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Leveraging the full potential of current and future gravitational wave detectors requires accurate waveform models that encompass the complete physical scenarios capable of generating detectable signals. In recent years, significant efforts have been dedicated to developing waveform models for binary black holes beyond the standard spin-aligned, quasi-circular case. In this talk, we will briefly discuss the effective-one-body approach, focusing on the TEOBResumS-Dalí model. We will demonstrate its applicability to the study of non-circularized binary black holes, including eccentric systems, dynamical captures, and scattering events. Finally, we will discuss the ringdown modeling and recent developments concerning the real m=0 modes.