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Иш: Testing linear non-minimal coupling in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si447.svg" display="inline" id="d1e4384"> <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 using X-ray binary pulsars constrained by NICER observations

  1. Anisotropic Stars II: Stability

    Krsna Dev, Marcelo Gleiser

    Мақола20034 иқтибос
    ABI

  2. On the stability and physical properties of an exact relativistic model for a superdense star

    Henning Knutsen

    Мақола19884 иқтибос
    ABI

  3. The MACHO Project: Microlensing Results from 5.7 Years of Large Magellanic Cloud Observations

    C. Alcock, R. A. Allsman, D. R. Alves +22

    Мақола20003 иқтибос
    ABI

  4. Observation of Gravitational Waves from Two Neutron Star–Black Hole Coalescences

    R. Abbott, T. D. Abbott, S. Abraham +97

    Мақола20213 иқтибос
    ABI

  5. Observation of Gravitational Waves from Two Neutron Star-Black Hole Coalescences

    R. Abbott, T. D. Abbott, S. Abraham +97

    Мақола20213 иқтибос
    ABI

  6. Сарлавҳасиз

    Бошқа3 иқтибос
    ABI

  7. Comment on “Energy conditions 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”

    Avik De, Loo Tee How

    Мақола20223 иқтибос
    ABI

  8. Investigation of Bardeen stellar structures in modified f(R,ϕ,X) theory of gravity

    Adnan Malik, Eman M. Moneer, Ayesha Sanaullah +2

    Мақола20243 иқтибос
    ABI

  9. Cracking of Homogeneous Self-Gravitating Compact Objects Induced by Fluctuations of Local Anisotropy

    A. Di Prisco, L. Herrera, Víctor Varela

    Мақола19973 иқтибос
    ABI

  10. On Stars, Their Evolution and Their Stability

    S. Chandrasekhar

    Мақола19843 иқтибос
    ABI

  11. A NICER View of the Massive Pulsar PSR J0740+6620 Informed by Radio Timing and XMM-Newton Spectroscopy

    Riley, Thomas E., Watts, Anna L., Ray, Paul S. +27

    Мақола20213 иқтибос
    ABI

  12. Сарлавҳасиз

    Бошқа2 иқтибос
    ABI

  13. Exact mapping between tensor and most general scalar power spectra

    Jose Beltrán Jiménez, Marcello Musso, Christophe Ringeval

    Мақола20132 иқтибос
    ABI

  14. Peering into the Dark Side: Magnesium Lines Establish a Massive Neutron Star in PSR J2215+5135

    M. Linares, T. Shahbaz, J. Casares

    Мақола20182 иқтибос
    ABI

  15. Quasinormal modes of dirty black holes in the effective theory of gravity with a third order curvature term

    Jerzy Matyjasek

    Мақола20202 иқтибос
    ABI

  16. Peering into the dark side: Magnesium lines establish a massive neutron star in PSR J2215+5135

    M. Linares, T. Shahbaz, J. Casares

    Мақола20182 иқтибос
    ABI

  17. Quasinormal modes of growing dirty black holes

    Jamie Bamber, Oliver J. Tattersall, Katy Clough +1

    Мақола20212 иқтибос
    ABI

  18. Сарлавҳасиз

    Бошқа2 иқтибос
    ABI

  19. Regge pole description of scattering by dirty black holes

    Théo Torres, Mohamed Ould El Hadj, Shi-Qian Hu +1

    Мақола20232 иқтибос
    ABI

  20. Charged stellar structure with Krori–Barua potentials in f(R,ϕ,X) gravity admitting Chaplygin equation of state

    Adnan Malik

    Мақола20242 иқтибос
    ABI

  21. Role of <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si1.svg"><mml:mi mathvariant="script">F</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mi mathvariant="script">Q</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="script">T</mml:mi><mml:mo stretchy="false">)</mml:mo></mml:math> gravity with class one space-time in constructing new spherically symmetric stellar solutions

    S. K. Maurya, Jitendra Kumar, Sourav Chaudhary +3

    Мақола20242 иқтибос
    ABI

  22. Self bound compact stars in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si13.svg" display="inline" id="d1e1787"><mml:mrow><mml:mi>f</mml:mi><mml:mrow><mml:mo>(</mml:mo><mml:mi>R</mml:mi><mml:mo>,</mml:mo><mml:mi>T</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mrow></mml:math> gravity admitting <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si179.svg" display="inline" id="d1e1804"><mml:mrow><mml:mi>C</mml:mi><mml:mi>F</mml:mi><mml:mi>L</mml:mi></mml:mrow></mml:math> equation of state in presence of non-minimal <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si542.svg" display="inline" id="d1e1814"><mml:mrow><mml:mi>Q</mml:mi><mml:mi>C</mml:mi><mml:mi>D</mml:mi></mml:mrow></mml:math> correction factor

    K. B. Goswami, Debadri Bhattacharjee, P. K. Chattopadhyay +1

    Мақола20242 иқтибос
    ABI

  23. Anisotropic quark stars in the modified f(Q, T) gravity: an application of the MIT bag model

    Hafiza Rizwana Kausar, Amal Majid, Bismah Nadeem

    Мақола20252 иқтибос
    ABI

  24. Anisotropic dark matter stars in gravity’s rainbow

    Takol Tangphati, İzzet Sakallı, Ayan Banerjee +1

    МақолаCosmology and Gravitation TheoriesThe European Physical Journal C20252 иқтибос
    ABI

  25. Dark-matter spike at the galactic center?

    Piero Ullio, Hongsheng Zhao, Marc Kamionkowski

    Мақола20012 иқтибос
    ABI