Angelica Albertini
PhD student in theoretical physics, working on gravitational waves.
Hello! I am a PhD student in theoretical physics affiliated to the Astronomical Institute of the Czech Academy of Sciences and to the Faculty of Mathematics and Physics of Charles University in Prague.
My research involves the gravitational waves (GWs) emitted by black hole binaries. In particular, I am dealing with waveform modelling within the effective-one-body (EOB) approach. This approach provides a powerful semi-analytical framework that allows to evaluate reliable GW templates for compact binary coalescences.
My current work aims at extending the validity of the EOB model TEOBResumS to the large-mass-ratio regime, in view of the needs of the next generation of GW detectors.
On this website you can find the list of my publications, the list of my talks and my cv. Click here to see my research metrics on iNSPIRE.
selected publications
- Effective-one-body waveforms for extreme-mass-ratio binaries: Consistency with second-order gravitational self-force quasicircular results and extension to nonprecessing spins and eccentricityPhys. Rev. D, 2024
- Comparing second-order gravitational self-force and effective one body waveforms from inspiralling, quasicircular and nonspinning black hole binaries. II. The large-mass-ratio casePhys. Rev. D, 2022
- Comparing second-order gravitational self-force, numerical relativity, and effective one body waveforms from inspiralling, quasicircular, and nonspinning black hole binariesPhys. Rev. D, 2022