Understand
Many beyond the Standard Model theories include a stable dark matter candidate that yields missing / invisible energy in collider detectors.
- If observed at the Large Hadron Collider, we must determine if its mass and other properties (and those of its partners) predict the correct dark matter relic density.
- We give a new procedure for determining its mass with small error.
Built on
B. C. Allanach et al
2000
Earlier work this paper cites.
B. C. Allanach et al
2001
Earlier work this paper cites.
B. K. Gjelsten, D. J. Miller and P. Osland, JHEP 0412
2004
Earlier work this paper cites.
Similar
K. Kawagoe, M. M. Nojiri and G. Polesello, Phys. Rev. D 71
2005
Cited alongside, same era.
D. J. Miller, P. Osland and A. R. Raklev, JHEP 0603
2006
Cited alongside, same era.
In a follow-up study, C. G. Lester discussed a likelihood method using all 5 mass shell constraints, which is in Part X of B. C. Allanach et al
Cited in the paper.
W. S. Cho, K. Choi, Y. G. Kim and C. B. Park, arXiv:0709.0288 [hep-ph]
Cited in the paper.
M. M. Nojiri, G. Polesello and D. R. Tovey, arXiv:0712.2718 [hep-ph]
Cited in the paper.
H. C. Cheng, D. Engelhardt, J. F. Gunion, Z. Han and B. McElrath, in preparation
Cited in the paper.
Cited in the paper.
Then
T. Sjostrand, S. Mrenna and P. Skands, JHEP 0605
2006
Later among the works it cites.
H. C. Cheng, J. F. Gunion, Z. Han, G. Marandella and B. McElrath, JHEP 0712
2007
Later among the works it cites.
Beyond the bibliography
alphaXiv searches the wider corpus for related work and actual follow-ups.
alphaXiv is searching for related work…