Auto-encoder model for faster generation of effective one-body gravitational waveform approximations

ArXi:2511.12642v2 Announce Type: replace-cross Upgrades to current gravitational wave detectors for the next observation run and upcoming third-generation observatories, like the Einstein telescope, are expected to have enormous improvements in detection sensitivities and compact object merger event rates. Estimation of source parameters for a wider parameter space that these detectable signals will lie in, will be a computational challenge.