Updated black-hole formation bounds show Population III stars can constrain bosonic asymmetric dark matter at lower masses than neutron stars when a Bose-Einstein condensate forms.
Title resolution pending
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
astro-ph.CO 1years
2024 1verdicts
CONDITIONAL 1representative citing papers
citing papers explorer
-
Constraining Asymmetric DM Properties by Black Hole Formation in Neutron Stars and Population III Stars
Updated black-hole formation bounds show Population III stars can constrain bosonic asymmetric dark matter at lower masses than neutron stars when a Bose-Einstein condensate forms.