REVIEW 2 cited by
Dark Matter and Dark Energy
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
Signed reviews
read the original abstract
This is a short review, aimed at a general audience, of several current subjects of research in cosmology. The topics discussed include the cosmic microwave background (CMB), with particular emphasis on its relevance for testing inflation; dark matter, with a brief review of astrophysical evidence and more emphasis on particle candidates; and cosmic acceleration and some of the ideas that have been put forward to explain it. A glossary of technical terms and acronyms is provided.
Forward citations
Cited by 2 Pith papers
-
Limits on the 21 cm power spectrum at z=6.5-7.0 from MWA observations
MWA's 268-hour dataset yields 21 cm power spectrum upper limits as low as (30.2)^2 mK^2, which rule out cold reionization models and indicate a heated intergalactic medium at z=6.5-7.0.
-
Quantifying the impacts of future gravitational-wave data on constraining interacting dark energy
Adding 1000 simulated Einstein Telescope standard sirens to current CMB, BAO, and supernova data would tighten H0 and matter density constraints by factors of 2 to 3 in four interacting dark energy models, with modest...
Discussion (0). Continue with ORCID to comment.