significantly for the two field orientations, there would be strong evidence that the weak interaction does violate parity conservation. In addition, the experiment was monitored over time as the apparatus slowly warmed up. The gamma ray anisotropy, measured in the direction of the magnetic field (polar direction) and perpendicular to this (equatorial direction) slowly vanished, indicating loss of
spin polarization with increasing temperature. The observed asymmetry of the electron counts in the two directions of the polarizing field should track the gamma ray anisotropy results.
Materials and methods The experimental challenge in this experiment was to obtain a high directional orientation or
polarization of the 60Co nuclei. For normal materials in spin state the fraction of polarization is proportional to the magnet moment of the nuclei, \mu, the applied field, and inversely proportional to temperature: f_N = \frac{1}{3}\frac{I+1}{I}\frac{\mu H}{kT}. Due to the very small magnetic moments of the nuclei, a magnetic field of about () is required at extremely low temperatures (around 0.01 K), a combination that is very difficult to achieve. In a
paramagnetic element the unpaired 3d or 4f electrons create a strong magnetic field, about (), at the nucleus. In that case, the fractional polarization becomes proportional to the fractional polarization of the electrons but is otherwise independent of the applied field. Thus for nuclei with magnetic moments in a paramagnetic material, aligning the electrons with a strong magnetic field has the side effect of aligning the nuclei. The concept can be paired with
adiabatic demagnetization, in which a paramagnetic salt is placed in an external magnetic field and heat caused by the alignment of the electrons is extracted by pumping the liquid helium to low pressure, giving a temperature 1.2 K. When the external field is removed, randomization of the electron spins cools the salt. A temperature of 0.01 K can be achieved by this process. Thus internal paramagnetism is manipulated to both cool the sample and provide the field to align the nuclei. This concept became known as the Rose–Gorter method. As was demonstrated by the NBS team in 1953, high nuclear polarization can be obtained even at low fields by using an anisotropic paramagnetic crystal like
cerium magnesium nitrate, a paramagnetic salt still favored for
magnetic refrigeration. Aligning the magnetically sensitive axis of the crystal horizontally allows a horizontal magnetic field to provide adiabatic cooling, while minimizing any reheating due to a vertical field used during the measurement phase of the experiment. The Wu team deposited radioactive cobalt as a 0.05 mm (0.002 in) layer on the surface of the cerium magnesium nitrate crystal, providing thermal bonding to allow the cooling of the crystal to cool the outer cobalt layer. The central bore of the horizontal refrigeration magnet was opened up to allow room for a vertical solenoid to be introduced. It would align the spin axis of the cobalt nuclei vertically, with a direction of spin that is determined by the direction of the field. A thin
anthracene crystal acting as a
scintillator was placed just above the cobalt-coated CeMg-nitrate crystal. Beta electrons exiting the cobalt layer and striking the anthracene produce a tiny light pulse, which was transmitted to a photomultiplier on the top of the apparatus via a lucite light pipe. The production of gamma-rays was monitored using equatorial and polar
scintillators and photomultipliers. The difference in counting rate between these location measures gamma-ray anisotropy. This anisotropy was continuously monitored over the next quarter-hour as the crystal warmed up and the anisotropy decreased. Likewise, beta-ray emissions were continuously monitored during this warming period. Then the entire process was repeated with the solenoid field reversed, creating the equivalent of a mirror image inversion.
Results The Wu paper reported a "large" beta-emission asymmetry between the two directions of nuclear spin polarization. This was sufficient to show that parity was not conserved, which was the key result of the paper. Specifically they found that "the emission of beta particles is more favored in the direction opposite to that of the nuclear spin". A quantitative value is more helpful for theoretical comparisons. As shown by Yang and Lee in the appendix to their theory paper, the weak interaction
Hamiltonian without parity conservation predicts an interference between parity-conserving and parity-non-conserving terms. The emitted electron angular distribution as a function of the angle
θ between the nuclear spin and the electron momentum vector would follow W(\theta) = 1 + A P \frac{v}{c}\cos\theta defines an asymmetry parameter . Here the polarization, of the nuclear spin, , is defined as P = \frac{\langle I_z\rangle}{I} and
v/
c is the ratio of the emitted electron speed to the
speed of light. The experiment only measured the angular distribution in two opposite directions along the magnetic field direction and observed a value of −0.25 for the subexpression in the expression above for the distribution: A P \frac{v}{c} = \frac{W(0) - W(\pi)}{W(0) + W(\pi)} = -0.25 The measurements gave and, from the gamma ray anisotropy, the polarization was 0.65. With these values and a correction for backscattering of electrons from the bulk crystal, the asymmetry comes out to −1. The paper would only claim a "lower limit" to the beta asymmetry of −0.7. This value was obtained by comparing the observed electron measurements to the gamma-ray measurements as well as other adjustments. Among the systematic checks, the observed electron asymmetry did not change sign when the horizontal field used for magnetic cooling was reversed, meaning that the asymmetry was not being caused by
remanent magnetization in the samples. Wu and her team had observed that the electrons were emitted in a direction preferentially opposite to that of the nuclear spin. Later refinements of the experiment established an asymmetry value was . == Mechanism and consequences ==