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We review the perhaps most exciting phenomenology of models with extra spatial dimensions and Planck scale near TeV: the production of mini black holes in ultrahigh energy particle collisions, and the discovery potential of cosmic…

High Energy Physics - Phenomenology · Physics 2007-05-23 Huitzu Tu

The existence of primordial black holes (PBHs), which may form from the collapse of matter overdensities shortly after the Big Bang, is still under debate. Among the potential signatures of PBHs are gravitational waves (GWs) emitted from…

It is generally believed that mini black holes decay by emitting elementary particles with a black body energy spectrum. The original calculation lead to the conclusion that about the 90% of the black hole mass is radiated away in the form…

High Energy Physics - Phenomenology · Physics 2009-11-11 Alex Casanova , Euro Spallucci

Using the BATSE survey data I find that quite small fraction of GRBs numbering 37 sources seems to emit the radiation similar to thermal bremsstrahlung in the range 20 to 300 keV. I suggest that these bursts may perhaps occur from collision…

Astrophysics · Physics 2009-06-25 B. E. Zhilyaev

It has been proposed that the first, intermediate-mass ($\approx 10^{5-6}~M_\odot$) black holes might form through direct collapse of unpolluted gas in atomic-cooling halos exposed to a strong Lyman-Werner (LW) or near-infrared (NIR)…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-18 Bin Yue , Andrea Ferrara , Ruben Salvaterra , Yidong Xu , Xuelei Chen

Primary proton-air interactions at ultra-high energies leave a physically interpretable imprint on the correlated fluctuations of the depth of shower maximum and the muon content in extensive air showers. This imprint reflects the…

High Energy Astrophysical Phenomena · Physics 2026-02-26 Lorenzo Cazon , Ruben Conceição , Miguel Alexandre Martins , Felix Riehn

Atmosphere-skimming showers are initiated by cosmic rays with incoming directions such that the full development of the cascade occurs inside the atmosphere without ever reaching the ground. This new class of showers has been observed in…

High Energy Astrophysical Phenomena · Physics 2024-09-25 Matias Tueros , Sergio Cabana-Freire , Jaime Álvarez-Muñiz

Cosmic rays from outer space enter the atmosphere with energies of up to 10^{11} GeV. The initial particle or a secondary hadron inside the shower may then interact with an air nucleon to produce nonstandard particles. In this article we…

High Energy Physics - Phenomenology · Physics 2008-11-26 J. I. Illana , M. Masip , D. Meloni

The Heitler-Matthews model for hadronic air showers will be extended to all the generations of electromagnetic subshowers in the hadronic cascade. The analysis is outlined in detail for showers initiated by primary protons. For showers…

High Energy Astrophysical Phenomena · Physics 2014-03-06 Hans Montanus

We revisit the role of primordial black holes (PBHs) as potential dark matter (DM) candidates, particularly focusing on light asteroid-mass PBHs. These PBHs are expected to emit particles through Hawking evaporation that can generate cosmic…

High Energy Astrophysical Phenomena · Physics 2026-03-26 Pedro De la Torre Luque , Jordan Koechler , Shyam Balaji

The interaction of ultra-high-energy cosmic rays with air nuclei triggers extensive air showers that reach their maximal energy deposition at the atmospheric depth $X_{\max}$. The distribution of this shower observable encodes information…

High Energy Astrophysical Phenomena · Physics 2025-10-27 Lorenzo Cazon , Ruben Conceição , Miguel Alexandre Martins , Felix Riehn

At ultra-high energies, the flux of cosmic rays is too low for direct measurements to be meaningful. When a cosmic ray enters the atmosphere, it initiates an extensive air shower, producing a cascade of secondary particles that propagate…

High Energy Astrophysical Phenomena · Physics 2025-08-25 Fiona Ellwanger , Darko Veberič

Black holes (BH), one of the most intriguing objects in the universe, can manifest themselves through electromagnetic radiation initiated by the accretion flow. Some stellar-mass BHs drive relativistic jets when accreting matter from their…

High Energy Astrophysical Phenomena · Physics 2026-01-01 The LHAASO Collaboration , Zhen Cao , Felix Aharonian , Yun-Xiang Bai , Yi-Wei Bao , Denis Bastieri , Xiao-Jun Bi , Yu-Jiang Bi , Wen-Yi Bian , Anatoly V Bukevich , Chengmiao Cai , Wen-Yu Cao , Zhe Cao , Jin Chang , Jin-Fan Chang , Aming Chen , En-Sheng Chen , Guohai Chen , Hua-Xi Chen , Liang Chen , Long Chen , Ming-Jun Chen , Ma-Li Chen , Qi-Hui Chen , Shi Chen , Su-Hong Chen , Song-Zhan Chen , Tian-Lu Chen , Xiao-Bin Chen , Xuejian Chen , Yang Chen , Ning Cheng , Yao-Dong Cheng , Ming Chung Chu , Ming-Yang Cui , Shu-Wang Cui , Xiao-Hong Cui , Yi-Dong Cui , Ben-Zhong Dai , Hong-Liang Dai , Zigao Dai , Danzeng Luobu , Yang-Xuan Diao , Xu-Qiang Dong , Kai-Kai Duan , Jun-Hui Fan , Yi-Zhong Fan , Jun Fang , Jian-Hua Fang , Kun Fang , Cun-feng Feng , Hua Feng , Li Feng , Shaohui Feng , Xiao-ting Feng , Yi Feng , You-liang Feng , Stefano Gabici , Bo Gao , Chuan-dong Gao , Qi Gao , Wei Gao , Wei-kang Gao , Maomao Ge , Ting-Ting Ge , Lisi Geng , Gwenael Giacinti , Guanghua Gong , Quanbu Gou , Min-Hao Gu , Fu-Lai Guo , Jing Guo , Xiao-Lei Guo , Yi-Qing Guo , Ying-Ying Guo , Yi-Ang Han , Otto A Hannuksela , Mariam Hasan , Hui-Hai He , Hao-Ning He , Jia-Yin He , Xinyu He , Yu He , Sergio Hernández-Cadena , Bo-Wen Hou , Chao Hou , Xian Hou , Hong-Bo Hu , Shi-Cong Hu , Chen Huang , Dai-Hui Huang , Jiajun Huang , Tian-Qi Huang , Wen-Jun Huang , Xing-Tao Huang , Xiao-Yuan Huang , Yong Huang , Yi-Yun Huang , Xiao-Lu Ji , Huan-Yu Jia , Kang Jia , Hou-Bing Jiang , Kun Jiang , Xiao-Wei Jiang , Ze-Jun Jiang , Min Jin , Samy Kaci , Ming-Ming Kang , Ivan Karpikov , Dmitry Khangulyan , Denis Kuleshov , Kirill Kurinov , Bing-Bing Li , Cheng Li , Cong Li , Dan Li , Fei Li , Haibo Li , Huicai Li , Jian Li , Jie Li , Kai Li , Long Li , Rong-Lan Li , Si-Da Li , Tian-Yang Li , Wen-Lian Li , Xiu-Rong Li , Xin Li , Yuan Li , Yizhuo Li , Zhe Li , Zhuo Li , En-Wei Liang , Yun-Feng Liang , Su-Jie Lin , Bing Liu , Cheng Liu , Dong Liu , Dang-Bo Liu , Hu Liu , Hai-Dong Liu , Jia Liu , Jia-Li Liu , Ji-Ren Liu , Mao-Yuan Liu , Ruo-Yu Liu , Si-Ming Liu , Wei Liu , X Liu , Yi Liu , Yu Liu , Yi-Nong Liu , Yu-Qing Lou , Qing Luo , Yu Luo , Hong-Kui Lv , Bo-Qiang Ma , Ling-Ling Ma , Xin-Hua Ma , Ji-Rong Mao , Zhen Min , Warit Mitthumsiri , Guo-Bin Mou , Hui-Jun Mu , Andrii Neronov , Kenny Chun Yu NG , Ming-Yang Ni , Lin Nie , Le-Jian Ou , Petchara Pattarakijwanich , Zhi-Yuan Pei , Jin-Can Qi , Meng-Yao Qi , Jia-Jun Qin , Ali Raza , Chong-Yang Ren , David Ruffolo , Alejandro Sáiz , Dmitri Semikoz , Lang Shao , Oleg Shchegolev , Yun-Zhi Shen , Xiang-Dong Sheng , Zhaodong Shi , Fu-Wen Shu , Hui-Chao Song , Yuri V Stenkin , Vladimir Stepanov , Yang Su , Dongxu Sun , Hao Sun , Qinning Sun , Xiaona Sun , Zhibin Sun , Nabeel Hussain Tabasam , Jumpei Takata , Pak Hin Thomas Tam , Hong-Bin Tan , Qingwen Tang , Ruiyi Tang , Zebo Tang , Wenwu Tian , Chaonan Tong , Li-Hong Wan , Chao Wang , Guangwei Wang , Hongguang Wang , Jiancheng Wang , Ke Wang , Kai Wang , Liping Wang , Lingyu Wang , Lu-Yao Wang , Ran Wang , Wei Wang , Xianggao Wang , Xin-Jian Wang , Xiang-Yu Wang , Yang Wang , Yu-Dong Wang , Zhong-Hai Wang , Zhong-Xiang Wang , Zheng Wang , Da-Ming Wei , Jun-Jie Wei , Yong-Jian Wei , Tao Wen , Shan-Shan Weng , Chao-Yong Wu , Han-Rong Wu , Qing-Wen Wu , Sha Wu , Xue-Feng Wu , Yu-Sheng Wu , Shao-qiang Xi , Jie Xia , Jun-Ji Xia , Guang-man Xiang , Di-xuan Xiao , Gang Xiao , Yu-liang Xin , Yi Xing , Ding-rong Xiong , Zeng Xiong , Dong-lian Xu , Reng-Feng Xu , Ren-Xin Xu , Wei-Li Xu , Liang Xue , Da-Hai Yan , Jing-Zhi Yan , Tian Yan , Chao-Wen Yang , Chu-Yuan Yang , Feng-Fan Yang , Li-Li Yang , Ming-Jie Yang , Rui-Zhi Yang , Wen-Xin Yang , Zihang Yang , Zhi-Guo Yao , Xuan-Ang Ye , Li-Qiao Yin , Na Yin , Xiao-Hao You , Zhi-Yong You , Yan-Hong Yu , Qiang Yuan , Hua Yue , Hou-Dun Zeng , Ting-Xuan Zeng , Wei Zeng , Xiangtao Zeng , Min Zha , Bin-Bin Zhang , Bing Theodore Zhang , Chao Zhang , Feng Zhang , Hong-Fei Zhang , Hai-Ming Zhang , Heng-Ying Zhang , Jian-Li Zhang , Li Zhang , Peng-Fei Zhang , Pei-Pei Zhang , Rui Zhang , Shao-Ru Zhang , Shou-Shan Zhang , Weiyan Zhang , Xiao Zhang , Xiao-Peng Zhang , Yi Zhang , Yong Zhang , Zhi-Peng Zhang , Jing Zhao , Lei Zhao , Li-Zhi Zhao , Shi-Ping Zhao , Xiao-Hong Zhao , Zihao Zhao , Fu Zheng , Wen-Juan Zhong , Bin Zhou , Hao Zhou , Jia-Neng Zhou , Meng Zhou , Ping Zhou , Rong Zhou , Xiao-Xi Zhou , Xun-Xiu Zhou , Ben-Yang Zhu , Cheng-Guang Zhu , Feng-Rong Zhu , Hui Zhu , Ke-Jun Zhu , Yuan-Chuan Zou , Xiong Zuo

Recently, an alleged plausible astrophysical scenario was proposed for the production of observed thermal gamma-ray bursts, via Hawking radiation emitted from a primordial black hole (PBH) freely falling into a more massive black hole. Here…

General Relativity and Quantum Cosmology · Physics 2022-02-08 Tyler McMaken

In models based on large extra dimensions where massive spin 2 exchange can dominate at high energies, the neutrino-proton cross section can rise to typical hadronic values at energies above 10^20 eV. The neutrino then becomes a candidate…

High Energy Physics - Phenomenology · Physics 2009-10-31 Ambar Jain , Pankaj Jain , Douglas W. McKay , John P. Ralston

The recent detection of the gravitational wave source GW150914 by the LIGO collaboration motivates a speculative source for the origin of ultrahigh energy cosmic rays as a possible byproduct of the immense energies achieved in black hole…

High Energy Astrophysical Phenomena · Physics 2016-06-01 Kumiko Kotera , Joseph Silk

Extensive Air Showers are still the only source of information on primary cosmic rays and their interactions at energies above PeV. However, this information is hidden inside the multiplicative character of the cascading process. Inspite of…

High Energy Physics - Phenomenology · Physics 2008-11-26 A. D. Erlykin

The origin of observed extremely high energy cosmic rays remains an astrophysical enigma. We show that a single evaporating primordial black hole should produce 8.5*10^14 particles over a 10^20 eV threshold. This emission results from…

Astrophysics · Physics 2011-05-23 Aurelien Barrau

High Energy Cosmic Rays (C.R.) versus Neutrino and Neutralino induced Air-Shower maybe tested at Horizons by their muons, gamma and Cerenkov blazing signals. Inclined and Horizontal C.R. Showers (70-90 zenith angle) produce secondary…

Astrophysics · Physics 2007-05-23 D. Fargion
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