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20102026
most citedThe Science of the Einstein Telescope

97 citations · 663 across the 44 of their papers we have counts for

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Showing 2023Show all

7 papers · 1 filter

gr-qc20231 cited

Effects of mass and self-interaction on nonlinear scalarization of scalar-Gauss-Bonnet black holes

Alexandre M. Pombo, Daniela D. Doneva

It was recently found that in certain flavours of scalar-Gauss-Bonnet gravity linearly stable bald black holes can co-exist with stable scalarized solutions. The transition between…

gr-qc2023

GRFolres: A code for modified gravity simulations in strong gravity

Llibert Aresté Saló, Sam E. Brady, Katy Clough +6

GRFolres is an open-source code for performing simulations in modified theories of gravity, based on the publicly available 3+1D numerical relativity code GRChombo. Note: Submitted…

gr-qc2023

Testing the limits of scalar-Gauss-Bonnet gravity through nonlinear evolutions of spin-induced scalarization

Daniela D. Doneva, Llibert Aresté Saló, Katy Clough +2

Quadratic theories of gravity with second order equations of motion provide an interesting model for testing deviations from general relativity in the strong gravity regime. Howeve…

gr-qc2023

Distinctive Features of Hairy Black Holes in Teleparallel Gauss-Bonnet Gravity

Sebastian Bahamonde, Daniela D. Doneva, Ludovic Ducobu +2

We examine the teleparallel formulation of non-minimally coupled scalar Einstein-Gauss-Bonnet gravity. In the teleparallel formulation, gravity is described by torsion instead of c…

gr-qc2023

Neutron stars in Gauss-Bonnet gravity -- nonlinear scalarization and gravitational phase transitions

Daniela D. Doneva, Christian J. Krüger, Kalin V. Staykov +1

It was recently discovered that scalarized neutron stars in scalar-tensor theories can undergo a gravitational phase transition to a non-scalarized (GR) state. Surprisingly, even t…

gr-qc2023

Differentially rotating scalarized neutron stars with realistic post-merger profile

Kalin V. Staykov, Daniela D. Doneva, Lavinia Heisenberg +2

The merger remnant of a binary neutron star coalescence is initially strongly differentially rotating. Some properties of these remnants can be accurately modeled through building…