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High-energy black hole production
High Energy Physics - Phenomenology · Submitted 7 Sep 2007
abstract compiled · 2026-09-23 · no language-model review
The authors' main claim 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 principles of quantum gravity.
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The abstract, sentence by sentence
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 principles of quantum gravity.
background contribution method result interpretation main claim
| # | sentence | role | the authors' own work | states the main conclusion | strength |
|---|---|---|---|---|---|
| s0 | Black hole production in high-energy collisions is briefly surveyed. | contribution 0.87 | 0.28 | 0.07 | asserted 0.70 |
| s1 | 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 principles of quantum gravity. | contribution 0.93 | 0.21 | 0.10 | asserted 0.91 |
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The paper
Original abstract
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 principles of quantum gravity.
Human review
References
How the literature uses it
11 arXiv papers cite this in 16 sentences
Papers citing it · 7 sentences without a confident label
Uses its data or values 1 paper
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Recent estimates [ref] , based on [ref] , give inelasticity $y$ of the order of 0.6–0.7, depending on $D$, dying off beyond impact parameters of about half the radius $R(√(ŝ))$.
Astrophysical implications of hypothetical stable TeV-scale black holes · Elementary cross sections · 0.92
Cites it as background 8 papers
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The standard approach [ref] (see [ref] for a recent review) to BH production at colliders assumes that BHs are formed directly in the collision of two SM particles.
Creating semiclassical black holes in collider experiments and keeping them on a string · Introduction · 0.95
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One of the most spectacular manifestations of nature realizing certain extra-dimensional scenarios [ref] could be the production of microscopic black holes at the LHC [ref] .[For reviews with more references see [ref] .] These are expected to undergo prompt, quasi-thermal, Hawking [ref] decay to large multiplicities of elementary particles, leading to very characteristic final states.
Astrophysical implications of hypothetical stable TeV-scale black holes · Introduction · 0.98
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This is all you need to set up an ultrahigh-energy collision.[While Lorentz invariance violation would change the nature of the problem, it would seem to reappear in a different guise, for example in the physics of black holes, like in the galaxy, formed from states that are not ultrarelativistic; such violation is also phenomenologically problematic.] Moreover, in recent years we have even been investigating models where, due to large or strongly-warped extra dimensions, the fundamental Planck scale $M_D$ could be as low as $∼TeV$, and such dynamics could be visible at LHC – for one review of this exciting possibility, see [ref] .
Beyond the Planck scale · Introduction · 0.82
What it cites · 71 sentences without a confident label
Contests 2 papers
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While inelasticity was considered in [ref] , its effects were underestimated based on these then state-of-the-art four-dimensional estimates – [ref] revealed that inelasticity increases with dimension.
High Energy Colliders as Black Hole Factories: The End of Short Distance Physics · Experimental expectations · contest 0.71
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While inelasticity was considered in [ref] , its effects were underestimated based on these then state-of-the-art four-dimensional estimates – [ref] revealed that inelasticity increases with dimension.
Classical Black Hole Production in High-Energy Collisions · Experimental expectations · contest 0.71
Uses data or values from 4 papers
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The trapped surface lower bounds of [ref] can be roughly parametrized by a curve of the form [equation] This parametrization follows from fig. 10 of [ref] , for $D=10$, with the cutoff taking into account a threshold of the form ([ref]).
Black hole formation in the grazing collision of high-energy particles · Experimental expectations · 0.88
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The trapped surface lower bounds of [ref] can be roughly parametrized by a curve of the form [equation] This parametrization follows from fig. 10 of [ref] , for $D=10$, with the cutoff taking into account a threshold of the form ([ref]).
Improved analysis of black hole formation in high-energy particle collisions · Experimental expectations · 0.88
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The trapped surface lower bounds of [ref] can be roughly parametrized by a curve of the form [equation] This parametrization follows from fig. 10 of [ref] , for $D=10$, with the cutoff taking into account a threshold of the form ([ref]).
Classical Black Hole Production in High-Energy Collisions · Experimental expectations · 0.88
Cites as support 5 papers
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However, such considerations also illustrate a narrowed parameter window where black hole production is possible, as has been stressed in [ref] .
Black Holes and Quantum Gravity at the LHC · Experimental expectations · 0.97
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However, such considerations also illustrate a narrowed parameter window where black hole production is possible, as has been stressed in [ref] .
Inelastic Black Hole Production and Large Extra Dimensions · Experimental expectations · 0.97
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These could produce an observable rate of black hole events [ref] .
Black Hole Production by Cosmic Rays · Experimental expectations · 0.96
Cites as background 17 papers
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Possible realizations of TeV-scale gravity include large extra dimensions [ref] and large warping [ref] .
Hierarchies from Fluxes in String Compactifications · Introduction · 0.91
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Possible realizations of TeV-scale gravity include large extra dimensions [ref] and large warping [ref] .
A Large Mass Hierarchy from a Small Extra Dimension · Introduction · 0.91
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(For more discussion see [ref] and references therein.) Classical production of black holes at high-energies was first studied by Penrose, who in unpublished work [ref] showed that a collision at zero impact parameter forms a closed-trapped surface.
Black Holes from Colliding Wavepackets · Formation · 0.91
Discussion
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