Abstract
Primordial black holes (PBHs) are probable candidates of dark matter (DM). In this review, we gathered data, evidence, and opinions from previous literatures to support the theory that PBHs are a form of DM. Besides, the formation of PBHs is introduced as well to give a more comprehensive description of PBHs. According to the results, the PBHs could assemble DM, or be DM itself, or generates DM, or influence DM. On the other hand, DM could have the similar influence on PBHs. Different relationships are discussed between PBHs and DM, including entropy, microlensing, distribution, growth rate, mass, and different detections (e.g., gammy ray). These results offer a guideline for future studies of PBHs.
Sign-in/Register to access full text options 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
