Paper Explainer: General Constraints on Isocurvature from the CMB and Ly-alpha Forest

Paper Explainer: General Constraints on Isocurvature from the CMB and Ly-alpha Forest

This is a paper explainer for my recent paper “General Constraints on Isocurvature from the CMB and Ly-$\alpha$ Forest” by myself, Peizhi Du (Rutgers postdoc until recently, now a newly-minted faculty member in China), Nicolas Fernandez (Rutgers postdoc), and my student Mitchell Weikert.

This is in some ways a follow up to our previous paper which I wrote about here

That paper had to do with a new physics scenario that creates “isocurvature” in the early Universe. This paper provides model-independent limits on isocurvature, using data from the Cosmic Microwave Background, the Lyman-alpha forest, and spectral distortions.

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Paper Explainer: Dark Radiation Isocurvature from Cosmological Phase Transitions

Paper Explainer: Dark Radiation Isocurvature from Cosmological Phase Transitions

I want to tell you about my most recent paper “Dark Radiation Isocurvature from Cosmological Phase Transitions,” which I wrote with my coauthors Mitch Weikert, Peizhi Du, and Nicolas Fernandez. Peizhi and Nico are postdocs here at Rutgers, and Mitch is my grad student. All three are great and fun to work with, and you should hire them.

As the title of the paper suggests, this is a project with a bunch of moving parts, and it’s not easy (even by the standards of theoretical physics research) to explain to outsiders. Which is unfortunate, because it has to do with what we know about the very early Universe, and how we know it. It’s one of those things that is really beautiful and tremendously informative, but complicated enough that its hard to convey how and why we know the things we know.

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