Unraveling the Mystery of Freeze-In Dark Matter
A new theory proposes how dark matter might form in the early universe.
Xinyue Yin, Shuai Xu, Sibo Zheng
― 7 min read
Table of Contents
- What is Freeze-In Dark Matter?
- The Higgs Portal
- The Two-Field Model
- The Role of Scalar Mediators
- Lack of Direct Signals
- Current Experimental Landscape
- The Importance of Coupling
- Phenomenology and Relic Density
- Challenges in Detection
- The LHC and Search for Signals
- Revisiting the Model
- Future Directions
- Conclusion
- Original Source
Dark matter is one of the great mysteries of modern physics. We can’t see it, but we know it’s there because of its gravitational effects on visible matter. Scientists believe dark matter makes up about 27% of the universe, but determining what it is has proven to be quite a challenge.
Among many theories, Freeze-in Dark Matter has caught the attention of researchers. This idea involves dark matter being produced in the early universe through processes that are quite different from the well-known freeze-out mechanisms. Here, we’re going to explore this concept, focusing on a particular model involving two types of fields interacting via the Higgs Portal.
What is Freeze-In Dark Matter?
Freeze-in dark matter is a theory about how dark matter was formed in the early universe. Unlike freeze-out mechanisms, where particles annihilate each other and leave behind a stable amount of dark matter, freeze-in dark matter is created without any initial interaction. It’s like sneaking in through the back door when there’s no one watching.
In simple terms, freeze-in occurs when dark matter particles are produced by other particles decaying or transforming into them as the universe cools down. This process results in a small but significant amount of dark matter that continues to exist today.
The Higgs Portal
Now, let’s introduce an important player in this game: the Higgs boson. This particle was famously discovered at the Large Hadron Collider (LHC) in 2012. Think of the Higgs boson like a bouncer at a nightclub, giving mass to other particles and helping them form the matter we know today.
The Higgs portal is a theoretical link between the Higgs boson and other hidden particles, like our dark matter candidates. This means that dark matter can interact with regular matter through the Higgs boson. If there’s a way for the Higgs to “speak” to dark matter, it could open up new possibilities for understanding its properties.
The Two-Field Model
Most dark matter models focus on one field—usually the one associated with dark matter itself. However, in this new approach, researchers propose a two-field model. This model includes both the dark matter and a “force mediator,” which helps to explain how dark matter interacts with ordinary matter.
Think of it this way: if dark matter is like a shy kid at a party, the force mediator is the friendly person helping them make connections. This setup allows dark matter to exist in a way that could potentially leave behind hints or signals that can be detected by experiments like those at the LHC.
The Role of Scalar Mediators
In this two-field model, researchers introduce a scalar mediator. This is just a fancy term for a type of particle that helps to mediate the interactions between dark matter and ordinary matter. The scalar mediator can decay into dark matter particles and, thus, produce detectable signals.
The scalar mediator needs to be a specific mass to ensure it can interact effectively with both the dark matter and the Higgs boson. Researchers found that within a certain mass range, they could derive limits on how much of this mediator could exist without being ruled out by existing experiments.
Lack of Direct Signals
One of the peculiar features of this approach is that traditional dark matter detection methods might not work well. While we might not find direct signals of dark matter, if our model is correct, the scalar mediator could still be detected at the LHC. This could occur through two channels: vector boson fusion or the mono-Z channel.
In simple terms, physicists are trying to find indirect evidence of dark matter by looking for the scalar mediator. It’s like trying to find a friend at a crowded mall by listening for their favorite music instead of looking directly for them.
Current Experimental Landscape
Currently, experiments like the LHC have not found definitive proof of dark matter particles. However, given the nature of freeze-in dark matter, researchers believe it might be too weakly coupled to ordinary matter to show up in Direct Detection experiments.
Instead, they’ve turned their attention to cosmic or astrophysical observations. These kinds of measurements have started to probe regions where this dark matter could exist. However, the two-field model offers a glimmer of hope that the LHC could change the game by detecting the scalar mediator.
The Importance of Coupling
In this context, coupling refers to how strongly the scalar mediator interacts with other particles. If the coupling is strong enough, it opens the door for potential detection at the LHC. Researchers are exploring different scenarios where the coupling varies, determining how it changes the limits for the range of the scalar mass.
This investigation is crucial because the scalar mediator needs to decay into two dark matter particles, which could lead to a missing energy signal. Missing energy is like when you’re playing hide and seek and notice that part of the group is mysteriously absent—the clues help you infer that something is going on.
Relic Density
Phenomenology andNext, let’s talk about phenomenology, which is just a fancy word for how physical theories play out in experiments. The researchers examine how dark matter gets produced and how it moves or interacts with other particles.
The concept of relic density helps us understand how much dark matter remains today. In the early universe, conditions were hot and dense, allowing dark matter to form through the decay of scalar mediators. As the universe cooled, fewer interactions occurred, leading to a stable amount of dark matter that we see now.
Challenges in Detection
Despite its intriguing properties, freeze-in dark matter presents some challenges. For one, the tiny interactions with ordinary matter mean that it’s incredibly difficult to detect directly. This is like trying to find a needle in a haystack while wearing a blindfold.
However, scientists are optimistic that indirect detection methods, such as observations of astrophysical phenomena or experiments at the LHC, may reveal the presence of dark matter.
The LHC and Search for Signals
The LHC is one of the most powerful particle colliders in the world. While traditional dark matter detection methods may fall short, the LHC could provide critical insights. The scalar mediator’s decay can lead to missing energy events that researchers hope to capture.
Scientists are keeping an eye on two specific processes at the LHC: vector boson fusion and the mono-Z channel. These processes are expected to create signals that hint at the presence of the scalar mediator, which in turn suggests the existence of freeze-in dark matter.
Revisiting the Model
The current work represents a revision of earlier models that primarily considered thermal dark matter. This new study emphasizes non-thermal explanations, which have not received as much attention.
By diving deeper into the two-field model involving the Higgs portal, researchers can explore new possibilities for detecting dark matter. The study aims to show how this non-thermal dark matter can be inferred from signals produced by the scalar mediator at the LHC.
Future Directions
As researchers continue to investigate dark matter, they’ll likely explore other portals besides the Higgs portal. These could include connections involving neutrinos or other particles. It’s an exciting field, and every new exploration might help us understand our universe a little better.
The hunt for dark matter is like a cosmic scavenger hunt—every finding leads to more questions and potential discoveries. Just as detectives search for clues to solve mysteries, scientists are piecing together the puzzle of dark matter.
Conclusion
In summary, freeze-in dark matter provides an intriguing avenue for understanding one of the universe’s biggest enigmas. By utilizing models involving two fields and the Higgs portal, researchers are paving the way for new discoveries.
Although direct detection methods may be limited, the LHC presents a unique opportunity to find indirect evidence of dark matter through the scalar mediator. As scientists refine their models and explore new avenues of detection, we can only hope that the answers to the dark matter mystery are just around the corner. After all, in the realm of physics, every mystery solved just leads to a new one, keeping scientists on their toes—as if they were in perpetual dance with the universe itself!
Title: LHC-friendly freeze-in dark matter via Higgs portal
Abstract: It is known that single-field freeze-in dark matter barely leaves footprints in dark matter direct detection and collider experiments. This situation can be altered in two-field context. In this work we propose a two-field freeze-in dark matter model through Higgs portal. The observed dark matter relic abundance is obtained by a decay of scalar mediator thermalized in the early Universe. While there is a lack of direct dark matter signals, the scalar mediator is in the reach of HL-LHC either through vector boson fusion or Mono-Z channel. Within allowed scalar mass window of 10-50 GeV, we use improved cuts to derive both $2\sigma$ exclusion and $5\sigma$ discovery limits, depending on the value of Higgs portal coupling. If verified, this scalar mediator signal allows us to infer the freeze-in dark matter.
Authors: Xinyue Yin, Shuai Xu, Sibo Zheng
Last Update: 2024-12-24 00:00:00
Language: English
Source URL: https://arxiv.org/abs/2412.18721
Source PDF: https://arxiv.org/pdf/2412.18721
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.