Northwestern University astrophysicists are part of an international team of scientists using advanced simulation tools that has predicted the existence of merging massive, 30 solar mass black hole binaries in Milky Way-like galaxies, challenging previous theories.
The team, which includes Northwestern’s Vicky Kalogera, used the POSYDON code’s recent major advancements in simulating binary-star populations to provide new insights into the formation mechanisms of merging black holes in galaxies like our own. The University of Geneva (UNIGE) led the study; the team also included scientists from the University of Florida and other institutions.
The results are published today (June 29) in the journal Nature Astronomy. The study is the first to utilize the newly released open-source POSYDON software to investigate merging binary black holes.
“Models prior to POSYDON predicted a negligible formation rate of merging binary black holes in galaxies similar to the Milky Way, and they particularly did not anticipate the existence of merging black holes as massive as 30 times the mass of our sun,” said Kalogera, a co-author of the study. “POSYDON has demonstrated that such massive black holes might exist in Milky Way-like galaxies, and we have provided a physical explanation for why this is possible.”
Kalogera is the Daniel I. Linzer Distinguished Professor of Physics and Astronomy in Northwestern’s Weinberg College of Arts and Sciences and director of the Center for Interdisciplinary Exploration and Research in Astrophysics (CIERA).