English

Remarks on the KARMEN Anomaly

High Energy Physics - Phenomenology 2009-09-25 v4 Astrophysics

Abstract

A recently reported anomaly in the time structure of signals in the KARMEN neutrino detector suggests the decay of a new particle xx, produced in π+μ+x\pi^+ \to \mu^+ x with mass mx=33.9m_x=33.9 MeV. We discuss the constraints and difficulties in interpreting xx as a neutrino. We show that a mainly-sterile neutrino scenario is compatible with all laboratory constraints, within narrow limits on the mixing parameters, although there are problems with astrophysical and cosmological constraints. This scenario predicts that appreciable numbers of other xx-decay events with different origins and time structures should also be observable in the KARMEN detector. Such xx-decay events should also be found in the LSND experiment and may be relevant to the search for νˉμνˉe\bar\nu_\mu\to\bar\nu_e oscillations.

Keywords

Cite

@article{arxiv.hep-ph/9503295,
  title  = {Remarks on the KARMEN Anomaly},
  author = {V. Barger and R. J. N. Phillips and S. Sarkar},
  journal= {arXiv preprint arXiv:hep-ph/9503295},
  year   = {2009}
}

Comments

Erratum concerning $x \to e^+ e^- \nu$ decays through FCNC appended to version published in Phys. Lett. B352 (1995) 365. Conclusions broadly unchanged. Latex, 14 pages, 2 postscript figures. Compressed postscript version including figures available at ftp://phenom.physics.wisc.edu/pub/preprints/1995/madph-95-875.ps.Z or at http://phenom.physics.wisc.edu/pub/preprints/1995/madph-95-875.ps.Z

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