scholarly journals Dark-matter pair production at the ILC in the littlest Higgs model with T -parity

2013 ◽  
Vol 37 (3) ◽  
pp. 033103
Author(s):  
Qing-Peng Qiao ◽  
Bin Xu
2010 ◽  
Author(s):  
Pedro Schwaller ◽  
George Alverson ◽  
Pran Nath ◽  
Brent Nelson
Keyword(s):  

2012 ◽  
Author(s):  
Ramona Groeber ◽  
Margarete Muehlleitner

2004 ◽  
Vol 70 (1) ◽  
Author(s):  
Liu Jing-Jing ◽  
Ma Wen-Gan ◽  
Li Gang ◽  
Zhang Ren-You ◽  
Hou Hong-Sheng

2008 ◽  
Vol 77 (7) ◽  
Author(s):  
Ethan M. Dolle ◽  
Shufang Su
Keyword(s):  

2012 ◽  
Vol 27 (07) ◽  
pp. 1250024
Author(s):  
DAPENG YANG ◽  
BINGFANG YANG ◽  
BIN XU

In the framework of the Left–Right Twin Higgs model, we studied the bottom-quark pair production via e+e- collision at the International Linear Collider. We calculated the bottom-quark pair production cross-section at tree level and the relevant differential distributions. The relative correction of the production cross-section is significant and the result will be a sensitive probe of the Left–Right Twin Higgs model.


2014 ◽  
Vol 89 (11) ◽  
Author(s):  
Shou-Jian Xiong ◽  
Wen-Gan Ma ◽  
Lei Guo ◽  
Chong Chen ◽  
Ren-You Zhang
Keyword(s):  

2009 ◽  
Vol 2009 (12) ◽  
pp. 027-027 ◽  
Author(s):  
A Freitas ◽  
P Schwaller ◽  
D Wyler
Keyword(s):  

2008 ◽  
Vol 23 (24) ◽  
pp. 2011-2022 ◽  
Author(s):  
DEBASISH MAJUMDAR ◽  
AMBAR GHOSAL

We investigate direct detection rates for Dark Matter candidates arise in a SU (2)L× U (1)Y with an additional doublet Higgs proposed by Barbieri, Hall and Rychkov. We refer to this model as "Heavy Higgs Model". The Standard Model Higgs mass comes out from this model is very heavy, so there is very slim chance that there is no Higgs boson mass below 200 GeV. The additional Higgs boson develops neither any VEV due to the choice of coefficient of the scalar potential of the model nor it has any coupling with fermions due to the incorporation of a discrete parity symmetry. Thus, the neutral components of the extra doublet are stable and can be considered as probable candidate of Cold Dark Matter. We have made calculations for three different types of Dark Matter experiments, namely, 76 Ge (like GENIUS), DAMA (NaI) and XENON (131 Xe ). Also demonstrated the annual variation of Dark Matter detection in case of all three


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