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The success of the first few years of LHC operations at CERN, and the expectation of more to come as the LHC performance improves, are already leading to discussions of what should be next for both proton-proton and electron-positron…

High Energy Physics - Experiment · Physics 2015-06-22 Burton Richter

We review the quantum field theory description of Hawking radiation from evaporating black holes and summarize what is known about Hawking radiation from black holes in more than four space-time dimensions. In the context of the Large Extra…

High Energy Physics - Theory · Physics 2021-04-07 Panagiota Kanti , Elizabeth Winstanley

Black holes are among the most intriguing objects in modern physics. Their influence ranges from powering quasars and other active galactic nuclei, to providing key insights into quantum gravity. We review the observational evidence for…

General Relativity and Quantum Cosmology · Physics 2008-11-26 Gary T. Horowitz , Saul A. Teukolsky

A case is made that in encounters with the earth's atmosphere, astrophysical little black holes (LBH) can manifest themselves as the core energy source of balllightning (BL). Relating the LBH incidence rate on earth to BL occurrence has the…

Astrophysics · Physics 2015-06-24 Mario Rabinowitz

A derivation of the Hawking effect is given which avoids reference to field modes above some cutoff frequency $\omega_c\gg M^{-1}$ in the free-fall frame of the black hole. To avoid reference to arbitrarily high frequencies, it is necessary…

High Energy Physics - Theory · Physics 2009-10-22 Ted Jacobson

The top quark will be produced copiously at the LHC. This will make both detailed physics studies and the use of top quark decays for detector calibration possible. This talk reviews plans and prospects for top physics activities in the…

High Energy Physics - Experiment · Physics 2019-08-15 Andrei Gaponenko

Black holes are probably among the most fascinating objects populating our universe. Their characteristic features found within general relativity, encompassing spacetime singularities, event horizons, and black hole thermodynamics, provide…

High Energy Physics - Theory · Physics 2015-06-18 Benjamin Koch , Frank Saueressig

It is argued that the signals expected from the evaporation of mini black holes - predicted in TeV-scale gravity models with large extra dimensions and possibly produced in ultra high energy collisions in the atmosphere - have…

High Energy Physics - Phenomenology · Physics 2007-05-23 Theodore N. Tomaras

Black holes are presumed to have an ideal ability to absorb and keep matter. Whatever comes close to the event horizon, a boundary separating the inside region of a black hole from the outside world, inevitably goes in and remains inside…

General Relativity and Quantum Cosmology · Physics 2007-05-23 M. Yu. Kuchiev

We discuss and compare definitions of a black hole based on the existence of event and apparent horizons. In this connection we present a non-singular model of a black hole with a closed apparent horizon and discuss its properties. We…

High Energy Physics - Theory · Physics 2014-11-26 Valeri P. Frolov

This is the third out of five chapters of the final report [1] of the Workshop on Physics at HL-LHC, and perspectives on HE-LHC [2]. It is devoted to the study of the potential, in the search for Beyond the Standard Model (BSM) physics, of…

High Energy Physics - Phenomenology · Physics 2019-08-14 X. Cid Vidal , M. D'Onofrio , P. J. Fox , R. Torre , K. A. Ulmer , A. Aboubrahim , A. Albert , J. Alimena , B. C. Allanach , C. Alpigiani , M. Altakach , S. Amoroso , J. K. Anders , J. Y. Araz , A. Arbey , P. Azzi , I. Babounikau , H. Baer , M. J. Baker , D. Barducci , V. Barger , O. Baron , L. Barranco Navarro , M. Battaglia , A. Bay , D. Bhatia , S. Biswas , D. Bloch , D. Bogavac , C. Borschensky , M. K. Bugge , D. Buttazzo , G. Cacciapaglia , L. Cadamuro , A. Calandri , D. A. Camargo , A. Canepa , L. Carminati , S. Carrá , C. A. Carrillo Montoya , A. Carvalho Antunes De Oliveira , F. L. Castillo , V. Cavaliere , D. Cavalli , C. Cecchi , A. Celis , A. Cerri , G. S. Chahal , A. Chakraborty , S. V. Chekanov , H. J. Cheng , J. T. Childers , M. Cirelli , O. Colegrove , G. Corcella , M. Corradi , M. J. Costa , R. Covarelli , N. P. Dang , A. Deandrea , S. De Curtis , H. De la Torre , L. Delle Rose , D. Del Re , A. Demela , S. Demers , R. Dermisek , A. De Santo , K. Deshpande , B. Dey , J. Donini , A. K. Duncan , V. Dutta , C. Escobar , L. Fanó , G. Ferretti , J. Fiaschi , O. Fischer , T. Flacke , E. D. Frangipane , M. Frank , G. Frattari , D. Frizzell , E. Fuchs , B. Fuks , E. Gabrielli , J. Gainer , Y. Gao , J. E. García Navarro , M. H. Genest , S. Giagu , G. F. Giudice , J. Goh , M. Gouzevitch , P. Govoni , A. Greljo , A. Grohsjean , A. Gurrola , G. Gustavino , C. Guyot , C. B. Gwilliam , S. Ha , U. Haisch , J. Haller , T. Han , D. Hayden , M. Heikinheimo , U. Heintz , C. Helsens , K. Hoepfner , J. M. Hogan , K. Huitu , P. Ilten , V. Ippolito , A. Ismail , A. M. Iyer , Sa. Jain , D. O. Jamin , L. Jeanty , T. Jezo , W. Johns , A. Kalogeropoulos , J. Karancsi , Y. Kats , H. Keller , A. Khanov , J. Kieseler , B. Kim , M. S. Kim , Y. G. Kim , M. Klasen , M. D. Klimek , R. Kogler , J. R. Komaragiri , M. Krämer , S. Kubota , A. K. Kulesza , S. Kulkarni , T. Lari , A. Ledovskoy , G. R. Lee , L. Lee , S. W. Lee , R. Leonardi , R. Les , I. M. Lewis , Q. Li , T. Li , I. T. Lim , S. H. Lim , K. Lin , Z. Liu , K. Long , M. Low , E. Lunghi , D. Madaffari , F. Mahmoudi , D. Majumder , S. Malvezzi , M. L. Mangano , E. Manoni , X. Marcano , A. Mariotti , M. Marjanovic , D. Marlow , J. Martin Camalich , P. Matorras Cuevas , M. McCullough , E. F. McDonald , J. Mejia Guisao , B. Mele , F. Meloni , I. -A. Melzer-Pellmann , C. Merlassino , A. B. Meyer , E. Michielin , A. J. Miller , L. Mittnacht , S. Mondal , S. Moretti , S. Mukhopadhyay , B. P. Nachman , K. Nam , M. Narain , M. Nardecchia , P. Nath , J. Navarro-González , A. Nisati , T. Nitta , D. L. Noel , M. M. Nojiri , J. P. Ochoa-Ricoux , H. Oide , M. L. Ojeda , S. Pagan Griso , E. Palencia Cortezon , O. Panella , P. Pani , L. Panizzi , L. Panwar , C. B. Park , J. Pazzini , K. Pedro , M. M. Perego , L. Perrozzi , B. A. Petersen , A. Pierce , G. Polesello , A. Policicchio , C. J. Potter , P. Pralavorio , M. Presilla , J. Proudfoot , F. S. Queiroz , G. Ramirez-Sanchez , D. Redigolo , A. Reimers , S. Resconi , M. Rimoldi , J. C. Rivera Vergara , T. Rizzo , C. Rogan , F. Romeo , R. Rosten , R. Ruiz , J. Ruiz-Alvarez , J. A. Sabater Iglesias , B. Safarzadeh Samani , S. Sagir , M. Saito , S. Saito , F. Sala , C. Salazar , A. Savin , R. Sawada , S. Sawant , I. Schienbein , M. Schlaffer , B. Schneider , S. C. Schuler , C. D. Sebastiani , S. Sekmen , M. Selvaggi , D. Sengupta , H. Serce , H. Serodio , L. Sestini , B. Shakya , B. Shams Es Haghi , P. Sheldon , S. Shin , F. Simonetto , L. Soffi , M. Spannowsky , J. Stupak , M. J. Sullivan , M. Sunder , Y. Takahashi , X. Tata , H. Teagle , K. Terashi , A. Tesi , A. Thamm , K. Tobioka , P. Tornambe , F. Trovato , D. Tsiakkouri , F. C. Ungaro , A. Urbano , E. Usai , N. Vanegas , L. Vaslin , C. Vázquez Sierra , I. Vivarelli , M. Vranjes Milosavljevic , H. Waltari , R. Wang , X. Wang , M. S. Weber , C. Weiland , M. Wielers , J. M. Williams , S. Willocq , D. Xu , K. Yagyu , E. Yazgan , R. Ye , H. D. Yoo , T. You , F. Yu , G. Zevi Della Porta , W. Zhang , C. Zhu , X. Zhuang , J. Zobec , J. Zupan , J. Zurita

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

Studying the threshold of black hole formation via numerical evolution has led to the discovery of fascinating nonlinear phenomena. Power-law mass scaling, aspects of universality, and self-similarity have now been found for a large variety…

General Relativity and Quantum Cosmology · Physics 2009-10-31 Steven L. Liebling

If Micro Black Holes (MBHs) can be produced at the LHC, they will decay very fast. We study hypothetical MBHs that do not decay; in particular, QCD effects on accretion by MBHs that are produced at rest. We explain why accretion of a…

High Energy Physics - Phenomenology · Physics 2010-01-07 Itzhak Goldman , Yuval Grossman , Shmuel Nussinov

(This is a general physics level overview article about hidden sectors, and how they motivate searches for long-lived particles. Intended for publication in Physics Today.) Searches for new physics at the Large Hadron Collider have so far…

High Energy Physics - Phenomenology · Physics 2017-06-15 David Curtin , Raman Sundrum

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

The concept of Large Extra Dimensions (LED) provides a way of solving the Hierarchy Problem which concerns the weakness of gravity compared with the strong and electro-weak forces. A consequence of LED is that miniature Black Holes…

High Energy Physics - Phenomenology · Physics 2008-11-26 Thomas J. Humanic , Benjamin Koch , Horst Stoecker

We argue that the signals expected from the evaporation of mini black holes - predicted in TeV-scale gravity models with large extra dimensions, and possibly produced in ultra high energy collisions in the atmosphere - are quite similar to…

High Energy Physics - Phenomenology · Physics 2015-01-21 A. Mironov , A. Morozov , T. N. Tomaras

It has been suggested that maximally spinning black holes can serve as particle accelerators, reaching arbitrarily high center-of-mass energies. Despite several objections regarding the practical achievability of such high energies, and…

General Relativity and Quantum Cosmology · Physics 2015-06-12 Sean T. McWilliams

We consider a cosmological scenario in which the expansion of the Universe is dominated by phantom dark energy and black holes which condense out of the latter component. The mass of black holes decreases via Hawking evaporation and by…

General Relativity and Quantum Cosmology · Physics 2015-05-13 Julio C. Fabris , Diego Pavon