Gravitational waves from the phase transition in the B-LSSM

Abstract

Based on the gauge symmetry group $SU(3{)}_C\otimes SU(2{)}_L\otimes U(1{)}_Y\otimes U(1{)}_{B-L}$, the minimal supersymmetric extension of the SM with local B-L gauge symmetry(B-LSSM) has been introduced. In this model, we study the Higgs masses with the one-loop zero temperature effective potential corrections. Besides, the finite temperature effective potentials connected with two $U(1{)}_{B-L}$ Higgs singlets are deduced specifically. Then we can obtain the gravitational wave spectrums generated from the strong first-order phase transition. In the B-LSSM, the gravitational wave signals can be as strong as $h^2{\Omega }_{GW}\sim 10^{-11}$, which may be detectable in the future experiments.

References in corpus (12)

• Gravitational Wave Production by Collisions: More Bubbles
• Dynamics of Non-renormalizable Electroweak Symmetry Breaking
• The Minimal Set of Electroweak Precision Parameters
• Production of Gravitational Waves in the nMSSM
• Spontaneous R-Parity Breaking and Left-Right Symmetry
• The gravitational waves from the first-order phase transition with a dimension-six operator
• The Fate of R-Parity
• Renormalization and two loop electroweak corrections to lepton anomalous dipole moments in the standard model and beyond (I): heavy fermion contributions
• New constraints on supersymmetric models from b -> s gamma
• CP-violation for Electroweak Baryogenesis from Dynamical CKM Matrix
• Search for Mono-Higgs Signals at the LHC in the B-L Supersymmetric Standard Model
• Constraints on Supersymmetric Flavour Models from b->s gamma

Cited by in corpus (1)

• Constraining the Cosmic Strings Gravitational Wave Spectra in No Scale Inflation with Viable Gravitino Dark matter and Non Thermal Leptogenesis