Examination of the calorimetric spectrum to determine the neutrino mass in low-energy electron capture decay
R. G. H. Robertson

TL;DR
This paper examines the calorimetric spectrum in low-energy electron capture decay, highlighting the complexities introduced by multiple vacancy states and satellites, which challenge the precise determination of neutrino mass.
Contribution
It reveals that the calorimetric spectrum's theoretical understanding is more complex than previously thought, especially due to multiple vacancy states and satellites.
Findings
Multiple vacancy states significantly affect the spectrum shape.
Shakeup and shakeoff satellites are present across the spectrum.
Spectrum shape uncertainties hinder sensitive neutrino mass measurements.
Abstract
The standard kinematic method for determining neutrino mass from the beta decay of tritium or other isotope is to measure the shape of the electron spectrum near the endpoint. It has been known for 30 years that a similar distortion of the "visible energy" remaining after electron capture is caused by neutrino mass. There has been a resurgence of interest in using this method with 163-Ho. Recent theoretical analyses offer reassurance that there are no significant theoretical uncertainties. We show that the situation is, however, more complicated, and that the spectrum shape is presently not well enough understood to permit a sensitive determination of the neutrino mass in this way. The theoretical analyses consider only single vacancy states in the daughter 163-Dy atom. It is necessary to consider configurations with more than one vacancy that can be populated owing to the change in…
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