Search results for "Astrophysics"

showing 10 items of 8341 documents

"Table 6" of "Search for new phenomena in dijet events using 37 fb$^{-1}$ of $pp$ collision data collected at $\sqrt{s}=$13 TeV with the ATLAS detect…

2017

The number of events normalized to bin width as a function of the chi angular separation between the two jets, compared to background prediction from Monte Carlo simulation and corresponding uncertainties, in [4.3-4.6] TeV dijet invariant mass region

13000.0P P --> jj + XDijet SpectrumAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::ExperimentDijet SearchAngular Search
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"Table 8" of "Search for new phenomena in dijet events using 37 fb$^{-1}$ of $pp$ collision data collected at $\sqrt{s}=$13 TeV with the ATLAS detect…

2017

The number of events normalized to bin width as a function of the chi angular separation between the two jets, compared to background prediction from Monte Carlo simulation and corresponding uncertainties, in [4.9-5.4] TeV dijet invariant mass region

13000.0P P --> jj + XDijet SpectrumAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::ExperimentDijet SearchAngular Search
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"Table 1" of "Measurement of the Inelastic Proton-Proton Cross Section at $\sqrt{s} = 13$ TeV with the ATLAS Detector at the LHC"

2016

The measured and extrapolated inelastic cross section. The statistical uncertainty is negligible and is therefore displayed as zero. The first systematic uncertainty is the experimental systematic uncertainty apart from the luminosity, the second is the luminosity uncertainty, and the third is the extrapolation uncertainty.

13000.0Proton-Proton ScatteringAstrophysics::High Energy Astrophysical PhenomenaIntegrated Cross SectionExclusiveHigh Energy Physics::ExperimentAstrophysics::Cosmology and Extragalactic AstrophysicsCross SectionSIGProton-Proton Total Cross SectionP P --> X
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"Table 25" of "Multiplicity dependence of K*(892)$^{0}$ and $\phi$(1020) production in pp collisions at $\sqrt{s}$ = 13 TeV"

2020

$\phi$ transverse momentum spectrum - V0M multiplicity class VII

13000.0YieldsAstrophysics::High Energy Astrophysical PhenomenaProton-Proton CollisionsMathematics::History and OverviewAstrophysics::Solar and Stellar AstrophysicsNuclear ExperimentSIGPhiResonanceQuantitative Biology::Cell BehaviorP P --> Phi+XV0M Multiplicity
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"Table 3" of "Measurement of the $ZZ$ Production Cross Section in $pp$ Collisions at $\sqrt{s}$ = 13 TeV with the ATLAS Detector"

2016

Measured fiducial cross section in the $\mu^+\mu^-\mu^+\mu^-$ channel. The first systematic uncertainty is the combined systematic uncertainty excluding luminosity uncertainty, the second is the luminosity uncertainty.

13000.0Z ProductionAstrophysics::High Energy Astrophysical PhenomenaP P --> Z0 Z0 XIntegrated Cross SectionAstrophysics::Cosmology and Extragalactic AstrophysicsCross SectionSIGMuon productionInclusiveProton-Proton ScatteringAstrophysics::Solar and Stellar AstrophysicsHigh Energy Physics::ExperimentZ pair ProductionAstrophysics::Galaxy Astrophysics
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"Table 1" of "Measurement of the $ZZ$ Production Cross Section in $pp$ Collisions at $\sqrt{s}$ = 13 TeV with the ATLAS Detector"

2016

Measured fiducial cross section in the $e^+e^-e^+e^-$ channel. The first systematic uncertainty is the combined systematic uncertainty excluding luminosity uncertainty, the second is the luminosity uncertainty.

13000.0Z ProductionElectron productionAstrophysics::High Energy Astrophysical PhenomenaP P --> Z0 Z0 XIntegrated Cross SectionAstrophysics::Cosmology and Extragalactic AstrophysicsCross SectionSIGInclusiveProton-Proton ScatteringAstrophysics::Solar and Stellar AstrophysicsHigh Energy Physics::ExperimentZ pair ProductionAstrophysics::Galaxy Astrophysics
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"Table 2" of "Measurement of the $ZZ$ Production Cross Section in $pp$ Collisions at $\sqrt{s}$ = 13 TeV with the ATLAS Detector"

2016

Measured fiducial cross section in the $e^+e^-\mu^+\mu^-$ channel. The first systematic uncertainty is the combined systematic uncertainty excluding luminosity uncertainty, the second is the luminosity uncertainty.

13000.0Z ProductionElectron productionAstrophysics::High Energy Astrophysical PhenomenaP P --> Z0 Z0 XIntegrated Cross SectionAstrophysics::Cosmology and Extragalactic AstrophysicsCross SectionSIGMuon productionInclusiveProton-Proton ScatteringAstrophysics::Solar and Stellar AstrophysicsHigh Energy Physics::ExperimentZ pair ProductionAstrophysics::Galaxy Astrophysics
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"Table 126" of "A measurement of soft-drop jet observables in $pp$ collisions with the ATLAS detector at $\sqrt{s} = 13$ TeV"

2021

Data from Fig 17c. The extracted quark-distribution from the unfolded charged-particle $R_g$ distribution for anti-kt R=0.8 jets with 600 < $p_T$ < 800 GeV, after the soft drop algorithm is applied for $\beta$ = 2, in data. All uncertainties described in the text are shown on the data. The distributions are normalized to the integrated cross section, $\sigma$.

13000.0substructureAstrophysics::High Energy Astrophysical PhenomenaP P --> JET JETHigh Energy Physics::ExperimentSoft dropRg
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"Table 124" of "A measurement of soft-drop jet observables in $pp$ collisions with the ATLAS detector at $\sqrt{s} = 13$ TeV"

2021

Data from Fig 17b. The extracted quark-distribution from the unfolded charged-particle $R_g$ distribution for anti-kt R=0.8 jets with 600 < $p_T$ < 800 GeV, after the soft drop algorithm is applied for $\beta$ = 1, in data. All uncertainties described in the text are shown on the data. The distributions are normalized to the integrated cross section, $\sigma$.

13000.0substructureAstrophysics::High Energy Astrophysical PhenomenaP P --> JET JETHigh Energy Physics::ExperimentSoft dropRg
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"Table 122" of "A measurement of soft-drop jet observables in $pp$ collisions with the ATLAS detector at $\sqrt{s} = 13$ TeV"

2021

Data from Fig 17a. The extracted quark-distribution from the unfolded charged-particle $R_g$ distribution for anti-kt R=0.8 jets with 600 < $p_T$ < 800 GeV, after the soft drop algorithm is applied for $\beta$ = 0, in data. All uncertainties described in the text are shown on the data. The distributions are normalized to the integrated cross section, $\sigma$.

13000.0substructureAstrophysics::High Energy Astrophysical PhenomenaP P --> JET JETHigh Energy Physics::ExperimentSoft dropRg
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