2006/06/21 by B. R. Heckel, Claire Cramer, C. E. Cramer +6 · 13 citations
Physics and Astronomy · #Dark Matter and Cosmic Phenomena #Neutrino Physics Research #Noncommutative and Quantum Gravity Theories #hep-ph
paper · pdf · doi:10.1103/physrevlett.97.021603
published as Phys.Rev.Lett.97:021603,2006 · 4 figures, accepted for publication in Physical Review Letters
arxiv created 2006/06/21 · openalex publication_date 2006/07/12 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/07/28
We used a torsion pendulum containing \ensuremath∼9\ifmmode×\else\texttimes\fi1022 polarized electrons to search for CP-violating interactions between the pendulum's electrons and unpolarized matter in the laboratory's surroundings or the Sun, and to test for preferred-frame effects that would precess the electrons about a direction fixed in inertial space. We find |gPegSN|/(\ensuremathℏc)<1.7\ifmmode×\else\texttimes\fi10^\ensuremath-36 and |gAegVN|/(\ensuremathℏc)<4.8\ifmmode×\else\texttimes\fi10^\ensuremath-56 for \ensuremathλ>1 AU. Our preferred-frame constraints, interpreted in the Kosteleck'y framework, set an upper limit on the parameter |\stackrel\texttildelow\mathbitbe|\ensuremath≤5.0\ifmmode×\else\texttimes\fi10^\ensuremath-21 eV that should be compared to the benchmark value me2/MPlanck=2\ifmmode×\else\texttimes\fi10^\ensuremath-17 eV.