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We establish the feasibility of measuring the neutron lifetime via an alternative, space-based class of methods, which use neutrons generated by galactic cosmic ray spallation of planets surfaces and atmospheres. Free neutrons decay via the weak interaction with a mean lifetime of around 880 s. This lifetime constrains the unitarity of the CKM matrix and is a key parameter for studies of Big-Bang nucleosynthesis. However, current laboratory measurements, using two independent approaches, differ by over 4$sigma$. Using data acquired in 2007 and 2008 during flybys of Venus and Mercury by NASAs MESSENGER spacecraft, which was not designed to make this measurement, we estimate the neutron lifetime to be $780pm60_textrm{stat}pm70_textrm{syst}$ s, thereby demonstrating the viability of this new approach.
We use data from the Lunar Prospector Neutron Spectrometer to make the second space-based measurement of the free neutron lifetime finding $tau_n=887 pm 14_text{stat}{:^{+7}_{-3:text{syst}}}$ s, which is within 1$sigma$ of the accepted value. This me
Free neutrons have a measured lifetime of 880 s, but disagreement between existing laboratory measurements of ~10 s have persisted over many years. This uncertainty has implications for multiple physics disciplines, including standard-model particle
A measurement of the neutron lifetime $tau_{n}$ performed by the absolute counting of in-beam neutrons and their decay protons has been completed. Protons confined in a quasi-Penning trap were accelerated onto a silicon detector held at a high potent
The neutron beta-decay lifetime plays an important role both in understanding weak interactions within the framework of the Standard Model and in theoretical predictions of the primordial abundance of 4He in Big Bang Nucleosynthesis. In previous work
A neutron decays into a proton, an electron, and an anti-neutrino through the beta-decay process. The decay lifetime ($sim$880 s) is an important parameter in the weak interaction. For example, the neutron lifetime is a parameter used to determine th