“A new lens” into the Universe’s most energetic particles

Osaka Metropolitan University scientists, in cooperation with researchers from the National Astronomical Observatory of Japan, have captured cosmic-ray extensive air showers with unprecedented precision using the prime-focus wide field camera mounted on the Subaru Telescope, situated atop Mauna Kea in Hawaii. Analyzing approximately 17,000 images captured between 2014 and 2020, they pinpointed 13 images containing extensive air showers, with a number of particle tracks far exceeding the usual count.

Cosmic-ray extensive air shower captured by the Subaru Telescope: An example of a cosmic-ray extensive air shower recorded by the Subaru Telescope. The highlighted tracks, which are mostly aligned in similar directions, show the shower particles induced from a high-energy cosmic ray.

Osaka, Japan - Showers in bathrooms bring us comfort; showers from space bring astrophysicists joy. Osaka Metropolitan University scientists have observed, with their novel method, cosmic-ray extensive air showers with unprecedented precision, opening the door to new insights into the Universe’s most energetic particles.

When a high energy cosmic ray collides with the Earth's atmosphere, it generates an enormous number of particles known as an extensive air shower. A research team led by Associate Professor Toshihiro Fujii from the Graduate School of Science and Nambu Yoichiro Institute of Theoretical and Experimental Physics at Osaka Metropolitan University, along with graduate student Fraser Bradfield, has discovered that the prime-focus wide field camera mounted on the Subaru Telescope, situated atop the Mauna Kea volcano in Hawaii, can capture these extensive air showers with extremely high resolution.

The Subaru Telescope was designed for observational astronomy. Cosmic rays, appearing as “tracks” on the observed images and obscuring the targeted stars or galaxies, are dismissed as noise by usual astronomical data processing. However, this team’s research focuses on that very “noise.” Analyzing approximately 17,000 images captured between 2014 and 2020, the research team pinpointed 13 images that contained extensive air showers. These images displayed a far larger number of particle tracks than usual.

“With conventional observation methods, it is challenging to distinguish between the types of particles that constitute extensive air showers,” explained Professor Fujii. “Our method, on the other hand, has the potential to determine the nature of individual particles.”

Professor Fujii added, “Furthermore, by integrating our method with conventional approaches, we hope to advance our understanding of extensive air showers. This technique may allow us to search for dark matter or other exotic particles, offering additional insights into the transition of the Universe into a matter-dominated era.”

Their results are set for publication in Scientific Reports on October 12, 2023.

 

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About OMU 

Osaka Metropolitan University is a new public university established in April 2022, formed by merger between Osaka City University and Osaka Prefecture University. For more research news visit https://www.omu.ac.jp/en/ or follow @OsakaMetUniv_en and #OMUScience.

Published: 12 Oct 2023

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Rina Matsuki

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Reference: 

Title: Observing Cosmic-Ray Extensive Air Showers with a Silicon Imaging Detector
DOI: 10.1038/s41598-023-42164-4
Author: Satoshi Kawanomoto, Michitaro Koike, Fraser Bradfield, Toshihiro Fujii, Yutaka Komiyama, Satoshi Miyazaki, Tomoki Morokuma, Hitoshi Murayama, Masamune Oguri, Tsuyoshi Terai
Published: October 12, 2023
URL: https://www.nature.com/articles/s41598-023-42164-4

Funding information:

This work was supported by JSPS KAKENHI Grant Number 20H00181, 20H05856, 22K21349, JP20H05852. This work was supported by JST, the establishment of university fellowships towards the creation of science technology innovation, Grant Number JPMJFS2138.