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Ушбу иш иқтибос қилган ишлар

87 та иш

Иш: Energy conditions in $f(Q, L_m)$ gravity

  1. Weyl type f(Q, T) gravity, and its cosmological implications

    Yixin Xu, Tiberiu Harko, Shahab Shahidi +1

    Мақола202016 иқтибос
    ABI

  2. Cosmic acceleration and energy conditions in symmetric teleparallel f(Q) gravity

    M. Koussour, S. H. Shekh, M. Bennai

    Мақола202216 иқтибос
    ABI

  3. A New Parametrization of Hubble Parameter in f(Q)$f(Q)$ Gravity

    M. Koussour, S. K. J. Pacif, M. Bennai +1

    Мақола202315 иқтибос
    ABI

  4. Constant sound speed and its thermodynamical interpretation in f(Q) gravity

    M. Koussour, Simran Arora, Dhruba Jyoti Gogoi +2

    Мақола202315 иқтибос
    ABI

  5. Cosmological constraints on alternative model to Chaplygin fluid revisited

    A. Hernández-Almada, Juan Magaña, Miguel A. García-Aspeitia +1

    Мақола201914 иқтибос
    ABI

  6. Сарлавҳасиз

    Бошқа14 иқтибос
    ABI

  7. Сарлавҳасиз

    Бошқа14 иқтибос
    ABI

  8. Accelerating Universe scenario in anisotropic <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si14.svg" display="inline" id="d1e530"><mml:mrow><mml:mi>f</mml:mi><mml:mrow><mml:mo>(</mml:mo><mml:mi>Q</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mrow></mml:math> cosmology

    M. Koussour, M. Bennai

    Мақола202214 иқтибос
    ABI

  9. Constraining the cosmological model using recent observational data*

    N. Myrzakulov, M. Koussour, Alnadhief H. A. Alfedeel +1

    Мақола202314 иқтибос
    ABI

  10. Quintessence Universe and cosmic acceleration in <i>f</i> (<i>Q</i>, <i>T</i>) gravity

    M. Koussour, N. Myrzakulov, S. H. Shekh +1

    Мақола202214 иқтибос
    ABI

  11. Holographic explanation of wide-angle power correlation suppression in the cosmic microwave background radiation

    Zhuoyi Huang, Bin Wang, Élcio Abdalla +1

    Мақола200613 иқтибос
    ABI

  12. Cosmology from Non‐Minimal Geometry‐Matter Coupling

    Berenice Santos Gonçalves, P. H. R. S. Moraes, B. Mishra

    Мақола202313 иқтибос
    ABI

  13. Investigating the dark energy phenomenon in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si14.svg" display="inline" id="d1e553"> <mml:mrow> <mml:mi>f</mml:mi> <mml:mrow> <mml:mo>(</mml:mo> <mml:mi>R</mml:mi> <mml:mo>,</mml:mo> <mml:msub> <mml:mrow> <mml:mi>L</mml:mi> </mml:mrow> <mml:mrow> <mml:mi>m</mml:mi> </mml:mrow> </mml:msub> <mml:mo>)</mml:mo> </mml:mrow> </mml:mrow> </mml:math> cosmological models with observational constraints

    S. Myrzakulova, M. Koussour, N. Myrzakulov

    Мақола202313 иқтибос
    ABI

  14. Constraints on bulk viscosity in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si256.svg" display="inline" id="d1e1685"><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 from H(z)/Pantheon+ data

    M. Koussour, Abdelghani Errehymy, Orhan Dönmez +4

    Мақола202413 иқтибос
    ABI

  15. Cosmological solutions and growth index of matter perturbations 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>Q</mml:mi><mml:mo stretchy="false">)</mml:mo></mml:math> gravity

    Wompherdeiki Khyllep, Andronikos Paliathanasis, Jibitesh Dutta

    Мақола202113 иқтибос
    ABI

  16. Exploring accelerated expansion in the universe: A study of <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si274.svg" display="inline" id="d1e325"><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 with parameterized EoS and cosmological constraints

    M. Koussour, N. Myrzakulov, Javlon Rayimbaev +2

    ПрепринтCosmology and Gravitation TheoriesChinese Journal of Physics202412 иқтибос
    ABI

  17. Generalizing the coupling between geometry and matter: $$f\left( R,L_m,T\right) $$ gravity

    Zahra Haghani, Tiberiu Harko

    Мақола202112 иқтибос
    ABI

  18. Energy conditions in <i>f</i> ( <i>R</i> , <i> L <sub>m</sub> </i> ) gravity

    Jun Wang, Kai Liao

    Мақола201212 иқтибос
    ABI

  19. Constant-roll and primordial black holes in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline" id="d1e1888" altimg="si282.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

    K. El Bourakadi, M. Koussour, Giovanni Otalora +2

    Мақола202312 иқтибос
    ABI

  20. Is cosmic speed-up due to new gravitational physics?

    Sean M. Carroll, Vikram Duvvuri, Mark Trodden +1

    Мақола200411 иқтибос
    ABI

  21. Gaussian process estimation of transition redshift

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

    Мақола202011 иқтибос
    ABI

  22. Сарлавҳасиз

    Бошқа11 иқтибос
    ABI

  23. Сарлавҳасиз

    Бошқа11 иқтибос
    ABI

  24. Сарлавҳасиз

    Бошқа11 иқтибос
    ABI

  25. Dynamical stability of new wormhole solutions via cold dark matter and solitonic quantum wave halos in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si2.svg" display="inline" id="d1e3341"><mml:mrow><mml:mi>f</mml:mi><mml:mrow><mml:mo>(</mml:mo><mml:mi mathvariant="script">R</mml:mi><mml:mo>,</mml:mo><mml:msub><mml:mrow><mml:mi mathvariant="script">L</mml:mi></mml:mrow><mml:mrow><mml:mi>m</mml:mi></mml:mrow></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:mrow></mml:math> gravity

    G. Mustafa, Faisal Javed, S. K. Maurya +2

    Мақола202411 иқтибос
    ABI