Gravitation & Cosmology

Papers
(The TQCC of Gravitation & Cosmology is 3. The table below lists those papers that are above that threshold based on CrossRef citation counts [max. 250 papers]. The publications cover those that have been published in the past four years, i.e., from 2020-04-01 to 2024-04-01.)
ArticleCitations
Dark Matter and Dark Radiation from Evaporating Kerr Primordial Black Holes21
Hybrid Metric-Palatini Gravity: Black Holes, Wormholes, Singularities, and Instabilities17
A Note on “Traversable Wormholes in Einstein–Dirac–Maxwell Theory”15
Remarks on Nonsingular Models of Hayward and Magnetized Black Hole with Rational Nonlinear Electrodynamics12
Accelerating Model of a Flat Universe in $$\boldsymbol{f(R,T)}$$ Gravity9
Big Rip and Big Crunch Cosmological Models in a Gravitational Field with Torsion9
Quantum Effects on Klein–Gordon Oscillator under a Cornell-type Potential in Kaluza–Klein Theory9
LRS Bianchi I Model with Bulk Viscosity in $$\boldsymbol{f(R,T)}$$ Gravity8
Cosmological Evolution of a Scalar-Charged Degenerate Cosmological Plasma with Higgs Scalar Fields7
Magnetically Charged AdS Black Holes and Joule–Thomson Expansion7
On Viability of Inflation in Nonminimal Kinetic Coupling Theory7
Constraining $$\boldsymbol{f(R,T)}$$ Gravity from the Dark Energy Density Parameter $$\boldsymbol{\Omega}_{\boldsymbol{\Lambda}}$$7
Interacting Holographic Dark Energy, the Present Accelerated Expansion and Black Holes7
Phase-Plane Analysis of FRW Cosmological Model with Variable $$\boldsymbol{\Lambda}$$ in Lyra Geometry6
Galactic Rotation Curves in Conformal Scalar-Tensor Gravity6
Constraints from Observational Data for a Running Cosmological Constant and Warm Dark Matter with Curvature6
Generation of Gravitational Waves by a Standing Electromagnetic Wave6
Cosmological Evolution of a Statistical System of Degenerate Scalarly Charged Fermions with an Asymmetric Scalar Doublet. I. Two-Component System of Assorted Charges5
Flow and Peculiar Velocities for Generic Motion in Spherically Symmetric Black Holes5
Stability of the Cosmological System of Degenerated Scalarly Charged Fermions and Higgs Scalar Fields. I. Mathematical Model of Linear Plane Perturbations5
Single-Field Model of Gravitational-Scalar Instability. I. Evolution of Perturbations5
The Kerr–Newman Black Hole Solution as Strong Gravity for Elementary Particles5
Sensitivity of the Gravity Assist to Variations of the Impact Parameter5
Anisotropic Model with Constant Jerk Parameter in $$\boldsymbol{f(R,T)}$$ Gravity5
Quintessence Behavior of New Tsallis Holographic Dark Energy in FRW Universe4
Nature of Higher-Dimensional Wormhole Mass Due to Accretion of Entropy Corrected Holographic and New Agegraphic Dark Energies4
Early Inflationary Phase with Canonical and Noncanonical Scalar Fields: A Symmetry-Based Approach4
Exact Cosmological Models in Modified $$\boldsymbol{f(R,L_{m})}$$ Gravity with Observational Constraints4
The Second Post-Newtonian Motion in Schwarzschild Spacetime4
Properties of the Vlasov–Maxwell–Einstein Equations and Their Application to the Problems of General Relativity4
Ruling Out Inflation Driven by a Power Law Potential: Kinetic Coupling Does Not Help4
Single-Field Model of Gravitational-Scalar Instability. II. Black Hole Formation4
Stability of the Cosmological System of Degenerate Scalarly Charged Fermions and Higgs Scalar Fields. II. Evolution of Short-wave Perturbations4
One-Loop Effective Action: Nonlocal Form Factors and Renormalization Group4
An Alternative Explanation of the Orbital Expansion of Titan and Other Bodies in the Solar System3
Two-Field Model of Gravitational-Scalar Instability and Formation of Supermassive Black Holes in the Early Universe3
Cosmological Density Perturbations from Matter Domination to Recombination in Newtonian and MONDian Gravity Scenarios3
Thermodynamic Properties of a Yukawa–Schwarzschild Black Hole in Noncommutative Gauge Gravity3
Diagnosing the Sharma–Mittal Holographic Dark Energy Model through the Statefinder3
Barrow Holographic Dark Energy with Hybrid Expansion Law3
Mass Generation by a Massless Scalar Field3
Axially Symmetric Type N Space-Time with a Naked Curvature Singularity and Closed Timelike Curves3
Stability of Thin Cylindrical Shell in Quadratic and Cubic Models of $$\boldsymbol{f(R)}$$ Gravity3
Spherically Symmetric Space-Times in Generalized Hybrid Metric-Palatini Gravity3
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