Topic: Space
Cosmic rays are powerful particles that travel across the universe. Scientists used a space telescope to discover a common feature shared by these particles and understand their origins.
Cosmic rays are incredibly powerful particles that have been traveling across the universe for millions of years. For over 100 years, scientists have been trying to understand where they come from and how they get accelerated to such high energies. Now, researchers using a space telescope called DAMPE have made an important discovery that could help answer these questions.
The DAMPE space telescope was launched in December 2015 to study cosmic rays and explore possible connections to dark matter. By examining highly precise data collected by the telescope, researchers discovered a universal pattern in the energy spectra of primary cosmic ray nuclei. This means that for every type of nucleus studied, the number of particles begins dropping much faster after reaching a certain threshold.
Scientists refer to this effect as 'spectral softening.' Normally, higher-energy cosmic rays become less common as energy increases. However, the DAMPE observations revealed that the decline becomes dramatically steeper beyond a rigidity of roughly 15 TV (teraelectron-volts). Rigidity describes how strongly a particle's path resists being bent by magnetic fields.
The findings strongly support theories suggesting that cosmic ray acceleration and movement through space are controlled by rigidity. At the same time, the data largely rules out competing explanations based on energy per nucleon (energy divided by the number of nucleons in the particle).
Why It Matters
Understanding how cosmic rays are created and move through space can help us better understand the universe and its mysteries. This discovery could also lead to new insights into dark matter, which is still a mystery.
Key Facts
- Cosmic rays are incredibly powerful particles that travel across the universe at extreme energies.
- The DAMPE space telescope was launched in December 2015 to study cosmic rays and explore possible connections to dark matter.
- Researchers discovered a universal pattern in the energy spectra of primary cosmic ray nuclei, which is known as 'spectral softening'.
- The decline in higher-energy cosmic rays becomes dramatically steeper beyond a rigidity of roughly 15 TV (teraelectron-volts).
- The findings strongly support theories suggesting that cosmic ray acceleration and movement through space are controlled by rigidity.
Key Terms
- Rigidity
- A measure of how strongly a particle's path resists being bent by magnetic fields
Implications
Understanding how cosmic rays are created and move through space can help us better understand the universe and its mysteries. This discovery could also lead to new insights into dark matter, which is still a mystery.
Source: https://www.sciencedaily.com/releases/2026/05/260513221809.htm
Journal Reference:
- Francesca Alemanno, Qi An, Philipp Azzarello, Felicia-Carla-Tiziana Barbato, Paolo Bernardini, Xiao-Jun Bi, Hugo Boutin, Irene Cagnoli, Ming-Sheng Cai, Elisabetta Casilli, Jin Chang, Deng-Yi Chen, Jun-Ling Chen, Zhan-Fang Chen, Zi-Xuan Chen, Paul Coppin, Ming-Yang Cui, Tian-Shu Cui, Ivan De Mitri, Francesco de Palma, Adriano Di Giovanni, Tie-Kuang Dong, Zhen-Xing Dong, Giacinto Donvito, Jing-Lai Duan, Kai-Kai Duan, Rui-Rui Fan, Yi-Zhong Fan, Fang Fang, Kun Fang, Chang-Qing Feng, Lei Feng, Sara Fogliacco, Jennifer-Maria Frieden, Piergiorgio Fusco, Min Gao, Fabio Gargano, Essna Ghose, Ke Gong, Yi-Zhong Gong, Dong-Ya Guo, Jian-Hua Guo, Shuang-Xue Han, Yi-Ming Hu, Guang-Shun Huang, Xiao-Yuan Huang, Yong-Yi Huang, Maria Ionica, Lu-Yao Jiang, Wei Jiang, Yao-Zu Jiang, Jie Kong, Andrii Kotenko, Dimitrios Kyratzis, Shi-Jun Lei, Bo Li, Manbing Li, Wen-Hao Li, Wei-Liang Li, Xiang Li, Xian-Qiang Li, Yao-Ming Liang, Cheng-Ming Liu, Hao Liu, Jie Liu, Shu-Bin Liu, Yang Liu, Francesco Loparco, Miao Ma, Peng-Xiong Ma, Tao Ma, Xiao-Yong Ma, Giovanni Marsella, Mario-Nicola Mazziotta, Dan Mo, Yu Nie, Xiao-Yang Niu, Andrea Parenti, Wen-Xi Peng, Xiao-Yan Peng, Chiara Perrina, Enzo Putti-Garcia, Rui Qiao, Jia-Ning Rao, Yi Rong, Ritabrata Sarkar, Pierpaolo Savina, Andrea Serpolla, Zhi Shangguan, Wei-Hua Shen, Zhao-Qiang Shen, Zhong-Tao Shen, Leandro Silveri, Jing-Xing Song, Hong Su, Meng Su, Hao-Ran Sun, Zhi-Yu Sun, Antonio Surdo, Xue-Jian Teng, Andrii Tykhonov, Gui-Fu Wang, Jin-Zhou Wang, Lian-Guo Wang, Shen Wang, Xiao-Lian Wang, Yan-Fang Wang, Da-Ming Wei, Jia-Ju Wei, Yi-Feng Wei, Di Wu, Jian Wu, Sha-Sha Wu, Xin Wu, Zi-Qing Xia, Zheng Xiong, En-Heng Xu, Hai-Tao Xu, Jing Xu, Zhi-Hui Xu, Zun-Lei Xu, Zi-Zong Xu, Guo-Feng Xue, Ming-Yu Yan, Hai-Bo Yang, Peng Yang, Ya-Qing Yang, Hui-Jun Yao, Yu-Hong Yu, Qiang Yuan, Chuan Yue, Jing-Jing Zang, Sheng-Xia Zhang, Wen-Zhang Zhang, Yan Zhang, Ya-Peng Zhang, Yi Zhang, Yong-Jie Zhang, Yong-Qiang Zhang, Yun-Long Zhang, Zhe Zhang, Zhi-Yong Zhang, Cong Zhao, Hong-Yun Zhao, Xun-Feng Zhao, Chang-Yi Zhou, Xun Zhu, Yan Zhu. Charge-dependent spectral softenings of primary cosmic rays below the knee. Nature, 2026; 653 (8113): 52 DOI: 10.1038/s41586-026-10472-0
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