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The Cosmological Parameters (2023)
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This is a review article for The Review of Particle Physics 2024 (aka the Particle Data Book), appearing as Chapter 25. It forms a compact review of knowledge of the cosmological parameters near the end of 2023. Topics included are Parametrizing the Universe; Extensions to the standard model; Probes; Bringing observations together; Outlook for the future.
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Cited by 4 Pith papers
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Expected redshift drift for tilted observers
Redshift drift for tilted observers consists of an FLRW background term plus directional corrections from peculiar expansion, projected shear, and acceleration along the line of sight.
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Cosmological constraining power of the redshifts, heights, and angular clustering of weak gravitational lensing peaks
In an idealized Euclid-like simulation forecast, the combined redshift distribution, height distribution, and angular clustering of weak-lensing peaks constrain cosmology better than shear two-point correlation functi...
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Expected redshift drift for tilted observers
For an observer with peculiar motion, the cosmic redshift-drift signal gains a dipolar correction proportional to the flow's projected expansion, shear, and acceleration; calibrated to CF4, it is subdominant and canno...
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The Degree of Fine-Tuning Needed for a Viable Universe: Not Fragile?
Most constants and cosmological parameters that control structure can vary by orders of magnitude and still yield long-lived universes with stars, planets, and complex nuclei; classic stellar fine-tuning cases are les...
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