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Related papers: Black hole/string ball production, possibly at LHC

200 papers

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

The correspondence principle between strings and black holes is a general framework for matching black holes and massive states of fundamental strings at a point where their physical properties (such as mass, entropy and temperature)…

High Energy Physics - Theory · Physics 2023-12-05 Nejc Čeplak , Roberto Emparan , Andrea Puhm , Marija Tomašević

We study the production cross section of a highly excited string with fixed angular momentum from an ultra-high energy collision of two light strings. We find that the cross section exhibits geometric behavior in a certain region of…

High Energy Physics - Theory · Physics 2009-02-26 Toshihiro Matsuo , Kin-ya Oda

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

If the fundamental planck scale is near a TeV, then parton collisions with high enough center-of-mass energy should produce black holes. The production rate for such black holes at LHC has been extensively studied for the case of a…

High Energy Physics - Phenomenology · Physics 2008-11-26 Andrew Chamblin , Gouranga C. Nayak

We make some observations regarding string/black hole correspondence with a view to understanding the nature of the quantum degrees of freedom of a black hole in string theory. In particular, we compare entropy change in analogous string…

High Energy Physics - Theory · Physics 2009-10-31 Ramzi R. Khuri

The correspondence principle offered a unique opportunity to test the Horowitz and Maldacena mechanism at correspondence point "the centre of mass energies around $(M_{s}/(g_{s})^{2})$". First by using Horowitz and Maldacena proposal, the…

High Energy Physics - Theory · Physics 2017-08-02 Alireza Sepehri , Somayyeh Shoorvazi , Mohammad Ebrahim Zomorrodian

The relevant physics for the possible formation of black holes in the LHC is discussed.

General Physics · Physics 2008-10-28 C Sivaram

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

For most black holes in string theory, the Schwarzschild radius in string units decreases as the string coupling is reduced. We formulate a correspondence principle, which states that (i) when the size of the horizon drops below the size of…

High Energy Physics - Theory · Physics 2009-10-09 Gary T. Horowitz , Joseph Polchinski

According to string theory, string ball is a highly excited long string which decays to standard model particles at the Hagedorn temperature with thermal spectrum. If there are extra dimensions, the string scale can be $\sim$ TeV, and we…

High Energy Physics - Phenomenology · Physics 2009-07-22 Gouranga C Nayak

Black hole production in high-energy collisions is briefly surveyed. Included is a summary of recent developments and open problems relevant to collider (LHC) production, as well as of some theoretical issues pointing towards fundamental…

High Energy Physics - Phenomenology · Physics 2008-11-26 Steven B. Giddings

In this chapter we review the current theoretical state of the art of small black holes at the LHC. We discuss the production mechanism for small non thermal black holes at the LHC and discuss new signatures due to a possible discrete mass…

High Energy Physics - Phenomenology · Physics 2013-01-10 Xavier Calmet , Dionysios Fragkakis , Nina Gausmann

With the advent of the LHC and the continuing influx of cosmological data, phenomenological aspects of string theory have received renewed attention in recent years and many problems have been properly incorporated in this framework. In…

High Energy Physics - Phenomenology · Physics 2015-05-13 Satoshi Nawata

We develop the general formalism for joining, splitting and interconnection of closed and open strings. As an application, we study examples of fundamental cosmic string collisions leading to gravitational collapse. We find that the…

High Energy Physics - Theory · Physics 2009-11-11 R. Iengo , J. Russo

We review recent progress in our understanding of the physics of black holes. In particular, we discuss the ideas from string theory that explain the entropy of black holes from a counting of microstates of the hole, and the related…

General Relativity and Quantum Cosmology · Physics 2009-11-07 Sumit R. Das , Samir D. Mathur

Relativistic current carrying strings moving axisymmetrically on the background of a Kerr black hole are studied. The boundaries and possible types of motion of a string with a given energy and current are found. Regions of parameters for…

General Relativity and Quantum Cosmology · Physics 2010-04-14 Ted Jacobson , Thomas P. Sotiriou

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

This paper reviews the role of black holes in the context of fundamental physics. After recalling some basic results stemming from Planckian string calculations, I present three examples of how stringy effects can improve the curvature…

General Relativity and Quantum Cosmology · Physics 2024-02-27 Piero Nicolini

We discuss the pair creation of black holes by the breaking of a cosmic string. We obtain an instanton describing this process from the $C$ metric, and calculate its probability. This is very low for the strings that have been suggested for…

General Relativity and Quantum Cosmology · Physics 2009-10-28 S. W. Hawking , Simon F. Ross
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