2022
DOI: 10.1016/j.astropartphys.2022.102686
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KATRIN background due to surface radioimpurities

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Cited by 11 publications
(15 citation statements)
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“…The resulting electrons are accelerated by qUana towards the detector, making them indistinguishable from signal electrons [14,18]. The unstable neutral particles are either 219 Rn and 220 Rn emanated from the getter pumps [19,20] or highly excited atoms sputtered off the inner spectrometer surfaces [21][22][23]. The sputtering mechanisms originate from both α-decays of 210 Po in the structural material and a Penning trap (e), which gives rise to accelerated positive ions from the volume between the two spectrometers [24].…”
Section: Methodsmentioning
confidence: 99%
“…The resulting electrons are accelerated by qUana towards the detector, making them indistinguishable from signal electrons [14,18]. The unstable neutral particles are either 219 Rn and 220 Rn emanated from the getter pumps [19,20] or highly excited atoms sputtered off the inner spectrometer surfaces [21][22][23]. The sputtering mechanisms originate from both α-decays of 210 Po in the structural material and a Penning trap (e), which gives rise to accelerated positive ions from the volume between the two spectrometers [24].…”
Section: Methodsmentioning
confidence: 99%
“…Depending on the excitation state of these Rydberg atoms, the ionization electrons will have energies in the meV range. This hypothesis is supported by detailed investigations, including short-term contamination with shorter-lived decay chains from 223 Ra and 228 Th sources [44]. Since the rate of ionization electrons detected depends on the volume imaged by the detector, this background can also be mitigated by the shifted analyzing plane (Sec.…”
Section: Backgroundsmentioning
confidence: 70%
“…As described in Sec. 2.3, our evidence suggests that a significant share of the background electrons in the KATRIN spectrometer originate from highly excited Rydberg atoms, which are ionized by the blackbody radiation emitted from the spectrometer walls at room temperature [44]. These secondary electrons possess very low starting energies [128], but are accelerated by the electric potential gradient of the spectrometer and essentially arrive with the same kinetic energy at the detector as the signal electrons.…”
Section: Active Transverse-energy Filtermentioning
confidence: 76%
“…The simulation considers the energy spectrum of background electrons which are ionized by black-body radiation at room temperature from hydrogen (36 %) and oxygen atoms (64 %) in highly excited Rydberg states. These Rydberg atoms are sputtered from the spectrometer walls due to α-decays of implanted 210 Pb progenies from the 222 Rn decay chain [5]. The Rydberg atom's energies from [6] are corrected for the surface binding energy and -after ionisation -the electron energy and direction are calculated with the Doppler shift of the Rydberg atoms taken into account.…”
Section: Countsmentioning
confidence: 99%
“…This corresponds to a cyclotron radius at the detector of less than 200 µm 2 . In contrast to the signal electrons, a significant share of the background electrons in the KATRIN spectrometer originate from highly excited, so-called Rydberg atoms, which are ionized by black-body radiation emitted from the spectrometer walls at room temperature [5]. These secondary electrons possess very low starting energies [6], but are accelerated by the electric potential gradient of the spectrometer and arrive at the detector with essentially the same kinetic energy as the signal electrons (which in the central region of the spectrometer also possess energies in the eV range).…”
Section: Introductionmentioning
confidence: 99%