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Search for dark matter in a signature with a four-prong large-radius jet in proton-proton collisions at s\sqrt{s} = 13 TeV

Using 138 fb1^{-1} of 13 TeV proton-proton collision data collected by the CMS detector, this study presents the first search for nonprompt dark matter candidates in a Lorentz-boosted topology featuring a four-prong large-radius jet and missing transverse momentum, finding no significant excess over Standard Model expectations and setting 95% confidence level upper limits on signal strength.

Original authors: CMS Collaboration

Published 2026-07-14
📖 5 min read🧠 Deep dive

Original authors: CMS 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 universe is a giant, cosmic party where most of the guests are invisible. We call these invisible guests Dark Matter. We know they're there because they have gravity (they pull on things), but we've never seen them, touched them, or caught them in the act.

For years, scientists have been trying to figure out what these invisible guests look like. One popular theory suggests that Dark Matter isn't just a single, boring particle. Instead, it might be part of a whole "Dark Sector" with its own family members, some of which are long-lived and travel a bit before disappearing.

In this paper, the CMS Collaboration (a massive team of scientists working at the Large Hadron Collider, or LHC, in Switzerland) decided to throw a very specific type of party to catch these guests. They smashed protons together at a speed of 13 TeV (a unit of energy) using data collected between 2016 and 2018. In total, they looked at a staggering 138 fb⁻¹ of data (that's a huge amount of collision records).

The Setup: The "Four-Pronged" Mystery

Here's the game plan the scientists used:

  1. The Bouncer: They imagined a heavy "mediator" particle (let's call it Y1) that acts like a bouncer. It doesn't let Dark Matter in directly; instead, it creates a pair of intermediate particles (χ2).
  2. The Long Walk: These χ2 particles are special. They are "long-lived," meaning they don't vanish instantly. They take a little walk away from the crash site before they decay.
  3. The Split: When χ2 finally stops, it splits into two things: a stable Dark Matter particle (χ1, which stays invisible and escapes) and a light boson (Y0).
  4. The Explosion: The light boson (Y0) immediately explodes into a pair of quarks. Since there are two χ2 particles, that means four quarks are created in total.
  5. The Jet: Because the original crash was so energetic, these four quarks are squished together so tightly that they look like a single, giant "jet" of particles with four distinct "prongs" (like a four-pronged fork).

The scientists were looking for a very specific signature: One giant jet with four prongs, plus a huge amount of missing energy. The missing energy is the two invisible Dark Matter particles (χ1) running away from the scene.

The Detective Work: The Graph Neural Network

Finding this specific four-pronged jet in a sea of billions of ordinary particle collisions is like finding a needle in a haystack, except the needle is made of invisible ink and the haystack is moving at the speed of light.

To solve this, the team used a super-smart computer brain called a Graph Neural Network (GNN).

  • Think of the jet as a social network. The particles inside the jet are the "people" (nodes), and their relationships are the "friendships" (edges).
  • The GNN looks at how these particles interact and move relative to each other. It's trained to spot the specific "social pattern" of a four-pronged Dark Matter jet, distinguishing it from the messy, random patterns of ordinary background noise (like standard quark jets).

The Results: The Party Was Quiet

The scientists analyzed the data, looking for an excess of these special events over what the Standard Model (our current best theory of physics) predicts.

The big news? The party was surprisingly quiet.

  • No significant excess was found. The number of events they saw matched the background noise perfectly.
  • They didn't find the "four-pronged" Dark Matter signature they were hunting for in the data.

What Does This Mean?

Since they didn't find the signal, they didn't discover Dark Matter. However, they didn't fail; they ruled out a lot of possibilities.

  • What they ruled out: They set strict "upper limits" (like a speed limit sign) on how often these specific Dark Matter scenarios could happen. If the Dark Matter particles had certain masses or if the "bouncer" (the mediator) had certain strengths, they should have seen them. Since they didn't, those specific combinations of mass and strength are now considered unlikely or impossible within the range they tested.
  • The Confidence: They are 95% confident in these limits. This means if they repeated the experiment 100 times, they would get these results 95 times if their model of the background was correct.

The Takeaway

This was the first search of its kind for this specific "Lorentz-boosted" (super-fast and squished) Dark Matter signature. While they didn't catch the invisible guests this time, they successfully mapped out the "no-go zones" for where these guests might be hiding.

They proved that if Dark Matter exists in this specific "long-lived, four-pronged" form, it's either much heavier, much weaker, or much rarer than their most optimistic guesses suggested. The search continues, but the map of the universe just got a little bit more detailed.

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