Could Primordial Black Holes Be the Missing Link to Dark Matter?

Could Primordial Black Holes Be the Missing Link to Dark Matter

Could Primordial Black Holes Be the Missing Link to Dark Matter?

The Laser Interferometer Gravitational-Wave Observatory (LIGO) has recorded mergers involving unusually massive black holes. These findings push the boundaries of classical black hole formation theories, which explain black holes as the remnants of massive stars collapsing under their gravity after exhausting their nuclear fuel. The existence of these unexpectedly large black holes suggests alternative origins, such as primordial black holes formed during the universe’s infancy.



Traditional Black Hole Formation Explained

Classical black hole formation occurs when massive stars, exceeding 20 times the Sun’s mass, reach the end of their life cycle. After burning through their nuclear fuel, these stars explode in supernovae, ejecting their outer layers. The remaining core collapses under its gravity. If the core’s mass surpasses a critical threshold, typically several solar masses, it forms a singularity—a point of infinite density enclosed by an event horizon, beyond which nothing, not even light, can escape.

Massive Black Holes Detected by LIGO Defy Expectations

Recent gravitational wave data from LIGO has revealed black holes that dwarf those commonly observed in the Milky Way. These massive black holes do not align with the conventional formation mechanisms described above. This anomaly has led researchers to hypothesize that these objects might be primordial black holes, born from density fluctuations in the early universe. Such primordial black holes could potentially explain phenomena like dark matter—a mysterious substance that makes up roughly 85% of the universe’s matter.

Image from NASA’s Hubble Space Telescope of a galaxy cluster that could contain dark matter (blue-shaded region).

Could Primordial Black Holes Explain Dark Matter?

Primordial black holes have been proposed as candidates for dark matter. These ancient objects could theoretically constitute up to 100% of dark matter while also accounting for the black hole merger rates observed by LIGO. However, their role in dark matter hinges on their abundance and detectability. If these black holes exist in the Milky Way’s dark matter halo, they should cause gravitational microlensing events—temporary brightening of distant stars as the black holes pass in front of them.

The Large Magellanic cloud. Credit: CTIO/NOIRLab/NSF/AURA/SMASH/D. Nidever (Montana State University) Image processing: Travis Rector (University of Alaska Anchorage), Mahdi Zamani & Davide de Martin.

Microlensing Studies Limit Primordial Black Hole Contributions

A recent study by Przemek Mroz and colleagues analyzed data from the Optical Gravitational Lensing Experiment (OGLE) to search for microlensing events caused by primordial black holes. The OGLE survey, conducted at the Las Campanas Observatory in Chile using a 1.3-meter telescope, has been monitoring the sky since 1992. Over 20 years of data focused on the Large Magellanic Cloud (LMC) were examined for long-timescale microlensing events, which would indicate the presence of supermassive primordial black holes.

Key Findings from the OGLE Survey

The analysis found no microlensing events lasting longer than a year—a key signature of massive primordial black holes. Shorter microlensing events were detected, but these are more likely attributed to stellar activity rather than primordial black holes. Based on these results:

Primordial black holes up to 6.3 million solar masses can account for no more than 1% of dark matter.

Larger primordial black holes, up to 860 million solar masses, cannot exceed 10% of dark matter.

Conclusions: Primordial Black Holes and Dark Matter

The OGLE findings strongly suggest that primordial black holes cannot constitute a significant fraction of dark matter. Despite their theoretical appeal and the intriguing possibility of their role in early cosmic structure, the data from microlensing studies in the LMC indicate their scarcity.

What’s Next for Dark Matter Research?

The quest to identify the nature of dark matter continues, with researchers exploring alternatives such as weakly interacting massive particles (WIMPs), axions, and other exotic particles. While LIGO’s observations challenge existing models of black hole formation, they also underscore the complexity of cosmic phenomena and the need for multi-pronged investigative approaches to unravel the mysteries of the universe.

Source: Could Primordial Black Holes Be the Missing Link to Dark Matter?

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