2009
DOI: 10.1088/1475-7516/2009/08/028
|View full text |Cite
|
Sign up to set email alerts
|

Full Boltzmann equations for leptogenesis including scattering

Abstract: We study the evolution of a cosmological baryon asymmetry produced via leptogenesis by means of the full classical Boltzmann equations, without the assumption of kinetic equilibrium and including all quantum statistical factors. Beginning with the full mode equations, we derive the usual equations of motion for the right-handed neutrino number density and integrated lepton asymmetry, and show explicitly the impact of each assumption on these quantities. For the first time, we investigate also the effects of sc… Show more

Help me understand this report
View preprint versions

Search citation statements

Order By: Relevance

Paper Sections

Select...
1
1
1
1

Citation Types

1
80
0
2

Year Published

2013
2013
2023
2023

Publication Types

Select...
6
1

Relationship

0
7

Authors

Journals

citations
Cited by 64 publications
(83 citation statements)
references
References 43 publications
1
80
0
2
Order By: Relevance
“…ref. [106]). Instead, one usually assumes kinetic equilibration of the mixing fields and approximates kinetic equations for the distribution functions by so-called rate equations for the corresponding number densities.…”
Section: Rate Equations In the Radiation-dominated Universementioning
confidence: 99%
“…ref. [106]). Instead, one usually assumes kinetic equilibration of the mixing fields and approximates kinetic equations for the distribution functions by so-called rate equations for the corresponding number densities.…”
Section: Rate Equations In the Radiation-dominated Universementioning
confidence: 99%
“…Therefore the right-hand side of Eq. (55) can be interpreted as a difference of two (integrated) Boltzmann-like equations-one for the particles and one for the antiparticles [23]. According to the physical interpretation of Eq.…”
Section: B Kadanoff-baym Equations For Leptonsmentioning
confidence: 99%
“…(55). Therefore, we insert the usual decomposition of the propagators G 2 fÁ; S; Sg into the spectral and statistical parts, Eq.…”
Section: Lepton Self-energiesmentioning
confidence: 99%
“…In the numerical computaion we use M φ /M 1 = 10 −5[105,106], where M φ is the Higgs thermal mass needed to cut off the infrared divergences of t channel process. For the the scattering cross sections please see Ref [107].…”
mentioning
confidence: 99%