2018
DOI: 10.1103/physrevd.97.015005
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Standard model with a complex scalar singlet: Cosmological implications and theoretical considerations

Abstract: We analyze the theoretical and phenomenological considerations for the electroweak phase transition and dark matter in an extension of the standard model with a complex scalar singlet (cxSM). In contrast with earlier studies, we use a renormalization group improved scalar potential and treat its thermal history in a gauge-invariant manner. We find that the parameter space consistent with a strong first-order electroweak phase transition (SFOEWPT) and present dark matter phenomenological constraints is signific… Show more

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Cited by 120 publications
(109 citation statements)
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“…This treatment has the advantage of being directly gauge-independent, numerically fast to evaluate, and still yields results comparable to a more thorough gaugeindependent treatment, as seen in Ref. [60]. Note that, in this context, the scalar field VEVs are manifestly gauge invariant, and we will identify these VEVs with the corresponding scalē v introduced above.…”
Section: Electroweak Phase Transitionmentioning
confidence: 86%
See 1 more Smart Citation
“…This treatment has the advantage of being directly gauge-independent, numerically fast to evaluate, and still yields results comparable to a more thorough gaugeindependent treatment, as seen in Ref. [60]. Note that, in this context, the scalar field VEVs are manifestly gauge invariant, and we will identify these VEVs with the corresponding scalē v introduced above.…”
Section: Electroweak Phase Transitionmentioning
confidence: 86%
“…For recent discussions of sphaleron rate computations in perturbation theory and the associated theoretical uncertainties see, e.g., Refs. [56,[58][59][60]. The dynamics of the expanding bubbles, together with the CPV transport dynamics, constitute the crucial elements for generating the left-handed number density that catalyses B + L generation.…”
Section: Overview Of Ewbgmentioning
confidence: 99%
“…However, as noted before in Eq. (3.7), this implies that 20) and therefore (v 1 , v 2 , 0) is always unstable.…”
Section: The Phase Diagram Of the Complete Thdsm Potentialmentioning
confidence: 90%
“…Both processes can be described by the same formalism as classical motion in Euclidean space [74]. In particular, such a solution is described by the action, 20) which can be assumed to be O(3)-symmetric in the high temperature limit [72]. Here,φ represents a solution of the Euclidean equation of motion found by computing the path that minimizes the energy [74,75].…”
Section: Bubble Nucleationmentioning
confidence: 99%
“…The gravitational wave must have an adjoint wave of matching field [35]. Because the energy of "dark matter" is the kinetic energy for expanding (or contracting) motion of universe, it is in the wrong direction to find the particle of the "dark matter" [36][37][38][39][40][41][42][43].…”
Section: Resultsmentioning
confidence: 99%