2019:groups:bsm:rdm
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2019:groups:bsm:rdm [2019/06/23 15:39] benjamin.fuks FeynRules/UFO/CalcHep model files are available |
2019:groups:bsm:rdm [2019/06/23 15:40] benjamin.fuks |
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| * The provided mathematica notebook has been used to generate {{ 2019:groups:bsm:lqdm.ufo.tgz | UFO}} and {{ 2019:groups:bsm:lqdm.ch.tgz | CalcHep}} model files. | * The provided mathematica notebook has been used to generate {{ 2019:groups:bsm:lqdm.ufo.tgz | UFO}} and {{ 2019:groups:bsm:lqdm.ch.tgz | CalcHep}} model files. | ||
| * Here is a {{ 2019:groups:bsm:note_benj.pdf | note }} detailing what has been implemented. The {{ 2019:groups:bsm:note_benj.tex | TeX }} version is also available. | * Here is a {{ 2019:groups:bsm:note_benj.pdf | note }} detailing what has been implemented. The {{ 2019:groups:bsm:note_benj.tex | TeX }} version is also available. | ||
| - | * **The model still needs to be double-checked by an independent pair of eyes!** | + | * Important message from Benj: **The model still needs to be double-checked by an independent pair of eyes!** |
| 2- RD explained by mS1=2 TeV, and both lq couplings being 1. (From D. Marzocca). Anomaly explained by lambda_bv * lambda_ctau / mS1^2. | 2- RD explained by mS1=2 TeV, and both lq couplings being 1. (From D. Marzocca). Anomaly explained by lambda_bv * lambda_ctau / mS1^2. | ||
2019/groups/bsm/rdm.txt ยท Last modified: 2019/06/27 17:19 by jose.zurita
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