Exploring the Expansion History of the Universe

Linder, Eric V.·2003·Physical Review Letters

Cited by (1,005)

Items 601–700 of 1,005

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  3. Euclid preparation
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  4. Does DESI 2024 confirm ΛCDM?
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  5. Test of the Chevallier-Polarski-Linder parametrization for rapid dark energy equation of state transitions
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  8. Oscillations in the dark energy equation of state: New MCMC lessons
    Ruth Lazkoz, Vincenzo Salzano, Irene Sendra · 2010 · Physics Letters B
  9. Strong gravitational lensing and dark energy complementarity
    Eric V. Linder · 2004 · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields
  10. Model Independent Reconstruction of the Expansion History of the Universe and the Properties of Dark Energy
    Arman Shafieloo · 2007
  11. Baryon oscillations and dark-energy constraints from imaging surveys
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  12. Observational Constraints on Dynamical Dark Energy with Pivoting Redshift
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  13. The role of LRG1 and LRG2’s monopole in inferring the DESI 2024 BAO cosmology
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  14. Modified gravity constraints from the full shape modeling of clustering measurements from DESI 2024
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  16. No redshift evolution of non-repeating fast radio burst rates
    Tetsuya Hashimoto, Tomotsugu Goto, Alvina Y L On, Ting-Yi Lu, Daryl Joe D Santos, Simon C-C Ho, Seong Jin Kim, Ting-Wen Wang, Tiger Yu-Yang Hsiao · 2020 · Monthly Notices of the Royal Astronomical Society
  17. Remarks on the formulation of the cosmological constant/dark energy problems
    Ishak, M · 2005 · CERN Document Server (European Organization for Nuclear Research)
  18. Probing Dynamics of Dark Energy with Supernova, Galaxy Clustering and the Three-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations
    Zhao, G B, Xia, J Q, Feng, B, Zhang, X · 2006 · CERN Document Server (European Organization for Nuclear Research)
  19. Cosmic voids: a novel probe to shed light on our Universe
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  20. Exponential quintessence: curved, steep and stringy?
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  21. Is the w0waCDM cosmological parameterization evidence for dark energy dynamics partially caused by the excess smoothing of Planck CMB anisotropy data?
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  22. Extended Chaplygin gas in Horava–Lifshitz gravity
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  23. Chasing the nonlinear evolution of matter power spectrum with a numerical resummation method: Solution of closure equations
    Takashi Hiramatsu, Atsushi Taruya · 2009 · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields
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  27. The ΛCDM Model in the Lead—A Bayesian Cosmological Model Comparison
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  28. PROBING DYNAMICS OF DARK ENERGY WITH SUPERNOVA, GALAXY CLUSTERING AND THE THREE-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE (WMAP) OBSERVATIONS
    GONG-BO ZHAO, JUN-QING XIA, XIN-MIN ZHANG, BO FENG · 2007 · International Journal of Modern Physics D
  29. Tightening the reins on nonminimal dark sector physics: Interacting dark energy with dynamical and nondynamical equation of state
    William Giarè, Yuejia Zhai, Supriya Pan, Eleonora Di Valentino, Rafael C. Nunes, Carsten van de Bruck · 2024 · Physical review. D/Physical review. D.
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    Tessa Baker, Philip Bull · 2015 · The Astrophysical Journal
  31. Cosmology with matter diffusion
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  33. Real-time cosmography with redshift derivatives
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  34. Latest astronomical constraints on some non-linear parametric dark energy models
    Weiqiang Yang, Supriya Pan, Andronikos Paliathanasis · 2018 · Monthly Notices of the Royal Astronomical Society
  35. New parametrized equation of state for dark energy surveys
    Luisa G. Jaime, Mariana Jaber, Celia Escamilla‐Rivera · 2018 · Physical review. D/Physical review. D.
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    J. E. Gonzalez, Micol Benetti, Rodrigo von Marttens, J. S. Alcaniz · 2021 · Journal of Cosmology and Astroparticle Physics
  37. Testable dark energy predictions from current data
    Michael J. Mortonson, Wayne Hu, Dragan Huterer A · 2010 · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields
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    J.-M. Virey, D. Talon-Esmieu, A. Ealet, Pierre Taxil, A. Tilquin · 2008 · Journal of Cosmology and Astroparticle Physics
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    Gong‐Bo Zhao, Hong Li, Eric V. Linder, Kazuya Koyama, David Bacon, Xinmin Zhang · 2012 · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields
  44. Cosmological systematics beyond nuisance parameters: form-filling functions
    T. Kitching, Adam Amara, Filipe Batoni Abdalla, Benjamin Joachimi, Alexandre R. Refregier · 2009 · Monthly Notices of the Royal Astronomical Society
  45. Revisiting the parametrization of equation of state of dark energy via SNIa data
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  46. Spherical collapse model in time varying vacuum cosmologies
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  47. Testing deviations from ΛCDM with growth rate measurements from six large-scale structure surveys atz= 0.06–1
    Shadab Alam, Shirley Ho, Alessandra Silvestri · 2016 · Monthly Notices of the Royal Astronomical Society
  48. Priors on the effective dark energy equation of state in scalar-tensor theories
    Marco Raveri, Philip Bull, Alessandra Silvestri, Levon Pogosian · 2017 · Physical review. D/Physical review. D.
  49. Tsallis holographic dark energy in Bianchi-I Universe using hybrid expansion law with k-essence
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  50. Dark energy parametrizations and the curvature of the universe
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  52. OBSERVATIONAL CONSTRAINTS ON DARK ENERGY MODEL
    YUNGUI GONG · 2005 · International Journal of Modern Physics D
  53. An old quasar in a young dark energy-dominated universe?
    2005
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  63. Reconstructing k-essence
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  64. Dark energy from a phantom field near a local potential minimum
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  65. Probing decisive answers to dark energy questions from cosmic complementarity and lensing tomography
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  73. High-redshift cosmography: Application and comparison with different methods
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  74. Reduction of Cosmological Data for the Detection of Time-varying Dark Energy Density
    Dick, J, Knox, L, Chu, M · 2006 · CERN Document Server (European Organization for Nuclear Research)
  75. Prospects of high redshift constraints on dark energy models with the E p, i − E iso correlation in long gamma ray bursts
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  77. Gaussian Process Modeling of Derivative Curves
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  82. Dark Energy simulations
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