Francesco Iacovelli
Research Subjects
Research Interests
Francesco Iacovelli has a total of 7 co-authors. Here are the top co-authors by number of shared publications:
- Edwin Genoud-Prachex
Institute for Theoretical Physics, Goethe University, 60438 Frankfurt am Main, Germany
2 shared publications - Matteo Schulz2 shared publications
- Michele Maggiore
Département de Physique Théorique, Université de Genève, 24 quai Ernest Ansermet, 1211 Genève 4, Switzerland
2 shared publications - Michele Mancarella
Dipartimento di Fisica "G. Occhialini" Università degli Studi di Milano-Bicocca Piazza della Scienza 3 20126 Milano Italy
2 shared publications - Michele Moresco
Dipartimento di Fisica e Astronomia “Augusto Righi” – Alma Mater Studiorum Università di Bologna
2 shared publications - Nicola Borghi
Dipartimento di Fisica e Astronomia "Augusto Righi" Università di Bologna via Piero Gobetti 93/2 I-40129 Bologna Italy
2 shared publications
Latest Publications
- Open Access
Gravitational-wave cosmology with dark sirens: state of the art and perspectives for 3G detectors
A joint fit of the mass and redshift distributions of the population of Binary Black Holes detected with Gravitational-Wave observations can be used to obtain constraints on the Hubble parameter and on deviations from General Relativity in the propagation of Gravitational Waves. We first present applications of this technique to the latest catalog of Gravitational-Wave events, focusing on the comparison of different parametrizations for the source-frame mass distribution of Black Hole Binaries. We find that models with more than one feature are favourite by the data, as suggested by population studies, even when varying the cosmology. Then, we discuss perspectives for the use of this technique with third generation Gravitational-Wave detectors, exploiting the recently developed Fisher information matrix Python code GWFAST.
Open AccessGravitational-wave cosmology with dark sirens: state of the art and perspectives for 3G detectors
A joint fit of the mass and redshift distributions of the population of Binary Black Holes detected with Gravitational-Wave observations can be used to obtain constraints on the Hubble parameter and on deviations from General Relativity in the propagation of Gravitational Waves. We first present applications of this technique to the latest catalog of Gravitational-Wave events, focusing on the comparison of different parametrizations for the source-frame mass distribution of Black Hole Binaries. We find that models with more than one feature are favourite by the data, as suggested by population studies, even when varying the cosmology. Then, we discuss perspectives for the use of this technique with third generation Gravitational-Wave detectors, exploiting the recently developed Fisher information matrix Python code GWFAST.
- Open Access
- 12 November 2022
- Published by Sissa Medialab Srl
- Vol. 414, 127
Gravitational-wave cosmology with dark sirens: state of the art and perspectives for 3G detectors
A joint fit of the mass and redshift distributions of the population of Binary Black Holes detected with Gravitational-Wave observations can be used to obtain constraints on the Hubble parameter and on deviations from General Relativity in the propagation of Gravitational Waves. We first present applications of this technique to the latest catalog of Gravitational-Wave events, focusing on the comparison of different parametrizations for the source-frame mass distribution of Black Hole Binaries. We find that models with more than one feature are favourite by the data, as suggested by population studies, even when varying the cosmology. Then, we discuss perspectives for the use of this technique with third generation Gravitational--Wave detectors, exploiting the recently developed Fisher information matrix Python code GWFAST.
- 12 November 2022
- Published by Sissa Medialab Srl
- Vol. 414, 127
Open AccessGravitational-wave cosmology with dark sirens: state of the art and perspectives for 3G detectors
A joint fit of the mass and redshift distributions of the population of Binary Black Holes detected with Gravitational-Wave observations can be used to obtain constraints on the Hubble parameter and on deviations from General Relativity in the propagation of Gravitational Waves. We first present applications of this technique to the latest catalog of Gravitational-Wave events, focusing on the comparison of different parametrizations for the source-frame mass distribution of Black Hole Binaries. We find that models with more than one feature are favourite by the data, as suggested by population studies, even when varying the cosmology. Then, we discuss perspectives for the use of this technique with third generation Gravitational--Wave detectors, exploiting the recently developed Fisher information matrix Python code GWFAST.