Simple Science

Cutting edge science explained simply

# Physics # High Energy Physics - Phenomenology

Axions and the Dark Matter Mystery

Investigating axions as a potential solution to dark matter.

Itay M. Bloch, Simon Knapen, Amalia Madden, Giacomo Marocco

― 5 min read


Axions: The Dark Matter Axions: The Dark Matter Enigma matter's secrets. Investigating axions to unravel dark
Table of Contents

Dark Matter is one of those big mysteries in physics. We know it's there because of its gravitational effects, but we can’t see it. One of the interesting candidates for dark matter is the axion. Originally, Axions were proposed to solve a confusing problem in particle physics, but they may also be responsible for the dark matter we can’t find.

What Are Axions?

Axions are tiny particles predicted by theoretical physics. They are believed to have a mass that is very small, somewhere between 1 microelectronvolt and 100 microelectronvolts. To put it simply, if you were to catch an axion in a jar, you’d need a very sophisticated setup-like a super-duper smart jar! Axions could also explain some of the missing pieces in our understanding of the universe, like why we observe dark matter.

How Do Axions Interact?

Axions have some unusual interactions. They can interact with other particles in ways that we don’t fully understand yet. This includes interactions with Nuclear Spins, which are like tiny magnets inside atomic nuclei. When axions come into contact with these nuclei, they can cause some action-like shaking things up and producing Phonons.

Phonons: The Sound of Physics

Phonons are a bit like the sound waves you hear when you pluck a guitar string or clap your hands. They are the building blocks of sound in solids, traveling through materials like waves. When axions interact with nuclei in certain materials, they can excite these phonons, leading to interesting effects.

The Role of Crystals

Crystals are solid materials whose atoms are arranged in a highly organized structure. When we talk about detecting axions, crystals are our playground! Specifically, when axions encounter a crystal, they can cause the atoms to vibrate, which in turn creates phonons. Different crystals might show different responses to axion interactions.

Exciting Phonons with Axions

So, how do we catch these phonons in action? When axions are absorbed by a crystal, they can produce phonons that have different energies. Because the nuclear spins in the crystal can be randomly oriented, it allows the axion to create a wide variety of phonons-not just a narrow band. This is like throwing a big party where everyone is dancing to all kinds of music instead of just one song!

Why the Mass Matters

The mass of axions is important. The range we are focusing on is very tiny-between 1 and 100 microelectronvolts. Unfortunately, this makes it tricky for scientists to detect them directly. We need very sensitive experiments to spot any interaction with axions, especially when it comes to producing phonons in materials.

Searching for Axions

While the quest for understanding dark matter continues, there are several experimental strategies being explored. Some experiments focus on detecting the energy from phonons created by axions. Others look for more subtle signals that might indicate axion interactions.

The Promise of New Experiments

In recent years, new technologies are emerging in the field of phonon detection. Devices like low-threshold calorimeters can help us detect individual phonons and could offer a real path towards discovering axions. These experiments aim to create an ideal environment where axions make their presence known, even if it's just a little noise.

Types of Crystals and Their Role

Various materials can be used to search for axions, but some work better than others. In particular, materials with light nuclei or those containing unpaired spins are of great interest. Scientists are like chefs, experimenting with different ingredients to find the best recipe for detecting axions.

The Challenge of Background Interference

One of the significant challenges in detecting axions is background noise. Just like trying to hear a quiet whisper at a loud party, it becomes crucial to filter out all other signals that do not come from axions. Scientists are working hard to develop methods to reduce these background events and improve sensitivity.

What Happens in the Lab?

In a lab setting, researchers may cool down crystal samples to incredibly low temperatures, aiming to reduce thermal noise. By conducting experiments underground, they can shield themselves from cosmic rays and other interference that might block their view of axions. Every detail counts in this complex game of hide-and-seek!

Going Deeper: Time-Dependent Electric Dipole Moments

There’s even more to axions! They can induce changes in the nuclei, leading to what scientists call electric dipole moments. Think of it like giving the atoms a little shake, which can help provoke more phonons. This extra layer of interaction can further complicate the search but also opens up new avenues for discovery.

Future Prospects

With advancements in technology and a growing understanding of axion interactions, researchers are hopeful. The next wave of experiments aims to push the boundaries, exploring new materials and techniques that could dramatically enhance detection sensitivity.

Conclusion: The Road Ahead

In the pursuit of understanding dark matter and the role of axions, every experiment is a step closer to piecing this cosmic puzzle together. Though the challenges are immense, the potential rewards are even greater, opening up a world of possibilities in our understanding of the universe. The journey may be long, but the excitement of discovery is just around the corner!

Original Source

Title: Broadband phonon production from axion absorption

Abstract: We show that axion dark matter in the range meV $\lesssim m_a\lesssim$ 100 meV can incoherently excite phonons in crystal targets with unpolarised nuclear spins. This can occur through its coupling to nuclear spins and/or through its induced time-dependent electric dipole moment in nuclei. Due to the random orientation of the nuclear spins, translation symmetry is broken in the phonon effective theory, allowing axion absorption to create phonons with unrestricted momentum. The absorption rate is therefore proportional to the phonon density of states, which generically has support across a wide range of energies, allowing for a broadband detection scheme. We calculate the absorption rate for solid $\text{H}_2$, $\text{D}_2$, $\text{Al}_2\text{O}_3$, $\text{GaAs}$, $\text{H}_2\text{O}$, $\text{D}_2\text{O}$, $\text{Be}$ and $\text{Li}_2 \text{O}$, and find that materials containing light, non-zero spin nuclei are the most promising. The predicted rates for the QCD axion are of the order of a few events / 10 kg-year exposure, setting an ambitious target for the required exposure and background suppression.

Authors: Itay M. Bloch, Simon Knapen, Amalia Madden, Giacomo Marocco

Last Update: 2024-11-15 00:00:00

Language: English

Source URL: https://arxiv.org/abs/2411.10542

Source PDF: https://arxiv.org/pdf/2411.10542

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.

More from authors

Similar Articles