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20002017
most citedA comparison of the Higgs sectors of the CMSSM and NMSSM for a 126 GeV Higgs boson

35 citations · 118 across the 7 of their papers we have counts for

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hep-ph2017★ 23 cited

Can we discover a light singlet-like NMSSM Higgs boson at the LHC?

C. Beskidt, W. de Boer, D. I. Kazakov

In the next-to minimal supersymmetric standard model (NMSSM) one additional singlet-like Higgs boson with small couplings to standard model (SM) particles is introduced. Although t…

hep-ph2014★ 12 cited

The impact of a 126 GeV Higgs on the neutralino mass

C. Beskidt, W. de Boer, D. I. Kazakov

We highlight the differences of the dark matter sector between the constrained minimal supersymmetric SM (CMSSM) and the next-to-minimal supersymmetric SM (NMSSM) including the 126…

hep-ph2013★ 35 cited

A comparison of the Higgs sectors of the CMSSM and NMSSM for a 126 GeV Higgs boson

C. Beskidt, W. de Boer, D. I. Kazakov

The recent discovery of a Higgs-like boson at the LHC with a mass of 126 GeV has revived the interest in supersymmetric models, which predicted a Higgs boson mass below 130 GeV lon…

hep-ph2008★ 6 cited

Long-lived Charginos in the Focus-point Region of the MSSM Parameter Space

A. V. Gladyshev, D. I. Kazakov, M. G. Paucar

We analyse the possibility to get light long-lived charginos within the framework of the MSSM with gravity mediated SUSY breaking. We find out that this possibility can be realized…

hep-ph2001★ 29 cited

The b->sgamma rate and Higgs boson limits in the Constrained Minimal Supersymmetric Model

W. de Boer, M. Huber, A. V. Gladyshev +1

New NLO b->sgamma calculations have become available using resummed radiative corrections. Using these calculations we perform a global fit of the supergravity inspired constrained…

hep-ph2000★ 1 cited

The b->sgamma decay rate in NLO, Higgs boson limits, and LSP masses in the CMSSM

W. de Boer, M. Huber, A. Gladyshev +1

New NLO b->sgamma calculations have become available. We observe that at large tanbeta the dominant NLO term of the chargino amplitude, which is proportional to mu.tanbeta^2, chang…