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Ушбу иш иқтибос қилган ишлар

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Иш: Linear redshift parametrization of deceleration parameter in f(R,Lm) gravity

  1. Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant

    Adam G. Riess, A. V. Filippenko, P. Challis +17

    Мақола1998108 иқтибос
    ABI

  2. <tt>emcee</tt>: The MCMC Hammer

    Daniel Foreman-Mackey, David W. Hogg, Dustin Lang +1

    Мақола2013108 иқтибос
    ABI

  3. Measurements of Ω and Λ from 42 High‐Redshift Supernovae

    S. Perlmutter, G. Aldering, G. Goldhaber +30

    Мақола1999103 иқтибос
    ABI

  4. <i>Planck</i> 2018 results

    N. Aghanim, Y. Akrami, M. Ashdown +97

    Мақола202090 иқтибос
    ABI

  5. Сарлавҳасиз

    Бошқа60 иқтибос
    ABI

  6. Detection of the Baryon Acoustic Peak in the Large‐Scale Correlation Function of SDSS Luminous Red Galaxies

    Daniel J. Eisenstein, Idit Zehavi, David W. Hogg +45

    Мақола200558 иқтибос
    ABI

  7. The cosmological constant problem

    Steven Weinberg

    Мақола198954 иқтибос
    ABI

  8. First‐Year <i>Wilkinson Microwave Anisotropy Probe</i> ( <i>WMAP</i> ) Observations: Determination of Cosmological Parameters

    David N. Spergel, Licia Verde, Hiranya V. Peiris +14

    Мақола200350 иқтибос
    ABI

  9. The cosmological constant and dark energy

    P. J. E. Peebles, Bharat Ratra

    Мақола200347 иқтибос
    ABI

  10. Baryon acoustic oscillations in the Sloan Digital Sky Survey Data Release 7 galaxy sample

    Will J. Percival, Beth Reid, Daniel J. Eisenstein +25

    Мақола200943 иқтибос
    ABI

  11. Non-Linear Lagrangians and Cosmological Theory

    H. A. Buchdahl

    Мақола197040 иқтибос
    ABI

  12. The Complete Light-curve Sample of Spectroscopically Confirmed SNe Ia from Pan-STARRS1 and Cosmological Constraints from the Combined Pantheon Sample

    D. Scolnic, D. O. Jones, A. Rest +37

    Мақола201839 иқтибос
    ABI

  13. Type Ia Supernova Discoveries at<i>z</i>&gt; 1 from the<i>Hubble Space Telescope</i>: Evidence for Past Deceleration and Constraints on Dark Energy Evolution

    Adam G. Riess, L. Strolger, J. Tonry +16

    Мақола200437 иқтибос
    ABI

  14. Raising the bar: new constraints on the Hubble parameter with cosmic chronometers at <i>z</i> ∼ 2

    M. Moresco

    Мақола201534 иқтибос
    ABI

  15. Dark energy cosmology: the equivalent description via different theoretical models and cosmography tests

    Kazuharu Bamba, Salvatore Capozzıello, Shin’ichi Nojiri +1

    Мақола201234 иқтибос
    ABI

  16. INTRODUCTION TO MODIFIED GRAVITY AND GRAVITATIONAL ALTERNATIVE FOR DARK ENERGY

    SHIN'ICHI NOJIRI, SERGEI D. ODINTSOV

    Мақола200731 иқтибос
    ABI

  17. Statefinder—A new geometrical diagnostic of dark energy

    Varun Sahni, Tarun Deep Saini, Alexei A. Starobinsky +1

    Мақола200329 иқтибос
    ABI

  18. Cosmic microwave background and supernova constraints on quintessence: Concordance regions and target models

    Robert R. Caldwell, Michael Doran

    Мақола200427 иқтибос
    ABI

  19. Two new diagnostics of dark energy

    Varun Sahni, Arman Shafieloo, Alexei A. Starobinsky

    Мақола200826 иқтибос
    ABI

  20. Сарлавҳасиз

    Бошқа25 иқтибос
    ABI

  21. Transition redshift: new kinematic constraints from supernovae

    J. V. Cunha, J. A. S. Lima

    Мақола200823 иқтибос
    ABI

  22. Observational constraints on two cosmological models of f(Q) theory

    M. Koussour, Avik De

    Мақола202322 иқтибос
    ABI

  23. f(R,L m ) gravity

    Tiberiu Harko, Francisco S. N. Lobo

    Мақола201022 иқтибос
    ABI

  24. Modified gravity with negative and positive powers of curvature: Unification of inflation and cosmic acceleration

    Shin’ichi Nojiri, Sergei D. Odintsov

    Мақола200321 иқтибос
    ABI

  25. Anisotropic nature of space–time in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline" id="d1e1494" altimg="si9.svg"> <mml:mrow> <mml:mi>f</mml:mi> <mml:mfenced open="(" close=")"> <mml:mrow> <mml:mi>Q</mml:mi> </mml:mrow> </mml:mfenced> </mml:mrow> </mml:math> gravity

    M. Koussour, S. H. Shekh, М. Беннаи

    Мақола202220 иқтибос
    ABI