Abstract
Heavy-Majorana-neutrino production and detection at colliders is examined. Majorana-neutrino decay is shown to be simply calculable from Dirac-neutrino results. Majorana-neutrino production {ital f{bar f}}{r arrow}{ital Z}{r arrow}{ital NN} is calculated and compared to Dirac-neutrino production. Near the threshold, the Dirac cross section rises much more quickly. Far above the threshold, the two types of neutrinos have the same spin-independent cross sections while the spin-dependent cross sections are very different. This difference could be observed in the correlations between the angle and energy dependence of the heavy-neutrino decay products.
Sign-in/Register to access full text options 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
