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Accreting black holes are believed to be sites of possible particle acceleration with favorable conditions also for effective gamma-ray production. However, because of photon-photon pair production, only low energy (MeV) gamma-rays can…

Astrophysics · Physics 2016-08-30 Felix Aharonian , Andrii Neronov

Quasars observed at redshifts $z\sim 6-7.5$ are powered by supermassive black holes which are too large to have grown from early stellar remnants without efficient super-Eddington accretion. A proposal for alleviating this tension is for…

High Energy Physics - Phenomenology · Physics 2023-06-28 Avi Friedlander , Sarah Schon , Aaron C. Vincent

The possibility of identifying some of Galactic gamma-ray sources as clusters of primordial black holes is discussed. The known scenarios of supermassive black hole formation indicate the multiple formation of lower-mass black holes. Our…

High Energy Astrophysical Phenomena · Physics 2012-12-12 K. M. Belotsky , A. V. Berkov , A. A. Kirillov , S. G. Rubin

The so-called "GeV-excess" of the diffuse Galactic gamma-ray emission is studied with a spectral template fit based on energy spectra. The spectral templates can be obtained in a data-driven way from the gamma-ray data, which avoids the use…

High Energy Astrophysical Phenomena · Physics 2017-09-13 Wim de Boer , Leo Bosse , Iris Gebauer , Alexander Neumann , Peter Biermann

The recent analyses of the Fermi Large Area Telescope data show an extended GeV $\gamma$-ray excess on top of the expected diffuse background in the Galactic center region, which can be explained with annihilating dark matter or a…

High Energy Astrophysical Phenomena · Physics 2015-04-23 Qiang Yuan , Kunihito Ioka

The evaporation of primordial black holes with a mass in the $1\ {\rm gram}\lesssim M_{\rm PBH}\lesssim$1000 kg range can lead to the production of dark matter particles of almost any mass in the range $0.1\ {\rm MeV}\lesssim m_{\rm…

Cosmology and Nongalactic Astrophysics · Physics 2019-05-06 Logan Morrison , Stefano Profumo , Yan Yu

Evidence of excess GeV emission nearly coinciding with the Galactic Centre has been interpreted as a possible signature of annihilating dark matter. In this paper, we argue that it seems too early to discard pulsars as a viable explanation…

High Energy Astrophysical Phenomena · Physics 2015-06-17 N. Mirabal

It has been proposed that the short period gamma-ray bursts, which occur at a rate of $\sim 10 {\rm yr^{-1}}$, may be evaporating primordial black holes (PBHs). Calculations of the present PBH evaporation rate have traditionally assumed…

Astrophysics · Physics 2014-10-13 Anne M. Green

In supergravity models, the evaporation of light Primordial Black Holes (PBHs) should be a source of gravitinos. By considering this process, new stringent limits are derived on the abundance of small black holes with initial masses less…

Astrophysics · Physics 2009-11-10 M. Yu Khlopov , A. Barrau , J. Grain

If the temperature of the hot thermal plasma in the Early Universe was within a few orders of magnitude of the Planck scale $M_{\rm Pl}$, then the hoop conjecture predicts the formation of microscopic black holes from particle collisions in…

High Energy Physics - Phenomenology · Physics 2023-10-03 Avi Friedlander , Ningqiang Song , Aaron C. Vincent

It has been conjectured that Micro Black Holes (MBH) may be formed in the presence of large extra dimensions. These MBHs have very small mass and they decay almost instantaneously. Taking into consideration quantum effects, they should…

High Energy Physics - Phenomenology · Physics 2013-12-17 Saeede Nafooshe , Martin O'Loughlin , Maria Vittoria Garzelli

An excess of gamma rays at GeV energies has been pointed out in the Fermi-LAT data. This signal comes from a narrow region centred around the Galactic center and has been interpreted as possible evidence for light dark matter particles…

High Energy Astrophysical Phenomena · Physics 2014-08-13 Thomas Lacroix , Celine Boehm , Joseph Silk

Due to their higher concentrations and small internal velocities, Milky Way subhalos can be at least as important as the smooth halo in accounting for the GeV positron excess via dark matter annihilation. After showing how this can be…

High Energy Astrophysical Phenomena · Physics 2010-08-13 Matthew D. Kistler , Jennifer M. Siegal-Gaskins

Following LIGO results of intermediate mass black holes mergers, the idea that dark matter is composed of Primordial Black Boles (PBH), made a recent comeback. PBHs might be formed in the early Universe through a variety of mechanisms, best…

High Energy Astrophysical Phenomena · Physics 2019-09-05 Thomas Tavernier , Jean-François Glicenstein , François Brun

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

Excess of gamma rays around the Galactic center (GC) observed in the Fermi Large Area Telescope (LAT) data is one of the most intriguing features in the gamma-ray sky. The spherical morphology and the spectral energy distribution with a…

High Energy Astrophysical Phenomena · Physics 2025-03-13 Dmitry V. Malyshev

Supermassive black holes (SMBHs) are common in local galactic nuclei, and SMBHs as massive as several billion solar masses already exist at redshift z=6. These earliest SMBHs may grow by the combination of radiation-pressure-limited…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-04 Zoltán Haiman

The production of Large Extra Dimension (LXD) Black Holes (BHs), with a new, fundamental mass scale of $M_f = 1$ TeV, has been predicted to occur at the Large Hadron Collider, LHC, with the formidable rate of $10^8$ per year in p-p…

High Energy Physics - Phenomenology · Physics 2008-11-26 Horst Stoecker

Massive Primordial Black Holes (MPBH) can be formed after inflation due to broad peaks in the primordial curvature power spectrum that collapse gravitationally during the radiation era, to form clusters of black holes that merge and…

Cosmology and Nongalactic Astrophysics · Physics 2017-06-28 Juan García-Bellido

Mirror matter models have been suggested recently as an explanation of neutrino puzzles and microlensing anomalies. We show that mirror supernovae can be a copious source of energetic gamma rays if one assumes that the quantum gravity scale…

Astrophysics · Physics 2011-05-23 R. N. Mohapatra , S. Nussinov , V. L. Teplitz