6.9k citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- Centre National de la Recherche ScientifiqueFR336 papers
- ETH ZurichCH215 papers
- Petersburg Nuclear Physics InstituteRU204 papers
- Massachusetts Institute of TechnologyUS182 papers
- European Organization for Nuclear ResearchCH168 papers
- Institut National de Physique Nucléaire et de Physique des ParticulesFR167 papers
- University of GenevaCH163 papers
- Hungarian Academy of SciencesHU159 papers
- California Institute of TechnologyUS145 papers
- Paul Scherrer InstituteCH143 papers
- University of BolognaIT143 papers
- University of MichiganUS143 papers
5 papers · 2 filters
Yukawa ratio predictions in non-renormalizable GUT models
Stefan Antusch, Christian Hohl, Vasja Susič
Since GUTs unify all fermions of the Standard Model plus a right-chiral neutrino in a representation per family, they have the potential to be maxim…
Comparatively Light Extra Higgs States as Signature of SUSY GUTs with 3rd Family Yukawa Unification
Stefan Antusch, Christian Hohl, Vasja Susic
We study rd family Yukawa unification in the context of supersymmetric (SUSY) GUTs and -motivated boundary conditions for the SUSY-breaking so…
Lepton-Trijet and Displaced Vertex Searches for Heavy Neutrinos at Future Electron-Proton Colliders
Stefan Antusch, Oliver Fischer, A. Hammad
Electron proton (ep) colliders could provide particle collisions at TeV energies with large data rates while maintaining the clean and pile~up-free environment of lepton colliders,…
Dark Matter Spin Characterisation in Mono- Channels
W. Abdallah, A. Hammad, S. Khalil +1
The Supersymmetric Standard Model (BLSSM) is an ideal testing ground of the spin nature of Dark Matter (DM) as it offers amongst its candidates both a spin-1/2 (the lightest…
Properties of oscillons in hilltop potentials: energies, shapes, and lifetimes
Stefan Antusch, Francesco Cefala, Francisco Torrenti
Oscillons are spatially localised strong fluctuations of a scalar field. They can e.g. form after inflation when the scalar field potential is shallower than quadratic away from th…