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  • Thumbnail for Deceleration parameterDeceleration parameter The deceleration parameter q {\displaystyle q} in cosmology is a dimensionless measure of the cosmic acceleration of the expansion of space in a... 6 KB (1,070 words) - 16:37, 2 August 2024
  • Thumbnail for Hubble's lawHubble's law (redirect from Hubble parameter) of the Hubble parameter changes over time, either increasing or decreasing depending on the value of the so-called deceleration parameter q, which is defined... 130 KB (12,871 words) - 04:02, 24 December 2024
  • Thumbnail for Accelerating expansion of the universeAccelerating expansion of the universe (category Pages using sidebar with the child parameter) deceleration of the universe's expansion that they introduced a so-called deceleration parameter q0. Recent observations indicate this deceleration parameter... 39 KB (4,805 words) - 08:34, 6 November 2024
  • Thumbnail for De Sitter universeDe Sitter universe (category Pages using sidebar with the child parameter) consistent through all space, but also through all time (since the deceleration parameter is q = − 1 {\displaystyle q=-1} ), thus satisfying the perfect cosmological... 6 KB (762 words) - 15:50, 16 June 2024
  • Thumbnail for UniverseUniverse (category Pages using sidebar with the child parameter) deceleration parameter, which most cosmologists expected to be positive and related to the matter density of the universe. In 1998, the deceleration parameter... 157 KB (16,470 words) - 14:11, 26 November 2024
  • image layout frameless Allan Sandage observational cosmology would be the search for two parameters: the Hubble constant H0 and the deceleration parameter q0. This paper influenced observational cosmology... 16 KB (1,702 words) - 23:36, 18 November 2024
  • image layout frameless Index of physics articles (D) Debye–Waller factor Decay chain Decay energy Decay heat Decay product Deceleration parameter Decibel Decollimation Deconfinement Decorrelation Decoy state Deep-dose... 17 KB (1,787 words) - 22:53, 7 October 2024
  • image layout frameless Angular diameter distance {\displaystyle q_{0}} is the present-day value of the deceleration parameter, which measures the deceleration of the expansion rate of the Universe; in the simplest... 6 KB (956 words) - 05:51, 19 November 2024
  • image layout frameless Latin letters used in mathematics, science, and engineering of a fraction the quotient resulting from integer division the deceleration parameter in cosmology electric charge of a particle a generalized coordinate... 40 KB (3,991 words) - 19:20, 11 October 2024
  • Thumbnail for Calán/Tololo SurveyCalán/Tololo Survey (category Articles using Infobox astronomical survey using locally defined parameters) led to the precise measurements of the Hubble Constant H0 and the deceleration parameter q0, the latter indicating the presence of a dark energy or cosmological... 5 KB (598 words) - 19:36, 15 July 2023
  • Thumbnail for Milne modelMilne model result in a linearly increasing scale factor for all time since the deceleration parameter is uniquely zero for such a model. Milne proposed that the universe's... 7 KB (742 words) - 01:42, 3 September 2024
  • Thumbnail for Tidal accelerationTidal acceleration (redirect from Tidal deceleration) will cause tidal deceleration of any remaining planets. Retrograde satellites: All retrograde satellites experience tidal deceleration to some degree because... 36 KB (4,749 words) - 18:19, 7 December 2024
  • Thumbnail for Brian SchmidtBrian Schmidt (category Pages using sidebar with the child parameter) Supernova Search Team to measure the expected deceleration of the universe and the deceleration parameter (q0) using distances to Type Ia supernovae. In... 34 KB (3,103 words) - 21:20, 25 November 2024
  • Thumbnail for Mark M. PhillipsMark M. Phillips leading to the precise measurements of the Hubble constant H0 and the deceleration parameter q0, the latter implying the existence of dark energy or a cosmological... 4 KB (356 words) - 21:06, 16 February 2023
  • image layout frameless Mattig formula distance. q 0 = Ω 0 / 2 {\displaystyle q_{0}=\Omega _{0}/2} is the deceleration parameter while Ω 0 {\displaystyle \Omega _{0}} is the density of matter in... 3 KB (608 words) - 19:40, 30 December 2018
  • Thumbnail for PKS 2215+020PKS 2215+020 quasar has a corresponding linear scale of 3.38 h−1 pc mas−1 and deceleration parameter of q0 = 0.5, which its radio spectral index of 2215+020 is a 5 GHz... 8 KB (890 words) - 13:54, 12 November 2024
  • Thumbnail for Mario HamuyMario Hamuy led to the precise measurements of the Hubble Constant H0 and the deceleration parameter q0, the latter indicating the presence of a dark energy or cosmological... 7 KB (595 words) - 12:49, 16 October 2024
  • image layout frameless China Light-Duty Vehicle Test Cycle adopted in Europe, the CLTC involves more frequent stops, accelerations, decelerations, and simulates urban traffic congestion with a lower speed limit of... 13 KB (1,574 words) - 17:35, 6 November 2024
  • image layout frameless Ronald Kantowski Branch, D. (1995). "The Effects of Inhomogeneities on Evaluating the Deceleration Parameter Q 0". The Astrophysical Journal. 447: 35–42. arXiv:astro-ph/9511108... 4 KB (412 words) - 23:13, 15 September 2024
  • Thumbnail for Nicholas B. SuntzeffNicholas B. Suntzeff (category Pages using sidebar with the child parameter) use Type Ia supernovae to measure the Hubble constant H0 and the deceleration parameter q0, ran from 1990 to 1995, and provided the pioneering method to... 21 KB (1,861 words) - 01:04, 17 November 2024
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