The Next-to-Minimal Supersymmetric Standard Model
By Ulrich Ellwanger, Cyril Hugonie, A. Teixeira. 2009
660 citations recorded by the source corpus.
Abstract We review the theoretical and phenomenological aspects of the Next-to-Minimal Supersymmetric Standard Model: the Higgs sector including radiative corrections and the 2-loop β -functions for all parameters of the general NMSSM; the tadpole and domain wall problems, baryogenesis; NMSSM phenomenology at colliders, B physics and dark matter; specific scenarios as the constrained NMSSM, gauge mediated supersymmetry breaking, U ( 1 ) ′ -extensions, CP and R-parity violation.
Subfields: Atomic and Molecular Physics, and Optics, Nuclear and High Energy Physics, Political Science and International Relations
View Paper: https://www.semanticscholar.org/paper/70e1b410149c2fcabc193a4cd942ca139008c1d8
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In Atomic and Molecular Physics, and Optics
In Nuclear and High Energy Physics
- Andrei Linde
- R. Kallosh
- Sergio Ferrara
- A. Proeyen
- Alessio Marrani
- Ulrich Ellwanger
- Zhaoxia Heng
- Jin Min Yang
In Political Science and International Relations
Citations in the corpus
- A non Standard Model Higgs at the LHC as a sign of naturalness (2011, background): “sides the case of an MSSM Higgs, two other cases: 1) MSSM with extra D-terms (DMSSM), where an extra quartic term for the Higgs is generated by an additional gauge sector that is broken above the electroweak scale [26], and 2) NMSSM [27](λSUSY [28, 29]), where the extra contribution to the Higgs mas”
- A SM-like Higgs near 125 GeV in low energy SUSY: a comparative study for MSSM and NMSSM (2012, methodology): “Compared with the MSSM, the Higgs sector in the NMSSM is rather complex, which can be seen from its superpotential and the corresponding soft-breaking terms given by [29, 30]”
- On naturalness of the MSSM and NMSSM (2012, neutral): “[29] and references therein.”
- Di-photon excess illuminates dark matter (2015, background): “ which we take to be a singlet of the Standard Model. Extra singlets are indeed ubiquitous in many scenarios of Beyond the Standard Model (BSM) physics, motivated either by naturalness considerations [38,39] or by dark matter physics [40{43]. Taking the large width constraint (1.3) at face value, it”
- WIMP dark matter candidates and searches—current status and future prospects (2017, background): “1;M 2;˛v u;v d. { 35 { The most popular extension of the MSSM is arguably the Next-to-Minimal Supersymmetric Standard Model (NMSSM), which can provide an elegant solution to the problem (see, e.g., [459] for a comprehensive review). In the NMSSM there is one additional kind of neutralino, the singli”
- A Higgs boson near 125 GeV with enhanced di-photon signal in the NMSSM (2011, methodology): “However, the lighter doublet-like CP-even state (corresponding to the SM-like Higgs boson HSM) can mix strongly with the real part of S and form eigenstates with reduced couplings to gauge bosons, quarks and leptons [15, 16, 19, 20, 22–30].”