TY - JOUR
T1 - Late-time entropy production due to the decay of domain walls
AU - Kawasaki, Masahiro
AU - Takahashi, Fuminobu
N1 - Funding Information:
F.T. is grateful to K. Ichikawa and M. Kakizaki for useful discussions. F.T. would like to thank the Japan Society for Promotion of Science for financial support.
PY - 2005/7/7
Y1 - 2005/7/7
N2 - It is shown that late-time decay of domain walls can dilute unwanted relics such as moduli, if the universe was dominated by frustrated domain walls with tension σ=(1-100TeV)3. Since energy density of the frustrated domain walls decreases as slow as the inverse of the scale factor, an overclosure limit on the axion decay constant fa is also considerably relaxed. In fact fa can be as large as the Planck scale, which may enable us to naturally implement the QCD axion in the string scheme. Furthermore, in contrast to thermal inflation models, the Affleck-Dine baryogenesis can generate enough asymmetry to explain the present baryon abundance, even in the presence of late-time entropy production.
AB - It is shown that late-time decay of domain walls can dilute unwanted relics such as moduli, if the universe was dominated by frustrated domain walls with tension σ=(1-100TeV)3. Since energy density of the frustrated domain walls decreases as slow as the inverse of the scale factor, an overclosure limit on the axion decay constant fa is also considerably relaxed. In fact fa can be as large as the Planck scale, which may enable us to naturally implement the QCD axion in the string scheme. Furthermore, in contrast to thermal inflation models, the Affleck-Dine baryogenesis can generate enough asymmetry to explain the present baryon abundance, even in the presence of late-time entropy production.
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U2 - 10.1016/j.physletb.2005.05.022
DO - 10.1016/j.physletb.2005.05.022
M3 - Article
AN - SCOPUS:20444395825
SN - 0370-2693
VL - 618
SP - 1
EP - 6
JO - Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics
JF - Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics
IS - 1-4
ER -