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20242026
most citedQuasinormal modes and their excitation beyond general relativity

36 citations · 71 across the 13 of their papers we have counts for

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gr-qc2026

Anisotropic Fluid Model for Massive Boson Stars: Spherically Symmetric Configurations

Ethan McKeever, Victor Guedes, Shu Yan Lau +1

Boson stars are among the best-studied exotic compact objects and constitute one of the few black-hole mimickers for which both the formation mechanism and dynamical behavior can b…

gr-qc2026

New Universal Relations for Magnetized Neutron Stars

Byon N. Jayawiguna, Siddarth Ajith, Takuya Katagiri +2

Unlike the neutron-star mass--radius relation, which depends sensitively on the internal stellar structure through the equation of state of dense nuclear matter, certain neutron-st…

gr-qc2026

Out-of-Equilibrium Effects in Non-Radial Relativistic Stellar Perturbations: A Model-Agnostic Formulation and Mode Analysis

Takuya Katagiri, Victor Guedes, Kent Yagi

We present a systematic, model-agnostic analysis of out-of-equilibrium effects, including viscosity and thermal conductivity, in non-radial oscillations of relativistic stars. Exte…

gr-qc2026

Spacetime Quasi-normal Mode Oscillations of Anisotropic Neutron Stars

Jihao Yu, Victor Guedes, Shu Yan Lau +2

Neutron star asteroseismology offers a unique opportunity to probe nuclear physics through stellar oscillations. Although the pressure inside of a neutron star is typically assumed…

gr-qc2024★ 4 cited

New modeling for hybrid stars with an elastic quark core

Zoey Zhiyuan Dong, Shu Yan Lau, Kent Yagi

Heavy neutron stars may contain solid quark cores as motivated by, e.g. the crystalline color superconducting phase, forming elastic hybrid stars (HSs). Many previous studies assum…

gr-qc2024★ 9 cited

Probing dark-matter effects with gravitational waves using the parameterized post-Einsteinian framework

Eileen Wilcox, David Nichols, Kent Yagi

A massive black hole can develop a dark-matter overdensity, and the dark matter changes the evolution of a stellar-mass compact object inspiraling around the massive black hole thr…

gr-qc2024★ 4 cited

Love-C relations for elastic hybrid stars

Zoey Zhiyuan Dong, Joshua Cole Faggert, Shu Yan Lau +1

Neutron stars (NSs) provide a unique laboratory to study matter under extreme densities. Recent observations from gravitational and electromagnetic waves have enabled constraints o…

gr-qc2024★ 10 cited

Nonradial instabilities in anisotropic neutron stars

Shu Yan Lau, Siddarth Ajith, Victor Guedes +1

Non-radial oscillation modes of a neutron star possess valuable information about its internal structure and nuclear physics. Starting from the quadrupolar order, such modes under…

gr-qc2024★ 36 cited

Quasinormal modes and their excitation beyond general relativity

Hector O. Silva, Giovanni Tambalo, Kostas Glampedakis +2

The response of black holes to small perturbations is known to be partially described by a superposition of quasinormal modes. Despite their importance to enable strong-field tests…