scholarly journals Classification of dark pion multiplets as dark matter candidates and collider phenomenology

2020 ◽  
Vol 2020 (2) ◽  
Author(s):  
Hugues Beauchesne ◽  
Giovanni Grilli di Cortona
2009 ◽  
Vol 2009 (09) ◽  
pp. 078-078 ◽  
Author(s):  
Chuan-Ren Chen ◽  
Mihoko M Nojiri ◽  
Seong Chan Park ◽  
Jing Shu ◽  
Michihisa Takeuchi

2013 ◽  
Vol 28 (34) ◽  
pp. 1330031 ◽  
Author(s):  
JENNIFER KILE

The current status of flavored dark matter (DM) is reviewed. We discuss the main experimental constraints on models of flavored DM and survey some possible considerations which are relevant for the constructions of models. We then review the application of existing flavor principles to DM, with an emphasis on minimal flavor violation, and discuss implications of flavored DM on collider phenomenology.


2021 ◽  
Author(s):  
Martin Stref ◽  
Thomas Lacroix ◽  
Gaétan Facchinetti ◽  
Judit Pérez-Romero ◽  
Julien LAVALLE ◽  
...  
Keyword(s):  

2007 ◽  
Vol 453 (2-4) ◽  
pp. 29-115 ◽  
Author(s):  
Dan Hooper ◽  
Stefano Profumo

2021 ◽  
Vol 2021 (4) ◽  
Author(s):  
Nicole F. Bell ◽  
Matthew J. Dolan ◽  
Leon S. Friedrich ◽  
Michael J. Ramsey-Musolf ◽  
Raymond R. Volkas

Abstract We examine the collider and dark matter phenomenology of the Standard Model extended by a hypercharge-zero SU(2) triplet scalar and gauge singlet scalar. In particular, we study the scenario where the singlet and triplet are both charged under a single ℤ2 symmetry. We find that such an extension is capable of generating the observed dark matter density, while also modifying the collider phenomenology such that the lower bound on the mass of the triplet is smaller than in minimal triplet scalar extensions to the Standard Model. A high triplet mass is in tension with the parameter space that leads to novel electroweak phase transitions in the early universe. Therefore, the lower triplet masses that are permitted in this extended model are of particular importance for the prospects of successful electroweak baryogenesis and the generation of gravitational waves from early universe phase transitions.


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