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000171268 0881_ $$aDESY-14-099; IPMU 14-0150; SISSA 39/2014/FISI; arXiv:1406.6300
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000171268 088__ $$2arXiv$$aarXiv:1406.6300
000171268 1001_ $$0P:(DE-H253)PIP1003059$$aBuchmuller, W.$$b0$$eCorresponding Author
000171268 245__ $$aThe Chaotic Regime of D-Term Inflation
000171268 260__ $$c2014
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000171268 520__ $$aWe consider D-term inflation for small couplings of the inflaton to matter fields. Standard hybrid inflation then ends at a critical value of the inflaton field that exceeds the Planck mass. During the subsequent waterfall transition the inflaton continues its slow-roll motion, whereas the waterfall field rapidly grows by quantum fluctuations. Beyond the decoherence time, the waterfall field becomes classical and approaches a time-dependent minimum, which is determined by the value of the inflaton field and the self-interaction of the waterfall field. During the final stage of inflation, the effective inflaton potential is essentially quadratic, which leads to the standard predictions of chaotic inflation. The model illustrates how the decay of a false vacuum of GUT-scale energy density can end in a period of `chaotic inflation'.
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000171268 650_7 $$2autogen$$ainflation: D-term
000171268 650_7 $$2autogen$$ainflation: chaos
000171268 650_7 $$2autogen$$ainflaton: potential
000171268 650_7 $$2autogen$$ainflaton: coupling
000171268 650_7 $$2autogen$$ainflation: hybrid
000171268 650_7 $$2autogen$$afluctuation: quantum
000171268 650_7 $$2autogen$$afalse vacuum: decay
000171268 650_7 $$2autogen$$adecoherence: time
000171268 650_7 $$2autogen$$aenergy: density
000171268 650_7 $$2autogen$$ascale: Planck
000171268 650_7 $$2autogen$$aslow-roll approximation
000171268 650_7 $$2autogen$$atime dependence
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000171268 7001_ $$0P:(DE-H253)PIP1013967$$aDomcke, V.$$b1
000171268 7001_ $$aSchmitz, K.$$b2
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000171268 9141_ $$y2014
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