Trieste, Italy (SPX) Jan 19, 2022 With a new computational approach, SISSA researchers have been...
In a first paper of a series just published in The Astrophysical Journal, the authors have investigated the demographics of stellar mass black holes, which are black holes with masses between a few to some hundred solar masses, that originated at the end of the life of massive stars.
According to the new research, a remarkable amount around 1% of the overall ordinary matter of the Universe is locked up in stellar mass black holes.
Astonishingly, the researchers have found that the number of black holes within the observable Universe at present time is about 40 trillions, 40 billion billions.
"A new method to calculate the number of black holes As the authors of the research explain:"This important result has been obtained thanks to an original approach which combines the state-of-the-art stellar and binary evolution code SEVN developed by SISSA researcher Dr. Mario Spera to empirical prescriptions for relevant physical properties of galaxies, especially the rate of star formation, the amount of stellar mass and the metallicity of the interstellar medium.
Exploiting these crucial ingredients in a selfconsistent approach, thanks to their new computation approach, the researchers have then derived the number of stellar black holes and their mass distribution across the whole history of the Universe.
What's the origin of most massive stellar black holes? The estimate of the number of black holes in the observable Universe is not the only issue investigated by the scientists in this piece of research.
In collaboration with Dr. Ugo Di Carlo and Prof. Michela Mapelli from University of Padova, they have also explored the various formation channels for black holes of different masses, like isolated stars, binary systems and stellar clusters.
According to their work, the most massive stellar black holes originate mainly from dynamical events in stellar clusters.
"Specifically, the researchers have shown that such events are required to explain the mass function of coalescing black holes as estimated from gravitational wave observations by the LIGO/Virgo collaboration. Lumen Boco, co-author of the paper, comments:"Our work provides a robust theory for the generation of light seeds formassive black holes at high redshift, and can constitute a starting point to investigate the origin of 'heavy seeds', that we will pursue in a forthcoming paper.
Alex Sicilia's work occurs in the context of a prestigious Innovative Training Network Project "BiD4BESt - Big Data Application for Black Hole Evolution Studies" co-PIed by Prof. Andrea Lapi from SISSA, that has been funded by the European Union with about 3.5 million Euros overall; it involves several academic and industrial partners, to provide Ph.D. training to 13 early stage researchers in the area of black hole formation and evolution, by exploiting advanced data science techniques.