2019:groups:bsm:rdm
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2019:groups:bsm:rdm [2019/06/27 08:27] benjamin.fuks |
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| 1- Expand existing UFO for dark matter: add yD coupling. Make it Micromegas friendly by including tildes for dark particles (see below for details on the model). In charge:JB, DS | 1- Expand existing UFO for dark matter: add yD coupling. Make it Micromegas friendly by including tildes for dark particles (see below for details on the model). In charge:JB, DS | ||
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| - | **From Benj:** | ||
| * FeynRules implementation (v2) + toy mathematica notebook: {{ 2019:groups:bsm:lqdm.fr.v2.tgz | here}}. | * FeynRules implementation (v2) + toy mathematica notebook: {{ 2019:groups:bsm:lqdm.fr.v2.tgz | here}}. | ||
| * CalcHEP/UFO v2 files: {{ 2019:groups:bsm:lqdm.ch.v2.tgz | CH}} and {{ 2019:groups:bsm:lqdm.ufo.v2.tgz | UFO}}. | * CalcHEP/UFO v2 files: {{ 2019:groups:bsm:lqdm.ch.v2.tgz | CH}} and {{ 2019:groups:bsm:lqdm.ufo.v2.tgz | UFO}}. | ||
2019/groups/bsm/rdm.txt ยท Last modified: 2019/06/27 17:19 by jose.zurita
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