Colored resonant signals at the LHC: largest rate and simplest topology
By T. Han, I. Lewis, Zhen Liu. 2010
172 citations recorded by the source corpus.
We study the colored resonance production at the LHC in a most general approach. We classify the possible colored resonances based on group theory decomposition, and construct their effective interactions with light partons. The production cross section from annihilation of valence quarks or gluons may be on the order of 400–1000 pb at LHC energies for a mass of 1 TeV with nominal couplings, leading to the largest production rates for new physics at the TeV scale, and simplest event topology with dijet final states. We apply the new dijet data from the LHC experiments to put bounds on various possible colored resonant states. The current bounds range from 0.9 to 2.7 TeV. The formulation is readily applicable for future searches including other decay modes.
Subfields: Artificial Intelligence, Nuclear and High Energy Physics
View Paper: https://www.semanticscholar.org/paper/bfd32ba111f984d245929fe93b862a5899d5c513
How researchers see this paper
The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.
In Artificial Intelligence
- Cms Collaboration
- Gudrun Heinrich
- Jean-Roch Vlimant
- Valentin Hirschi
- P. Nason
- Ansgar Denner
- L. Harland–Lang
- Juan Rojo
In Nuclear and High Energy Physics
- Cms Collaboration
- Atlas Collaboration
- Gudrun Heinrich
- Ansgar Denner
- Stefan Kallweit
- Stefan Dittmaier
- M. Grazzini
- Juan Rojo
Citations in the corpus
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- Search for narrow and broad dijet resonances in proton-proton collisions at $\sqrt{s}=$ 13 TeV and constraints on dark matter mediators and other new particles (2018, background): “Limits are compared to predicted cross sections for string resonances [23, 24], excited quarks [26, 27], axigluons [28], colorons [29], scalar diquarks [25], color-octet scalars [30], new gauge bosons W′ and Z′ with SM-like couplings [32], dark matter mediators for mDM = 1 GeV [34, 35], and RS gravi”
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