Black holes, TeV-scale gravity and the LHC

Elizabeth Winstanley

RECORD

Black holes, TeV-scale gravity and the LHC

Elizabeth Winstanley

High Energy Physics - Theory · Submitted 23 Jun 2013

abstract compiled · 2026-09-23 · no language-model review

The authors' main claim We give an overview of some of the fundamental ideas of the large extra dimensions scenarios and the resulting black hole processes at the LHC.

how it is stated · asserted 0.81 read the record →

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The compiled record

The paper's own sentences, arranged. Each label is drawn from a closed vocabulary; the number beside it is the probability the classifier gave that label. Numbers in the tables are the authors', checked by code. No sentence in this record was written by a model.

Open the compiled record

Compiled by classifier-1.13-20260917 via OpenRouter, question bank abstract-p1-20260923, 2026-09-23: 1 request, 4,178 input tokens, $0.0002 reported.

What the abstract itself states, as probabilities: claims first 0.02 · states limitation 0.05 · human participants 0.02 · controlled comparison 0.02 · randomized assignment 0.01 · states quantitative result 0.20 · compares with prior results 0.05 · mentions code or data availability 0.01.

The abstract, sentence by sentence

arXiv listing abstract v2. Results and the main claim are underlined; show every role.

Over the past 15 years models with large extra space-time dimensions have been extensively studied. We have learned from these models that the energy scale of quantum gravity may be many orders of magnitude smaller than the conventional value of 10^19 GeV. This raises the tantalizing prospect of probing quantum gravity effects at the LHC. Of the possible quantum gravity processes at the LHC, the formation and subsequent evaporation of microscopic black holes is one of the most spectacular. We give an overview of some of the fundamental ideas of the large extra dimensions scenarios and the resulting black hole processes at the LHC.

background contribution method result interpretation main claim

What the classifier reports for each sentence. The number is the probability it gave the label.
#	sentence	role	the authors' own work	states the main conclusion	strength
s0	Over the past 15 years models with large extra space-time dimensions have been extensively studied.	background 1.00	0.03	0.02	asserted 1.00
s1	We have learned from these models that the energy scale of quantum gravity may be many orders of magnitude smaller than the conventional value of 10^19 GeV.	background 0.99	0.12	0.11	hedged possibility 0.96
s2	This raises the tantalizing prospect of probing quantum gravity effects at the LHC.	background 0.70	0.05	0.12	hedged possibility 0.84
s3	Of the possible quantum gravity processes at the LHC, the formation and subsequent evaporation of microscopic black holes is one of the most spectacular.	background 0.77	0.05	0.12	asserted 0.89
s4	We give an overview of some of the fundamental ideas of the large extra dimensions scenarios and the resulting black hole processes at the LHC.	contribution 0.99	0.67	0.08	asserted 0.81

What kind of paper the classifier reports this is: review 1.00 · evidence from literature 0.68.

What was examined, and what was not

sources read

arXiv listing abstract v2

not examined

full text
figures and tables
references and citing sentences
relations to other papers

levels run

P abstract

not run

S sections
T body sentences
C citations
R cross-paper relations

Every quoted sentence on this record is the authors'. Every label is from Pith's closed vocabulary, with the probability shown beside it. Every number in the measurements table is the authors', checked by code. Record as JSON

The paper

Original abstract

Over the past 15 years models with large extra space-time dimensions have been extensively studied. We have learned from these models that the energy scale of quantum gravity may be many orders of magnitude smaller than the conventional value of 10^19 GeV. This raises the tantalizing prospect of probing quantum gravity effects at the LHC. Of the possible quantum gravity processes at the LHC, the formation and subsequent evaporation of microscopic black holes is one of the most spectacular. We give an overview of some of the fundamental ideas of the large extra dimensions scenarios and the resulting black hole processes at the LHC.

Human review

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How the literature uses it

1 arXiv paper cite this in 1 sentence

Each citing sentence is taken from the citing paper's LaTeX source and typed by Pith's classifier. A label appears at probability 0.8 or more (0.95 for support), a contest at 0.7 or more; the quoted words are the citing authors'. How each label was checked · JSON

What it cites · 2 sentences without a confident label

Uses data or values from 2 papers

ATLAS rule out semi-classical black holes having masses lower than about 4 TeV/c$^2$ for six extra dimensions and $E_*$ about 2 TeV [ref] , while CMS have slightly higher lower bounds on the semi-classical black hole mass for the same values of $E_*$ [ref] .

Search for microscopic black holes in pp collisions at sqrt(s) = 8 TeV · Experimental searches · 0.95
As an example of the results from numerical relativity, four-dimensional calculations indicate that about 50% of the initial energy of the colliding particles is radiated away in the ultra-relativistic limit [ref] .

Universality, maximum radiation and absorption in high-energy collisions of black holes with spin · Balding phase · 0.95

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