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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) hypothetically generated in the first instants of life of the Universe are potential dark matter (DM) candidates. Focusing on PBHs masses in the range $[5 \times10^{14} - 5 \times 10^{15}]$g, we point out that…

High Energy Physics - Phenomenology · Physics 2022-04-14 Roberta Calabrese , Damiano F. G. Fiorillo , Gennaro Miele , Stefano Morisi , Antonio Palazzo

The Hawking evaporation of primordial black holes (PBH) reheats the Universe locally, forming hot spots that survive throughout their lifetime. We propose to use the temperature profile of such hot spots to calculate the decay rate of…

High Energy Physics - Phenomenology · Physics 2024-10-15 Louis Hamaide , Lucien Heurtier , Shi-Qian Hu , Andrew Cheek

Sterile neutrinos ($\nu_s$s) are well-motivated and actively searched for hypothetical neutral particles that would mix with the Standard Model active neutrinos. They are considered prime warm dark matter (DM) candidates, typically when…

High Energy Physics - Phenomenology · Physics 2024-08-01 Muping Chen , Graciela B. Gelmini , Philip Lu , Volodymyr Takhistov

Primordial black holes (PBHs) formed from the collapse of density fluctuations provide a unique window into the physics of the early Universe. Their evaporation through Hawking radiation around the epoch of Big Bang nucleosynthesis (BBN)…

Cosmology and Nongalactic Astrophysics · Physics 2026-05-07 Quan-feng Wu , Xun-Jie Xu

The KM3NeT Collaboration recently announced the detection of a neutrino with energy 220 PeV. One possible source of such ultra-high-energy particles is the rapid emission of energetic Hawking radiation from a primordial black hole (PBH)…

High Energy Physics - Phenomenology · Physics 2025-09-24 Alexandra P. Klipfel , David I. Kaiser

Primordial black holes~(PBHs) formed in the early Universe are well-motivated dark matter~(DM) candidates over a wide range of masses. These PBHs could emit detectable signals in the form of photons, electrons, and neutrinos through Hawking…

High Energy Physics - Phenomenology · Physics 2024-09-25 Qishan Liu , Kenny C. Y. Ng

The study of primordial black holes (PBHs) and the Hawking radiation they produce represents a significant step toward understanding the role of these phenomena in the cosmological evolution of the Universe. PBHs could be a component of…

Cosmology and Nongalactic Astrophysics · Physics 2025-03-04 Yu. A. Lysyy , P. A. Kislitsyn , A. V. Ivanchik

A black hole is expected to end its lifetime in a cataclysmic runaway burst of Hawking radiation, emitting all Standard Model particles with ultra-high energies. Thus, the explosion of a nearby primordial black hole (PBH) has been proposed…

High Energy Physics - Phenomenology · Physics 2026-01-14 Lua F. T. Airoldi , Gustavo F. S. Alves , Yuber F. Perez-Gonzalez , Gabriel M. Salla , Renata Zukanovich Funchal

Primordial black holes (PBHs) are a potential dark matter candidate whose masses can span over many orders of magnitude. If they have masses in the $10^{15}-10^{17}$ g range, they can emit sizeable fluxes of MeV neutrinos through…

High Energy Physics - Phenomenology · Physics 2022-02-02 Valentina De Romeri , Pablo Martínez-Miravé , Mariam Tórtola

Primordial black holes (PBHs) formed in the early Universe are sources of neutrinos emitted via Hawking radiation. Such astrophysical neutrinos could be detected at Earth and constraints on the abundance of comet-mass PBHs could be derived…

High Energy Physics - Phenomenology · Physics 2022-09-30 Nicolás Bernal , Víctor Muñoz-Albornoz , Sergio Palomares-Ruiz , Pablo Villanueva-Domingo

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 capable of emitting extremely energetic particles independent of their interactions with the Standard Model. In this work, we investigate whether PBHs evaporating in the early universe could be responsible…

High Energy Physics - Phenomenology · Physics 2025-02-28 Quan-feng Wu , Xun-Jie Xu

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) in the mass range $10^{17} - 10^{23}~{\rm gm}$ are considered as possible dark matter candidates as they are not subject to big-bang nucleosynthesis constraints and behave like cold dark matter. If PBHs are…

General Relativity and Quantum Cosmology · Physics 2022-06-01 Semin Xavier , Alan Sunny , S. Shankaranarayanan

We review the formation and evaporation of primordial black holes (PBHs) and their possible contribution to dark matter. Various constraints suggest they could only provide most of it in the mass windows $10^{17}$ - $10^{23}\,$g or $10$ -…

Cosmology and Nongalactic Astrophysics · Physics 2022-05-03 Bernard Carr , Florian Kuhnel

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

We investigate the influence of hadron injection from evaporating primordial black holes (PBHs) in the early stage of the primordial nucleosynthesis era (t = 10^{-3} - 10^4 sec). The emitted quark-antiquark pairs or gluons immediately…

Astrophysics · Physics 2008-11-26 K. Kohri , Jun'ichi Yokoyama

There are ongoing efforts in detecting Hawking radiation from primordial black holes (PBH) formed during the early universe. Here we put an upper limit on the PBH number density that could have been formed prior to the big bang…

General Physics · Physics 2010-06-29 C. Sivaram , Kenath Arun

When light primordial black holes (PBHs) evaporate in the early Universe, they locally reheat the surrounding plasma, creating hot spots with temperatures that can be significantly higher than the average plasma temperature. In this work,…

High Energy Physics - Phenomenology · Physics 2024-09-05 Jacob Gunn , Lucien Heurtier , Yuber F. Perez-Gonzalez , Jessica Turner
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