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Electroweak Baryogenesis and Dark Matter in the nMSSM
High Energy Physics - Phenomenology · Submitted 21 Apr 2004
abstract compiled · 2026-09-23 · no language-model review
The authors' main claim We demonstrate that a strong, first order electroweak phase transition, necessary for electroweak baryogenesis, may arise in regions of parameter space where the lightest neutralino provides an acceptable dark matter candidate.
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The abstract, sentence by sentence
We examine the possibility of electroweak baryogenesis and dark matter in the nMSSM, a minimal extension of the MSSM with a singlet field. This extension avoids the usual domain wall problem of the NMSSM, and also appears as the low energy theory in models of dynamical electroweak symmetry breaking with a so-called fat-Higgs boson. We demonstrate that a strong, first order electroweak phase transition, necessary for electroweak baryogenesis, may arise in regions of parameter space where the lightest neutralino provides an acceptable dark matter candidate. We investigate the parameter space in which these two properties are fulfilled and discuss the resulting phenomenology. In particular, we show that there are always two light CP-even and one light CP-odd Higgs bosons with masses smaller than about 250 GeV. Moreover, in order to obtain a realistic relic density, the lightest neutralino mass tends to be smaller than $M_Z/2$, in which case the lightest Higgs boson decays predominantly into neutralinos.
background contribution method result interpretation main claim
| # | sentence | role | the authors' own work | states the main conclusion | strength |
|---|---|---|---|---|---|
| s0 | We examine the possibility of electroweak baryogenesis and dark matter in the nMSSM, a minimal extension of the MSSM with a singlet field. | contribution 0.90 | 0.73 | 0.06 | hedged possibility 0.78 |
| s1 | This extension avoids the usual domain wall problem of the NMSSM, and also appears as the low energy theory in models of dynamical electroweak symmetry breaking with a so-called fat-Higgs boson. | background 0.98 | 0.11 | 0.04 | asserted 0.74 |
| s2 | We demonstrate that a strong, first order electroweak phase transition, necessary for electroweak baryogenesis, may arise in regions of parameter space where the lightest neutralino provides an acceptable dark matter candidate. | result 0.96 | 0.93 | 0.64 | hedged possibility 0.91 |
| s3 | We investigate the parameter space in which these two properties are fulfilled and discuss the resulting phenomenology. | contribution 0.94 | 0.88 | 0.07 | asserted 0.53 |
| s4 | In particular, we show that there are always two light CP-even and one light CP-odd Higgs bosons with masses smaller than about 250 GeV. | result 1.00 | 0.93 | 0.19 | asserted 1.00 |
| s5 | Moreover, in order to obtain a realistic relic density, the lightest neutralino mass tends to be smaller than $M_Z/2$, in which case the lightest Higgs boson decays predominantly into neutralinos. | result 0.94 | 0.87 | 0.13 | asserted 0.55 |
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The paper
Original abstract
We examine the possibility of electroweak baryogenesis and dark matter in the nMSSM, a minimal extension of the MSSM with a singlet field. This extension avoids the usual domain wall problem of the NMSSM, and also appears as the low energy theory in models of dynamical electroweak symmetry breaking with a so-called fat-Higgs boson. We demonstrate that a strong, first order electroweak phase transition, necessary for electroweak baryogenesis, may arise in regions of parameter space where the lightest neutralino provides an acceptable dark matter candidate. We investigate the parameter space in which these two properties are fulfilled and discuss the resulting phenomenology. In particular, we show that there are always two light CP-even and one light CP-odd Higgs bosons with masses smaller than about 250 GeV. Moreover, in order to obtain a realistic relic density, the lightest neutralino mass tends to be smaller than $M_Z/2$, in which case the lightest Higgs boson decays predominantly into neutralinos.
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References
How later papers used it
51 later papers cite it
1 later paper by other authors is listed below: 1 compared its own results with it. 1 more paper by the same authors is listed: 1 used its method or tool.
Uses its method or tool 1 of 2 papers with this label · 1 by the same authors
By the same authors
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Replaced the singlet by its extreme value as a function of the Higgs boson fields, leading to this paper's expression for the potential.
Light Dark Matter and the Electroweak Phase Transition in the NMSSM (2011) (same authors) · 0.84 · paraphrased: the licence does not allow quoting
Compares with it 1 of 2 papers with this label
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Reported a small difference among the results of another work, this paper and its own results.
Electroweak Symmetry Breaking and Singlino Dark Matter with Deflected Anomaly Mediation (2009) · 1.00 · paraphrased: the licence does not allow quoting
How the literature uses it
50 arXiv papers cite this in 84 sentences
Papers citing it · 48 sentences without a confident label
Uses its method or tool 2 papers
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The electroweak symmetry breaking and the phase transition properties are mostly dependent on the minima of the potential, therefore we shall replace $S$ by its extreme value as a function of the Higgs boson fields: [equation] This leads to the expression [ref] [equation] where $ϕ=√(|H_u|^2+|H_d|^2)$ and $ã=λA_λsin(β) cos(β)$. $m_ϕ^2(T)=m_ϕ^2(0)+cT^2$, and $c$ is determined by the all weak scale particles that couple to the Higgs and contribute to the finite temperature potential.
Light Dark Matter and the Electroweak Phase Transition in the NMSSM · Electroweak Phase Transition in a Simplified Model · 0.84
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The semi-analytical approach adopted here closely follows [ref] .
Electroweak Phase Transition in a Right-Handed Neutrino Superfield Extended NMSSM · A simplified model to understand EWPT in NMSSM+ one RHN model · 0.98
Compares with it 2 papers
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The main differences between our work and Ref. [ref] are the following: (1) The soft SUSY-breaking parameters are taken as $m_q̃=m_t̃=500$ GeV and $A_t=100$ GeV.
Electroweak phase transitions in the secluded U(1)-prime-extended MSSM · Comparisons · 0.96
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Therefore there is small difference among the results of [ref] and [ref] and our results.
Electroweak Symmetry Breaking and Singlino Dark Matter with Deflected Anomaly Mediation · The Landau pole · 1.00
Cites it as support 2 papers
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For larger $λ$, the SM-like $h^0$ Higgs can decay predominantly into pairs of these neutralinos producing invisible Higgs decays [ref] .
Physics searches at the LHC · Extended supersymmetric models · 0.96
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In both cases, strong constraints from the upper bound on the (neutron) electric dipole moments have to be respected, which is possible in the nMSSM [ref] .
The Next-to-Minimal Supersymmetric Standard Model · Electroweak baryogenesis · 0.98
Cites it as background 26 papers
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From Eq. ([ref]) and Eq. ([ref]), the potential and the triple Higgs coupling are given by [equation] This case has been studied in the literature in various contexts [ref] .
Probing the Electroweak Phase Transition at the LHC · Higgs Potential of order $(ϕ^†ϕ)^3$ · 0.95
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The corresponding simplest extension of the MSSM is the Minimal Non–minimal Supersymmetric Standard Model (MNSSM) [ref] , [ref] , [ref] – [ref] .
Theoretical upper bound on the mass of the LSP in the MNSSM · Superpotential · 0.93
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So far, electroweak baryogenesis have been studied in the singlet extended MSSM models: the NMSSM [ref] , the nMSSM [ref] , the UMSSM [ref] and the sMSSM [ref] .
CP violation in the secluded U(1)'-extended MSSM · Introduction · 0.87
Discussion
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