Flavour Changing Neutral Current decays at LHCb

This paper summarizes recent LHCb results on Flavour Changing Neutral Current decays, including a legacy measurement of B0K0μ+μB^0\to K^{*0}\mu^+\mu^- using 8.4 fb1^{-1} of Run 1 and 2 data, to search for New Physics and investigate long-standing tensions with Standard Model predictions in bsμ+μb\to s\mu^+\mu^- transitions.

Original authors: Christoph Langenbruch (for the LHCb collaboration)

Published 2026-05-19
📖 5 min read🧠 Deep dive

Original authors: Christoph Langenbruch (for the LHCb collaboration)

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

Imagine the Standard Model of particle physics as a very strict rulebook for how the universe's smallest building blocks behave. In this rulebook, there is a specific rule: a heavy particle called a "bottom quark" is generally forbidden from turning into a lighter "strange quark" while simultaneously creating a pair of electrons or muons (heavy cousins of electrons) without changing its electric charge. This is called a Flavour Changing Neutral Current (FCNC) decay.

Think of it like a bank vault that is supposed to be impenetrable. According to the rulebook, you can't just walk in and swap the gold for silver. However, the rulebook allows for a tiny, sneaky loophole: if you borrow a particle for a split second from the "quantum vacuum" (a virtual particle), you might be able to sneak the swap through. Because this requires a "loan" from the quantum world, it happens very rarely and very slowly.

Why is this exciting?
If "New Physics" (mysterious, undiscovered particles or forces) exists, it could act like a master thief with a master key. It could make these forbidden swaps happen much more often than the rulebook predicts, or change how they happen. The LHCb experiment at CERN is like a high-speed security camera system designed to catch these rare, sneaky swaps.

Here is a breakdown of what the paper found, using simple analogies:

1. The Detective Work: Counting the Rare Swaps

The scientists looked at billions of collisions to find specific decays where a bottom quark turns into a strange quark and a pair of muons (bsμ+μb \to s\mu^+\mu^-).

  • The Result: They found that these decays happen slightly less often than the Standard Model predicts. Imagine if the rulebook said a specific rare event should happen 100 times a year, but the camera only caught it 80 times.
  • The Catch: The rulebook's prediction isn't perfect because it has to guess how messy "hadronic" (strong force) interactions work. It's like trying to predict the exact path of a leaf in a hurricane; the wind (hadronic uncertainty) makes it hard to be 100% sure of the baseline.

2. The "Twist" in the Story: Angular Analysis

It's not just about how many times the swap happens, but how the particles fly out. Imagine a spinning top. If you know the rules, you can predict exactly which way the top will wobble.

  • The Finding: In the decay of a specific particle called B0B^0 into a K0K^{*0} and two muons, the "wobble" (angular distribution) didn't match the prediction. In the middle range of energies, the data was off by about 2.6 to 2.7 "standard deviations" (a statistical way of saying "this is weird").
  • The "Magic Number": When they tried to fix the math by adjusting one specific "knob" in the theory (called C9C_9), they found they needed to turn it quite a bit to match the data. This adjustment had a significance of about 4 sigma. In the world of particle physics, 3 sigma is a "hint," and 5 sigma is a "discovery." They are sitting right on the edge of a discovery, but not quite there yet.

3. The "Charm Loop" Problem

Why aren't they declaring a discovery yet?
The paper explains that the "rulebook" (Standard Model) has a fuzzy area called the "charm loop." Imagine trying to calculate the speed of a car, but you don't know exactly how much friction the tires have on the road. The "charm loop" is a complex quantum effect involving charm quarks that is very hard to calculate precisely.

  • The Conclusion: The tension between the data and the theory might be because the "friction" (hadronic uncertainty) is different than we thought, not because there is a new thief (New Physics). Until we understand the friction better, we can't be sure if the car is speeding because of a new engine or just bad tires.

4. Other Findings

  • Radiative Decays (Light and Magic): They also looked at decays where a photon (light) is emitted. They found these happen exactly as the rulebook predicts, which is good news—it means the rulebook works well in some areas.
  • Lepton Universality (The Equal Opportunity Rule): The Standard Model says electrons and muons should be treated exactly the same (except for their weight). The scientists checked this by comparing how often the swap happens with muons versus electrons. In the high-energy range, the ratio was 1.08, which is very close to the expected 1.0. This suggests that, in this specific high-energy zone, the "Equal Opportunity" rule still holds true.
  • New Data (Run 3): The experiment has started collecting a massive new batch of data (Run 3). They tested their new camera system with a "control" decay (a known event) and found it works perfectly. This gives them confidence that their future measurements will be even more precise.

The Bottom Line

The LHCb team has found some very intriguing "glitches" in the universe's rulebook. The data suggests that heavy particles are behaving slightly differently than expected, particularly in how they spin and how often they decay.

However, the paper is cautious. It says, "We see a tension, but it might just be because our understanding of the messy background (hadronic uncertainties) isn't perfect yet." It's like hearing a strange noise in your house; it could be a ghost (New Physics), or it could just be the pipes settling (theoretical uncertainty).

To solve the mystery, the scientists need two things:

  1. Better Theory: Mathematicians need to calculate the "friction" (hadronic effects) more precisely.
  2. More Data: The new, massive dataset from Run 3 will allow them to measure these rare events with such precision that the answer will eventually become clear.

For now, the universe is still holding its secrets, but the clues are getting clearer.

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