2023
DOI: 10.1007/jhep08(2023)029
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Electroweak phase transition in a right-handed neutrino superfield extended NMSSM

Abstract: Supersymmetric models with singlet extensions can accommodate single- or multi-step first-order phase transitions (FOPT) along the various constituent field directions. Such a framework can also produce Gravitational Waves, detectable at the upcoming space-based interferometers, e.g., U-DECIGO. We explore the dynamics of electroweak phase transition and the production of Gravitational Waves in an extended set-up of the Next-to-Minimal Supersymmetric Standard Model (NMSSM) with a Standard Model singlet right-ha… Show more

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Cited by 5 publications
(1 citation statement)
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“…In fact, there exist limits like PQ-symmetry-limit (κ → 0) or Rsymmetry-limit (A κ , A λ → 0), where a light CP-odd Higgs bosons would follow naturally [17]. A light scalar helps to accomplish different goals: (i) to satisfy the dark matter abundance of the Universe through resonance annihilations of light Singlino-like or Bino-like DM pairs, (ii) to initiate a strong first-order electroweak phase transition, which also yields the promising conditions for electroweak baryogenesis [18][19][20][21][22][23], (iii) to boost the BSM contributions to the anomalous magnetic moment of the muon [24][25][26][27] or the W boson mass at one-loop [28][29][30] or even at the two-loop [29]. Thus, the quest of probing light scalars is of interest, especially since this is one of the salient features of the NMSSM.…”
Section: Introductionmentioning
confidence: 99%
“…In fact, there exist limits like PQ-symmetry-limit (κ → 0) or Rsymmetry-limit (A κ , A λ → 0), where a light CP-odd Higgs bosons would follow naturally [17]. A light scalar helps to accomplish different goals: (i) to satisfy the dark matter abundance of the Universe through resonance annihilations of light Singlino-like or Bino-like DM pairs, (ii) to initiate a strong first-order electroweak phase transition, which also yields the promising conditions for electroweak baryogenesis [18][19][20][21][22][23], (iii) to boost the BSM contributions to the anomalous magnetic moment of the muon [24][25][26][27] or the W boson mass at one-loop [28][29][30] or even at the two-loop [29]. Thus, the quest of probing light scalars is of interest, especially since this is one of the salient features of the NMSSM.…”
Section: Introductionmentioning
confidence: 99%