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Determining the neutrino mass with Cyclotron Radiation Emission Spectroscopy - Project 8

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arxiv 1703.02037 v1 pith:Z4GJYI3R submitted 2017-03-06 physics.ins-det hep-exnucl-ex

Determining the neutrino mass with Cyclotron Radiation Emission Spectroscopy - Project 8

classification physics.ins-det hep-exnucl-ex
keywords massneutrinoexperimentcrestechniquetritiumabsoluteachieve
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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The most sensitive direct method to establish the absolute neutrino mass is observation of the endpoint of the tritium beta-decay spectrum. Cyclotron Radiation Emission Spectroscopy (CRES) is a precision spectrographic technique that can probe much of the unexplored neutrino mass range with $\mathcal{O}({\rm eV})$ resolution. A lower bound of $m(\nu_e) \gtrsim 9(0.1)\, {\rm meV}$ is set by observations of neutrino oscillations, while the KATRIN Experiment - the current-generation tritium beta-decay experiment that is based on Magnetic Adiabatic Collimation with an Electrostatic (MAC-E) filter - will achieve a sensitivity of $m(\nu_e) \lesssim 0.2\,{\rm eV}$. The CRES technique aims to avoid the difficulties in scaling up a MAC-E filter-based experiment to achieve a lower mass sensitivity. In this paper we review the current status of the CRES technique and describe Project 8, a phased absolute neutrino mass experiment that has the potential to reach sensitivities down to $m(\nu_e) \lesssim 40\,{\rm meV}$ using an atomic tritium source.

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    Presents the science case, reference design, and project plan for the CMB-S4 ground-based CMB experiment.