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The Mystery of Dark Matter and CP Violation

Exploring the connections between dark matter and charge-parity violation in physics.

Ferruccio Feruglio, Robert Ziegler

― 6 min read


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Table of Contents

Dark Matter has become one of the biggest mysteries in modern physics. It's like trying to find a missing sock in an overstuffed drawer; you know it's there, you just can't see it. Scientists believe dark matter makes up a significant part of the universe, but we have yet to directly detect it. This elusive substance doesn't emit light or energy, which makes it hard to study.

What is Dark Matter?

Imagine walking into a room filled with invisible furniture. You can feel it bumping into you, but you can't see it or touch it. That's essentially what dark matter is. It's a form of matter that doesn't interact with light, meaning we can't see it with our eyes or telescopes. However, we know it's out there because of its gravitational effects on visible matter, like stars and galaxies.

The Strong CP Problem

Now, let's talk about another curious case in physics known as the "strong CP problem." This problem questions why the universe appears to have very little CP (charge-parity) violation in its strong interactions. You might think of CP violation as a quirky phenomenon that happens when certain particles behave differently from their mirror-image counterparts. It's like if you had a twin who always wore mismatched socks; it’s unusual, but not harmful.

In the world of particle physics, we expect some level of CP violation due to the way particles interact. However, experiments show that this violation is much weaker than we would expect. This discrepancy is known as the strong CP problem.

Solutions on the Table

Many scientists have proposed various solutions to tackle the issue of dark matter and CP violation. One intriguing idea involves an extra particle called the CPon, which could explain both mysteries. Think of the CPon as a quirky cousin who shows up at family gatherings and somehow ties together the unrelated threads of family drama.

What is the CPon?

So, what exactly is the CPon? Picture a tiny particle that can influence the behavior of other particles through its interactions. It’s like the party planner who organizes all the other guests at a gathering. The CPon could play a crucial role in explaining why the universe behaves the way it does regarding charge-parity violation and how dark matter fits into the big picture.

The Role of Supersymmetry

Supersymmetry is another key player in this tale. It's a theoretical idea suggesting that every particle has a "superpartner" with different properties. If this theory holds true, it could provide a framework for understanding the universe's mysteries. Imagine having a superhero counterpart who helps you with your mission; that's what supersymmetry brings to the table.

In this scenario, supersymmetry allows for the inclusion of the CPon as a viable dark matter candidate. This extra particle could help solve the strong CP problem while also making dark matter a little less mysterious.

CPon Properties and Interactions

The CPon is proposed to have specific interactions with other particles, which could lead to observable effects. However, because it's expected to be very light, detecting it directly is a tricky business. It’s like trying to find a feather in a windstorm; it doesn't leave behind obvious traces.

The interactions of the CPon with other particles are complex and not straightforward. It involves various couplings that depend on the energy scales of interactions. Think of it as a game of telephone where the message gets distorted as it travels, making it hard to trace back to the source accurately.

Dark Matter Production in the Universe

One of the proposed ways the CPon could contribute to dark matter is through a process known as Freeze-in. In this analogy, imagine a cold winter night where snowflakes start to settle down. The dark matter particles can ‘freeze in’ as the universe cools, leading to the abundance we observe today.

Early Universe Dynamics

During the early stages of the universe, conditions were very different. It was too hot for particles like the CPon to form. As the universe expanded and cooled, these particles could start to settle in, much like how your body finally warms up after stepping inside from the cold.

In this low-energy environment, the CPon could find a balance between the various particles around, contributing to dark matter. The CPon doesn't need to be in thermal equilibrium with other particles but can still be produced through interactions, much like a surprise party that pops up unexpectedly.

Constraints and Experimental Challenges

While the idea of the CPon sounds promising, it faces many constraints. Think of it as being put through a rigorous audition process; it must demonstrate that it can fit into the existing framework of physics without causing any contradictions. Scientists use established experiments and observations to set limits on the properties of the CPon.

For instance, if the CPon interacts too much with ordinary matter, it could lead to detectable signals that haven't been observed. This is akin to expecting to hear a loud noise but instead finding everything eerily quiet. Thus, there are boundaries within which the CPon must operate to remain consistent with current scientific understanding.

The Search for the CPon

The ongoing hunt for dark matter and solutions to the strong CP problem involves intense research and experimentation. Scientists are using state-of-the-art telescopes and particle accelerators to look for signs of the CPon and dark matter interactions. It's like a treasure hunt where every clue could lead to groundbreaking discoveries.

Future Outlook

The future of research in this area is filled with excitement and hope. New technologies and experimental techniques might bring us closer to uncovering the secrets of dark matter and its relationship with CP violation. Picture scientists like detectives, piecing together a puzzle that could fundamentally change our understanding of the universe.

Conclusion

The interplay between dark matter and CP violation manifests through fascinating concepts like the CPon and supersymmetry. While the mysteries of the universe continue to baffle and inspire, researchers are determined to make sense of it all. With determination and curiosity, the quest to uncover the hidden heroes of our cosmos carries on.

Original Source

Title: CPon Dark Matter

Abstract: We study a class of supersymmetric models where the strong CP problem is solved through spontaneous CP violation, carried out by a complex scalar field that determines the Yukawa couplings of the theory. Assuming that one real component of this field - the CPon - is light, we examine the conditions under which it provides a viable Dark Matter candidate. The CPon couplings to fermions are largely determined by the field-dependent Yukawa interactions, and induce couplings to gauge bosons at 1-loop that are suppressed by a special sum rule. All couplings are suppressed by an undetermined UV scale, which needs to exceed $10^{12}$ GeV in order to satisfy constraints on excessive stellar cooling and rare Kaon decays. The CPon mass is limited from below by 5th force experiments and from above by X-ray telescopes looking for CPon decays to photons, leaving a range roughly between 10 meV and 1 MeV. Everywhere in the allowed parameter space the CPon can saturate the observed Dark Matter abundance through an appropriate balance of misalignment and freeze-in production from heavy SM fermions.

Authors: Ferruccio Feruglio, Robert Ziegler

Last Update: 2024-11-12 00:00:00

Language: English

Source URL: https://arxiv.org/abs/2411.08101

Source PDF: https://arxiv.org/pdf/2411.08101

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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