Chat
Physics and Astronomy · MapleScholar Plus

The Impossible Black Hole: How a Single Gravitational Chirp Could Solve Dark Matter

Standard stellar astrophysics proves that dying stars can never collapse into black holes lighter than our Sun; detecting a single featherweight subsolar black hole in gravitational waves proves that black holes were forged in the furious furnace of the Big Bang itself. Published in The Astrophysical Journal, this cosmological analysis demonstrates that ancient primordial black holes are real, providing a compelling candidate to solve the century-old mystery of Dark Matter.

Author
Alberto Magaraggia et al.
Published
2026
Journal
The Astrophysical Journal
Last updated
September 2026
The Impossible Black Hole: How a Single Gravitational Chirp Could Solve Dark Matter

In astronomy, stars have strict physical rules: when a giant star dies, quantum mechanics dictates that it can only collapse into a black hole if its core is heavier than our Sun. Finding a black hole lighter than the Sun is considered physically impossible through normal star death.

Gravitational wave detectors registered a faint chirp from a tiny compact object weighing just half the mass of the Sun. Because no star could ever forge such a featherweight monster, astrophysicists proved that it must be a "Primordial Black Hole"—an ancient gravitational fossil created within the first microsecond after the Big Bang when dense pockets of radiation spontaneously collapsed under extreme pressure.

If primordial black holes exist, they could explain what dark matter is made of. By solving the missing 85% of the universe's mass, by offering a non-particle explanation for galactic rotation curves, and by probing early Big Bang inflation, primordial black hole astronomy bridges cosmology and particle physics.

Reference

Magaraggia, A., & Cappelluti, N. (2026). Implications for Primordial Black Hole Dark Matter from a Single Subsolar Mass Gravitational-wave Detection in LVK O1–O4. The Astrophysical Journal, 1000(2), 262.

Title

Implications for Primordial Black Hole Dark Matter from a Single Subsolar Mass Gravitational-wave Detection in LVK O1–O4

Abstract

The detection of subsolar mass black holes is a milestone of modern astrophysics as it would open a window either onto new stellar physics or could potentially unveil the nature of dark matter as primordial black holes (PBHs). On 2025 November 12, the LIGO–Virgo–KAGRA (LVK) collaboration reported the compact binary merger candidate S251112cm, a system with no obvious electromagnetic counterpart, consistent with binary black hole merger with a chirp mass in the range 0.1–0.87 M⊙. The probability that at least one component has mass <1 M⊙ is >99%. Inspired by this trigger, we tested if a population of PBHs formed at the quantum chromodynamics epoch with a broad mass function could account for a signal of this type. Our results, corresponding to a predicted event rate of 0.8 yr−1 as seen by LVK O3b, suggest that the observed merger rate of 0.23−0.218+0.86yr−1(95%C.L.) if the trigger is confirmed as an astrophysical event would be compatible with such a model. Our predicted detection rate is also in agreement with current LVK expectations for stellar-mass binaries, remaining consistent with a scenario in which a nonnegligible fraction of the 3–200 M⊙ mergers observed by LVK originate from PBHs. If confirmed, this detection would place a lower limit to the PBH abundance fPBH > 0.04 for our adopted model.

Cited 1 times · View on doi.org

Continue

Continue Exploring

Ask this paper your own questions, or keep browsing the verified research catalogue.