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Observing cosmic-ray extensive air showers with a silicon imaging detector
Satoshi Kawanomoto1, Michitaro Koike2, Fraser Bradfield3
1National Astronomical Observatory of Japan, Osawa, Mitaka, Tokyo, 181-8588, Japan. kawanomoto.satoshi@nao.ac.jp.
Researchers developed a new method using the Subaru Hyper Suprime-Cam (HSC) to observe extensive air showers. This technique allows detailed study of individual particles, aiding cosmic ray research.
Area of Science:
- Astrophysics and particle physics
- Cosmic ray physics
Background:
- High-energy cosmic rays create extensive air showers, offering insights into extreme universal phenomena.
- Observing these showers is crucial for understanding particle acceleration and propagation.
Purpose of the Study:
- To introduce and evaluate a novel method for observing extensive air showers.
- To demonstrate the capability of silicon imaging detectors for detailed shower analysis.
- To explore the potential of this method for reconstructing primary cosmic ray properties.
Main Methods:
- Utilizing the Subaru Hyper Suprime-Cam (HSC) silicon imaging detector for shower observation.
- Measuring individual secondary particles within extensive air showers.
- Integrating HSC data with a surface detector array for comprehensive analysis.
Main Results:
- Successfully observed extensive air showers using the Subaru HSC.
- Demonstrated the ability to measure individual secondary particles with high precision.
- Showcased the potential for reconstructing the incident direction of primary cosmic rays.
Conclusions:
- The Subaru HSC offers a powerful new tool for detailed extensive air shower studies.
- Combining silicon imaging detectors with surface arrays enhances the study of cosmic ray properties.
- This method opens avenues for interdisciplinary research in high-energy astrophysics.
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