Light Gluino And Tevatroin Dijet Angular Distributions

Details Light Gluino And Tevatroin Dijet Angular Distributions Light Gluino And Tevatroin Dijet Angular Distributions

1997-02-11

arxiv.org/abs/hep-ph/9702301v1

Phys.Lett.B412:86-90,1997

Physics

High Energy Physics

High Energy Physics - Phenomenology

10 pages, LaTeX with 2 epsf figures

Scientific paper

10.1016/S0370-2693(97)01063-0

We consider the effects of a light gluino on the dijet angular distributions in p - pbar collisions at sqrt(s)=1800 GeV. We show that the slower running of alpha_s and the production q qbar, g g -> Gino Gino do not significantly alter the expected angular distributions. On the other hand, single U, D squark production q g -> Q Gino with subsequent Q -> q g results in dijets whose angular distributions are dramatically different from that in SM. The CDF data on dijet angular distributions with integrated luminosity of 106 pb^(-1) exclude U, D squarks in the mass ranges 170 < m < 650 and 190 < m < 600 GeV, We consider lower energies as well and show that in a future experimental analysis for dijet mass below 240 GeV squarks could be observed or ruled out.

Affiliated with

Also associated with

No associations

Rating

Light Gluino And Tevatroin Dijet Angular Distributions 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 Light Gluino And Tevatroin Dijet Angular Distributions, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Light Gluino And Tevatroin Dijet Angular Distributions will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-393220