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We argue that black holes microstates leave an imprint on the gravitational vacuum through their virtual fluctuations. This imprint yields a power law fall off -- rather than an exponential fall off -- for the entanglement of planck scale…

High Energy Physics - Theory · Physics 2025-05-16 Samir D. Mathur

In string theory, black holes have a minimum mass below which they transition into highly excited long and jagged strings --- ``string balls''. These are the stringy progenitors of black holes; because they are lighter, in theories of…

High Energy Physics - Phenomenology · Physics 2009-11-07 Savas Dimopoulos , Roberto Emparan

Black holes could be produced at the Large Hadron Collider in TeV-scale gravity scenarios. We discuss missing energy mechanisms in black hole production and decay in large extra-dimensional models. In particular, we examine how graviton…

High Energy Physics - Phenomenology · Physics 2014-11-18 Douglas M. Gingrich

Recent calculations applying statistical mechanics indicate that in a setting with compactified large extra dimensions a black hole might evolve into a (quasi-)stable state with mass close to the new fundamental scale $M_f$. Black holes and…

High Energy Physics - Phenomenology · Physics 2009-11-10 Sabine Hossenfelder , Marcus Bleicher , Stefan Hofmann , Horst Stöcker , Ashutosh V. Kotwal

It is argued that the cross section for production of large black holes, for which a semiclassical description is applicable, cannot be given by the geometric area of the black hole horizon, as claimed recently in the literature. Rather the…

High Energy Physics - Phenomenology · Physics 2010-05-28 M. B. Voloshin

In this talk I briefly discuss some features of a striking signature of TeV quantum gravity/strings and large extra dimensions: the production of exotic objects such as black holes, and their stringy precursors, the string resonances at…

High Energy Physics - Phenomenology · Physics 2007-05-23 Roberto Emparan

In TeV-scale gravity scenarios with large extra dimensions, black holes may be produced at future colliders. Good arguments have been made for why general relativistic black holes may be just out of reach of the Large Hadron Collider (LHC).…

High Energy Physics - Phenomenology · Physics 2008-12-30 Douglas M. Gingrich , Kevin Martell

We estimate the rate at which collisions between ultra-high energy cosmic rays can form small black holes in models with extra dimensions. If recent conjectures about false vacuum decay catalyzed by black hole evaporation apply, the lack of…

High Energy Physics - Phenomenology · Physics 2019-03-13 Katherine J. Mack , Robert McNees

If TeV-scale gravity describes nature, black holes will be produced in particle accelerators, perhaps even with impressive rates at the Large Hadron Collider. Their decays, largely via the Hawking process, will be spectacular. Black holes…

High Energy Physics - Theory · Physics 2016-09-06 Steven B. Giddings

We examine the rates for the production of black holes(BH) at the LHC in light of the exponential suppression of the geometric cross section estimate recently proposed by Voloshin. We show that the resulting production rates will still be…

High Energy Physics - Phenomenology · Physics 2014-11-17 Thomas G. Rizzo

If a cosmological first-order phase transition occurs sufficiently slowly, delayed vacuum decay may lead to the formation of primordial black holes. Here we consider a simple model as a case study of how the abundance of the produced black…

High Energy Physics - Phenomenology · Physics 2025-05-20 Yanda Wu , Stefano Profumo

We consider black hole production at the LHC in a generic scenario with many extra dimensions where the Standard Model fields are confined to a brane. With $\sim 20$ dimensions the hierarchy problem is shown to be naturally solved without…

High Energy Physics - Phenomenology · Physics 2009-11-11 JoAnne L. Hewett , Ben Lillie , Thomas G. Rizzo

I argue that the true quantum gravity scale cannot be much larger than the Planck length, because if it were then the quantum gravity-induced fluctuations in $\Lam$ would be insufficient to produce the observed cosmic ``dark energy''. If…

General Relativity and Quantum Cosmology · Physics 2015-06-25 Rafael D. Sorkin

The coupling of a string to gravity allows for Schwarzschild black holes whose entropy to area relation is $S=(A/4)(1-4\mu)$, where $\mu$ is the string tension. This departure from the A/4 universality results from a string instanton…

High Energy Physics - Theory · Physics 2009-10-28 Francois Englert , Laurent Houart , Paul Windey

Within the scenario of large extra dimensions, the Planck scale is lowered to values soon accessible. Among the predicted effects, the production of TeV mass black holes at the {\sc LHC} is one of the most exciting possibilities. Though the…

High Energy Physics - Phenomenology · Physics 2009-11-11 Benjamin Koch , Marcus Bleicher , Sabine Hossenfelder

As was suggested about a year ago, one of the most dramatic consequences of low-scale (~1 TeV) quantum gravity is copious production of mini black holes at future accelerators and in ultra-high-energy cosmic ray collisions. Hawking…

High Energy Physics - Phenomenology · Physics 2007-05-23 Greg Landsberg

We investigate the possibility for cosmic ray experiments to discover non-thermal small black holes with masses in the TeV range. Such black holes would result due to the impact between ultra high energy cosmic rays or neutrinos with nuclei…

High Energy Physics - Phenomenology · Physics 2015-06-04 Xavier Calmet , Lauretiu Ioan Caramete , Octavian Micu

We investigate the pair creation of magnetically charged black holes on a cosmic string in the presence of a background magnetic field. The string may either break or fray to produce a pair of accelerating black holes described by Ernst…

High Energy Physics - Theory · Physics 2021-03-24 Amjad Ashoorioon , Mohammad Bagher Jahani Poshteh

Fundamental string theory has been used to show that low energy excitations of certain black holes are described by a two dimensional conformal field theory. This picture has been found to be extremely robust. In this paper it is argued…

High Energy Physics - Theory · Physics 2009-09-17 Juan M. Maldacena , Andrew Strominger

One of the most dramatic consequences of low-scale (~1 TeV) quantum gravity in models with large or warped extra dimension(s) is copious production of mini black holes at future colliders and in ultra-high-energy cosmic ray collisions.…

High Energy Physics - Phenomenology · Physics 2015-06-25 Greg Landsberg