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Tritium Beta Spectrum Measurement and Neutrino Mass Limit from Cyclotron Radiation Emission Spectroscopy.

Authors :
Ashtari Esfahani A
Böser S
Buzinsky N
Carmona-Benitez MC
Claessens C
de Viveiros L
Doe PJ
Fertl M
Formaggio JA
Gaison JK
Gladstone L
Grando M
Guigue M
Hartse J
Heeger KM
Huyan X
Johnston J
Jones AM
Kazkaz K
LaRoque BH
Li M
Lindman A
Machado E
Marsteller A
Matthé C
Mohiuddin R
Monreal B
Mueller R
Nikkel JA
Novitski E
Oblath NS
Peña JI
Pettus W
Reimann R
Robertson RGH
Rosa De Jesús D
Rybka G
Saldaña L
Schram M
Slocum PL
Stachurska J
Sun YH
Surukuchi PT
Tedeschi JR
Telles AB
Thomas F
Thomas M
Thorne LA
Thümmler T
Tvrznikova L
Van De Pontseele W
VanDevender BA
Weintroub J
Weiss TE
Wendler T
Young A
Zayas E
Ziegler A
Source :
Physical review letters [Phys Rev Lett] 2023 Sep 08; Vol. 131 (10), pp. 102502.
Publication Year :
2023

Abstract

The absolute scale of the neutrino mass plays a critical role in physics at every scale, from the subatomic to the cosmological. Measurements of the tritium end-point spectrum have provided the most precise direct limit on the neutrino mass scale. In this Letter, we present advances by Project 8 to the cyclotron radiation emission spectroscopy (CRES) technique culminating in the first frequency-based neutrino mass limit. With only a cm^{3}-scale physical detection volume, a limit of m_{β}<155  eV/c^{2} (152  eV/c^{2}) is extracted from the background-free measurement of the continuous tritium beta spectrum in a Bayesian (frequentist) analysis. Using ^{83m}Kr calibration data, a resolution of 1.66±0.19  eV (FWHM) is measured, the detector response model is validated, and the efficiency is characterized over the multi-keV tritium analysis window. These measurements establish the potential of CRES for a high-sensitivity next-generation direct neutrino mass experiment featuring low background and high resolution.

Details

Language :
English
ISSN :
1079-7114
Volume :
131
Issue :
10
Database :
MEDLINE
Journal :
Physical review letters
Publication Type :
Academic Journal
Accession number :
37739382
Full Text :
https://doi.org/10.1103/PhysRevLett.131.102502