activity
20102026
most citedThe Science of the Einstein Telescope

97 citations · 712 across the 52 of their papers we have counts for

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Showing 2025Show all

9 papers · 1 filter

astro-ph.HE2025

Differentially rotating neutron stars with dark matter cores

Lorenzo Cipriani, Violetta Sagun, Kalin V. Staykov +2

Dark matter is expected to accumulate inside neutron stars, modifying the structure of isolated stars and influencing both the dynamics of binary mergers and the evolution of the r…

gr-qc2025★ 3 cited

Quasi-Normal Mode Ringing of Binary Black Hole Mergers in Scalar-Gauss-Bonnet Gravity

Zexin Hu, Daniela D. Doneva, Stoytcho S. Yazadjiev +1

Observations of gravitational waves (GWs) generated by binary black hole (BBH) mergers provide us with a powerful way to explore the strong and highly dynamical regime of gravity t…

gr-qc2025

Ringdown mode amplitudes of charged binary black holes

Zexin Hu, Daniela D. Doneva, Ziming Wang +4

The ringdown phase of the binary black hole (BBH) merger provides a clean and direct probe of strong-field gravity and tests of the nature of black holes. The quasinormal mode (QNM…

gr-qc2025

Challenges in the nonlinear evolution of unequal mass binaries in sGB gravity

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

It has only recently become possible to simulate the full nonlinear dynamics of binary black holes in scalar-Gauss-Bonnet theories of gravity. The simulations remain technically ch…

gr-qc2025

No-hair theorems in General Relativity and scalar-tensor theories

Stoytcho Yazadjiev, Daniela Doneva

In the present review, we consider the status of the classification of the vacuum, stationary and asymptotically flat black holes in scalar-tensor gravity. Contrary to the similar…

gr-qc2025★ 4 cited

Rotating scalarized black holes: the role of the coupling

Kalin V. Staykov, Daniela D. Doneva, Pedro G. S. Fernandes +1

We perform an in-depth analysis of rotating scalarized black holes in scalar-Gauss-Bonnet gravity, where scalarization is induced by the spacetime curvature. Our results show that…