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Иш: Role of three coupling parameters on maximum mass and stability: Theoretical insights into relativistic massive compact objects in mass gap under <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si334.svg" display="inline" id="d1e10703"><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> action

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

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

    Мақола1999103 иқтибос
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  2. f(R) Theories

    Antonio De Felice, Shinji Tsujikawa

    Мақола201039 иқтибос
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  3. General Relativistic Fluid Spheres

    H. A. Buchdahl

    Мақола195930 иқтибос
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  4. Modified gravity theories on a nutshell: Inflation, bounce and late-time evolution

    S. Nojiri, S.D. Odintsov, V.K. Oikonomou

    Мақола201728 иқтибос
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  5. Cracking of self-gravitating compact objects

    L. Herrera

    Мақола199226 иқтибос
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  6. f(Q, T) gravity

    Yixin Xu, Guangjie Li, Tiberiu Harko +1

    Мақола201925 иқтибос
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  7. Сарлавҳасиз

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  8. New general relativity

    Kenji Hayashi, Takeshi Shirafuji

    Мақола197918 иқтибос
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  9. Weyl type f(Q, T) gravity, and its cosmological implications

    Yixin Xu, Tiberiu Harko, Shahab Shahidi +1

    Мақола202016 иқтибос
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  10. Hairy black holes by gravitational decoupling

    Jorge Ovalle, R. Casadio, E. Contreras +1

    Мақола202015 иқтибос
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  11. Сарлавҳасиз

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