2006/06/30 by F. del Águila, F. del Aguila, J. A. Aguilar-Saavedra +2
Physics and Astronomy · #Dark Matter and Cosmic Phenomena #Dirac (video compression format) #MAJORANA #Neutrino #Neutrino Physics Research #Nuclear physics #Particle physics #Particle physics theoretical and experimental studies #Physics #hep-ph
paper · pdf · doi:10.1088/1742-6596/53/1/032
published as J.Phys.Conf.Ser.53:506-527,2006 · LaTeX 32 pages. This review summarises and extends work presented at several conferences. To appear in the proceedings of CORFU2005. References added
arxiv created 2006/07/13 · openalex publication_date 2006/11/01 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
Large colliders are not sensitive to light neutrino masses and character, but they can produce new heavy neutrinos, allowing also for the determination of their Dirac or Majorana nature. We review the discovery limits at the next generation of large colliders.