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Cosmic ray puzzle resolved as scientists hyperlink ‘knee’ formation to black holes

November 17, 2025
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Cosmic ray puzzle resolved as scientists hyperlink ‘knee’ formation to black holes
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LHAASO uncovers mystery of cosmic ray "knee" formation
LHAASO experiment. Credit score: LHAASO Collaboration

Milestone outcomes launched by the Massive Excessive Altitude Air Bathe Observatory (LHAASO) on November 16 have solved a decades-old thriller in regards to the cosmic ray power spectrum—which reveals a pointy lower in cosmic rays above 3 PeV, giving it an uncommon knee-like form.

The reason for the “knee” has remained unclear since its discovery practically 70 years in the past. Scientists have speculated that it’s linked to the acceleration restrict of the astrophysical sources of cosmic rays and displays the transition of the cosmic ray power spectrum from one power-law distribution to a different.

Now, nevertheless, two current research—revealed in Nationwide Science Evaluate and Science Bulletin, respectively—exhibit that micro-quasars pushed by black gap system accretion are highly effective particle accelerators within the Milky Method and are the seemingly supply of the “knee.” The research additionally advance our understanding of the intense bodily processes of black gap techniques.

The analysis was carried out by researchers from the Institute of Excessive Vitality Physics of the Chinese language Academy of Sciences (CAS), Nanjing College, the College of Science and Know-how of China of CAS, La Sapienza College of Rome, and different establishments.

Micro-quasars recognized as cosmic accelerators

Black holes, some of the enigmatic objects within the universe, generate relativistic jets when accreting materials from companion stars in binary techniques, forming “micro-quasars.” On this research, LHAASO systematically detected for the primary time ultra-high-energy gamma rays from 5 micro-quasars: SS 433, V4641 Sgr, GRS 1915+105, MAXI J1820+070, and Cygnus X-1.

Particularly, the ultra-high-energy radiation from SS 433 was discovered to overlap with an enormous atomic cloud, strongly suggesting that the high-energy protons are accelerated by the black gap and collide with surrounding matter.

The proton power on this system exceeded 1 PeV, with a complete energy output of roughly 1032 joules per second, equal to the power launched per second by 4 trillion of essentially the most highly effective hydrogen bombs. The gamma-ray power from V4641 Sgr was discovered to succeed in 0.8 PeV, making it one other “tremendous PeV particle accelerator,” whereas the father or mother particles producing these gamma rays had energies exceeding 10 PeV.

These outcomes show that micro-quasars are vital PeV particle accelerators within the Milky Method, addressing a long-standing situation in science: Whereas supernova remnants had been traditionally acknowledged as cosmic ray sources, each observational and theoretical research have proven that they can’t speed up cosmic rays to the energies of the “knee” and past.

Challenges in measuring cosmic ray spectra

To totally perceive this phenomenon, exact measurements of the power spectra of the assorted cosmic ray species together with their respective “knees” are important. Step one is to measure the power spectrum of the lightest nuclei—protons. Nonetheless, cosmic rays within the “knee” area are sparse and satellite tv for pc detectors have restricted acceptance, making detection akin to discovering a needle in a haystack.

In ground-based oblique measurements of cosmic ray particles, it’s not possible to keep away from atmospheric interference. This makes it tough to tell apart protons from different nuclei. For a very long time, this measurement was thought of not possible.

On this research, leveraging its world-leading ground-based cosmic ray observational gear, LHAASO developed multi-parameter measurement methods and chosen a big statistical pattern of high-purity protons, permitting for exact measurement of their power spectrum, with precision corresponding to that of satellite tv for pc experiments. This measurement revealed an power spectrum construction that was completely surprising, clearly displaying a brand new “high-energy part” as an alternative of a easy transition between power-law spectra.

A number of accelerators form cosmic ray origins

LHAASO’s new findings, along with the low-energy part measured by the space-borne AMS-02 experiment and the intermediate-energy part measured by the space-borne DArk Matter Particle Explorer (DAMPE) experiment, revealed the existence of a number of accelerators inside the Milky Method, with every possessing its personal distinctive acceleration functionality and power vary. The “knee” represents the acceleration restrict of the sources answerable for producing the high-energy part.

The complicated construction of the proton power spectrum signifies that cosmic ray protons within the PeV power vary primarily originate from “new sources” reminiscent of micro-quasars, which have an acceleration restrict considerably greater than that of supernova remnants. This allows them to generate high-energy cosmic rays that exceed the “knee.”

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Breakthroughs join black holes to cosmic rays

These two discoveries help one another, presenting a complete scientific image. This not solely marks a major development in resolving the long-standing thriller of the “knee” origin, but additionally presents essential observational proof for understanding the function of black holes within the origin of cosmic rays.

LHAASO’s hybrid detector array design permits for the detection of cosmic ray sources via ultra-high-energy gamma rays, whereas enabling exact measurement of cosmic ray particles within the neighborhood of the photo voltaic system. This strategy presents insights into the acceleration capabilities of sources at PeV energies and the spectral traits they contribute to cosmic rays. For the primary time, the “knee” construction has been observationally related to a particular sort of astrophysical supply—the black gap jet system.

LHAASO, which was designed, constructed, and is operated by Chinese language scientists, has taken the lead in high-energy cosmic-ray analysis on account of its sensitivity in each gamma ray astronomical exploration and cosmic ray precision measurement. It has achieved a sequence of discoveries which have a worldwide affect, thereby contributing to our data of the intense bodily processes within the universe.

Extra info:
Science Bulletin (2025). DOI: 10.1016/j.scib.2025.10.048

Nationwide Science Evaluate (2025).

Supplied by
Chinese language Academy of Sciences


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