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Ушбу иш иқтибос қилган ишлар

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Иш: Charged Spherical Solution in Torsion and Matter Coupling Gravity and Influence of Torsion Parameter and Electric Charge on Compact Stars in Lower Mass Gap

  1. Weak-field spherically symmetric solutions 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>T</mml:mi><mml:mo stretchy="false">)</mml:mo></mml:math>gravity

    Matteo Luca Ruggiero, Ninfa Radicella

    Мақола20153 иқтибос
    ABI

  2. General Solution for a Class of Static Charged Spheres

    Ranjan Sharma, S. Mukherjee, Sunil D. Maharaj

    Мақола20013 иқтибос
    ABI

  3. Electrically charged compact stars and formation of charged black holes

    Subharthi Ray, Aquino L. Espíndola, M. Malheiro +2

    Мақола20033 иқтибос
    ABI

  4. Data-driven reconstruction of the late-time cosmic acceleration with <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline" id="d1e500" altimg="si183.svg"> <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> gravity

    Xin Ren, Thomas Hong Tsun Wong, Yi-Fu Cai +1

    Мақола20213 иқтибос
    ABI

  5. Viable<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>T</mml:mi><mml:mo stretchy="false">)</mml:mo></mml:math>models are practically indistinguishable from<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>Λ</mml:mi><mml:mi>CDM</mml:mi></mml:math>

    Savvas Nesseris, Spyros Basilakos, Emmanuel N. Saridakis +1

    Мақола20133 иқтибос
    ABI

  6. Reconstruction 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>T</mml:mi><mml:mo stretchy="false">)</mml:mo></mml:math>gravity: Rip cosmology, finite-time future singularities, and thermodynamics

    Kazuharu Bamba, Ratbay Myrzakulov, Shin’ichi Nojiri +1

    Мақола20123 иқтибос
    ABI

  7. Gauss-Bonnet dark energy

    Shin’ichi Nojiri, Sergei D. Odintsov, Misao Sasaki

    Мақола20053 иқтибос
    ABI

  8. Transition redshift in<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>f</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mi>T</mml:mi><mml:mo stretchy="false">)</mml:mo></mml:mrow></mml:math>cosmology and observational constraints

    Salvatore Capozzıello, Orlando Luongo, Emmanuel N. Saridakis

    Мақола20153 иқтибос
    ABI

  9. Moments of inertia for neutron and strange stars: limits derived for the Crab pulsar

    M. Bejger, P. Haensel

    Мақола20023 иқтибос
    ABI

  10. Trace-anomaly driven inflation in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si1.gif" overflow="scroll"><mml:mi>f</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mi>T</mml:mi><mml:mo stretchy="false">)</mml:mo></mml:math> gravity and in minimal massive bigravity

    Kazuharu Bamba, Shin’ichi Nojiri, Sergei D. Odintsov

    Мақола20143 иқтибос
    ABI

  11. Gravitational collapse in<i>f</i>(<i>R</i>) theories

    José A. R. Cembranos, Álvaro de la Cruz-Dombriz, B. Montes Núñez

    Мақола20123 иқтибос
    ABI

  12. Was GW190814 a Black Hole–Strange Quark Star System?

    Ignazio Bombaci, A. Drago, Domenico Logoteta +2

    Мақола20213 иқтибос
    ABI

  13. Anisotropic compact stellar solution in general relativity

    Lipi Baskey, Saibal Ray, Shyam Das +2

    Мақола20233 иқтибос
    ABI

  14. Accelerating<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>T</mml:mi><mml:mo stretchy="false">)</mml:mo></mml:math>gravity models constrained by recent cosmological data

    V. F. Cardone, Ninfa Radicella, S. Camera

    Мақола20122 иқтибос
    ABI

  15. Regular black holes in<i>f</i>(<i>T</i>) Gravity through a nonlinear electrodynamics source

    Ednaldo L.B. Junior, Manuel E. Rodrigues, Mahouton J.S. Houndjo

    Мақола20152 иқтибос
    ABI

  16. Сарлавҳасиз

    Бошқа2 иқтибос
    ABI

  17. The Multi-messenger Matrix: The Future of Neutron Star Merger Constraints on the Nuclear Equation of State

    Ben Margalit, Brian D. Metzger

    Мақола20192 иқтибос
    ABI

  18. Сарлавҳасиз

    Бошқа2 иқтибос
    ABI

  19. Interpreting cosmological tensions from the effective field theory of torsional gravity

    Sheng-Feng Yan, Pierre Zhang, Jiewen Chen +3

    Мақола20202 иқтибос
    ABI

  20. A pulsar in a binary with a compact object in the mass gap between neutron stars and black holes

    E D Barr, Arunima Dutta, P. C. C. Freire +22

    Мақола20242 иқтибос
    ABI

  21. Anisotropic compact stars in complexity formalism and isotropic stars made of anisotropic fluid under minimal geometric deformation (MGD) context in $$f(\mathscr {T})$$ gravity-theory

    S. K. Maurya, Abdelghani Errehymy, Megandhren Govender +3

    Мақола20232 иқтибос
    ABI

  22. Constraining physical parameters of DESs via the secondary component of the GW190814 event and other self-bound NS pulsars in f(Q)-gravity theory

    Piyali Bhar, Abdelghani Errehymy, Saibal Ray

    Мақола20232 иқтибос
    ABI

  23. Cosmological observational constraints on the power law f(Q) type modified gravity theory

    Sanjay Mandal, Sneha Pradhan, P. K. Sahoo +1

    Мақола20232 иқтибос
    ABI

  24. Сарлавҳасиз

    Бошқа2 иқтибос
    ABI

  25. How Does the Electromagnetic Field Couple to Gravity, in Particular to Metric, Nonmetricity, Torsion, and Curvature?

    Friedrich W. Hehl, Yuri N. Obukhov

    Боб20072 иқтибос
    ABI