Studente IRACI, FRANCESCO
Facoltà/Dipartimento Dipartimento di Fisica e Astronomia "Galileo Galilei" - DFA
Corso di studio ASTROPHYSICS AND COSMOLOGY Laurea Magistrale (D.M. 270/2004)
Anno Accademico 2021
Titolo originale Impact of core-collapse supernova models on the population of binary black holes
Abstract in italiano With an initial population of isolated binary stars, I am using the population synthesis code SEVN which describes stellar evolution with a set of precomputed look-up tables. I am running the code for a wide range of metallicities in order to have a complete landscape of remnants coming from metal poor and metal rich stars. For each of them I use three Core collapse supernova models: rapid, delayed and compactness. I compare the outcomes with pythons scripts, studying the black hole mass spectrum and the relation between zero-age main sequence mass and the black hole mass.
Abstract in inglese With an initial population of isolated binary stars, I am using the population synthesis code SEVN which describes stellar evolution with a set of precomputed look-up tables. I am running the code for a wide range of metallicities in order to have a complete landscape of remnants coming from metal poor and metal rich stars. For each of them I use three Core collapse supernova models: rapid, delayed and compactness. I compare the outcomes with pythons scripts, studying the black hole mass spectrum and the relation between zero-age main sequence mass and the black hole mass.
Parola chiave binary black holes
star: binaries
supernovae
Relatore MAPELLI, MICHELA
Appare nelle tipologie: Lauree magistrali
File in questo prodotto:
File Dimensione Formato  
Iraci_Francesco.pdf 10.07 MB Adobe PDF Visualizza/Apri

The text of this website © Università degli studi di Padova. Full Text are published under a non-exclusive license. Metadata are under a CC0 License

Utilizza questo identificativo per citare o creare un link a questo documento: http://hdl.handle.net/20.500.12608/37076