REVIEW 2 cited by
Unveiling dark forces with measurements of the Large Scale Structure of the Universe
Not yet reviewed by Pith; the record is open.
This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.
SPECIMEN: schema-true, not a live event
T0 review · schema-true
One-sentence machine reading of the paper's core claim.
pith:XXXXXXXX · record.json · timestamp
read the original abstract
Cosmology offers opportunities to test Dark Matter independently of its interactions with the Standard Model. We study the imprints of long-range forces acting solely in the dark sector on the distribution of galaxies, the so-called Large Scale Structure (LSS). We derive the strongest constraint on such forces from a combination of Planck and BOSS data. Along the way we consistently develop, for the first time, the Effective Field Theory of LSS in the presence of new dynamics in the dark sector. We forecast that future surveys will improve the current bound by an order of magnitude.
Forward citations
Cited by 2 Pith papers
-
Natural Phantom Crossing from Axion-WIMP Interactions
A Z_N-symmetric WIMP sector stores the initial axion value in its relic distribution and later generates a finite-density axion potential, producing an apparent late-time phantom crossing without ghosts.
-
Scale-dependent bias and mode coupling in redshift-space clustering near the BAO scale
A biased-tracer clustering model that adds scale-dependent density/velocity bias and mode coupling accurately describes BAO-scale redshift-space multipoles in simulations, and scale-dependent bias matters more than mo...
Discussion (0). Sign in to comment.