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2015

Generating the cosmic microwave background power asymmetry with $g_{NL}$

Kenton, Zachary, Mulryne, David J., Thomas, Steven

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We consider a higher order term in the $\delta N$ expansion for the CMB power asymmetry generated by a superhorizon isocurvature field fluctuation.

The term can generate the asymmetry without requiring a large value of $f_{NL}$.
Instead it produces a non-zero value of $g_{NL}$.
A combination of constraints lead to an allowed region in $f_{NL}-g_{NL}$ space.

Generating the cosmic microwave background power asymmetry with $g_{NL}$ · Around

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