Testing the AMSB Model via $e^+e^- \to \tildeχ^+ \tildeχ^- γ$}

Physics – High Energy Physics – High Energy Physics - Phenomenology

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

10pages, Latex style, 4 figs, revised version

Scientific paper

10.1016/S0370-2693(01)00672-4

The possibility of detecting the signature of a nearly invisible charged wino ($\CH$) decaying into a soft pion and the LSP($\LSP$), predicted by the Anomaly Mediated Symmetry Breaking model, via the process $e^+e^-\r\gamma{\tilde\chi}^{+}{\tilde\chi}^{-}$ at the Next Linear Collider has been explored. Using the recently, proposed bounds on slepton and wino masses derived from the condition of stability of the electroweak symmetry breaking vacuum and employing some standared kinematical cuts to supress the background, we find that almost the whole of the allowed parameter space with the slepton mass less than 1 TeV, can be probed at $\sqrt{s}$ 500 GeV. Determination of the slepton and the chargino masses from this signal is a distinct possiblity. Any violation of the above mass bound will suggest that the standard vacuum is unstable and we are living in a false vacuum.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Testing the AMSB Model via $e^+e^- \to \tildeχ^+ \tildeχ^- γ$} does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Testing the AMSB Model via $e^+e^- \to \tildeχ^+ \tildeχ^- γ$}, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Testing the AMSB Model via $e^+e^- \to \tildeχ^+ \tildeχ^- γ$} will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-626487

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.