New probes of initial state of quantum fluctuations during inflation
New probes of initial state of quantum fluctuations during inflation
New probes of initial state of quantum fluctuations during inflation
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Galaxy clustering modified<br />
by the squeezed limit<br />
• The existence <strong>of</strong> long-wavelength ζ changes the smallscale<br />
power <strong>of</strong> δm.<br />
• A positive long-wavelength ζ -> more power<br />
on small scales.<br />
• More power on small scales -> more galaxies formed.<br />
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