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The Mystery of Dark Matter and WIMPs

Exploring the hidden roles of secluded WIMPs and Dirac neutrinos in dark matter.

Kimy Agudelo, Diego Restrepo, Andrés Rivera, David Suarez

― 6 min read


Unraveling Dark Matter Unraveling Dark Matter Mysteries shape our universe's hidden aspects. Secluded WIMPs and Dirac neutrinos
Table of Contents

In our universe, there is a lot more going on than what we can see. While visible matter, like stars and planets, makes up a small part of the overall mass of the universe, the majority is believed to be composed of dark matter. Dark matter is mysterious because it doesn’t emit, absorb, or reflect light, making it nearly impossible to detect directly. Scientists think it's out there because of its gravitational effects on visible matter.

What Are WIMPs?

One of the leading candidates for dark matter is known as WIMPs, or Weakly Interacting Massive Particles. These particles are thought to have mass and interact with regular matter only through gravity and possibly the weak nuclear force. In essence, they're like that friend who shows up to parties but never speaks to anyone—present, but not easily noticed.

The Concept of Secluded WIMPs

Now, imagine these WIMPs hanging out in their own private universe, far from the limelight of regular matter. This is where the "secluded" aspect comes in. Secluded WIMPs interact mainly with each other and have a very weak connection with the particles we know and love, like electrons and protons. This makes them intriguing candidates for explaining dark matter.

Dirac Neutrinos: The Hidden Players

Speaking of elusive characters, neutrinos are tiny particles that are generated in nuclear reactions, like those happening in the sun. They hardly interact with anything and can zip through galaxies as if they’re on the express train. There are two types of neutrinos: Dirac and Majorana. Dirac neutrinos behave like regular particles, while Majorana neutrinos are their own antiparticles.

In our story, we focus on Dirac neutrinos. Unlike Majorana neutrinos, where the lines between particles and antiparticles get blurred, Dirac neutrinos can be distinguished from their counterparts.

The Role of Extra Symmetries

Now, here comes the twist. To understand these secluded WIMPs and Dirac neutrinos, scientists propose adding something called an "extra Abelian gauge symmetry." Think of it as giving our secluded WIMPs and Dirac neutrinos an exclusive club membership that allows them to interact in ways that regular matter cannot.

This symphony of particle interactions lets us explore how dark matter and neutrinos could work together to create a coherent story about the universe's makeup.

How Do WIMPs Relate to Dark Matter Abundance?

For dark matter to be stable and not disappear into thin air, it needs to have the right properties to keep it around. The theory of secluded WIMPs suggests that these particles can convert into lighter, mediating particles. This process is essential in determining how much dark matter remains post-Big Bang.

When particles of dark matter collide, they can produce lighter particles that can then decay into the regular matter we are familiar with, such as neutrinos. When this interaction is just right, we can maintain the perfect balance of dark matter in the cosmos.

The Role of Mediators: Dark Higgs and Dark Photon

To keep things running smoothly in the secluded WIMP scenario, two important characters come into play: the dark Higgs and the dark photon.

  • The dark Higgs is kind of like a bouncer at the club, controlling how particles get in and out and making sure they behave.
  • The dark photon is like the club's DJ, playing tunes that allow particles to interact in specific ways.

Together, these mediators influence how WIMPs and Dirac neutrinos perform their cosmic dance.

Neutrino Masses: How Do They Fit In?

We can't have a proper party without a good reason for the guests to be there. In the case of Dirac neutrinos, they need a mechanism to explain why they have mass. In the standard model of particle physics, there wasn't a clear way to give neutrinos their needed mass without breaking rules.

This is where the extra symmetry and the secluded WIMP framework come in handy. Using the dark Higgs, we can define a process that generates neutrino masses at a unique level. It’s a bit like discovering a secret ingredient to make a dish taste better.

The Role of Cosmology

Cosmology looks at the universe's history and evolution. It suggests that for dark matter to be a viable candidate, there needs to be a stable, neutral particle. In a similar vein, neutrinos must fit into this cosmic picture by having a mechanism to generate mass.

This connection between dark matter and neutrino masses creates a more thorough understanding of how the universe ticked during its infancy.

Interactions of Dark Matter with Standard Model Particles

As secluded WIMPs interact with regular particles, they can gradually transform into forms that we can observe. Because their interactions are limited, they do not clutter up measurements, allowing scientists to study them without too much noise.

In practical terms, if we could observe these interactions, it would offer us a glimpse into the dark sector. We’d get insights into how this secluded material and the regular matter communicate—giving scientists a better preview of the universe’s true nature.

Experimental Tests and Predictions

Though secluded WIMPs are difficult to observe directly, scientists are always on the lookout for clues from particle detectors and other experiments. They want to see if they can spot any signs that might indicate these elusive particles exist and how they interact with neutrinos.

Future experiments, like DARWIN, are particularly promising. They aim to detect potential signals from dark matter interactions—which would help us paint a more complete picture of the universe’s structure.

A Recipe for Compatibility

To make the secluded WIMP model work beautifully, it needs to check off a few boxes. For instance, it must align with cosmological observations, such as measurements of the cosmic microwave background and the formation of galaxies.

The model also needs to hold up against theoretical constraints, ensuring it doesn't contradict any established laws of physics. If the secluded WIMP hypothesis can satisfy these criteria, we can be more confident that it tells us something valuable about dark matter and neutrinos.

The Big Picture

So, where does all this lead us? If secluded WIMPs exist and can produce Dirac neutrinos, it could reshape our understanding of both dark matter and particle physics. It serves as a bridge between the visible universe we understand and the dark, hidden universe that remains elusive.

In this sense, dark matter isn’t just about filling in the gaps in our knowledge; it’s also about connecting different parts of a grand cosmic puzzle. As we continue our search, every experiment brings us one step closer to discovering how our universe operates.

Conclusion

To wrap things up, secluded WIMPs and Dirac neutrinos play critical roles in the ongoing saga of dark matter. These elusive players are not just figures in a theoretical game; they hold the keys to more profound mysteries about our universe's composition and behavior.

In our quest for knowledge, each new piece of information brings us closer to understanding the invisible realms that influence our visible reality. Perhaps one day, we might just crack the code on dark matter, leaving behind a clearer, more complete model of the universe—and who knows, maybe even a reason to throw a cosmic dance party!

Original Source

Title: Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry

Abstract: Scenarios for secluded WIMP dark matter models have been extensively studied in simplified versions. This paper shows a complete UV realization of a secluded WIMP dark matter model with an extra Abelian gauge symmetry that includes two-component dark matter candidates, where the dark matter conversion process plays a significant role in determining the relic density in the Universe. The model contains two new unstable mediators: a dark Higgs and a dark photon. It generates Dirac neutrino masses and can be tested in future direct detection experiments of dark matter. The model is also compatible with cosmological and theoretical constraints, including the branching ratio of Standard model particles into invisible, Big Bang nucleosynthesis restrictions, and the number of relativistic degrees of freedom in the early Universe, even without kinetic mixing.

Authors: Kimy Agudelo, Diego Restrepo, Andrés Rivera, David Suarez

Last Update: 2024-12-18 00:00:00

Language: English

Source URL: https://arxiv.org/abs/2412.02027

Source PDF: https://arxiv.org/pdf/2412.02027

Licence: https://creativecommons.org/publicdomain/zero/1.0/

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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