DOAJ Open Access 2023

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

Raghav Narasimha Della Vincent Arun Kenath Chandra Sivaram

Abstrak

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 effects of Dark Matter (DM) in the progenitors of PISN in terms of luminosity, lifetime and temperature and have shown that in the presence of DM particles, the progenitors can overcome the PISN stage to collapse into a black hole (BH) as a remnant.

Topik & Kata Kunci

Mechanical drawing. Engineering graphics Physical and theoretical chemistry

Penulis (4)

Raghav Narasimha

Della Vincent

Arun Kenath

Chandra Sivaram

Format Sitasi

APA MLA BibTeX

Narasimha, R., Vincent, D., Kenath, A., Sivaram, C. (2023). Escaping the Pair-Instability Mass Gap with the Help of Dark Matter. https://doi.org/10.3390/ECU2023-14059

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Informasi Jurnal

Tahun Terbit: 2023
Sumber Database: DOAJ
DOI: 10.3390/ECU2023-14059
Akses: Open Access ✓