Constraining the Neutrino Mass Using Cyclotron Radiation Emission Spectroscopy

dc.contributor.advisorRybka, Gray
dc.contributor.authorAshtari Esfahani, Ali
dc.date.accessioned2020-10-26T20:45:31Z
dc.date.available2020-10-26T20:45:31Z
dc.date.issued2020-10-26
dc.date.submitted2020
dc.descriptionThesis (Ph.D.)--University of Washington, 2020
dc.description.abstractThe existing prototype to demonstrate the viability of the Cyclotron Radiation Emission Spectroscopy (CRES) has been upgraded to incorporate tritium compatibility. The spectrum of the conversion electrons from $^{83m}Kr$ has been measured with great linearity and a precision of $2 \ eV$ over the energy range of $17-32 \eV$. The first tritium beta-spectrum using CRES has also been measured to conclude an endpoint value of $E_0 = 18574.1 \pm (17.2)_{stat.} + \left(^{+12.5}_{-21.1}\right)_{sys.} \ eV$. The recorded tritium spectrum is analyzed to set the first CRES limit on the neutrino mass, $m_\beta \ < 146 \ eV \ \ (90\% \ C.L.)$.
dc.embargo.termsOpen Access
dc.format.mimetypeapplication/pdf
dc.identifier.otherAshtariEsfahani_washington_0250E_22209.pdf
dc.identifier.urihttp://hdl.handle.net/1773/46557
dc.language.isoen_US
dc.rightsnone
dc.subjectCyclotron Radiation Emission Spectroscopy (CRES)
dc.subjectNeutrino Mass
dc.subjectPhysics
dc.subject.otherPhysics
dc.titleConstraining the Neutrino Mass Using Cyclotron Radiation Emission Spectroscopy
dc.typeThesis

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