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Insertion of STC into TRT at the Department of Physics, Oxford
Credit: CERN

David Wark

Professor of Particle Physics

Sub department

  • Particle Physics

Research groups

  • Accelerator Neutrinos
dave.wark@physics.ox.ac.uk
Telephone: 01865 (2)73400
Denys Wilkinson Building, room 626
  • About
  • Publications

Particle physics: Wobbly oscillations.

Nature 447:7140 (2007) 43-46
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No neutrinos is good news

Nature Physics Springer Nature 1:3 (2005) 137-138
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Neutrinos: ghosts of matter

Physics World IOP Publishing 18:6 (2005) 29-36
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Another route to cp violation beyond the SM – The neutron EDM

Proceedings of Science 21 (2005)

Authors:

M Van Der Grinten, CA Baker, K Green, PS Iaydjiev, SN Ivanov, DL Wark, DD Doyle, PG Harris, DJR May, JM Pendlebury, DJ Richardson, DB Shiers, KF Smith, P Geltenbort

Abstract:

The neutron electric dipole moment (EDM) experiment at the Institut Laue-Langevin (ILL) has completed data taking and subsequently the systematic errors have been evaluated. In this paper the experimental technique is discussed and results of the experiment are given. The experiment is based on a precision measurement of the Larmor precession frequency of neutrons in a magnetic field and employs a cohabiting mercury magnetometer. We have reached a final statistical precision of 1.5 × 10-26 e cm, the systematic potential for error, dominated by geometric phase shifts due to magnetic field inhomogeneities in the experiment, is found to be of the same order as the statistical precision obtained.

Neutrino mass measurements.

Philosophical transactions. Series A, Mathematical, physical, and engineering sciences 361:1812 (2003) 2527-2551

Abstract:

Before we can be sure we have a dark-matter problem we have to first be certain that no known particle can account for the missing matter. The last possibility has long been the neutrino, which, while massless in the Standard Model of particle physics, is the second most numerous particle in the Universe (after the photon) and thus (if massive) a potential source of substantial unaccounted for mass. Recent neutrino oscillation measurements have, in fact, confirmed that the Standard Model is incomplete and that neutrinos have mass. However, recent measurements have confirmed that the resulting mass is insufficient for neutrinos to make up the bulk of the dark matter. In fact, observations of the matter distribution in the Universe are now competing with laboratory measurements in their sensitivity to the absolute masses of neutrinos. The article discusses all these measurements and gives some guesses about where we may get in our measurements of neutrino masses in the future.
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