Muon trident process at far-forward LHC detectors

This paper investigates the feasibility of observing the muon trident process, including the first potential detection of electromagnetic τ+τ\tau^+\tau^- pair production and QED bound states, at the LHC's far-forward FASERν\nu and FASERν\nu2 detectors through μ\mu-tungsten collisions.

Reinaldo Francener, Victor P. Goncalves, Gabriel Rabelo-Soares

Published Tue, 10 Ma
📖 4 min read🧠 Deep dive

Imagine the Large Hadron Collider (LHC) as a massive, high-speed particle racetrack. Usually, we watch the main event: protons smashing into protons in the center of the ring. But this paper is about looking at the "backstage" of the race, specifically at the very far end of the track where a tiny, specialized camera (called a detector) is waiting to catch particles that fly straight ahead.

Here is the story of what the authors are investigating, explained simply:

1. The Setup: The "Muon Mailman"

In the chaos of proton collisions, a huge number of muons (heavy cousins of electrons) are created. They zip forward like a high-speed mail delivery service, heading straight toward the far-forward detectors (FASERν\nu and FASERν2\nu2).

Usually, these muons just pass through the detector's layers of tungsten (a very heavy metal) like ghosts. But sometimes, something interesting happens.

2. The Main Event: The "Muon Trident"

The paper studies a rare event called the Muon Trident Process.

  • The Analogy: Imagine a muon is a fast-moving billiard ball. It zooms toward a heavy tungsten nucleus (which is like a giant, stationary bowling ball).
  • The Collision: As the muon passes the tungsten, it doesn't just bounce off. Instead, the intense electromagnetic force acts like a whip. The muon "whips" the vacuum of space, and suddenly, two new particles pop into existence out of thin air.
  • The Result: The original muon keeps going (but slightly slower), and now there are three particles leaving the scene: the original muon plus the new pair. It looks like a trident (a three-pronged spear), hence the name.

The authors calculated how often this happens when the new pair is:

  • Electrons (e+ee^+e^-): Very common. Like catching raindrops in a bucket.
  • Muons (μ+μ\mu^+\mu^-): Less common. Like catching snowflakes.
  • Taus (τ+τ\tau^+\tau^-): Extremely rare. Like catching a specific, rare bird that only flies at high speeds.

Why does this matter?
The authors predict that the FASERν\nu detector will see billions of electron pairs and thousands of muon pairs. But the big news is about the Taus. They predict that for the first time ever, we might actually see a muon create a pair of Taus. This would be a historic first observation of this specific type of "magic trick" in physics.

3. The Special Case: The "Exotic Couples" (QED Bound States)

The paper also looks at a weirder possibility. What if the two new particles created don't just fly apart, but immediately grab onto each other to form a temporary "couple"?

  • Positronium: An electron and a positron holding hands. The authors predict we will see millions of these.
  • True Muonium: A muon and an anti-muon holding hands. This is the "holy grail" of this study. It has never been seen before.
    • The Challenge: These couples are very fragile. They break apart almost instantly.
    • The Prediction: The current detector (FASERν\nu) might be too small to catch enough of them (less than one event). However, the upgraded detector (FASERν2\nu2), which will be much larger and run longer, might finally catch about 60 of these "True Muonium" couples.

4. The "Why" and the "How"

  • The "Why": By counting how many of these events happen, physicists can test if our current laws of physics (the Standard Model) are perfect. If the numbers don't match the predictions, it could mean there is "New Physics" hiding in the shadows. It also helps us understand how muons lose energy when traveling through materials (like lead or tungsten), which is crucial for designing future particle accelerators.
  • The "How": The authors used powerful computer simulations (like a virtual physics lab) to calculate the odds. They looked at the math of how light and matter interact at the highest energies possible.

Summary in a Nutshell

This paper is a "menu" for what the FASERν\nu detectors will see in the coming years.

  1. Electron pairs: We will see a flood of them (billions).
  2. Muon pairs: We will see a steady stream (thousands).
  3. Tau pairs: We might finally see the first-ever examples of this rare event.
  4. True Muonium: The upgraded detector might finally catch the elusive "muon couple" that has never been observed before.

It's like saying, "We know the main race is exciting, but if you look at the very edge of the track with a super-magnifying glass, you might just see a brand-new species of butterfly that no one has ever seen before."