User Tools

Site Tools


2019:groups:bsm:rdm

Differences

This shows you the differences between two versions of the page.

Link to this comparison view

Both sides previous revision Previous revision
Next revision
Previous revision
Next revision Both sides next revision
2019:groups:bsm:rdm [2019/06/25 16:30]
benjamin.fuks
2019:groups:bsm:rdm [2019/06/27 08:27]
benjamin.fuks
Line 1: Line 1:
 Project Acronym: RDM Project Acronym: RDM
  
-Interested people: Benj, Andreas Goudelis, Genevieve Belanger, Dipan Sengupta, Aoife Bharucha, José Zurita, Jose Miguel No, Jordan Bernigaud, Jan Heisig, Giacomo Polesello, Priscilla Pani, Biplob Bhattacherjee,​ Andre Lessa, Cedric Delaunay+Interested people: Benj, Andreas Goudelis, Genevieve Belanger, Dipan Sengupta, Aoife Bharucha, José Zurita, Jose Miguel No, Jordan Bernigaud, Jan Heisig, Giacomo Polesello, Priscilla Pani, Biplob Bhattacherjee,​ Andre Lessa, Cedric Delaunay, Adil Jueid.
  
 [Feel free to add your name here and edit tasks!] [Feel free to add your name here and edit tasks!]
Line 14: Line 14:
  
 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 
-**From Benj: the yD coupling is included already. What is wrong with it?**+ 
 +**From Benj:** 
 +  * 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}}.
  
 2- Check flavor constraints:​ how much can we relax y^L_{3X}, y^{R}_{23} / mS1^2 = 1/(4 TeV^2)? Interest is to lower mS1 and the couplings as much as possible without colliding with other flavor bounds coming from e.g: D-Dbar mixing (that would apply on combinations of couplings and masses, y^{R}_{23}^2 / mS1^2 ). Persons in charge: MN, JB, AB 2- Check flavor constraints:​ how much can we relax y^L_{3X}, y^{R}_{23} / mS1^2 = 1/(4 TeV^2)? Interest is to lower mS1 and the couplings as much as possible without colliding with other flavor bounds coming from e.g: D-Dbar mixing (that would apply on combinations of couplings and masses, y^{R}_{23}^2 / mS1^2 ). Persons in charge: MN, JB, AB
2019/groups/bsm/rdm.txt · Last modified: 2019/06/27 17:19 by jose.zurita