{ "id": "hep-ph/9310349", "version": "v1", "published": "1993-10-26T03:47:52.000Z", "updated": "1993-10-26T03:47:52.000Z", "title": "Closing the Windows on Mev Tau Neutrinos", "authors": [ "K. S. Babu", "T. M. Gould", "I. Z. Rothstein" ], "comment": "8 pgs. LaTeX (1 uuencoded fig., also available on request), Bartol-930XXX, JHU-TIPAC-930026, UM-TH-93-26", "journal": "Phys.Lett.B321:140-144,1994", "doi": "10.1016/0370-2693(94)90340-9", "categories": [ "hep-ph" ], "abstract": "In this note, we analyze various constraints on the ``visible'' decay modes of a massive $\\tau $ neutrino, $\\nu_\\tau\\rightarrow\\nu^\\prime\\,\\gamma $ and $\\nu_\\tau\\rightarrow\\nu^\\prime\\, e^+ e^-$, where $\\nu^\\prime$ is a light neutrino. The BEBC beam dump experiment provides model-independent constraints on these modes. The lifetime for the $\\nu^\\prime\\, e^+e^-$ mode is constrained to be $\\tau_{\\nu^\\prime\\, e^+e^-} \\ge 0.18~(m_{\\nu_\\tau}/MeV)~sec.$ We point out that the same experiment implies a similar constraint on the $\\nu^\\prime\\,\\gamma$ mode. This results in a new upper limit on the transition magnetic moment of $\\nu_\\tau$, $\\mu_{\\rm tran} \\le 1.1 \\times 10^{-9} (MeV/m_{\\nu_\\tau})^2 \\mu_B $. Furthermore, a limit on the electric charge of $\\nu_\\tau$ may be obtained, $Q_{\\nu_\\tau} \\le 4 \\times 10^{-4}e$. Combining these constraints with those arising from supernova observations and primordial nucleosynthesis calculations, we show that these ``visible'' decays cannot be the dominant decay modes of the $\\tau$ neutrino.", "revisions": [ { "version": "v1", "updated": "1993-10-26T03:47:52.000Z" } ], "analyses": { "keywords": [ "mev tau neutrinos", "constraint", "bebc beam dump experiment", "transition magnetic moment", "primordial nucleosynthesis calculations" ], "tags": [ "journal article" ], "note": { "typesetting": "LaTeX", "pages": 0, "language": "en", "license": "arXiv", "status": "editable", "inspire": 359417 } } }