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PHYS08200605006 D.K. Hazra - Homi Bhabha National Institute

PHYS08200605006 D.K. Hazra - Homi Bhabha National Institute

PHYS08200605006 D.K. Hazra - Homi Bhabha National Institute

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CHAPTER 5. THE SCALAR BI-SPECTRUM DURING PREHEATING<br />

whereγ(b,x) is the incomplete Gamma function (see, for example, Refs. [115, 116]), while<br />

the quantity C is a dimensionless constant of integration. Then, the relation between the<br />

incomplete Gamma and the Gamma functions allows us to express the function K(t) as<br />

follows:<br />

K(t) ≃ t e<br />

4a 2 e<br />

∫ t<br />

[<br />

d¯t 6<br />

cos 2 (m¯t+∆) 5<br />

(<br />

tē<br />

t<br />

) 1/3 ( ) ( ) 2 5<br />

+e 2i∆ (−2imt e ) −5/3 tē<br />

Γ<br />

3 t<br />

( ) 4/3 ( ) ( ) 2<br />

−e 2i(m¯t+∆) (−2imt e ) −1 tē 5<br />

+e −2i∆ (2imt e ) −5/3 tē<br />

Γ<br />

t 3 t<br />

( ) 4/3 ( ) ] 2<br />

−e −2i(m¯t+∆) (2imt e ) −1 tē tē<br />

+C<br />

t t<br />

≃ 3t4/3 e<br />

10a 2 e<br />

∫ t<br />

d¯t ¯t −1/3<br />

+··· . (5.23)<br />

cos 2 (m¯t+∆)<br />

In arriving at the final equality, we have used the asymptotic property of the incomplete<br />

Gamma function [115, 116] and have retained only the dominant term in inverse power<br />

ofmt. The final expression above can be integrated by parts to arrive at<br />

∫ t<br />

K(t) ≃ 3t4/3 e<br />

t −1/3 tan(mt+∆)+ t4/3 e<br />

d¯t ¯t −4/3 tan(m¯t+∆). (5.24)<br />

10ma 2 e 10ma 2 e<br />

The second term containing the integral in this expression is of the order of the other<br />

terms that we have already neglected and, hence, it too can be ignored. As a result, the<br />

growing mode of the curvature perturbation can be written as<br />

[<br />

]<br />

f k ≃ A k 1− 3 k 2 t 4/3<br />

e<br />

10 a 2 e mt tan(mt+∆) 1/3<br />

[<br />

= A k 1− 1 ( ) ]<br />

2 k H<br />

5 aH m tan(mt+∆) , (5.25)<br />

in perfect agreement with the result that has been obtained recently in the literature [64].<br />

It is evident from the above expression that the evolution of the curvature perturbation<br />

will contain sharp spikes during preheating, a feature that is clearly visible in Figure 5.3<br />

wherein we have plotted the above analytical expression as well as the corresponding<br />

numerical result (in this context, also see Figure 4 in the first reference in Refs. [63], where<br />

the spikes are also clearly visible).<br />

It is important that we make a couple of remarks concerning the appearance of the<br />

spikes in the evolution of the curvature perturbation. Firstly, as the spikes are encountered<br />

both analytically and numerically, evidently, they are not artifacts of the adopted<br />

96

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