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20102026
most citedDark Matter Benchmark Models for Early LHC Run-2 Searches: Report of the ATLAS/CMS Dark Matter Forum

411 citations · 756 across the 34 of their papers we have counts for

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hep-ph2017★ 14 cited

Colder Freeze-in Axinos Decaying into Photons

Kyu Jung Bae, Ayuki Kamada, Seng Pei Liew +1

We point out that 7 keV axino dark matter (DM) in the R-parity violating (RPV) supersymmetric (SUSY) Dine-Fischler-Srednicki-Zhitnitsky model can simultaneously reproduce the 3.5ke…

hep-ph2017★ 52 cited

Light Axinos from Freeze-in: production processes, phase space distributions, and Ly- forest constraints

Kyu Jung Bae, Ayuki Kamada, Seng Pei Liew +1

We consider freeze-in production of 7 keV axino dark matter (DM) in the supersymmetric Dine-Fischler-Srednicki-Zhitnitsky (DFSZ) model in light of the 3.5 keV line excess. The warm…

hep-ph2016★ 30 cited

Mono-X Versus Direct Searches: Simplified Models for Dark Matter at the LHC

Seng Pei Liew, Michele Papucci, Alessandro Vichi +1

We consider simplified models for dark matter (DM) at the LHC, focused on mono-Higgs, -Z, or -b produced in the final state. Our primary purpose is to study the LHC reach of a rela…

hep-ph2016★ 63 cited

Effects of QCD bound states on dark matter relic abundance

Seng Pei Liew, Feng Luo

We study scenarios where there exists an exotic massive particle charged under QCD in the early Universe. We calculate the formation and dissociation rates of bound states formed b…

hep-ph2016★ 7 cited

Models of 750 GeV quarkonium and the LHC excesses

Koichi Hamaguchi, Seng Pei Liew

We investigate models involving a vector-like quark X, which forms a 750 GeV bound state and reproduces the observed diphoton signals at the LHC, in connection with other excesses…

hep-ph2015★ 12 cited

Testing ATLAS Diboson Excess with Dark Matter Searches at LHC

Seng Pei Liew, Satoshi Shirai

The ATLAS collaboration has recently reported a 2.6 sigma excess in the search for a heavy resonance decaying into a pair of weak gauge bosons. Only fully hadronic final states are…