Measurement of Min inimum Bia ias Observables wit ith ATLAS
Jiří Kvita, 28th Nov 2016 Palacký University, RCPTM, Olomouc, Czech Republic On behalf of the ATLAS collaboration
Observables wit ith ATLAS J i Kvita, 28 th Nov 2016 Palac k - - PowerPoint PPT Presentation
Measurement of Min inimum Bia ias Observables wit ith ATLAS J i Kvita, 28 th Nov 2016 Palac k University, RCPTM, Olomouc, Czech Republic On behalf of the ATLAS collaboration Outline Motivation ATLAS Inner Detector Samples,
Jiří Kvita, 28th Nov 2016 Palacký University, RCPTM, Olomouc, Czech Republic On behalf of the ATLAS collaboration
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radiation detectors, providing excellent position, vertex and PID resolution.
material or via decays.
IBL, allowed by a novel reduced-radius beam pipe.
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Positions of clusters in IBL, pixel, strip and TRT detectors. IBL insertion
radiation detectors, providing excellent position, vertex and PID resolution.
material or via decays.
IBL, allowed by a novel reduced-radius beam pipe.
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Positions of clusters in IBL, pixel, strip detectors. IBL insertion
different rapidity and multiplicity regions.
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different rapidity and multiplicity regions which are all probed by data.
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decay and few silicon hits.
systematics uncertainty.
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prompt particles, strange baryons (EPOS) and out-of-kinematic region fractions:
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particles multiplicity best described by EPOS.
well the η shape.
describe the pT dependence.
general purpose tune (SPS and Tevatron data).
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and Monash tunes, and EPOS.
described by QGSJET, which also deviates at large multiplicities.
general purpose tune.
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nch >= 2 nch >= 6 nch >= 20 nch >= 50
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describe η shape but fails at overall normalization.
dependence description, where QGSJET shows largest deviations.
while EPOS is best.
low and high nch.
structures.
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particles multiplicity best described by EPOS.
the η dependence.
describe the nch pT dependence.
(which is a 7 TeV tune)
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and Monash tunes, and EPOS, which are all 7 TeV tunes.
described by QGSJET.
interactions in material.
parameter distribution.
MC to match observed yield in data.
analysis phase space defined as |d0| < 1.5 mm (dashed vertical lines)
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shape but fails at overall normalization.
and total cross-section expected to be better described by an coming Pythia A3 tune.
dependence description, where QGSJET shows largest deviations.
while EPOS is best.
low and high nch.
also available in the |η|<0.8 phase-space to compare to ALICE and CMS.
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particles multiplicities per event per unit η in central region at
for comparion.
MC generators and their tunes observed.
EPOS, and Pythia Monash and A2 tunes.
multiplicities.
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nch >= 2 nch >= 6 nch >= 20 nch >= 50
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