Abstract

Experimental studies of neutron decay, n→peν[over ¯], exhibit two anomalies. The first is a 8.6(2.1)s, roughly 4σ difference between the average beam measured neutron lifetime, τ_{n}^{beam}=888.0(2.0) s, and the more precise average trapped ultracold neutron determination, τ_{n}^{trap}=879.4(6) s. The second is a 5σ difference between the pre2002 average axial coupling, g_{A}, as measured in neutron decay asymmetries g_{A}^{pre2002}=1.2637(21), and the more recent, post2002, average g_{A}^{post2002}=1.2755(11), where, following the UCNA Collaboration division, experiments are classified by the date of their most recent result. In this Letter, we correlate those τ_{n} and g_{A} values using a (slightly) updated relation τ_{n}(1+3g_{A}^{2})=5172.0(1.1) s. Consistency with that relation and better precision suggest τ_{n}^{favored}=879.4(6) s and g_{A}^{favored}=1.2755(11) as preferred values for those parameters. Comparisons of g_{A}^{favored} with recent lattice QCD and muonic hydrogen capture results are made. A general constraint on exotic neutron decay branching ratios, <0.27%, is discussed and applied to a recently proposed solution to the neutron lifetime puzzle.

Highlights

  • Experimental studies of neutron decay, n → peν, exhibit two anomalies

  • The second is a 5σ difference between the pre2002 average axial coupling, gA, as measured in neutron decay asymmetries gpAre2002 1⁄4 1.2637ð21Þ, and the more recent, post2002, average gpAost2002 1⁄4 1.2755ð11Þ, where, following the UCNA Collaboration division, experiments are classified by the date of their most recent result

  • The neutron lifetime, τn, and its axial-current coupling, gA 1⁄4 GA=GV, are important weak interaction parameters used in nuclear, particle, and astrophysics, as well as cosmology [1,2,3,4,5,6]

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Summary

Alberto Sirlin

The neutron lifetime, τn, and its axial-current coupling, gA 1⁄4 GA=GV, are important weak interaction parameters used in nuclear, particle, and astrophysics, as well as cosmology [1,2,3,4,5,6]. An area of particular importance is the dependence of primordial nucleosynthesis and cosmic microwave background anisotropies on τn and gA [9,10] Despite their central role in weak interaction phenomenology, τn and gA values have changed, sometimes dramatically, with time. The most precise τn and gA experimental measurements have generally been carried out independently of one another, prevailing values at a given time were known to be correlated through the relationship τnð þ 3g2AÞ 1⁄4 constant, with the constant determined by the standard model (SM) neutron decay rate prediction.

Published by the American Physical Society
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