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The Enigma of Dark Matter: A Scientific Pursuit

Scientists chase dark matter, unraveling its influence on the universe.

Anupam Ghosh, Partha Konar, Sudipta Show

― 5 min read


Chasing the Mystery of Chasing the Mystery of Dark Matter influence on the universe. Uncovering dark matter's hidden
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Dark Matter is like the superhero of the universe-it's everywhere, but we can't see it! This mysterious substance makes up about 27% of the universe, spinning galaxies and influencing cosmic events without ever showing itself. Scientists know it exists because they can see its effects on visible matter, such as stars and galaxies. However, no one has ever actually spotted a dark matter particle.

The Quest for Answers

Researchers have been searching for clues about dark matter's nature for decades. One of the most popular candidates for dark matter is something called WIMP, which is short for “Weakly Interacting Massive Particle.” Sorry, WIMP, but after many tests, you still can't seem to find any friends in the lab. Despite a lot of effort, scientists couldn't catch even a glimpse of WIMP; it remains elusive.

But don't worry! Even if WIMP didn’t come through, the quest isn't over. Scientists are looking at other candidates for dark matter. Among them, we have FIMP-short for “Feebly Interacting Massive Particle.” FIMP has a low-profile way of sneaking in, making it harder to detect compared to WIMP, but it might just be the key to the dark matter puzzle.

The Early Universe's Secrets

To understand dark matter, we first need to look back at the early universe. Right after the Big Bang, the universe was a wild place. It was heating up, cooling down, and expanding rapidly. Think of it as an energetic teenager going through all the changes of growing up. During this time, interactions between particles were really wild.

Under normal circumstances, scientists assume that radiation ruled the early universe. But what if that's not the whole story? What if there were hidden influences at play, such as a quick expansion phase that made things more chaotic? This could change everything we know about dark matter.

The Role of Vector-like Quarks

In this new picture of the universe, we have vector-like quarks, which are heavy particles that interact with dark matter through weak forces. Think of them as the cool kids in the particle playground, playing games with the dark matter. When these quarks decay, they produce dark matter, and that's where the action happens.

These quarks can be produced in large amounts at powerful Particle Colliders like the Large Hadron Collider (LHC). Scientists hope to catch a glimpse of them, as they might provide valuable information about dark matter production.

Challenges of Detection

Now, here's the catch: detecting dark matter is a lot like trying to find a needle in a haystack while blindfolded. The interactions with regular matter are faint, so picking them out among the noisy background from all the other particles can be a real headache.

Scientists are particularly interested in cases where the new heavy particles decay quickly, producing dark matter in the process. However, this fast decay can hide the signals they want to detect. In a universe where things are expanding quickly, the rules of the game change altogether, making detection even trickier.

A New Strategy for Searching Dark Matter

Since the usual approaches for searching for dark matter aren't cutting it, researchers are proposing new strategies. One idea is focusing on specific signals that result from the decay of vector-like quarks. By creating events with strong missing energy (thanks to the sneaky dark matter) and certain jet structures (those are just groups of particles flowing out from the decay), scientists hope to catch dark matter in the act!

Using advanced techniques like boosted decision trees, which are fancy ways of sorting through data, researchers can better analyze potential dark matter signals amidst all the chaos at the collider. It's like trying to find gold in a river of rocks-only, in this case, the gold might not even be visible!

The Impact of Cosmology on Dark Matter

As scientists look into these new avenues, they have to consider how the universe's expansion impacts the search. In different cosmological scenarios, the rules can change, and dark matter's properties may also shift. One cosmological picture is like a gentle breeze, where things expand gradually. Another scenario is as if the universe suddenly decided to bolt forward like a sprinter!

Studying how these cosmic factors affect dark matter production might give us a clearer picture of its nature. Different conditions in the early universe can lead to various interactions, changing how researchers approach dark matter detection in the present.

Why This Matters

Understanding dark matter is like solving a huge cosmic mystery. The more we uncover about this invisible force, the closer we get to understanding how the entire universe works. What does dark matter tell us about galaxy formation? How does it influence the cosmic web? Each discovery brings us one step closer to grasping the universe's biggest secrets.

Conclusion

In summary, the study of dark matter is no easy feat, with many twists and turns along the way. Researchers must navigate through a wide range of theoretical landscapes, challenging detection methods, and the ever-changing rules of cosmology. But with persistence and innovative thinking, they might just crack the code and uncover the true nature of dark matter-whatever it might be. So, buckle up, folks, because the universe still has a lot to reveal!

Original Source

Title: Collider fingerprints of freeze-in production of dark matter amidst the fast expansion phase of Universe

Abstract: We examine a simple dark sector extension where the observed dark matter (DM) abundance arises from a freeze-in process through the decay of heavy vector-like quarks into a scalar dark matter candidate. The detection prospects of such DM are challenging due to the feeble nature of the interactions, but these vector-like quarks can be produced copiously at the LHC, where they decay to Standard Model quarks along with DM. Depending on the decay rate, this scenario is typically probed through long-lived particle or displaced vertex signatures, assuming a radiation-dominated background. An alternative hypothesis suggests that the Universe may have experienced a rapid expansion phase instead of the standard radiation-dominated one during freeze-in. This would significantly alter the dark matter phenomenology, requiring a substantial increase in the interaction rate to match the observed relic density, resulting in the rapid decay of the parent particle. As a result, much of the parameter space for this scenario is beyond the reach of traditional long-lived particle and displaced vertex searches. Due to this non-standard cosmic evolution, existing constraints do not cover the expanded dark matter parameter space. We propose a complementary search strategy to explore this scenario, offering additional limits alongside searches for long-lived particles and displaced vertices. In our search, we investigate the FIMP dark matter model at the LHC using boosted fatjets and significant missing transverse momentum. To improve precision, we include one-loop QCD corrections for LHC production processes and employ a boosted decision tree multivariate analysis, leveraging jet substructure variables to explore a vast parameter space for this minimally extended FIMP dark matter model at the 14 TeV LHC.

Authors: Anupam Ghosh, Partha Konar, Sudipta Show

Last Update: 2024-11-14 00:00:00

Language: English

Source URL: https://arxiv.org/abs/2411.09464

Source PDF: https://arxiv.org/pdf/2411.09464

Licence: https://creativecommons.org/licenses/by/4.0/

Changes: This summary was created with assistance from AI and may have inaccuracies. For accurate information, please refer to the original source documents linked here.

Thank you to arxiv for use of its open access interoperability.

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