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Deceleration parameter

  • The Hubble Constant H0 --- Describing How Fast the Universe Is Expanding A˙ (T) H(T) = , A(T) = the Cosmic Scale Factor A(T)

    The Hubble Constant H0 --- Describing How Fast the Universe Is Expanding A˙ (T) H(T) = , A(T) = the Cosmic Scale Factor A(T)

  • Measuring Dark Energy and Primordial Non-Gaussianity: Things to (Or Not To?) Worry About!

    Measuring Dark Energy and Primordial Non-Gaussianity: Things to (Or Not To?) Worry About!

  • Arxiv:Astro-Ph/9805201V1 15 May 1998 Hitpe Stubbs Christopher .Phillips M

    Arxiv:Astro-Ph/9805201V1 15 May 1998 Hitpe Stubbs Christopher .Phillips M

  • ASTRON 329/429, Fall 2015 – Problem Set 3

    ASTRON 329/429, Fall 2015 – Problem Set 3

  • Cosmological Consequences of a Parametrized Equation of State

    Cosmological Consequences of a Parametrized Equation of State

  • From Cosmic Deceleration to Acceleration: New Constraints from SN Ia and BAO/CMB

    From Cosmic Deceleration to Acceleration: New Constraints from SN Ia and BAO/CMB

  • Expanding Universe: Slowdown Or Speedup?

    Expanding Universe: Slowdown Or Speedup?

  • Sne Ia Redshift in a Nonadiabatic Universe

    Sne Ia Redshift in a Nonadiabatic Universe

  • Linear and Non-Linear Regression: the Hubble Plot Using Type-1A Supernovae

    Linear and Non-Linear Regression: the Hubble Plot Using Type-1A Supernovae

  • Power Spectrum of the SDSS Luminous Red Galaxies: Constraints on Cosmological Parameters

    Power Spectrum of the SDSS Luminous Red Galaxies: Constraints on Cosmological Parameters

  • Local Determination of the Hubble Constant and the Deceleration Parameter

    Local Determination of the Hubble Constant and the Deceleration Parameter

  • Astrophysical Cosmology 4 2004/2005 Solution Set 4

    Astrophysical Cosmology 4 2004/2005 Solution Set 4

  • Cosmological Parameters AST 541, Fall 2018

    Cosmological Parameters AST 541, Fall 2018

  • Time Evolution of Various Cosmological Parameters and Their Inter-Dependence in the Framework of Brans-Dicke Theory

    Time Evolution of Various Cosmological Parameters and Their Inter-Dependence in the Framework of Brans-Dicke Theory

  • Constraining the Hubble Parameter Using Distance Modulus – Redshift Relation

    Constraining the Hubble Parameter Using Distance Modulus – Redshift Relation

  • Fundamentals of Cosmology (4) Observational Tests of Cosmological Models

    Fundamentals of Cosmology (4) Observational Tests of Cosmological Models

  • THE CARNEGIE SUPERNOVA PROJECT: FIRST NEAR-INFRARED HUBBLE DIAGRAM to Z ∼ 0.7∗

    THE CARNEGIE SUPERNOVA PROJECT: FIRST NEAR-INFRARED HUBBLE DIAGRAM to Z ∼ 0.7∗

  • Brian P. Schmidt Australian National University, Weston Creek, Australia

    Brian P. Schmidt Australian National University, Weston Creek, Australia

Top View
  • Cosmological Constraints on the Coupling Model from Observational Hubble Parameter and Baryon Acoustic Oscillation Measurements
  • Is the Transition Redshift a New Cosmological Number?
  • The Role of Quantum Expansion in Cosmic Evolution
  • 15. the Pocket Cosmology 125
  • Cosmology in Terms of the Deceleration Parameter. Part I
  • 5.1 Introduction
  • Cosmological Formulas, Since It Was My Feeling That I Often and Repeatedly Wasted Time in Re-Deriving Distances, Volume Elements, Look-Back Times, Etc
  • A Low Hubble Constant from Galaxy Distribution Observations
  • Cosmology AS7009, 2008 Lecture 5
  • Evolution of the Distance Scale Factor and the Hubble Parameter in the Light of Planck’S Results
  • Viscous Cosmology in New Holographic Dark Energy Model and the Cosmic Acceleration
  • Model Independent Constraints on Transition Redshift
  • The Picture of Our Universe: a View from Modern Cosmology
  • Evidence for Anisotropy of Cosmic Acceleration? Jacques Colin1, Roya Mohayaee1, Mohamed Rameez2, and Subir Sarkar3
  • Anisotropic Cosmological Model in a Modified Theory of Gravitation
  • Deceleration Parameter I a Few Others… Definition
  • Lecture 16 : Cosmological Models I
  • A Parametric Reconstruction of the Deceleration Parameter


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