
Alchemist's Dream Realized As Lead Turned Into Gold at Large Hadron Collider
Based on facts, either observed and verified firsthand by the reporter, or reported and verified from knowledgeable sources.
Newsweek AI is in beta. Translations may contain inaccuracies—please refer to the original content.
Fulfilling the dream of medieval alchemists, physicists have observed the transmutation of lead into gold—through nuclear physics at the Large Hadron Collider (LHC), the world's most powerful particle accelerator.
For centuries, this idea of turning lead into gold—chrysopoeia—seemed out of reach. The two metals share a similar density, but modern science later proved they are distinct elements and chemically non-interchangeable.
However, gold can be produced, albeit in microscopic amounts, at the heart of ALICE (A Large Ion Collider Experiment), one of the four main instruments on the LHC at CERN, the European Organization for Nuclear Research.
The ALICE experiment is dedicated to heavy-ion physics and investigates matter under extreme energy densities. During high-energy collisions of lead nuclei at the LHC, scientists can momentarily recreate quark–gluon plasma, a state of matter that existed just millionths of a second after the Big Bang.
Still, gold is not born from these direct crashes. Instead, it forms in a more subtle scenario—when lead nuclei almost collide head-on, but miss.
"It is impressive to see that our detectors can handle head-on collisions producing thousands of particles, while also being sensitive to collisions where only a few particles are produced at a time, enabling the study of electromagnetic 'nuclear transmutation' processes," ALICE spokesperson Marco Van Leeuwen, said in a statement.
An image of the tunnel inside a large hadron collider.
An image of the tunnel inside a large hadron collider.
Getty Images
In near-miss encounters, intense electromagnetic fields surrounding the rapidly moving lead nuclei generate brief pulses of photons. T
When these photons interact with nuclei, they cause a phenomenon known as electromagnetic dissociation, in which protons and neutrons are ejected from a nucleus.
In rare cases, three protons are knocked out of a lead nucleus, leaving behind gold in its place.
The ALICE team used specialized instruments known as Zero Degree Calorimeters (ZDC) to measure these rare events.
By detecting the number of protons and neutrons ejected in collisions, researchers were able to distinguish between the creation of other heavy elements like thallium and mercury—and gold.
Sadly, the resulting gold nuclei do not stick around for long. Traveling at nearly the speed of light, they smash into the walls of the collider or its components and disintegrate almost instantly into smaller particles.
Still, the numbers are impressive: during Run 2 of the LHC (2015–2018), about 86 billion gold nuclei were produced. Run 3 has already nearly doubled that count.
Yet despite this, the total mass of gold created is vanishingly small—trillions of times less than what would be needed to make, say, a wedding ring.
While that may dash the hopes of some, the experiment opens a new window into how elements are formed and how electromagnetic fields can manipulate atomic nuclei.
It also highlights the extraordinary sensitivity of the ALICE detector, which was designed not for gold-making, but to probe the universe's earliest moments.
Do you have a tip on a science story that Newsweek should be covering? Do you have a question about particle physics? Let us know via science@newsweek.com.
Reference
ALICE Collaboration, Acharya, S., Agarwal, A., Aglieri Rinella, G., Aglietta, L., Agnello, M., Agrawal, N., Ahammed, Z., Ahmad, S., Ahn, S. U., Ahuja, I., Akindinov, A., Akishina, V., Al-Turany, M., Aleksandrov, D., Alessandro, B., Alfanda, H. M., Alfaro Molina, R., Ali, B., ... Zurlo, N. (2025). Proton emission in ultraperipheral Pb-Pb collisions at $sqrt{{s}_{NN}}=5.02$ TeV. Physical Review C, 111(5). https://doi.org/10.1103/PhysRevC.111.054906
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We know that this is possible because spacecraft from NASA and other space agencies produce much less accidental radiation than private satellites do. But companies can only mitigate a satellite's UEMR before it is launched into space. Once in LEO, "they are hard to fix," Winkel said, so it is vital that they are tested for leaks before launch. "If satellite operators care about the UEMR, we will be OK," Di Vruno said. "It will be more difficult to conduct radio astronomy than it is now, but we understand technology evolves and we will evolve with it." Astronomers can also limit the impacts of radio pollution by removing the interfering signals from their datasets. However, this "cleaning" may cause astronomers to miss crucial data that is masked by the interference. "The amount of data you have to discard or the effort that you need to put in to somehow clean the data also increases the more interference there is," Winkel said. One way around this is to collect more data so that there is more left once you've cleaned it, but this also makes it much more expensive to do research, he added. By working together, satellite operators and radio astronomers can solve the radio pollution issue without any external help, Thomson said. "But inevitably, satellite operators and the radio astronomy community have different goals, priorities and budgets, and finding workable solutions is no easy feat." Because private companies and scientists have different priorities, the most effective solution to the problem is to impose strict limits on the amount of UEMR that private spacecraft can give off, experts told Live Science. "We would, of course, be more relaxed if proper regulation was in place," Winkel said. 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