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An analysis of the influence of background subtraction and quenching on jet observables in heavy-ion collisions

High Energy Physics - Phenomenology · Submitted 6 Nov 2012

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

The authors' main claim The average background level and fluctuations affect both single inclusive spectra and dijet asymmetries, although differently for different subtraction setups.

how it is stated · asserted 1.00 read the record →

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arXiv ID1211.1161 (version 2)
Pith IDV3VGL37B, Pith's permanent record of this paper and its review
CitationLeticia Cunqueiro, Liliana Apolin\'ario, N\'estor Armesto. "An analysis of the influence of background subtraction and quenching on jet observables in heavy-ion collisions." arXiv:1211.1161 (2012). https://pith.science/paper/V3VGL37B
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What the abstract itself states, as probabilities: claims first 0.03 · states limitation 0.26 · human participants 0.01 · controlled comparison 0.26 · randomized assignment 0.01 · states quantitative result 0.05 · compares with prior results 0.83 · mentions code or data availability 0.02.

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

Subtraction of the large background in reconstruction is a key ingredient in jet studies in high-energy heavy-ion collisions at RHIC and the LHC. Here we address the question to which extent the most commonly used subtraction techniques are able to eliminate the effects of the background on the most commonly discussed observables at present: single inclusive jet distributions, dijet asymmetry and azimuthal distributions. We consider two different background subtraction methods, an area-based one implemented through the FastJet pack- age and a pedestal subtraction method, that resemble the ones used by the experimental collaborations at the LHC. We also analyze different ways of defining the optimal parame- ters in the second method. We use a toy model that easily allows variations of the background characteristics: average background level and fluctuations and azimuthal structure, but cross- checks are also done with a Monte Carlo simulator. Furthermore, we consider the influence of quenching using Q-PYTHIA on the dijet observables with the different background subtrac- tion methods and, additionally, we examine the missing momentum of particles. The average background level and fluctuations affect both single inclusive spectra and dijet asymmetries, although differently for different subtraction setups. A large azimuthal modulation of the background has a visible effect on the azimuthal dijet distributions. Quenching, as imple- mented in Q-PYTHIA, substantially affects the dijet asymmetry but little the azimuthal dijet distributions. Besides, the missing momentum characteristics observed in the experiment are qualitatively reproduced by Q-PYTHIA.

background contribution method result interpretation main claim

What the classifier reports for each sentence. The number is the probability it gave the label.
#sentencerolethe authors' own workstates the main conclusionstrength
s0 Subtraction of the large background in reconstruction is a key ingredient in jet studies in high-energy heavy-ion collisions at RHIC and the LHC. background 1.00 0.05 0.03 asserted 1.00
s1 Here we address the question to which extent the most commonly used subtraction techniques are able to eliminate the effects of the background on the most commonly discussed observables at present: single inclusive jet distributions, dijet asymmetry and azimuthal distributions. contribution 0.83 0.37 0.04 unclear 0.81
s2 We consider two different background subtraction methods, an area-based one implemented through the FastJet pack- age and a pedestal subtraction method, that resemble the ones used by the experimental collaborations at the LHC. method 0.97 0.81 0.03 asserted 0.96
s3 We also analyze different ways of defining the optimal parame- ters in the second method. method 0.94 0.92 0.02 asserted 0.60
s4 We use a toy model that easily allows variations of the background characteristics: average background level and fluctuations and azimuthal structure, but cross- checks are also done with a Monte Carlo simulator. method 1.00 0.93 0.02 asserted 0.98
s5 Furthermore, we consider the influence of quenching using Q-PYTHIA on the dijet observables with the different background subtrac- tion methods and, additionally, we examine the missing momentum of particles. contribution 0.58 0.92 0.04 asserted 0.83
s6 The average background level and fluctuations affect both single inclusive spectra and dijet asymmetries, although differently for different subtraction setups. result 1.00 0.92 0.21 asserted 1.00
s7 A large azimuthal modulation of the background has a visible effect on the azimuthal dijet distributions. result 1.00 0.88 0.10 asserted 0.99
s8 Quenching, as imple- mented in Q-PYTHIA, substantially affects the dijet asymmetry but little the azimuthal dijet distributions. result 1.00 0.89 0.21 asserted 1.00
s9 Besides, the missing momentum characteristics observed in the experiment are qualitatively reproduced by Q-PYTHIA. result 0.97 0.84 0.08 asserted 0.93

What kind of paper the classifier reports this is: simulation study 1.00 · evidence from simulation or computation 1.00.

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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

Subtraction of the large background in reconstruction is a key ingredient in jet studies in high-energy heavy-ion collisions at RHIC and the LHC. Here we address the question to which extent the most commonly used subtraction techniques are able to eliminate the effects of the background on the most commonly discussed observables at present: single inclusive jet distributions, dijet asymmetry and azimuthal distributions. We consider two different background subtraction methods, an area-based one implemented through the FastJet pack- age and a pedestal subtraction method, that resemble the ones used by the experimental collaborations at the LHC. We also analyze different ways of defining the optimal parame- ters in the second method. We use a toy model that easily allows variations of the background characteristics: average background level and fluctuations and azimuthal structure, but cross- checks are also done with a Monte Carlo simulator. Furthermore, we consider the influence of quenching using Q-PYTHIA on the dijet observables with the different background subtrac- tion methods and, additionally, we examine the missing momentum of particles. The average background level and fluctuations affect both single inclusive spectra and dijet asymmetries, although differently for different subtraction setups. A large azimuthal modulation of the background has a visible effect on the azimuthal dijet distributions. Quenching, as imple- mented in Q-PYTHIA, substantially affects the dijet asymmetry but little the azimuthal dijet distributions. Besides, the missing momentum characteristics observed in the experiment are qualitatively reproduced by Q-PYTHIA.

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References
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20 arXiv papers cite this in 22 sentences

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

Papers citing it · 13 sentences without a confident label

Cites it as background 9 papers

What it cites · 64 sentences without a confident label

Uses the method or tool of 10 papers
Uses data or values from 10 papers
Compares with 8 papers
  • The increase of $q̂$ induces momentum imbalance: for $q̂=8$ GeV$^2$/fm, the $A_J$ distribution is in qualtitative agreement with experimental data (the agreement seems better when considering the difference between the CMS Monte Carlo and CMS data [ref] ).On the other hand, in spite of the shower being degraded in energy so that a significant $A_J$ is induced by quenching, the azimuthal dijet correlation is not very strongly modified, in apparent conflict with the generic link between energy loss and broadening [ref] .

    Jet quenching · Asymmetry · 0.98

  • The increase of $q̂$ induces momentum imbalance: for $q̂=8$ GeV$^2$/fm, the $A_J$ distribution is in qualtitative agreement with experimental data (the agreement seems better when considering the difference between the CMS Monte Carlo and CMS data [ref] ).On the other hand, in spite of the shower being degraded in energy so that a significant $A_J$ is induced by quenching, the azimuthal dijet correlation is not very strongly modified, in apparent conflict with the generic link between energy loss and broadening [ref] .

    Jet Quenching in Heavy Ion Collisions · Asymmetry · 0.98

  • The increase of $q̂$ induces momentum imbalance: for $q̂=8$ GeV$^2$/fm, the $A_J$ distribution is in qualtitative agreement with experimental data (the agreement seems better when considering the difference between the CMS Monte Carlo and CMS data [ref] ).On the other hand, in spite of the shower being degraded in energy so that a significant $A_J$ is induced by quenching, the azimuthal dijet correlation is not very strongly modified, in apparent conflict with the generic link between energy loss and broadening [ref] .

    The theory and phenomenology of perturbative QCD based jet quenching · Asymmetry · 0.98

Cites as support 1 paper
Cites as background 6 papers
  • The effect of background fluctuations on jet observables has extensively been discussed in [ref] .

    Fluctuations and asymmetric jet events in PbPb collisions at the LHC · Background energy and event-by-event fluctuations · 0.95

  • On the other hand, jet studies in hadronic collisions demand a procedure in order to separate jet constituents from the background of soft particles not coming from the shower of a hard parton, see [ref] and refs. therein.

    Towards Jetography · Introduction · 0.83

  • Among the different hard probes, the suppression of energetic particles and of jet-like correlations generically called jet quenching, see [ref] for recent reviews, lies among the most prominent ones.

    Jet quenching · Introduction · 1.00

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