Understand
We construct a basis for effective operators responsible for interactions between the Standard Model and a dark sector composed of particles with spin less or equal to 1.
- Redundant operators are eliminated using dim-4 equations of motion.
- We consider simple scenarios where the dark matter components are stabilized against decay by Z2 symmetries.
- We determine operators which are loop-generated within an underlying theory and those that are potentially tree-level generated.
Built on
W. Buchmuller and D. Wyler, Nucl. Phys. B 268
1986
Earlier work this paper cites.
H. D. Politzer, Nucl. Phys. B 172
1994
Earlier work this paper cites.
H. Ruegg and M. Ruiz-Altaba, Int. J. Mod. Phys. A 19
2004
Earlier work this paper cites.
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Cited alongside, same era.
S. Bhattacharya, A. Drozd, B. Grzadkowski and J. Wudka, JHEP 1310
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Cited alongside, same era.
Cited in the paper.
Then
2013
Later among the works it cites.
B. Grzadkowski, M. Iskrzynski, M. Misiak and J. Rosiek, JHEP 1010
2013
Later among the works it cites.
2014
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