Stellar Initial Mass Function (IMF) Probed with Supernova Rates and Neutrino Background: Cosmic-average IMF Slope Is ≃2–3 Similar to the Salpeter IMF

The stellar initial mass function (IMF) is expressed by ϕ ( m ) ∝ m ^− ^α with the slope α , and known as a poorly constrained but very important function in studies of star and galaxy formation. There are no sensible observational constraints on the IMF slopes beyond the Milky Way and nearby galaxi...

Ausführliche Beschreibung

Bibliographische Detailangaben
Hauptverfasser: Shohei Aoyama, Masami Ouchi, Yuichi Harikane
Format: Artikel
Sprache:English
Veröffentlicht: IOP Publishing 2023-01-01
Schriftenreihe:The Astrophysical Journal
Schlagworte:
Online Zugang:https://doi.org/10.3847/1538-4357/acba87