Slides from the talk - CP3-Origins
Slides from the talk - CP3-Origins
Slides from the talk - CP3-Origins
You also want an ePaper? Increase the reach of your titles
YUMPU automatically turns print PDFs into web optimized ePapers that Google loves.
The matter bispectrum and PNG: large scales<br />
In Perturbation Theory ...<br />
P = P 0 + P loop<br />
G<br />
[P 0]+P loop<br />
NG [P 0,B 0 ]<br />
matter power spectrum<br />
Linear power<br />
spectrum<br />
Gravity-induced<br />
contributions<br />
(depending on P0 alone)<br />
Additional gravity-induced contributions<br />
present only for NG initial conditions (B0)<br />
B = B 0 + B tree<br />
G<br />
[P 0 ]+B loop<br />
G<br />
[P 0]+B loop<br />
NG [P 0,B 0 ]<br />
& bispectrum<br />
Primordial<br />
component<br />
If B0 was <strong>the</strong> only effect of NG initial conditions on <strong>the</strong> LSS<br />
<strong>the</strong>n future, large volume surveys (~100 Gpc 3 ) could<br />
provide:<br />
ΔfNL local < 5 and ΔfNL eq < 10<br />
Scoccimarro, ES & Zaldarriaga (2004), ES & Komatsu (2007)
Change language