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Primordial Black Holes (PBHs) may have been created by density fluctuations in the early Universe and could be as massive as $> 10^9$ solar masses or as small as the Planck mass. It has been postulated that a black hole has a temperature…

Primordial Black Holes (PBHs) are gravitationally collapsed objects that may have been created by density fluctuations in the early universe and could have arbitrarily small masses down to the Planck scale. Hawking showed that due to…

High Energy Astrophysical Phenomena · Physics 2015-10-21 A. A. Abdo , A. U. Abeysekara , R. Alfaro , B. T. Allen , C. Alvarez , J. D. Álvarez , R. Arceo , J. C. Arteaga-Velázquez , T. Aune , H. A. Ayala Solares , A. S. Barber , B. M. Baughman , N. Bautista-Elivar , J. Becerra Gonzalez , E. Belmont , S. Y. BenZvi , D. Berley , M. Bonilla Rosales , J. Braun , R. A. Caballero-Lopez , K. S. Caballero-Mora , A. Carramiñana , M. Castillo , C. Chen , G. E. Christopher , U. Cotti , J. Cotzomi , E. de la Fuente , C. De León , T. DeYoung , R. Diaz Hernandez , L. Diaz-Cruz , J. C. Díaz-Vélez , B. L. Dingus , M. A. DuVernois , R. W. Ellsworth , D. W. Fiorino , N. Fraija , A. Galindo , F. Garfias , M. M. González , J. A. Goodman , V. Grabski , M. Gussert , Z. Hampel-Arias , J. P. Harding , E. Hays , C. M. Hoffman , C. M. Hui , P. Hüntemeyer , A. Imran , A. Iriarte , P. Karn , D. Kieda , B. E. Kolterman , G. J. Kunde , A. Lara , R. J. Lauer , W. H. Lee , D. Lennarz , H. León Vargas , E. C. Linares , J. T. Linnemann , M. Longo , R. Luna-GarcIa , J. H. MacGibbon , A. Marinelli , S. S. Marinelli , H. Martinez , O. Martinez , J. Martínez-Castro , J. A. J. Matthews , J. McEnery , E. Mendoza Torres , A. I. Mincer , P. Miranda-Romagnoli , E. Moreno , T. Morgan , M. Mostafá , L. Nellen , P. Nemethy , M. Newbold , R. Noriega-Papaqui , T. Oceguera-Becerra , B. Patricelli , R. Pelayo , E. G. Pérez-Pérez , J. Pretz , C. Rivière , D. Rosa-González , J. Ryan , H. Salazar , F. Salesa , A. Sandoval , P. M. Saz Parkinson , M. Schneider , A. Shoup , S. Silich , G. Sinnis , A. J. Smith , D. Stump , K. Sparks Woodle , R. W. Springer , I. Taboada , P. A. Toale , K. Tollefson , I. Torres , T. N. Ukwatta , V. Vasileiou , L. Villaseñor , G. P. Walker , T. Weisgarber , S. Westerhoff , D. A. Williams , I. G. Wisher , J. Wood , G. B. Yodh , P. W. Younk , D. Zaborov , A. Zepeda , H. Zhou

Many early universe theories predict the creation of Primordial Black Holes (PBHs). The PBHs could have masses ranging from the Planck mass to 10^5 solar masses or higher depending on the formation scenario. Hawking showed that any Black…

High Energy Astrophysical Phenomena · Physics 2015-11-02 J. T. Linnemann , D. Stump , S. S. Marinelli , T. Yapici , K. Tollefson , T. N. Ukwatta , J. H. MacGibbon

Primordial Black Holes (PBHs) are of interest in many cosmological contexts. PBHs lighter than about 1012 kg are predicted to be directly detectable by their Hawking radiation. This radiation should produce both a diffuse extragalactic…

High Energy Astrophysical Phenomena · Physics 2015-03-05 Jane H MacGibbon , Tilan N. Ukwatta , J. T. Linnemann , S. S. Marinelli , D. Stump , K. Tollefson

Many early universe theories predict the creation of Primordial Black Holes (PBHs). PBHs could have masses ranging from the Planck mass to 10^5 solar masses or higher depending on the size of the universe at formation. A Black Hole (BH) has…

High Energy Astrophysical Phenomena · Physics 2016-04-27 T. N. Ukwatta , D. R. Stump , J. T. Linnemann , J. H. MacGibbon , S. S. Marinelli , T. Yapici , K. Tollefson

Primordial Black Holes (PBHs) are hypothetical black holes predicted to have been formed from density fluctuations in the early Universe. PBHs with an initial mass around $10^{14}-10^{15}$g are expected to end their evaporation at present…

High Energy Astrophysical Phenomena · Physics 2023-05-10 H. E. S. S. collaboration , : , F. Aharonian , F. Ait Benkhali , J. Aschersleben , M. Boettcher , M. Backes , V. Barbosa Martins , R. Batzo , Y. Becherini , D. Berge , B. Bi , C. Boisson , J. Bolmont , M. de Bony de Lavergne , J. Borowska , F. Bradascio , R. Brose , F. Brun , B. Bruno , T. Bulik , C. Burger-Scheidlin , S. Caro , S. Casanova , J. Celic , M. Cerruti , T. Chand , A. Chen , O. Chibueze , G. Cotter , J. Damascene Mbarubucyeye , A. Djannati-Atai , K. Egberts , C. van Eldik , J. -P. Ernenwein , M. Fussling , A. Fiasson , G. Fichet de Clairfontaine , G. Fontaine , S. Gabici , S. Ghafourizadeh , G. Giavitto , D. Glawion , J. F. Glicenstein , G. Grolleron , M. -H. Grondin , L. Haerer , M. Haupt , J. A. Hinton , W. Hofmann , M. Holler , D. Horns , Zhiqiu Huang , M. Jamrozy , F. Jankowsky , V. Joshi , I. Jung-Richardt , E. Kasai , K. Katarzynski , B. Khelifi , S. Klepser , W. Kluzniak , Nu. Komin , K. Kosack , D. Kostunin , T. L. Holch , R. G. Lang , S. Le Stum , F. Leitl , A. Lemiere , J. -P. Lenain , F. Leuschner , T. Lohse , A. Luashvili , I. Lypova , J. Mackey , D. Malyshev , V. Marandon , P. Marchegiani , P. Marinos , G. Marti-Devesa , R. Marx , A. Mitchell , R. Moderski , L. Mohrmann , A. Montanari , E. Moulin , J. Muller , K. Nakashima , M. de Naurois , J. Niemiec , P. O'Brien , S. Ohm , L. Olivera-Nieto , E. de Ona Wilhelmi , M. Ostrowski , G. Puehlhofer , S. Panny , M. Panter , R. D. Parsons , G. Peron , A. Priyana Noel , D. A. Prokhorov , H. Prokoph , M. Punch , A. Quirrenbach , P. Reichherzer , O. Reimer , F. Rieger , G. Rowell , B. Rudak , H. Rueda Ricarte , V. Sahakian , H. Salzmann , D. A. Sanchez , A. Santangelo , M. Sasaki , H. M. Schutte , U. Schwanke , J. N. S. Shapopi , H. Sol , A. Specovius , S. Spencer , L. Stawarz , R. Steenkamp , S. Steinmassl , C. Steppa , I. Sushch , H. Suzuki , T. Takahashi , T. Tanaka , T. Tavernier , C. Thorpe-Morgan , N. Tsuji , Y. Uchiyama , M. Vecchi , J. Veh , C. Venter , J. Vink , S. J. Wagner , R. White , A. Wierzcholska , Yu Wun Wong , M. Zacharias , D. Zargaryan , A. A. Zdziarski , A. Zech , S. Zouari , N. Zywucka

Primordial Black Holes~(PBHs) are hypothetical black holes with a wide range of masses that formed in the early universe. As a result, they may play an important cosmological role and provide a unique probe of the early universe. A PBH with…

High Energy Astrophysical Phenomena · Physics 2025-11-04 Zhen Cao , F. Aharonian , Y. X. Bai , Y. W. Bao , D. Bastieri , X. J. Bi , Y. J. Bi , W. Bian , A. V. Bukevich , C. M. Cai , W. Y. Cao , Zhe Cao , J. Chang , J. F. Chang , A. M. Chen , E. S. Chen , G. H. Chen , H. X. Chen , Liang Chen , Long Chen , M. J. Chen , M. L. Chen , Q. H. Chen , S. Chen , S. H. Chen , S. Z. Chen , T. L. Chen , X. B. Chen , X. J. Chen , Y. Chen , N. Cheng , Y. D. Cheng , M. C. Chu , M. Y. Cui , S. W. Cui , X. H. Cui , Y. D. Cui , B. Z. Dai , H. L. Dai , Z. G. Dai , Danzengluobu , Y. X. Diao , X. Q. Dong , K. K. Duan , J. H. Fan , Y. Z. Fan , J. Fang , J. H. Fang , K. Fang , C. F. Feng , H. Feng , L. Feng , S. H. Feng , X. T. Feng , Y. Feng , Y. L. Feng , S. Gabici , B. Gao , C. D. Gao , Q. Gao , W. Gao , W. K. Gao , M. M. Ge , T. T. Ge , L. S. Geng , G. Giacinti , G. H. Gong , Q. B. Gou , M. H. Gu , F. L. Guo , J. Guo , X. L. Guo , Y. Q. Guo , Y. Y. Guo , Y. A. Han , O. A. Hannuksela , M. Hasan , H. H. He , H. N. He , J. Y. He , X. Y. He , Y. He , S. Hernández-Cadena , B. W. Hou , C. Hou , X. Hou , H. B. Hu , S. C. Hu , C. Huang , D. H. Huang , J. J. Huang , T. Q. Huang , W. J. Huang , X. T. Huang , X. Y. Huang , Y. Huang , Y. Y. Huang , X. L. Ji , H. Y. Jia , K. Jia , H. B. Jiang , K. Jiang , X. W. Jiang , Z. J. Jiang , M. Jin , S. Kaci , M. M. Kang , I. Karpikov , D. Khangulyan , D. Kuleshov , K. Kurinov , B. B. Li , Cheng Li , Cong Li , D. Li , F. Li , H. B. Li , H. C. Li , Jian Li , Jie Li , K. Li , L. Li , R. L. Li , S. D. Li , T. Y. Li , W. L. Li , X. R. Li , Xin Li , Y. Li , Y. Z. Li , Zhe Li , Zhuo Li , E. W. Liang , Y. F. Liang , S. J. Lin , B. Liu , C. Liu , D. Liu , D. B. Liu , H. Liu , H. D. Liu , J. Liu , J. L. Liu , J. R. Liu , M. Y. Liu , R. Y. Liu , S. M. Liu , W. Liu , X. Liu , Y. Liu , Y. Liu , Y. N. Liu , Y. Q. Lou , Q. Luo , Y. Luo , H. K. Lv , B. Q. Ma , L. L. Ma , X. H. Ma , J. R. Mao , Z. Min , W. Mitthumsiri , G. B. Mou , H. J. Mu , A. Neronov , K. C. Y. Ng , M. Y. Ni , L. Nie , L. J. Ou , P. Pattarakijwanich , Z. Y. Pei , J. C. Qi , M. Y. Qi , J. J. Qin , A. Raza , C. Y. Ren , D. Ruffolo , A. Sáiz , D. Semikoz , L. Shao , O. Shchegolev , Y. Z. Shen , X. D. Sheng , Z. D. Shi , F. W. Shu , H. C. Song , Yu. V. Stenkin , V. Stepanov , Y. Su , D. X. Sun , H. Sun , Q. N. Sun , X. N. Sun , Z. B. Sun , N. H. Tabasam , J. Takata , P. H. T. Tam , H. B. Tan , Q. W. Tang , R. Tang , Z. B. Tang , W. W. Tian , C. N. Tong , L. H. Wan , C. Wang , G. W. Wang , H. G. Wang , J. C. Wang , K. Wang , Kai Wang , Kai Wang , L. P. Wang , L. Y. Wang , L. Y. Wang , R. Wang , W. Wang , X. G. Wang , X. J. Wang , X. Y. Wang , Y. Wang , Y. D. Wang , Z. H. Wang , Z. X. Wang , Zheng Wang , D. M. Wei , J. J. Wei , Y. J. Wei , T. Wen , S. S. Weng , C. Y. Wu , H. R. Wu , Q. W. Wu , S. Wu , X. F. Wu , Y. S. Wu , S. Q. Xi , J. Xia , J. J. Xia , G. M. Xiang , D. X. Xiao , G. Xiao , Y. L. Xin , Y. Xing , D. R. Xiong , Z. Xiong , D. L. Xu , R. F. Xu , R. X. Xu , W. L. Xu , L. Xue , D. H. Yan , T. Yan , C. W. Yang , C. Y. Yang , F. F. Yang , L. L. Yang , M. J. Yang , R. Z. Yang , W. X. Yang , Z. H. Yang , Z. G. Yao , X. A. Ye , L. Q. Yin , N. Yin , X. H. You , Z. Y. You , Q. Yuan , H. Yue , H. D. Zeng , T. X. Zeng , W. Zeng , X. T. Zeng , M. Zha , B. B. Zhang , B. T. Zhang , C. Zhang , F. Zhang , H. Zhang , H. M. Zhang , H. Y. Zhang , J. L. Zhang , Li Zhang , P. F. Zhang , P. P. Zhang , R. Zhang , S. R. Zhang , S. S. Zhang , W. Y. Zhang , X. Zhang , X. P. Zhang , Yi Zhang , Yong Zhang , Z. P. Zhang , J. Zhao , L. Zhao , L. Z. Zhao , S. P. Zhao , X. H. Zhao , Z. H. Zhao , F. Zheng , W. J. Zhong , B. Zhou , H. Zhou , J. N. Zhou , M. Zhou , P. Zhou , R. Zhou , X. X. Zhou , X. X. Zhou , B. Y. Zhu , C. G. Zhu , F. R. Zhu , H. Zhu , K. J. Zhu , Y. C. Zou , X. Zuo , S. Wang , Xin Zhang

Primordial black holes (PBHs), more generally, BHs, undergo evaporation and, in principle, will end their lives in bursts of very high-energy gamma rays. The notable aspect of the PBHs with an initial mass of $\sim10^{14}$ g is that they…

High Energy Astrophysical Phenomena · Physics 2024-10-28 Chen Yang , Sai Wang , Meng-Lin Zhao , Xin Zhang

Primordial Black Holes (PBHs) created early in the universe are dark matter candidates. One method of detecting these PBHs is through their Hawking radiation. PBHs created with an initial mass of 5.0 x 10^14 g should be evaporating today…

High Energy Astrophysical Phenomena · Physics 2013-08-23 T. U. Ukwatta , D. Stump , J. T. Linnemann , K. Tollefson , V. Vasileiou , G. Sinnis , J. H. MacGibbon

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

Primordial black holes (PBHs) are thought to have been formed as a result of density fluctuations in the very early Universe. It is suggested that PBHs of mass $\sim 5 \times 10^{14} \mathrm{\ g}$ or less have evaporated through the release…

High Energy Astrophysical Phenomena · Physics 2019-09-04 Sajan Kumar

Primordial Black Holes (PBHs) are remnants of objects formed in the early Universe. Their lifetime is an increasing function of their mass, so PBHs in the right mass range can end their lives in an evaporation event that is potentially…

High Energy Astrophysical Phenomena · Physics 2021-08-25 R. López-Coto , M. Doro , A. de Angelis , M. Mariotti , J. P. Harding

Black holes with masses below approximately $10^{15}$ g are expected to emit gamma rays with energies above a few tens of MeV, which can be detected by the Fermi Large Area Telescope (LAT). Although black holes with these masses cannot be…

High Energy Astrophysical Phenomena · Physics 2018-02-02 LAT Collaboration

As the lifetime of a black hole decreases, the energy of the Hawking radiation it emits increases, ultimately culminating in its disappearance through a powerful burst of gamma rays. For primordial black holes (PBHs) with an initial mass of…

High Energy Astrophysical Phenomena · Physics 2025-09-03 Chen Yang , Jun-Da Pan , Xin Zhang

Primordial Black Holes (PBHs) are candidates for dark matter as well as ultra-high energy cosmic rays. PBHs are speculated to exist over a large range of masses, from below $10^{15}$ g to $10^3$ M$_\odot$. Here we search for PBHs with an…

High Energy Astrophysical Phenomena · Physics 2019-08-16 Pranav Dave , Ignacio Taboada

Primordial black holes (PBHs) with mass $10^{16}-10^{17}$ g almost escape constraints from observations so could essentially contribute to dark matter density. Hawking evaporation of such PBHs produces with a steady rate $\gamma$- and…

Cosmology and Nongalactic Astrophysics · Physics 2015-02-26 K. M. Belotsky , A. A. Kirillov

Recent developments in the study of primordial black holes (PBHs) will be reviewed, with particular emphasis on their formation and evaporation. PBHs could provide a unique probe of the early Universe, gravitational collapse, high energy…

Astrophysics · Physics 2008-11-26 B. J. Carr

Primordial Black Holes (PBHs), which may have been created in the early Universe, are predicted to be detectable by their Hawking radiation. The Fermi Gamma-ray Space Telescope observatory offers increased sensitivity to the gamma-ray…

High Energy Astrophysical Phenomena · Physics 2010-03-26 T. N. Ukwatta , Jane H. MacGibbon , W. C. Parke , K. S. Dhuga , S. Rhodes , A. Eskandarian , N. Gehrels , L. Maximon , D. C. Morris

Black hole relics are of significant interest in cosmology and theoretical physics. In this work, we consider tiny primordial black holes (PBHs) ( $M_{\text {PBH }} \lesssim 10^7 \mathrm{~g}$ ) which are generated soon after the end of…

High Energy Physics - Phenomenology · Physics 2025-12-30 Misao Sasaki , Jianing Wang

Primordial black holes (PBH), while still constituting a viable dark matter component, are expected to evaporate through Hawking radiation. Assuming the semi-classical approximation holds up to near the Planck scale, PBHs are expected to…

High Energy Physics - Phenomenology · Physics 2025-03-11 Valentina De Romeri , Yuber F. Perez-Gonzalez , Agnese Tolino
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