Comparative half-life 2026-10-18
The product of a dimensionless beta-decay statistical phase-space factor and the partial half-life for the transition. The tabulated normally means . Factoring out this approximate phase space dependence allows comparisons of nuclear weak matrix elements. Strong superallowed Fermi transitions have small ; forbidden beta decays generally have larger values, with nuclear-structure exceptions and overlaps between categories.
Past exam of the particle and nuclear physics course of the University of Cambridge 2017 3 Solution 2026-10-18
Alpha lifetimes and competing beta decays. The Geiger-Nuttall law follows approximately from quantum tunnelling through the daughter’s Coulomb barrier. Increasing shortens the barrier and greatly increases the decay rate; increasing the daughter charge makes the barrier harder to penetrate. A useful local parametrization isUsing the supplied nuclear masses, no electron-mass subtraction is needed for alpha decay. The calculated Q values areCalibrate the two constants to the two supplied even-even thorium half-lives. Their daughter charges are both 88, soThis gives the order-of-magnitude estimatesHere . The known beta-minus decay rates are approximately and , respectively. Thus the reference alpha branching fractions are only about and . Beta decay overwhelmingly removes the parents before alpha emission, explaining why the alpha branches are not seen in the stated chain.
These estimates are local extrapolations, not precision predictions. In particular, actinium is odd-odd, so extrapolating an even-even Geiger-Nuttall law neglects nuclear-structure and angular-momentum hindrance. Such effects can further suppress its alpha branch.
Allowed daughter spin and parity. The even-even parent in its ground state and the alpha particle both have . The total final angular momentum must be zero, so coupling daughter spin to relative orbital momentum requires . Parity conservation gives . The alpha-decay angular-momentum and parity selection rule is thereforeThese are the natural parity states. Restricting the list to even spin would be too strong; even-spin rotational bands are a further structural specialization.
Ground-state line and recoil. The nuclear alpha-decay recoil correction givesFor the thorium ground-state decay, this predicts , with daughter recoil about . This is close to the highest measured line, : the difference is , or . Conversely that line implies . The quoted nuclear masses have only five decimal places in atomic mass units; rounding three such entries can shift their mass difference by up to about . Thus the requested approximate agreement is supported, but the rounded table does not reproduce the line energy exactly. Dropping daughter recoil would give an error around instead.
Excited levels. Relative to the highest line, the two alpha-energy deficits are and . Multiplying by the common recoil factor givesA deformed even-even nucleus has a ground-state nuclear rotational band with and . Its to excitation ratio is , with the observed ratio about below this ideal value. The likely assignments are therefore and rotational excitations, with modest departures from a rigid constant-inertia rotor. The ratio supports this interpretation; it is not a unique spin measurement by itself.
Sargent comparison. For beta-minus decay using nuclear masses, subtract the emitted electron rest mass:The simple version of Sargent's rule would predictThe measured rate ratio is the inverse half-life ratio,The naive fifth-power estimate is about times larger. It correctly predicts the much faster actinium decay but fails quantitatively. The small radium endpoint is far below the electron rest mass, violating the negligible-mass approximation behind the fifth power; Coulomb distortion of the emitted electron, different nuclear matrix elements and different daughter excitations also matter. The rounded mass difference makes the very small radium especially uncertain. The appropriate comparison of individual branches uses the actual endpoint-dependent statistical factor and comparative half-life, not a universal fifth power of the ground-state release.
Beta selection rules and the four observed branches. The radium parent has , so the ground-state transition is a unique forbidden beta decay of second order: it preserves parity and requires three units of angular momentum. For the increasing daughter excitation energies, the endpoints decrease. The assignments areFor , zero lepton orbital angular momentum and lepton-pair spin one give an allowed beta decay of Gamow-Teller transition type. The branches need odd lepton orbital angular momentum, with lowest value one, and are forbidden beta decays of first order; they are not unique because they do not have the maximal transfer at that order.
The absence of a listed ground-state branch is consistent with its stronger forbiddenness. The two allowed branches carry in total, and the nearly equal-endpoint pair favours the allowed branch by four to one. These trends support the classification. However, first-forbidden branches still carry , and the lower-endpoint first-forbidden branch is stronger than the higher-endpoint one. Thus selection-rule labels alone do not explain all intensities: nuclear overlaps and the endpoint-dependent phase space are indispensable. “Forbidden” means suppressed at leading order, not impossible.
Use the leading lepton-orbital classification of a beta decay transition. For lepton-pair orbital angular momentum , Fermi transitions have pair spin and total lepton angular momentum ; Gamow-Teller transitions have and . Addition of angular momentum requireswhile the nuclear parity change requires . The least allowed gives the order: means an allowed beta decay, and an th-forbidden beta decay. Fermi-type and Gamow-Teller-type below refer to these spin-independent and spin-dependent contributions, including their higher-orbital generalizations.
- For , the nuclear spin changes by and parity is unchanged. An lepton pair cannot carry ; would have the wrong parity. At , Fermi transitions can carry , and Gamow-Teller transitions can carry , including the permitted transfers and . Therefore this is a second-forbidden, nonunique transition, with both Fermi-type and Gamow-Teller-type contributions permitted. The quantum numbers do not determine their actual relative matrix elements.
- For , and parity is unchanged. Already carries . The operator for a Fermi transition has rank zero and cannot connect these unequal nuclear spins. This is an allowed Gamow-Teller transition. The decrease of atomic number makes the nuclear conversion proton-to-neutron; the angular momentum classification applies to either the energetically available beta-plus decay or electron capture branch.
- For , requires transfer and a parity change. The lowest possible orbital order is . The pair for a Fermi transition then has only , whereas the pair for a Gamow-Teller transition can attain . Thus this is a first-forbidden unique Gamow-Teller-type transition. Here unique means the maximal transfer at the leading orbital order, as in a unique forbidden beta decay.
- For , permits the scalar operator for a Fermi transition with . The allowed Gamow-Teller transition operator has rank one, and the triangle rule excludes . Interpreting the printed logarithm in the usual comparative half-life convention gives
In the order listed, the concise classification is