Abstract

We find that the difference between ${N}_{\ensuremath{\nu}}=\frac{{\ensuremath{\Gamma}}_{\mathrm{inv}}}{{\ensuremath{\Gamma}}_{\overline{\ensuremath{\nu}}\ensuremath{\nu}}^{\mathrm{SM}}}$ and ${\overline{N}}_{\ensuremath{\nu}}=\frac{{\ensuremath{\Gamma}}_{\mathrm{inv}}}{{\ensuremath{\Gamma}}_{\overline{l}l}}\frac{{\ensuremath{\Gamma}}_{\overline{l}l}^{\mathrm{SM}}}{{\ensuremath{\Gamma}}_{\overline{\ensuremath{\nu}}\ensuremath{\nu}}^{\mathrm{SM}}}$ can be used as an indicator of possible extensions of the standard model. This test will be possible, however, only after the top-quark mass measurement. We illustrate our point by an example of a left-right symmetric model with the Higgs sector containing one bidoublet and two triplets and the additional assumption that there is no fine-tuning in neutrino Yukawa couplings. If this is the case, the difference between ${N}_{\ensuremath{\nu}}$ and ${\overline{N}}_{\ensuremath{\nu}}$ could be a test for the bidoublet contents, assuming that nonstandard radiative corrections are negligible.

Full Text
Paper version not known

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 call

Disclaimer: 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.