Knowing how long a free neutron can last outside a nucleus is important to our understanding of the fundamental structure of matter. It could also show if there are other fundamental particles yet to be discovered.
“The neutron lifetime is key to answering several big questions in cosmology and particle physics, for our understanding of the crucial early state of the universe and the behavior of fundamental particles,” Wilson said.
The neutron lifetime is the easiest and most direct way of measuring the weak force, one of just four fundamental forces in nature. The weak force governs certain types of radioactive decay, including the natural breakdown of lone neutrons into a proton, electron and antineutrino. It even kicks off the nuclear fusion reaction that powers the Sun and other stars.
The problem is nobody can agree on how long a free neutron can last. Since the early 1990s, researchers have tried two lab-based methods to determine the time: the so-called “bottle” method, which traps neutrons in a bottle and tracks how long they take to radioactively decay, and the “beam” method, which fires a beam of neutrons and scores the number of protons created by radioactive decay.
The bottle method says the lifetime is 14 minutes and 39 seconds. The beam method says the lifetime is nine seconds longer, at 14 minutes and 48 seconds. And although scientists suspect there’s a systematic error in one or both methods, nobody can deduce what that error is.
Space-based measurements offer an alternative, independent method from lab-based experiments, said Jacob Kegerreis, a physicist at Durham University and a study co-author. “[It] may be a way to resolve the current conflict on which method is the most reliable.”
Scientists have suggested various forms of space-based measurements to determine the neutron lifetime since 1959, but Wilson, Kegerreis and the team were the first to show it could be done.
Their method relies on neutrons released into space by cosmic rays colliding with atoms on a planet’s surface or in its atmosphere. The farther the neutrons travel from the planet’s surface, the more time passes and the more neutrons decay. By collecting neutrons at various altitudes and comparing that data with a model of neutron production, transport and detection from that planetary body, scientists can estimate the neutron lifetime. Last year’s results from MESSENGER data at Venus and Mercury showed a neutron lifetime of about 13 minutes.
Because of several systematic errors, however (such as the encounter being just 45 minutes along a quirky orbit and the uncertainty about Venus’ and Mercury’s elemental composition, which is critical to knowing how many neutrons would decay before reaching the spacecraft), that data was limited. So, the group turned to Lunar Prospector neutron data that was collected during its first two days of operation in orbit around the Moon.
“There’s a lot that we know about the Moon compared with Venus and especially Mercury,” Kegerreis said. “Combined with the multiple orbits we could use of Lunar Prospector around the Moon compared with the one-off flyby we had for MESSENGER past Venus, that made this new result significantly more accurate and reliable.”