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Ушбу иш иқтибос қилган ишлар

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Иш: Exploring cosmological evolution and constraints in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si145.svg" display="inline" id="d1e758"><mml:mrow><mml:mi>f</mml:mi><mml:mrow><mml:mo>(</mml:mo><mml:mi>T</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mrow></mml:math> teleparallel gravity

  1. Accelerating universe from F(T) gravity

    Ratbay Myrzakulov

    Мақола201113 иқтибос
    ABI

  2. The teleparallel equivalent of general relativity

    J. W. Maluf

    Мақола201313 иқтибос
    ABI

  3. Сарлавҳасиз

    Бошқа12 иқтибос
    ABI

  4. From cosmic deceleration to acceleration: new constraints from SN Ia and BAO/CMB

    R Giostri, M. Vargas dos Santos, I Waga +3

    Мақола201211 иқтибос
    ABI

  5. Gaussian process estimation of transition redshift

    J. F. Jesus, R. Valentim, A. A. Escobal +1

    Мақола202011 иқтибос
    ABI

  6. Сарлавҳасиз

    Бошқа11 иқтибос
    ABI

  7. Сарлавҳасиз

    Бошқа11 иқтибос
    ABI

  8. HUBBLE PARAMETER MEASUREMENT CONSTRAINTS ON THE REDSHIFT OF THE DECELERATION–ACCELERATION TRANSITION, DYNAMICAL DARK ENERGY, AND SPACE CURVATURE

    Omer Farooq, Foram Ranjeet Madiyar, Bharat Ratra +1

    Мақола201710 иқтибос
    ABI

  9. A comprehensive parametrization approach for the Hubble parameter in scalar field dark energy models

    M. Koussour, N. Myrzakulov, S. Myrzakulova +1

    Мақола202310 иқтибос
    ABI

  10. Teleparallel Gravity: An Introduction

    R. Aldrovandi, R. Aldrovandi, J. G. Pereira

    Китоб201210 иқтибос
    ABI

  11. Сарлавҳасиз

    Бошқа9 иқтибос
    ABI

  12. Measuring the Baryon Acoustic Oscillation scale using the Sloan Digital Sky Survey and 2dF Galaxy Redshift Survey

    Will J. Percival, Shaun Cole, Daniel J. Eisenstein +4

    Мақола20079 иқтибос
    ABI

  13. Cosmological inflation in<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>F</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mi>R</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="script">G</mml:mi><mml:mo stretchy="false">)</mml:mo></mml:math>gravity

    Mariafelicia De Laurentis, Mariacristina Paolella, Salvatore Capozzıello

    Мақола20159 иқтибос
    ABI

  14. Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics beyond ΛCDM

    Adam G. Riess, Stefano Casertano, Wenlong Yuan +2

    Мақола20199 иқтибос
    ABI

  15. Сарлавҳасиз

    Бошқа8 иқтибос
    ABI

  16. HUBBLE PARAMETER MEASUREMENT CONSTRAINTS ON THE REDSHIFT OF THE DECELERATION-ACCELERATION TRANSITION, DYNAMICAL DARK ENERGY, AND SPACE CURVATURE

    Farooq, O., Madiyar, F. R., Crandall, S. +1

    Мақола20178 иқтибос
    ABI

  17. <i>WMAP</i> constraints on low redshift evolution of dark energy

    H. K. Jassal, J. S. Bagla, Τ. Padmanabhan

    Мақола20058 иқтибос
    ABI

  18. Сарлавҳасиз

    Бошқа8 иқтибос
    ABI

  19. Modeling wormholes in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>f</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mi>R</mml:mi><mml:mo>,</mml:mo><mml:mi>T</mml:mi><mml:mo stretchy="false">)</mml:mo></mml:math> gravity

    P. H. R. S. Moraes, P. K. Sahoo

    Мақола20178 иқтибос
    ABI

  20. Confronting the relaxation mechanism for a large cosmological constant with observations

    Spyros Basilakos, Florian Bauer, Joan Solà

    Мақола20127 иқтибос
    ABI

  21. Correcting Type Ia Supernova Distances for Selection Biases and Contamination in Photometrically Identified Samples

    R. Keßler, D. Scolnic

    Мақола20177 иқтибос
    ABI

  22. Cosmography of<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>f</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mi>R</mml:mi><mml:mo stretchy="false">)</mml:mo></mml:math>gravity

    Salvatore Capozzıello, V. F. Cardone, Vincenzo Salzano

    Мақола20087 иқтибос
    ABI

  23. Acceleration of the universe: a reconstruction of the effective equation of state

    Ankan Mukherjee

    Мақола20167 иқтибос
    ABI

  24. Fitting <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline" id="d1e4298" altimg="si614.svg"> <mml:mrow> <mml:mi>f</mml:mi> <mml:mrow> <mml:mo>(</mml:mo> <mml:mi>Q</mml:mi> <mml:mo>,</mml:mo> <mml:mi>T</mml:mi> <mml:mo>)</mml:mo> </mml:mrow> </mml:mrow> </mml:math> gravity models with a <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline" id="d1e4315" altimg="si606.svg"> <mml:mi>Λ</mml:mi> </mml:math> CDM limit using <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline" id="d1e4320" altimg="si18.svg"> <mml:mrow> <mml:mi>H</mml:mi> <mml:mrow> <mml:mo>(</mml:mo> <mml:mi>z</mml:mi> <mml:mo>)</mml:mo> </mml:mrow> </mml:mrow> </mml:math> and Pantheon data

    José Antonio Nájera, Amanda Fajardo

    Мақола20217 иқтибос
    ABI

  25. On the stability of the cosmological solutions in <i>f</i> ( <i>R</i> , <i>G</i> ) gravity

    Álvaro de la Cruz-Dombriz, Diego Sáez-Gómez

    Мақола20127 иқтибос
    ABI