The Role of Axion-like Particles in Dark Matter and Wormholes
Exploring axion-like particles and their connection to dark matter and wormholes.
Dhong Yeon Cheong, Koichi Hamaguchi, Yoshiki Kanazawa, Sung Mook Lee, Natsumi Nagata, Seong Chan Park
― 6 min read
Table of Contents
- What Are Axion-like Particles?
- The Strong CP Problem
- Dark Matter Investigation
- Enter the Wormholes
- The Role of Gravity
- Before and After Inflation
- Finding the Sweet Spot
- The Wacky World of Symmetry Breaking
- Exploring the Mass Range
- Constraints and Challenges
- The Cosmic String Connection
- Putting It All Together
- Future Directions
- Conclusion
- Original Source
- Reference Links
Imagine a universe filled with mysterious stuff that we can't see but know is there. This stuff is called Dark Matter. Scientists have been scratching their heads trying to figure out what it is. One of the exciting ideas is that a certain type of particle, called Axion-like Particles (ALPs), could play a role in making up this dark matter. And guess what? Wormholes might have something to do with it!
What Are Axion-like Particles?
Before diving into wormholes, let’s talk about axion-like particles. ALPs are theoretical particles that arise from certain physics models. They are not just hanging around; they have properties that could allow them to help solve some big questions in science, like the nature of dark matter and the Strong CP Problem.
The Strong CP Problem
The strong CP problem is a fancy term that describes why we do not see certain behaviors in particles that we expect to. In simple terms, it’s like a puzzle: scientists know something is missing but can’t quite figure out the exact pieces. ALPs might be one of those pieces that help fit the puzzle together.
Dark Matter Investigation
Now, let’s get to dark matter. We can’t see it, but we know it makes up a good chunk of the universe. Think of it like a mysterious friend at a party-everyone knows they are there, but no one really knows what they look like. Scientists are exploring many theories about what dark matter could be, and ALPs are front and center in these discussions.
Enter the Wormholes
Now here’s where it gets a bit wacky: wormholes. These are theoretical passages through space-time that could connect distant parts of the universe. Picture a wormhole like a shortcut through a cosmic cheat sheet. If these wormholes exist, they could have an effect on ALPs, contributing to their mass and how they behave in space.
The Role of Gravity
Gravity isn't just about keeping us on the ground; it has a significant role in shaping the universe. It's a tough boss, even for particles. ALPs can gain mass due to gravitational effects, which is crucial for making them potential players in the dark matter game. This means that the way gravity acts can indeed affect the properties of ALPs.
Before and After Inflation
Inflation is not just what happens when you eat too many beans; it's also a theory describing the rapid expansion of the universe right after the Big Bang. This period plays a crucial role in how particles like ALPs came to be. Scientists believe that different production mechanisms, both before and after inflation, can explain how ALPs might exist.
Pre-Inflationary Production
Before inflation, things were chaotic. Think of it as a crowded subway train where everyone is jostling for space. In this scenario, ALPs could form through something called the misalignment mechanism, where they settle into states that give them mass.
Post-Inflationary Production
Once inflation cools down and the universe becomes more stable, things change. ALPs can still form, and this time, Cosmic Strings, which are like defects in the fabric of space-time, can help produce them. So not only do we have the chaotic environment before inflation, but we also have more order after inflation, both contributing to our mysterious dark matter candidates.
Finding the Sweet Spot
To make sure ALPs fit into the dark matter puzzle, scientists are looking for just the right conditions. They investigate the parameters that would allow ALPs to thrive as dark matter. It's like trying to bake a cake: you have to get the temperature and ingredients just right.
The Wacky World of Symmetry Breaking
Now let’s talk about symmetries. In physics, symmetries are like rules of a game. When something breaks those rules, we see changes, and that’s what symmetry breaking is all about. Gravity can cause global symmetries to break, and this process can lead to mass for our friend ALP. This relationship is crucial for exploring how ALPs could contribute to dark matter.
Exploring the Mass Range
ALPs can have a wide range of masses, depending on how the universe evolved and what forces acted upon them. This variability is excellent for scientists looking for dark matter candidates because it gives them many options to play with. The more they explore this mass range, the better they can understand the universe.
Constraints and Challenges
It’s not all fun and games, though. There are rules and constraints scientists have to work within. These constraints help them understand what mass ranges for ALPs make sense and which don’t. So, while scientists are dreaming up possibilities, they have to keep their feet on the ground and follow the rules of physics.
The Cosmic String Connection
Cosmic strings are like a spaghetti highway in the universe-long, thin, and possibly tangled. These strings can be created during symmetry breaking and have a role in producing ALPs. The decay of these strings could contribute to dark matter, underscoring how interconnected these cosmic events are.
Putting It All Together
After diving through wormholes, axion-like particles, and cosmic strings, we can finally see how these ideas fit together in a broader picture of dark matter. ALPs could be a significant component of dark matter, with various mechanisms at play for their production. Wormholes offer a unique perspective on how gravity can shape particles and their masses, leading to potential candidates for the invisible stuff that makes up our universe.
Future Directions
So where do we go from here? Scientists are just scratching the surface of these ideas. There’s still much to learn! Future research could further unravel the mysteries of ALPs, wormholes, and dark matter. The questions are many, and the universe is a big place filled with puzzles waiting to be solved.
Conclusion
The quest to understand dark matter is like a detective story that science is still unraveling. The relationship between gravity, axion-like particles, and wormholes offers exciting avenues to explore. As researchers continue to investigate these cosmic possibilities, who knows what other surprises the universe holds in store?
Title: Wormhole-Induced ALP Dark Matter
Abstract: Non-perturbative gravitational effects induce explicit global symmetry breaking terms within axion models. These exponentially suppressed terms in the potential give a mass contribution to the axion-like particles (ALPs). In this work we investigate this scenario with a scalar field charged under a global $U(1)$ symmetry and having a non-minimal coupling to gravity. Given the exponential dependence, the ALP can retain a mass spanning a wide range, which can act as a dark matter component. We specify pre-inflationary and post-inflationary production mechanisms of these ALPs, with the former from the misalignment mechanism and the latter from both the misalignment and cosmic-string decay. We identify the allowed parameter ranges that explain the dark matter abundance for both a general inflation case and a case where the radial mode scalar drives inflation, each in metric and Palatini formalisms. We show that the ALP can be the dominant component of the dark matter in a wide range of its mass, $m_{a} \in [10^{-21}~\mathrm{eV},\, \mathrm{TeV}]$, depending on the inflationary scenario and the $U(1)$ breaking scale. These results indicate that ALPs can be responsible for our dark matter abundance within a setup purely from non-perturbative gravitational effects.
Authors: Dhong Yeon Cheong, Koichi Hamaguchi, Yoshiki Kanazawa, Sung Mook Lee, Natsumi Nagata, Seong Chan Park
Last Update: 2024-11-12 00:00:00
Language: English
Source URL: https://arxiv.org/abs/2411.07713
Source PDF: https://arxiv.org/pdf/2411.07713
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.