Rotating black holes in 4D Einstein-Gauss-Bonnet gravity and its shadow
Recently there has been a surge of interest in regularizing, a D→ 4 limit of, the Einstein-
Gauss-Bonnet (EGB) gravity, and the resulting regularized 4D EGB gravity has nontrivial …
Gauss-Bonnet (EGB) gravity, and the resulting regularized 4D EGB gravity has nontrivial …
[HTML][HTML] Anisotropic quark stars in Einstein-Gauss-Bonnet theory
Recent progress in the determination of both masses and radii of neutron stars has put
strong constraints on the equation of state (EoS) above the nuclear saturation density. Within …
strong constraints on the equation of state (EoS) above the nuclear saturation density. Within …
Radiating black holes in the novel 4D Einstein–Gauss–Bonnet gravity
Abstract Recently Glavan and Lin (2020) formulated a novel Einstein–Gauss–Bonnet gravity
in which the Gauss–Bonnet coupling has been rescaled as α∕(D− 4) and the 4 D theory is …
in which the Gauss–Bonnet coupling has been rescaled as α∕(D− 4) and the 4 D theory is …
Anisotropic stars in 4D Einstein–Gauss–Bonnet gravity
The current trend concerning dense matter physics at sufficiently high densities and low
temperatures is expected to behave as a degenerate Fermi gas of quarks forming Cooper …
temperatures is expected to behave as a degenerate Fermi gas of quarks forming Cooper …
[HTML][HTML] Minimally deformed anisotropic stars by gravitational decoupling in Einstein–Gauss–Bonnet gravity
In this article, we develop a theoretical framework to study compact stars in Einstein gravity
with the Gauss–Bonnet (GB) combination of quadratic curvature terms. We mainly analyzed …
with the Gauss–Bonnet (GB) combination of quadratic curvature terms. We mainly analyzed …
Phase transition of AdS black holes in 4D EGB gravity coupled to nonlinear electrodynamics
Abstract Einstein–Gauss–Bonnet (EGB) gravity is an outcome of quadratic curvature
corrections to the Einstein–Hilbert gravity action in the form of a Gauss–Bonnet (GB) term in …
corrections to the Einstein–Hilbert gravity action in the form of a Gauss–Bonnet (GB) term in …
Quark stars in the Einstein–Gauss–Bonnet theory: A new branch of stellar configurations
The observations of pulsars heavier than 2 M⊙ have put strong constraints on the equation
of state (EoS) above nuclear saturation density. For this reason, the internal structure of a …
of state (EoS) above nuclear saturation density. For this reason, the internal structure of a …
Dust collapse in 4d einstein–gauss–bonnet gravity
We consider gravitational collapse in the recently proposed 4D limit of Einstein–Gauss–
Bonnet gravity. We show that for collapse of a sphere made of homogeneous dust the …
Bonnet gravity. We show that for collapse of a sphere made of homogeneous dust the …
Exploring perfect fluid dark matter with EHT results of Sgr A* through rotating 4D-EGB black holes
We investigate the rotating 4D Gauss–Bonnet (GB) black holes surrounded by Perfect Fluid
Dark Matter (PFDM) using the Event Horizon Telescope (EHT) observations of Sagittarius …
Dark Matter (PFDM) using the Event Horizon Telescope (EHT) observations of Sagittarius …
Regular black holes in Einstein-Gauss-Bonnet gravity
Einstein-Gauss-Bonnet theory, a natural generalization of general relativity to a higher
dimension, admits a static spherically symmetric black hole which was obtained by …
dimension, admits a static spherically symmetric black hole which was obtained by …