Search results for "GH"

showing 10 items of 37181 documents

"Figure 9" of "Cold-nuclear-matter effcts on heavy-quark production in d+Au collisions at sqrt(s_NN)=200 GeV"

2023

Heavy flavor electron $R_{dA}$ 20-40% $d$+Au collisions. The nuclear modification factor, $R_{dA}$, for electrons from open heavy flavor decays, for the (a) most central and (b) most peripheral centrality bins.

$d$ + Au$\implies$ CHARGED Xheavy flavor electronlight flavor mesonsmass-dependent Cronin enhancementRelativistic Heavy Ion Collider$p + p$ $\implies$ CHARGED Xheavy $D$ meson familyheavy flavor mesons200.0ppg131
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"Figure 7" of "Cold-nuclear-matter effcts on heavy-quark production in d+Au collisions at sqrt(s_NN)=200 GeV"

2023

Heavy flavor electron $R_{dA}$ 0-100% d+Au collisions. The nuclear modification factors $R_{dA}$ and $R_{AA}$ for minimum bias $d$+Au and Au+Au collisions, for the $\pi^{0}$ and $e^{\pm}_{HF}$. The two boxes on the right side of the plot represent the global uncertainties in the $d$+Au (left) and Au+Au (right) values of $N_{coll}$ . An additional common global scaling uncertainty of 9.7% on $R_{dA}$ and $R_{AA}$ from the $p+p$ reference data is omitted for clarity.

$d$ + Au$\implies$ CHARGED Xheavy flavor electronlight flavor mesonsmass-dependent Cronin enhancementRelativistic Heavy Ion Collider$p + p$ $\implies$ CHARGED Xheavy $D$ meson familyheavy flavor mesons200.0ppg131
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"Figures 3-6" of "Cold-nuclear-matter effcts on heavy-quark production in d+Au collisions at sqrt(s_NN)=200 GeV"

2023

Heavy flavor electron yield, $d$+Au $\implies$ CHARGED X. Electrons from heavy flavor decays, separated by centrality. The lines represent a fit to the previous $p+p$ result [23], scaled by $N_{coll}$. The inset shows the ratio of photonic background electrons determined by the converter and cocktail methods for Minimum Bias $d$+Au collisions, with error bars (boxes) that represent the statistical uncertainty on the converter data (systematic uncertainty on the photonic-electron cocktail).

$d$ + Au$\implies$ CHARGED Xheavy flavor electronlight flavor mesonsmass-dependent Cronin enhancementRelativistic Heavy Ion Collider$p + p$ $\implies$ CHARGED Xheavy $D$ meson familyheavy flavor mesons200.0ppg131
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"Figure 10" of "Cold-nuclear-matter effcts on heavy-quark production in d+Au collisions at sqrt(s_NN)=200 GeV"

2023

Heavy flavor electron $R_{dA}$ 40-60% $d$+Au collisions. The nuclear modification factor, $R_{dA}$, for electrons from open heavy flavor decays, for the (a) most central and (b) most peripheral centrality bins.

$d$ + Au$\implies$ CHARGED Xheavy flavor electronlight flavor mesonsmass-dependent Cronin enhancementRelativistic Heavy Ion Collider$p + p$ $\implies$ CHARGED Xheavy $D$ meson familyheavy flavor mesons200.0ppg131
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"Figures 1-2" of "Cold-nuclear-matter effcts on heavy-quark production in d+Au collisions at sqrt(s_NN)=200 GeV"

2023

Heavy flavor electron yield, Run-8 $p$ + $p$, $d$+Au collisions. Electrons from heavy flavor decays, separated by centrality. The lines represent a fit to the previous $p+p$ result [23], scaled by $N_{coll}$. The inset shows the ratio of photonic background electrons determined by the converter and cocktail methods for Minimum Bias $d$+Au collisions, with error bars (boxes) that represent the statistical uncertainty on the converter data (systematic uncertainty on the photonic-electron cocktail).

$d$ + Au$\implies$ CHARGED Xheavy flavor electronlight flavor mesonsmass-dependent Cronin enhancementRelativistic Heavy Ion Collider$p + p$ $\implies$ CHARGED Xheavy $D$ meson familyheavy flavor mesons200.0ppg131
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"Table 35" of "Search for pairs of highly collimated photon-jets in $pp$ collisions at $\sqrt{s}$ = 13 TeV with the ATLAS detector"

2018

Fraction of photons with a value of shower shape variable $\Delta E$ lower than the threshold, for photons originating from the BSM process $X\rightarrow\gamma\gamma$, where the $X$ particle is a high-mass narrow-width scalar particle originating from the gluon--gluon fusion process.

$pp\rightarrow X \rightarrow \gamma\gamma$Astrophysics::High Energy Astrophysical PhenomenaCategory fractionHigh Energy Physics::PhenomenologyHigh Energy Physics::Experiment13000Photon-jet
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"Table 34" of "Search for pairs of highly collimated photon-jets in $pp$ collisions at $\sqrt{s}$ = 13 TeV with the ATLAS detector"

2018

Selection efficiency for photons originating from the BSM process $X\rightarrow\gamma\gamma$, where the $X$ particle is a high-mass narrow-width scalar particle originating from the gluon--gluon fusion process.

$pp\rightarrow X \rightarrow \gamma\gamma$High Energy Physics::LatticeHigh Energy Physics::PhenomenologySelection efficiency13000Photon-jet
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"Table 28" of "Search for pairs of highly collimated photon-jets in $pp$ collisions at $\sqrt{s}$ = 13 TeV with the ATLAS detector"

2018

Fraction of reconstructed photons with a value of shower shape variable $\Delta E$ lower than the threshold, for reconstructed photons originating from the decay $a\rightarrow 3\pi^0\rightarrow 6\gamma$ with $m_a$ = 0.5 GeV.

$pp\rightarrow X \rightarrow aa \rightarrow 6\pi^0$Astrophysics::High Energy Astrophysical PhenomenaCategory fractionHigh Energy Physics::PhenomenologyHigh Energy Physics::Experiment13000Photon-jet
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"Table 32" of "Search for pairs of highly collimated photon-jets in $pp$ collisions at $\sqrt{s}$ = 13 TeV with the ATLAS detector"

2018

Fraction of reconstructed photons with a value of shower shape variable $\Delta E$ lower than the threshold, for reconstructed photons originating from the decay $a\rightarrow 3\pi^0\rightarrow 6\gamma$ with $m_a$ = 5 GeV.

$pp\rightarrow X \rightarrow aa \rightarrow 6\pi^0$Astrophysics::High Energy Astrophysical PhenomenaCategory fractionHigh Energy Physics::PhenomenologyHigh Energy Physics::Experiment13000Photon-jet
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"Table 33" of "Search for pairs of highly collimated photon-jets in $pp$ collisions at $\sqrt{s}$ = 13 TeV with the ATLAS detector"

2018

Fraction of reconstructed photons with a value of shower shape variable $\Delta E$ lower than the threshold, for reconstructed photons originating from the decay $a\rightarrow 3\pi^0\rightarrow 6\gamma$ with $m_a$ = 10 GeV.

$pp\rightarrow X \rightarrow aa \rightarrow 6\pi^0$Astrophysics::High Energy Astrophysical PhenomenaCategory fractionHigh Energy Physics::PhenomenologyHigh Energy Physics::Experiment13000Photon-jet
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