Litcius/Paper detail

Anisotropic stars in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline" id="d1e1238" altimg="si6.svg"> <mml:mrow> <mml:mn>4</mml:mn> <mml:mi>D</mml:mi> </mml:mrow> </mml:math> Einstein–Gauss–Bonnet gravity

Takol Tangphati, Anirudh Pradhan, Ayan Banerjee, Grigoris Panotopoulos

2021Physics of the Dark Universe48 citationsDOIOpen Access PDF

Topics & Concepts

PhysicsQuark starStrange matterAnisotropyStarsContext (archaeology)QuarkCompact starEquation of stateAstrophysicsDegenerate energy levelsFermi Gamma-ray Space TelescopeGravitationQuantum electrodynamicsPulsarNeutron starColor superconductivityParticle physicsCoupling (piping)Stellar structureClassical mechanicsNeutrinoInstabilityQuark–gluon plasmaDark matterCosmologyTheoretical physicsGeneral relativityCoupling constantTop quarkTop quark condensateNuclear matterStrange quarkNonlinear systemStandard Model (mathematical formulation)Pulsars and Gravitational Waves ResearchCosmology and Gravitation TheoriesBlack Holes and Theoretical Physics
Anisotropic stars in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline" id="d1e1238" altimg="si6.svg"> <mml:mrow> <mml:mn>4</mml:mn> <mml:mi>D</mml:mi> </mml:mrow> </mml:math> Einstein–Gauss–Bonnet gravity | Litcius