Florian Staub
CERN
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Featured researches published by Florian Staub.
Reports on Progress in Physics | 2016
Sergey Alekhin; Wolfgang Altmannshofer; Takehiko Asaka; Brian Batell; Fedor Bezrukov; K. Bondarenko; Alexey Boyarsky; Ki-Young Choi; Cristobal Corral; Nathaniel Craig; David Curtin; Sacha Davidson; André de Gouvêa; Stefano Dell'Oro; Patrick deNiverville; P. S. Bhupal Dev; Herbi K. Dreiner; Marco Drewes; Shintaro Eijima; Rouven Essig; Anthony Fradette; Bjorn Garbrecht; Belen Gavela; Gian Francesco Giudice; Mark D. Goodsell; Dmitry Gorbunov; Stefania Gori; Christophe Grojean; Alberto Guffanti; Thomas Hambye
This paper describes the physics case for a new fixed target facility at CERN SPS. The SHiP (search for hidden particles) experiment is intended to hunt for new physics in the largely unexplored domain of very weakly interacting particles with masses below the Fermi scale, inaccessible to the LHC experiments, and to study tau neutrino physics. The same proton beam setup can be used later to look for decays of tau-leptons with lepton flavour number non-conservation, [Formula: see text] and to search for weakly-interacting sub-GeV dark matter candidates. We discuss the evidence for physics beyond the standard model and describe interactions between new particles and four different portals-scalars, vectors, fermions or axion-like particles. We discuss motivations for different models, manifesting themselves via these interactions, and how they can be probed with the SHiP experiment and present several case studies. The prospects to search for relatively light SUSY and composite particles at SHiP are also discussed. We demonstrate that the SHiP experiment has a unique potential to discover new physics and can directly probe a number of solutions of beyond the standard model puzzles, such as neutrino masses, baryon asymmetry of the Universe, dark matter, and inflation.
Advances in High Energy Physics | 2015
Florian Staub
I give an overview about the features the Mathematica package SARAH provides to study new models. In general, SARAH can handle a wide range of models beyond the MSSM coming with additional chiral superfields, extra gauge groups, or distinctive features like Dirac gaugino masses. All of these models can be implemented in a compact form in SARAH and are easy to use: SARAH extracts all analytical properties of the given model like two-loop renormalization group equations, tadpole equations, mass matrices, and vertices. Also one- and two-loop corrections to tadpoles and self-energies can be obtained. For numerical calculations SARAH can be interfaced with other tools to get the mass spectrum, to check flavour or dark matter constraints, and to test the vacuum stability or to perform collider studies. In particular, the interface to SPheno allows a precise prediction of the Higgs mass in a given model comparable to MSSM precision by incorporating the important two-loop corrections. I show in great detail with the example of the B-L-SSM how SARAH together with SPheno, HiggsBounds/HiggsSignals, FlavorKit, Vevacious, CalcHep, MicrOmegas, WHIZARD, and MadGraph can be used to study all phenomenological aspects of a model.
European Physical Journal C | 2015
Mark D. Goodsell; Kilian Nickel; Florian Staub
We present an extension to the Mathematica package SARAH which allows for Higgs mass calculations at the two-loop level in a wide range of supersymmetric (SUSY) models beyond the MSSM. These calculations are based on the effective potential approach and include all two-loop corrections which are independent of electroweak gauge couplings. For the numerical evaluation Fortran code for SPheno is generated by SARAH. This allows the prediction of the Higgs mass in more complicated SUSY models with the same precision that most state-of-the-art spectrum generators provide for the MSSM.
Computer Physics Communications | 2016
Florian Staub; Peter Athron; Ulrich Ellwanger; Ramona Gröber; Margarete Mühlleitner; P. Slavich; Alexander Voigt
The publicly available spectrum generators for the NMSSM often lead to different predictions for the mass of the standard model-like Higgs boson even if using the same renormalization scheme and two-loop accuracy. Depending on the parameter point, the differences can exceed 5 GeV, and even reach 8 GeV for moderate superparticle masses of up to 2 TeV. It is shown here that these differences can be traced back to the calculation of the running standard model parameters entering all calculations, to the approximations used in the two-loop corrections included in the different codes, and to different choices for the renormalization conditions and scales. In particular, the importance of the calculation of the top Yukawa coupling is pointed out.
Journal of High Energy Physics | 2016
Alberto Salvio; Florian Staub; Alfredo Urbano; Alessandro Strumia
A bstractMotivated by the 750 GeV diphoton excess found at LHC, we compute the maximal width into γγ that a neutral scalar can acquire through a loop of charged fermions or scalars as function of the maximal scale at which the theory holds, taking into account vacuum (meta)stability bounds. We show how an extra gauge symmetry can qualitatively weaken such bounds, and explore collider probes and connections with Dark Matter.
Journal of High Energy Physics | 2015
Mark D. Goodsell; Manuel E. Krauss; Tobias Müller; Werner Porod; Florian Staub
A bstractWe perform the first analysis of Dark Matter scenarios in a constrained model with Dirac Gauginos. The model under investigation is the Constrained Minimal Dirac Gaugino Supersymmetric Standard model (CMDGSSM) where the Majorana mass terms of gauginos vanish. However, R-symmetry is broken in the Higgs sector by an explicit and/or effective Bμ-term. This causes a mass splitting between Dirac states in the fermion sector and the neutralinos, which provide the dark matter candidate, become pseudo-Dirac states. We discuss two scenarios: the universal case with all scalar masses unified at the GUT scale, and the case with non-universal Higgs soft-terms. We identify different regions in the parameter space which fulfill all constraints from the dark matter abundance, the limits from SUSY and direct dark matter searches and the Higgs mass. Most of these points can be tested with the next generation of direct dark matter detection experiments.
Journal of High Energy Physics | 2015
Kilian Nickel; Florian Staub
A bstractWe present a precise analysis of the Higgs mass corrections stemming from vectorlike top partners in supersymmetric models. We reduce the theoretical uncertainty compared to previous studies in the following aspects: (i) including the one-loop threshold corrections to SM gauge and Yukawa couplings due to the presence of the new states to obtain the DR¯
Physics Letters B | 2016
Graham G. Ross; Florian Staub; Kai Schmidt-Hoberg
Physics Letters B | 2015
Herbi K. Dreiner; Kilian Nickel; Florian Staub
\overline{\mathrm{DR}}
Journal of High Energy Physics | 2016
Martin Hirsch; Manuel E. Krauss; Toby Opferkuch; Werner Porod; Florian Staub