TY - JOUR
T1 - Preheating with extra dimensions
AU - Tsujikawa, Shinji
PY - 2000
Y1 - 2000
N2 - We investigate preheating in a higher-dimensional generalized Kaluza-Klein theory with a quadratic inflaton potential V(φ) = 1/2m2φ2 including metric perturbations explicitly. The system we consider is the multi-field model where there exists a dilaton field σ which corresponds to the scale of compactifications and another scalar field χ coupled to inflaton with the interaction 1/2g2φ2χ2 + g-2φ3χ. In the case of g̃ = 0, we find that the perturbation of dilaton does not undergo parametric amplification while the χ field fluctuation can be enhanced in the usual manner by parametric resonance. In the presence of the g-2φ3χ coupling, the dilaton fluctuation in sub-Hubble scales is modestly amplified by the growth of metric perturbations for the large coupling g̃. In super-Hubble scales, the enhancement of the dilaton fluctuation as well as metric perturbations is weak, taking into account the backreaction effect of created χ particles. We argue that not only is it possible to predict the ordinary inflationary spectrum in large scales but extra dimensions can be held static during preheating in our scenario.
AB - We investigate preheating in a higher-dimensional generalized Kaluza-Klein theory with a quadratic inflaton potential V(φ) = 1/2m2φ2 including metric perturbations explicitly. The system we consider is the multi-field model where there exists a dilaton field σ which corresponds to the scale of compactifications and another scalar field χ coupled to inflaton with the interaction 1/2g2φ2χ2 + g-2φ3χ. In the case of g̃ = 0, we find that the perturbation of dilaton does not undergo parametric amplification while the χ field fluctuation can be enhanced in the usual manner by parametric resonance. In the presence of the g-2φ3χ coupling, the dilaton fluctuation in sub-Hubble scales is modestly amplified by the growth of metric perturbations for the large coupling g̃. In super-Hubble scales, the enhancement of the dilaton fluctuation as well as metric perturbations is weak, taking into account the backreaction effect of created χ particles. We argue that not only is it possible to predict the ordinary inflationary spectrum in large scales but extra dimensions can be held static during preheating in our scenario.
KW - Cosmology of Theories beyond the SM
KW - Extra Large Dimensions
KW - Physics of the Early Universe
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U2 - 10.1088/1126-6708/2000/07/024
DO - 10.1088/1126-6708/2000/07/024
M3 - Article
AN - SCOPUS:7744234174
SN - 1029-8479
VL - 4
SP - XXXIII-25
JO - Journal of High Energy Physics
JF - Journal of High Energy Physics
IS - 7 PART A
ER -