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The Search for Dark Matter: Axions and Pulsars

Scientists explore ultralight axions using pulsars to solve dark matter's mystery.

N. K. Porayko, P. Usynina, J. Terol-Calvo, J. Martin Camalich, G. M. Shaifullah, A. Castillo, D. Blas, L. Guillemot, M. Peel, C. Tiburzi, K. Postnov, M. Kramer, J. Antoniadis, S. Babak, A. -S. Bak Nielsen, E. Barausse, C. G. Bassa, C. Blanchard, M. Bonetti, E. Bortolas, P. R. Brook, M. Burgay, R. N. Caballero, A. Chalumeau, D. J. Champion, S. Chanlaridis, S. Chen, I. Cognard, G. Desvignes, M. Falxa, R. D. Ferdman, A. Franchini, J. R. Gair, B. Goncharov, E. Graikou, J. -M. Grießmeier, Y. J. Guo, H. Hu, F. Iraci, D. Izquierdo-Villalba, J. Jang, J. Jawor, G. H. Janssen, A. Jessner, R. Karuppusamy, E. F. Keane, M. J. Keith, M. A. Krishnakumar, K. Lackeos, K. J. Lee, K. Liu, Y. Liu, A. G. Lyne, J. W. McKee, R. A. Main, M. B. Mickaliger, I. C. Niţu, A. Parthasarathy, B. B. P. Perera, D. Perrodin, A. Petiteau, A. Possenti, H. Quelquejay Leclere, A. Samajdar, S. A. Sanidas, A. Sesana, L. Speri, R. Spiewak, B. W. Stappers, S. C. Susarla, G. Theureau, E. van der Wateren, A. Vecchio, V. Venkatraman Krishnan, J. Wang, L. Wang, Z. Wu

― 5 min read


Chasing Dark Matter's Chasing Dark Matter's Axions for dark matter clues. Scientists hunt axions using pulsars
Table of Contents

Dark Matter is one of the great mysteries in modern science. While we can't see it or touch it, we know it exists because of how it affects things we can observe, like stars and galaxies. Imagine trying to solve a puzzle with missing pieces. That's what scientists are doing when they try to figure out what dark matter is. One of the exciting candidates for dark matter is something called ultralight Axions, which sound like characters from a sci-fi movie but are actually tiny particles that might help explain the universe's hidden mass.

The Mysterious Nature of Dark Matter

To understand dark matter, you have to picture a universe filled with invisible stuff. Scientists think about 27% of the universe is made up of dark matter. The rest? That’s mostly ordinary matter, the kind we are familiar with—like stars, planets, and your leftover pizza.

But here’s the kicker: we can’t see dark matter. We know it’s there because of its gravitational effects. It pulls and shapes galaxies and clusters, just like a puppet master pulling strings. People have proposed many ideas about what dark matter could be, and one of the most intriguing is ultralight axion dark matter.

What Are Axions?

Picture a tiny particle so light that it barely has any mass. These are axions, which are hypothetical particles that could help solve the dark matter mystery. They were first introduced in the 1970s to explain a different problem in physics, but they quickly became a hopeful candidate for dark matter.

Think of axions as the shy cousins of other particles. They don’t like to interact with anything much, which makes them very difficult to detect. But if we could find them, it could change our understanding of the universe.

The Role of Pulsars

Now, let’s throw some pulsars into the mix. A pulsar is like a cosmic lighthouse, sending beams of radiation into space. Imagine you are at the beach, and someone is waving a flashlight in the air. If you’re standing in the right spot, you’ll see the light. Pulsars are similar, and they help us detect changes in things like radiation and Polarization.

Polarization is a way light waves can be oriented in a specific direction. When light travels through a medium affected by axions, its polarization can change. By observing the light from pulsars, scientists can search for signs of axions.

How Do We Search for Axions?

To find these elusive axions, scientists analyze the light coming from pulsars. They look for subtle changes in the polarization of the light. It’s not easy; it’s like trying to hear a faint whisper in a crowded room.

They use advanced techniques to sift through tons of data, hoping to catch a glimpse of the axion's effects. One method they use is called the Lomb-Scargle periodogram. It helps scientists find periodic Signals in their data, much like tuning a radio to find a specific station.

So far, researchers have looked at many pulsars, trying to detect signals that might indicate the presence of axions. They gather data from various radio telescopes in Europe, which act like big ears listening for the faint sounds of axions.

The Challenges of Detecting Dark Matter

Detecting dark matter is no walk in the park. It’s like trying to catch smoke with your bare hands. There are many factors that can interfere with the signals researchers hope to find. These include other cosmic sources such as radio waves emitted by nearby stars and even the ionosphere, which can distort signals that pass through it.

Even with the best tools and methods, researchers sometimes find signals that aren’t from dark matter at all. They might just be artifacts from the equipment or interference from other sources. So, they need to be careful and methodical in their search.

The Results So Far

Recent efforts to find ultralight axions are ongoing and have yielded some interesting results. For example, researchers have analyzed data from 12 of the brightest pulsars, looking for signs of changes in polarization.

The findings so far have been both exciting and a bit of a bummer. While some signals were detected, they mostly pointed to interference and not the presence of axions. For now, scientists have set upper limits on the possible interaction strength between axions and light. This means they can still rule out certain aspects of axions, but they haven’t found the smoking gun yet.

The Future of Axion Research

Scientists are not giving up. The hunt for ultralight axions will continue, and new technology could provide better ways to search for these particles. The quest to understand dark matter mirrors the search for the Holy Grail of physics, where each discovery provides a piece of the puzzle, and every failure brings them closer to the truth.

Future studies may involve more advanced telescopes and new techniques, opening doors to fresh discoveries. As more data is gathered and technology improves, the search for axions may finally yield results that could explain dark matter's mysteries.

Conclusion

The journey of figuring out what dark matter is made of continues to be a thrilling ride. Ultrawide axions represent a glimmer of hope in this quest, and pulsars provide a unique tool for this exciting adventure. As researchers scan the heavens, they not only search for these tiny particles but also push the boundaries of human understanding of the universe.

So, while dark matter remains elusive, the search for answers fuels scientific exploration, reminding us that even the greatest mysteries can inspire incredible journeys of discovery. Who knows? Maybe one day, we’ll look back at these early efforts with a smile, thinking about how we once tried to catch a whisper in the cosmic wind.

Original Source

Title: Searches for signatures of ultra-light axion dark matter in polarimetry data of the European Pulsar Timing Array

Abstract: Ultra-light axion-like particles (ALPs) can be a viable solution to the dark matter problem. The scalar field associated with ALPs, coupled to the electromagnetic field, acts as an active birefringent medium, altering the polarisation properties of light through which it propagates. In particular, oscillations of the axionic field induce monochromatic variations of the plane of linearly polarised radiation of astrophysical signals. The radio emission of millisecond pulsars provides an excellent tool to search for such manifestations, given their high fractional linear polarisation and negligible fluctuations of their polarisation properties. We have searched for the evidence of ALPs in the polarimetry measurements of pulsars collected and preprocessed for the European Pulsar Timing Array (EPTA) campaign. Focusing on the twelve brightest sources in linear polarisation, we searched for an astrophysical signal from axions using both frequentist and Bayesian statistical frameworks. For the frequentist analysis, which uses Lomb-Scargle periodograms at its core, no statistically significant signal has been found. The model used for the Bayesian analysis has been adjusted to accommodate multiple deterministic systematics that may be present in the data. A statistically significant signal has been found in the dataset of multiple pulsars with common frequency between $10^{-8}$ Hz and $2\times10^{-8}$ Hz, which can most likely be explained by the residual Faraday rotation in the terrestrial ionosphere. Strong bounds on the coupling constant $g_{a\gamma}$, in the same ballpark as other searches, have been obtained in the mass range between $6\times10^{-24}$ eV and $5\times10^{-21}$ eV. We conclude by discussing problems that can limit the sensitivity of our search for ultra-light axions in the polarimetry data of pulsars, and possible ways to resolve them.

Authors: N. K. Porayko, P. Usynina, J. Terol-Calvo, J. Martin Camalich, G. M. Shaifullah, A. Castillo, D. Blas, L. Guillemot, M. Peel, C. Tiburzi, K. Postnov, M. Kramer, J. Antoniadis, S. Babak, A. -S. Bak Nielsen, E. Barausse, C. G. Bassa, C. Blanchard, M. Bonetti, E. Bortolas, P. R. Brook, M. Burgay, R. N. Caballero, A. Chalumeau, D. J. Champion, S. Chanlaridis, S. Chen, I. Cognard, G. Desvignes, M. Falxa, R. D. Ferdman, A. Franchini, J. R. Gair, B. Goncharov, E. Graikou, J. -M. Grießmeier, Y. J. Guo, H. Hu, F. Iraci, D. Izquierdo-Villalba, J. Jang, J. Jawor, G. H. Janssen, A. Jessner, R. Karuppusamy, E. F. Keane, M. J. Keith, M. A. Krishnakumar, K. Lackeos, K. J. Lee, K. Liu, Y. Liu, A. G. Lyne, J. W. McKee, R. A. Main, M. B. Mickaliger, I. C. Niţu, A. Parthasarathy, B. B. P. Perera, D. Perrodin, A. Petiteau, A. Possenti, H. Quelquejay Leclere, A. Samajdar, S. A. Sanidas, A. Sesana, L. Speri, R. Spiewak, B. W. Stappers, S. C. Susarla, G. Theureau, E. van der Wateren, A. Vecchio, V. Venkatraman Krishnan, J. Wang, L. Wang, Z. Wu

Last Update: 2024-12-03 00:00:00

Language: English

Source URL: https://arxiv.org/abs/2412.02232

Source PDF: https://arxiv.org/pdf/2412.02232

Licence: https://creativecommons.org/licenses/by-sa/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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