Non-Gaussian bubbles in the sky
- fNL(θ, φ) ≡ 3
- (δT(θ, φ)/ ¯
T)3 (δT/ ¯ T)22
Y TP
YUKAWA INSTITUTE FOR THEORETICAL PHYSICS
Non-Gaussian bubbles in the sky T ) - - PowerPoint PPT Presentation
Non-Gaussian bubbles in the sky T ) 2 2 T ) 3 ( T ( , ) / ( T/ f NL ( , ) 3
YUKAWA INSTITUTE FOR THEORETICAL PHYSICS
YUKAWA INSTITUTE FOR THEORETICAL PHYSICS
3
http://journalofcosmology.com
L(x) −
L
6
int
10
dt
int
(φ(x); x)
13
16
m/H = 0.3, HRW = 0.2π H/φ0 = 0.001 λ = 0.005,
005, rφ = 0.1, |x0| = r∗ = 2, Hte = 50.
σ(χ) = σT for 0 χ < HRW, σF for HRW < χ π.
f (cen)
NL
≈ 3×10−4 λ r3
φ sin3(
HRW) A4
ζ exp
H )2Hte
m
φ0
.
18
t t
C C
x
Re Im
×
i /2
C C’
R
C×Σt dtd3xLI
R
C×Σt dtd3xLI
R-region C-region L-region E-region reheating bubble nucleation bubble wall
ˆ) ≈ 40r3
φ
81ζ22 δφ3(|x0 + r∗ ˆ n|, t∗) φ3
te
ζ ≡ 6.25 × 10−10
ζφ = 1 3 δρφ ρφ
= 1 3
φ0 + δφ2 φ2
,
can be written in terms of the cu (δT/T)(ˆ n) = (1/5) ζ(x0 + r∗ ˆ n, t∗),
T)3 (δT/ ¯ T)22