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gr-qc2026
Testing compact binary nature in eccentric orbits with third-generation detectors
Syed U. Naqvi, Kaushik Paul, Chandra Kant Mishra
The spin-induced quadrupole moment (SIQM) of a compact object provides a direct null test of the Kerr hypothesis. Most existing gravitational-wave tests of SIQM assume quasi-circul…
gr-qc2026
Large mass-ratio () inspiral-merger-ringdown model for eccentric binary black holes
Pratul Manna, Tamal RoyChowdhury, Chandra Kant Mishra
We present , a fully analytical entric-rid-nspiral-erger-ingdown model for the quadrupole ($\e…
gr-qc2026
Testing the Kerr hypothesis beyond the quadrupole with GW241011
Rimo Das, N. V. Krishnendu, M. Saleem +2
All multipole moments of a Kerr black hole are uniquely determined by its mass and spin. Gravitational wave observations can test this prediction by measuring spin-induced multipol…