Search for the charmonium weak decay J/ψDˉ0Kˉ0+c.c.J/\psi\to\bar{D}^0\bar{K}^{*0}+{\rm c.c.}

Using a sample of over 10 billion J/ψJ/\psi events collected by the BESIII detector, researchers searched for the rare weak decay J/ψDˉ0Kˉ0+c.c.J/\psi\to\bar{D}^0\bar{K}^{*0}+{\rm c.c.}, found no significant signal, and established a new upper limit on its branching fraction of 1.4×1071.4\times10^{-7} at the 90% confidence level, improving upon previous limits by an order of magnitude.

Original authors: BESIII Collaboration, M. Ablikim, M. N. Achasov, P. Adlarson, X. C. Ai, R. Aliberti, A. Amoroso, Q. An, Y. Bai, O. Bakina, Y. Ban, H. -R. Bao, V. Batozskaya, K. Begzsuren, N. Berger, M. Berlowski, M.
Published 2026-05-19
📖 5 min read🧠 Deep dive

Original authors: BESIII Collaboration, M. Ablikim, M. N. Achasov, P. Adlarson, X. C. Ai, R. Aliberti, A. Amoroso, Q. An, Y. Bai, O. Bakina, Y. Ban, H. -R. Bao, V. Batozskaya, K. Begzsuren, N. Berger, M. Berlowski, M. Bertani, D. Bettoni, F. Bianchi, E. Bianco, A. Bortone, I. Boyko, R. A. Briere, A. Brueggemann, H. Cai, M. H. Cai, X. Cai, A. Calcaterra, G. F. Cao, N. Cao, S. A. Cetin, X. Y. Chai, J. F. Chang, G. R. Che, Y. Z. Che, C. H. Chen, Chao Chen, G. Chen, H. S. Chen, H. Y. Chen, M. L. Chen, S. J. Chen, S. L. Chen, S. M. Chen, T. Chen, X. R. Chen, X. T. Chen, X. Y. Chen, Y. B. Chen, Y. Q. Chen, Y. Q. Chen, Z. J. Chen, Z. K. Chen, J. C. Cheng, S. K. Choi, X. Chu, G. Cibinetto, F. Cossio, J. Cottee-Meldrum, J. J. Cui, H. L. Dai, J. P. Dai, X. C. Dai, A. Dbeyssi, R. E. de Boer, D. Dedovich, C. Q. Deng, Z. Y. Deng, A. Denig, I. Denysenko, M. Destefanis, F. De Mori, B. Ding, X. X. Ding, Y. Ding, Y. Ding, Y. X. Ding, J. Dong, L. Y. Dong, M. Y. Dong, X. Dong, M. C. Du, S. X. Du, S. X. 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Original paper licensed under CC BY 4.0 (http://creativecommons.org/licenses/by/4.0/). This is an AI-generated explanation of the paper below. It is not written or endorsed by the authors. For technical accuracy, refer to the original paper. Read full disclaimer

The Big Picture: Hunting for a "Ghost" in a Crowd of Particles

Imagine the J/ψJ/\psi particle as a very heavy, energetic celebrity. For decades, physicists have watched this celebrity perform its usual tricks: breaking apart into other particles via the "Strong Force" (like a heavy weight dropping and shattering) or the "Electromagnetic Force" (like a spark jumping between wires). These are loud, common, and well-understood events.

However, there is a very rare, quiet trick this celebrity should be able to do according to the rules of the Standard Model (the rulebook of physics): a Weak Decay. This is like the celebrity trying to whisper a secret message that changes their identity entirely. The paper searches for one specific whisper: the J/ψJ/\psi turning into a Dˉ0\bar{D}^0 and a Kˉ0\bar{K}^{*0}.

The problem? This whisper is incredibly faint. The paper predicts that for every 100 million times the J/ψJ/\psi does its loud, normal tricks, it might only whisper this secret once (or even less).

The Setup: The Giant Camera (BESIII)

To catch this whisper, the researchers used the BESIII detector, which is essentially a giant, high-tech 360-degree camera sitting at the BEPCII collider in China.

  • The Data: They didn't just take a few photos; they took 10 billion pictures of J/ψJ/\psi particles. That is a massive crowd.
  • The Strategy: Because the "whisper" is so rare, the researchers had to be incredibly careful not to get tricked by "fake whispers" (background noise). They used a "blind" strategy: they set up their rules for what counts as a signal using computer simulations first, then looked at a small slice of real data to test their rules, and only then looked at the full 10 billion events. This ensures they didn't accidentally bias the results to find what they wanted to find.

The Detective Work: How They Found the "Ghost"

The specific decay they are looking for (J/ψDˉ0Kˉ0J/\psi \to \bar{D}^0 \bar{K}^{*0}) is tricky because one of the particles produced is a neutrino.

  • The Invisible Neighbor: A neutrino is like a ghost that passes through walls. It has no electric charge and barely interacts with anything. The camera (BESIII) cannot see it directly.
  • The Clue: Since the camera can't see the ghost, the scientists look for missing energy. Imagine a billiard table where you hit a ball, and you know exactly how fast it should go. If the ball stops short, you know something invisible (the ghost) must have taken some of the energy.
  • The Reconstruction: The scientists looked for the other pieces of the puzzle: a Kaon, a Pion, and an Electron. They checked if these pieces fit together perfectly except for the missing energy carried away by the invisible neutrino. If the math added up perfectly with a "ghost" in the middle, it was a candidate signal.

The Challenge: The "Cosplay" Problem

The biggest hurdle was background noise.

Imagine a crowded party where you are looking for a specific person wearing a red hat. But, thousands of other people are wearing red hats, or they are wearing blue hats but holding red balloons, or they are wearing red hats but standing in the shadows.

  • In this experiment, the "noise" came from other common particle decays where a pion (a common particle) was mistakenly identified as an electron (the signal particle).
  • Sometimes, a photon (light particle) would escape the camera's view, making it look like a neutrino was there.
  • The researchers had to build very strict "bouncers" at the door of their analysis to filter out these impostors. They checked angles, energy levels, and timing to ensure the "electron" was really an electron and not a "cosplayer" (a misidentified pion).

The Result: Silence is Golden

After sifting through 10 billion events and applying all these strict filters, the researchers looked at the final pile of candidates.

  • The Finding: They found zero clear signals. The number of events they saw was actually slightly lower than what they expected from background noise (a statistical fluctuation).
  • The Conclusion: They did not find the whisper. The J/ψJ/\psi did not perform this specific weak decay in their sample.

However, "not finding it" is still a scientific victory. Because they looked at such a huge sample (10 billion events) and found nothing, they can say with high confidence: "If this decay happens, it happens less than 1 time in every 7 million J/ψJ/\psi particles."

They set a new Upper Limit of 1.4×1071.4 \times 10^{-7}. This means they have improved the sensitivity of the search by 10 times compared to the previous best attempt.

Why Does This Matter?

Think of the Standard Model as a map. The map predicts that this "weak decay" exists, but it should be extremely rare.

  • If the researchers had found it happening more often than the map predicted, it would mean the map is wrong and there is "New Physics" (like a hidden tunnel or a secret passage) that we don't know about.
  • Since they didn't find it, the map remains consistent with reality. The "ghost" is still hiding, but we now know exactly how good at hiding it is.

In summary: The BESIII team took 10 billion photos of a subatomic particle, used a clever "missing energy" trick to look for a ghost, and found nothing. But by proving the ghost is even rarer than we thought, they tightened the rules of the universe and ruled out several theories that predicted the ghost should be easier to find.

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