Primordial Black Holes as Viable Candidates for Dark Matter

Thursday 20 March 2025


The search for dark matter, a mysterious substance thought to make up approximately 27% of our universe’s mass-energy budget, has been ongoing for decades. Scientists have proposed various theories and mechanisms to explain its existence, but so far, none have been proven conclusively. A recent study published in the journal Physical Review D suggests that primordial black holes (PBHs) could be a viable candidate for dark matter.


The concept of PBHs dates back to the 1970s, when physicist Stephen Hawking proposed that tiny black holes could form during the early stages of the universe’s evolution. These miniature black holes would have been created by density fluctuations in the primordial plasma and would have evaporated quickly due to Hawking radiation.


The new study reexamines this idea, proposing that PBHs could be formed through a different mechanism: the supercooled radion phase transition (PT) in warped extra-dimensional models. In these models, the universe underwent a rapid cooling process, causing the formation of density fluctuations that would eventually collapse into PBHs.


The researchers used numerical simulations to study the properties of these PBHs and their potential impact on the cosmic microwave background radiation (CMB). They found that the predicted CMB signals from these PBHs are consistent with current observational data. Furthermore, they showed that the required mass range for these PBHs is within the detectable range of future gravitational wave detectors like LISA and ET.


The implications of this study are significant. If confirmed, PBHs could provide a new window into understanding dark matter’s properties and behavior. Future observations with next-generation telescopes and gravitational wave detectors could potentially confirm or rule out this hypothesis, providing crucial insights into the nature of dark matter.


In addition to their potential as dark matter candidates, PBHs could also serve as probes for testing theories of gravity and the early universe. Their formation and evolution would be influenced by various physical processes, such as Hawking radiation and gravitational wave emission. By studying these effects, scientists could gain a better understanding of fundamental physics and potentially uncover new phenomena.


The search for dark matter is an ongoing effort, with multiple approaches being explored simultaneously. The PBH hypothesis offers a unique perspective on this problem, highlighting the potential benefits of interdisciplinary research between cosmology, particle physics, and gravitational wave astronomy.


Cite this article: “Primordial Black Holes as Viable Candidates for Dark Matter”, The Science Archive, 2025.


Primordial Black Holes, Dark Matter, Cosmic Microwave Background Radiation, Supercooled Radion Phase Transition, Warped Extra-Dimensional Models, Gravitational Wave Detectors, Lisa, Et, Hawking Radiation, Gravitational Waves.


Reference: Anish Ghoshal, Eugenio Megias, Germano Nardini, Mariano Quiros, “Complementary Probes of Warped Extra Dimension: Colliders, Gravitational Waves and Primordial Black Holes from Phase Transitions” (2025).


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