Escaping the Pair-Instability Mass Gap with the Help of Dark Matter

Black Holes are not expected to form in the mass range of 60 M<sub>⊙</sub> to 130 M<sub>⊙</sub> because of the Pair-Instability Supernova (PISN). However, the recent observational evidence of GW190521 does not comply with the existing theory. Here, we have looked into the eff...

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Bibliographic Details
Main Authors: Raghav Narasimha, Della Vincent, Arun Kenath, Chandra Sivaram
Format: Article
Language:English
Published: MDPI AG 2023-03-01
Series:Physical Sciences Forum
Subjects:
Online Access:https://www.mdpi.com/2673-9984/7/1/24