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開始行:
[[UTAPwiki/セミナー/初期宇宙・相対論速報]]
Speaker: Jun'ichi Yokoyama (RESCEU)
Title: Spontaneous genesis after G-inflation
Abstract:
In kinetically driven G-inflation, the Universe after inf...
is dominated by the kinetic energy density of a free scal...
whose energy density is dissipated in proportion to $a^{-...
so that the cosmic expansion law is like $a(t) \propto t^...
The reheating is achieved by gravitational particle produ...
or through direct coupling preserving the shift symmetry ...
model. We discuss spontaneous baryogenesis and asymmetric
dark matter genesis may be possible if these charge densi...
have a derivative coupling with the inflaton.
&br;
終了行:
[[UTAPwiki/セミナー/初期宇宙・相対論速報]]
Speaker: Jun'ichi Yokoyama (RESCEU)
Title: Spontaneous genesis after G-inflation
Abstract:
In kinetically driven G-inflation, the Universe after inf...
is dominated by the kinetic energy density of a free scal...
whose energy density is dissipated in proportion to $a^{-...
so that the cosmic expansion law is like $a(t) \propto t^...
The reheating is achieved by gravitational particle produ...
or through direct coupling preserving the shift symmetry ...
model. We discuss spontaneous baryogenesis and asymmetric
dark matter genesis may be possible if these charge densi...
have a derivative coupling with the inflaton.
&br;
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