2 papers
gr-qc2026
Estimation of the MTOV precision for ET, CE, and NEMO from the post-merger of BNS coalescences
Gabriela Conde-Saavedra, Odylio Denys Aguiar, Henrique P. de Oliveira +1
The detection of the gravitational waves produced after the coalescence of two neutron stars is greatly anticipated because it will be able to provide information about matter in e…
gr-qc2025
Distorted black holes: a characteristic view
H. P. de Oliveira
We investigate the interaction between a non-rotating black hole and incoming gravitational waves using the characteristic formulation of the Einstein field equations, framed as a…