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Black Hole Remnants at the LHC
High Energy Physics - Phenomenology · Submitted 12 Jul 2005
abstract compiled · 2026-09-23 · no language-model review
The authors' main claim We find the total transverse momentum of the black hole event to be significantly dominated by the presence of a remnant mass providing a strong experimental signature for black hole remnant formation.
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.
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The abstract, sentence by sentence
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 final phases of the black hole's evaporation are still unknown, the formation of a black hole remnant is a theoretically well motivated expectation. We analyze the observables emerging from a black hole evaporation with a remnant instead of a final decay. We show that the formation of a black hole remnant yields a signature which differs substantially from a final decay. We find the total transverse momentum of the black hole event to be significantly dominated by the presence of a remnant mass providing a strong experimental signature for black hole remnant formation.
background contribution method result interpretation main claim
| # | sentence | role | the authors' own work | states the main conclusion | strength |
|---|---|---|---|---|---|
| s0 | Within the scenario of large extra dimensions, the Planck scale is lowered to values soon accessible. | background 1.00 | 0.05 | 0.02 | asserted 0.92 |
| s1 | Among the predicted effects, the production of TeV mass black holes at the {\sc LHC} is one of the most exciting possibilities. | background 1.00 | 0.04 | 0.03 | hedged possibility 0.76 |
| s2 | Though the final phases of the black hole's evaporation are still unknown, the formation of a black hole remnant is a theoretically well motivated expectation. | background 0.89 | 0.05 | 0.05 | asserted 0.81 |
| s3 | We analyze the observables emerging from a black hole evaporation with a remnant instead of a final decay. | contribution 0.99 | 0.88 | 0.05 | asserted 0.85 |
| s4 | We show that the formation of a black hole remnant yields a signature which differs substantially from a final decay. | result 0.96 | 0.89 | 0.29 | asserted 1.00 |
| s5 | We find the total transverse momentum of the black hole event to be significantly dominated by the presence of a remnant mass providing a strong experimental signature for black hole remnant formation. | result 0.99 | 0.95 | 0.86 | asserted 1.00 |
What was examined, and what was not
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- P abstract
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- C citations
- R cross-paper relations
The paper
Original abstract
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 final phases of the black hole's evaporation are still unknown, the formation of a black hole remnant is a theoretically well motivated expectation. We analyze the observables emerging from a black hole evaporation with a remnant instead of a final decay. We show that the formation of a black hole remnant yields a signature which differs substantially from a final decay. We find the total transverse momentum of the black hole event to be significantly dominated by the presence of a remnant mass providing a strong experimental signature for black hole remnant formation.
Human review
References
How the literature uses it
14 arXiv papers cite this in 21 sentences
Papers citing it · 9 sentences without a confident label
Uses its method or tool 2 papers
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while those labeled with “C” were produced using the Charybdis2 generator: * C1: rotating; * C2: nonrotating; * C3: rotating with the evaporation model in Ref. [ref] ; * C4: rotating with the Yoshino–Rychkov (YR) loss model [ref] , which is a conservative bound that includes impact parameter considerations; * C5: rotating, stable-remnant model [ref] , where the stable remnant must be a colorless object essentially equivalent to a quark-antiquark bound state; * C6: rotating, boiling remnant model [ref] , where the remnant continues to evaporate until a maximum Hawking temperature equal to is reached.
A search for microscopic black holes, string balls, and sphalerons in proton-proton collisions at $\sqrt{s}$ = 13 TeV · Data and simulated samples · 0.90
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Such an approach has been used in previous generators [ref] .
Monte Carlo event generator for black hole production and decay in proton-proton collisions · Class Member Functions · 0.92
Cites it as background 8 papers
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Previous studies of black hole remnants considered a high initial mass ($∼10$ TeV) black hole and examined its decay down to the Planck scale [ref] .
Noncommutative geometry inspired black holes in higher dimensions at the LHC · Results · 0.80
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In fact, it has been suggested that microscopic black holes could be created in particle accelerators [ref] and numerous studies have been carried out to determine the feasibility of their production [ref] and to characterize their observational signatures [ref] .
Semiclassical geons at particle accelerators · Introduction · 0.93
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The possibility of a final black hole remnant with mass of the order of the Planck scale has been studied [ref] .
Missing energy in black hole production and decay at the Large Hadron Collider · Introduction · 0.81
Discussion
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