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Exploring the Universe's Vast Cosmic Voids

A look into cosmic voids and their role in understanding the universe.

Hernan Rincon, Segev BenZvi, Kelly Douglass, Dahlia Veyrat, Jessica Nicole Aguilar, Steven Ahlen, Davide Bianchi, David Brooks, Todd Claybaugh, Shaun Cole, Axel de la Macorra, Peter Doel, Andreu Font-Ribera, Jaime E. Forero-Romero, Enrique Gaztañaga, Satya Gontcho A Gontcho, Gaston Gutierrez, Klaus Honscheid, Cullan Howlett, Stephanie Juneau, Robert Kehoe, Sergey Koposov, Andrew Lambert, Martin Landriau, Laurent Le Guillou, Aaron Meisner, Ramon Miquel, John Moustakas, Gustavo Niz, Will Percival, Francisco Prada, Ignasi Pérez-Ràfols, Graziano Rossi, Eusebio Sanchez, Michael Schubnell, Hee-Jong Seo, David Sprayberry, Gregory Tarlé, Benjamin Alan Weaver, Hu Zou

― 4 min read


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Table of Contents

Welcome to the fascinating world of Cosmic Voids! Picture the universe as a big, starry room filled with furniture (that’s clumps of Galaxies) and, of course, plenty of empty spaces (voids). This article takes you on a journey through these voids and their significance in understanding the universe. We’ll explore how we created a catalog of voids using data from the Dark Energy Spectroscopic Instrument (DESI) and why it matters.

What Are Cosmic Voids?

Cosmic voids are large, empty spaces in the universe. They are the opposite of galaxy clusters, which are densely filled with stars and galaxies. Voids can be enormous, stretching tens of millions of light-years across. Imagine finding a giant room in your house with nothing but a single light bulb hanging from the ceiling-this is sort of what a void looks like in the cosmos!

The Universe’s Structure

The universe is not just a random scattering of stuff. It has a structure, like a web with thick strands of galaxies (called filaments) and large gaps in between (the voids). Understanding this structure helps scientists learn about how the universe evolved over time.

The Role of DESI

The DESI project is a massive telescope that helps us gather data about galaxies and quasars. It’s like a cosmic vacuum cleaner, sucking up information about millions of stars. This data has been crucial for identifying and cataloging voids, which are essential for studying the universe’s expansion and the mysterious dark energy.

Our Catalog Creation

In our quest to catalog voids, we took a sample of galaxies from the Bright Galaxy Survey collected by DESI. Using two different methods, we identified and classified the voids.

The Void-Finding Algorithms

  1. VoidFinder: Think of this as a cosmic detective. VoidFinder scans through data and identifies regions that are mostly empty. It looks at the distance between galaxies and decides which areas can be classified as voids.

  2. The Watershed Algorithm (V): This method works like a team of squirrels gathering nuts. It identifies zones based on their local density. It can spot smaller voids and even combine regions to create a clearer picture of the voids.

The Results

After applying these methods, we discovered a significant number of voids.

  • 1,484 voids were found using VoidFinder.
  • 386 voids were discovered using the watershed algorithm (with a pruning method called REVOLVER).
  • 295 voids came from another pruning method called VIDE.

Comparing with SDSS

To check if our findings were accurate, we compared our void catalog with another database called the Sloan Digital Sky Survey (SDSS). Though both catalogs showed consistent properties for voids, we noted differences in the volume that the voids covered. This difference likely stems from the different ways galaxies were selected in each survey.

The Importance of Voids

Why should we care about these cosmic voids? They tell us a lot about the universe's expansion and the odd stuff like dark energy that makes the universe grow faster. The spherical shape of voids also makes them useful for various tests to confirm our theories about the universe.

The Evolution of Voids

Voids are not static; they change over time. As galaxies move and evolve, voids can expand or contract. If you think of galaxies as being part of a big cosmic party, then voids are the dance floor-sometimes it gets crowded, other times it feels empty!

Future Research

As the DESI survey continues, we expect to gather more data about voids. With this, we can study voids over time and understand how they impact galaxy formation.

Data Collection Process

With each data release, we will refine our catalog of voids. Our goal is to include all available data from DESI and make updated catalogs that can be accessed by other scientists for future research.

Conclusion

In summary, the study of cosmic voids gives us a unique view of the universe. It helps us understand how galaxies and voids fit together like pieces of a cosmic jigsaw puzzle. By cataloging these voids, we can make significant strides in our understanding of the universe, dark energy, and how everything works.

So next time you look up at the night sky, remember that among all those stars and galaxies, there are vast, empty voids just waiting to be explored!

Original Source

Title: DESIVAST: A Catalog of Low-Redshift Voids using Data from the DESI DR1 Bright Galaxy Survey

Abstract: We present three separate void catalogs created using a volume-limited sample of the DESI Year 1 Bright Galaxy Survey. We use the algorithms VoidFinder and V2 to construct void catalogs out to a redshift of z=0.24. We obtain 1,461 interior voids with VoidFinder, 420 with V2 using REVOLVER pruning, and 295 with V2 using VIDE pruning. Comparing our catalog with an overlapping SDSS void catalog, we find generally consistent void properties but significant differences in the void volume overlap, which we attribute to differences in the galaxy selection and survey masks. These catalogs are suitable for studying the variation in galaxy properties with cosmic environment and for cosmological studies.

Authors: Hernan Rincon, Segev BenZvi, Kelly Douglass, Dahlia Veyrat, Jessica Nicole Aguilar, Steven Ahlen, Davide Bianchi, David Brooks, Todd Claybaugh, Shaun Cole, Axel de la Macorra, Peter Doel, Andreu Font-Ribera, Jaime E. Forero-Romero, Enrique Gaztañaga, Satya Gontcho A Gontcho, Gaston Gutierrez, Klaus Honscheid, Cullan Howlett, Stephanie Juneau, Robert Kehoe, Sergey Koposov, Andrew Lambert, Martin Landriau, Laurent Le Guillou, Aaron Meisner, Ramon Miquel, John Moustakas, Gustavo Niz, Will Percival, Francisco Prada, Ignasi Pérez-Ràfols, Graziano Rossi, Eusebio Sanchez, Michael Schubnell, Hee-Jong Seo, David Sprayberry, Gregory Tarlé, Benjamin Alan Weaver, Hu Zou

Last Update: 2024-10-31 00:00:00

Language: English

Source URL: https://arxiv.org/abs/2411.00148

Source PDF: https://arxiv.org/pdf/2411.00148

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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