3 papers
gr-qc2025
Black-Hole Cartography
Richard Dyer, Christopher J. Moore
Quasinormal modes (QNMs) are usually characterized by their time dependence; oscillations at specific frequencies predicted by black hole (BH) perturbation theory. QNMs are routine…
astro-ph.HE2024
Eccentric Signatures of Stellar-Mass Binary Black Holes with Circumbinary Disks in LISA
Isobel M. Romero-Shaw, Samir Goorachurn, Magdalena Siwek +1
Stellar-mass binary black holes may have circumbinary disks if formed through common-envelope evolution or within gaseous environments. Disks can drive binaries into wider and more…
astro-ph.HE2024
Expected insights on type Ia supernovae from LISA's gravitational wave observations
Valeriya Korol, Riccardo Buscicchio, Ruediger Pakmor +3
The nature of progenitors of Type Ia supernovae has long been debated, primarily due to the elusiveness of the progenitor systems to traditional electromagnetic observation methods…