activity
20242026
collaborators

6 papers

gr-qc2026

Hybrid Stars with Post-Merger Rotation Profiles

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

We study the effect of differential rotation on hybrid stars with the first-order deconfinement phase transition from hadronic to color superconducting quark matter. The differenti…

gr-qc2026

Phase transition structure of scalarized neutron stars: the effect of rotation and linear coupling

Kalin V. Staykov, Fethi M. Ramazanoğlu, Daniela D. Doneva +1

There has been a recent revival in understanding the spontaneous scalarization phenomenon in scalar-tensor gravity as a phase transition. Using the tools of the Landau theory, we n…

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

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…

gr-qc2025

Axisymmetric stability of neutron stars as extreme rotators in massive scalar-tensor theory

Alan Tsz-Lok Lam, Kalin V. Staykov, Hao-Jui Kuan +2

Differentially rotating scalarized neutron stars, mimickers of binary merger remnants, can possess an enormous angular momentum larger than what could possibly be sustained in a ne…

gr-qc2024

Neutron stars in extended scalar-Gauss-Bonnet gravity: the richness of the solution spectrum

Kalin V. Staykov, Peter Y. Yordanov, Daniela D. Doneva +1

Neutron stars are natural laboratories for testing gravity in the strong field regime. That is why the full spectrum of neutron star solutions in different modified theories should…