Analysis of singularity-free cores: Exact two-fluid solutions for anisotropic stars in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si4.svg" display="inline" id="d1e467"> <mml:mrow> <mml:mi>f</mml:mi> <mml:mrow> <mml:mo>(</mml:mo> <mml:mi>R</mml:mi> <mml:mo>)</mml:mo> </mml:mrow> </mml:mrow> </mml:math> gravity
Tayyaba Naz, Adnan Malik, Khadija Akbar, M. Zeeshan Gul
Topics & Concepts
PhysicsQuark starStrange matterAnisotropyStarsBaryonEquation of stateEmbeddingPulsarMetric (unit)Stability (learning theory)Field (mathematics)Compact starAstrophysicsParticle physicsStrange quarkQuarkStellar structureComponent (thermodynamics)Exact solutions in general relativityMathematical physicsPhase transitionEnergy densityBaryon numberPhase (matter)Theoretical physicsDark matterMixing (physics)Energy (signal processing)Classical mechanicsSkyrmionTensor (intrinsic definition)Nuclear matterNeutron starField equationQuark modelPulsars and Gravitational Waves ResearchHigh-Energy Particle Collisions ResearchAstrophysical Phenomena and Observations