Pith. sign in

REVIEW 2 cited by

The Physics of Microwave Background Anisotropies

Not yet reviewed by Pith; the record is open.

Re-run · record.json Download PDF Read on arXiv ↗

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

arxiv astro-ph/9604166 v1 pith:GHYXXJH5 submitted 1996-04-28 astro-ph

Wayne Hu (IAS , Princeton) , Naoshi Sugiyama (Kyoto) , Joseph Silk (UC Berkeley) This is my paper · ORCID
classification astro-ph
keywords anisotropiesbackgroundmicrowaveamountanisotropycontentcosmiccosmological
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
read the original abstract

Cosmic microwave background anisotropies provide a vast amount of cosmological information. Their full physical content and detailed structure can be understood in a simple and intuitive fashion through a systematic investigation of the individual mechanisms for anisotropy formation.

Discussion (0). Continue with ORCID to comment.

Forward citations

Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. CAPMAP: A New Instrument to Measure the E-mode CMB Polarization on Angular Scales of 4 arcmin to 40 arcmin

    astro-ph.IM 2024-11 conditional novelty 6.0 of 10

    The CAPMAP instrument, a four-element 90 GHz correlation polarimeter array, was built, calibrated, and shown to be sensitive enough to measure the CMB E-mode polarization at multipoles 500 to 1500.

  2. Origin of cosmological neutrino mass bounds: background $\textit{versus}$ perturbations

    astro-ph.CO 2024-11 conditional novelty 6.0 of 10

    The CMB bound on the sum of neutrino masses comes mostly from the background energy density of massive neutrinos, not from their free-streaming effects.

Pith tools