Search results for "High Energy Physics"

showing 10 items of 17560 documents

"16-Anti3He" of "Multiplicity dependence of light (anti-)nuclei production in p-Pb collisions at $\sqrt{s_{\rm{NN}}}$ = 5.02 TeV"

2019

Transverse momentum distribution of $^{3}\overline{\mathrm{He}}$ for all non single diffractive (NSD) p-Pb collisions.

$1/N_{\mathrm{ev}}\mathrm{d}^{2}N/(\mathrm{d}y\mathrm{d}p_{T})$High Energy Physics::PhenomenologyNuclear Experiment
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"Table 5" of "The ALICE Transition Radiation Detector: construction, operation, and performance"

2017

Most probable charge deposit signal normalised to that of minimum ionising particles as a function of $\beta\gamma$ for cosmic-ray muons (dE/dx + TR). Statistical uncertainties as vertical error bars. Uncertainties in momentum and thus $\beta \gamma$ determination are drawn as horizontal error bars.

$Q_{\rm MPV}/Q_{\rm MPV}^{\rm mip}$Astrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::Experiment
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"Table 4" of "The ALICE Transition Radiation Detector: construction, operation, and performance"

2017

Most probable charge deposit signal normalised to that of minimum ionising particles as a function of $\beta\gamma$ for cosmic-ray muons (dE/dx). Statistical uncertainties as vertical error bars. Uncertainties in momentum and thus $\beta \gamma$ determination are drawn as horizontal error bars.

$Q_{\rm MPV}/Q_{\rm MPV}^{\rm mip}$Astrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::Experiment
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"Table 4" of "Multiplicities of charged pions and unidentified charged hadrons from deep-inelastic scattering of muons off an isoscalar target"

2017

Multiplicities of unidentified negatively charged hadrons from semi-inclusive deep-inelastic scattering of muons off an isoscalar target, $M^{h^{-}}$, in bins of $x$, $y$, and $z$. Also given are the diffractive vector meson correction to the hadron count, $DVM^{h^{-}}$, and DIS count, $DVM^{DIS}$, as well as the radiative correction factors to the hadron count, $\eta^{h^{-}}$, and DIS count, $\eta^{DIS}$. The correction factors were applied to the raw multiplicity to arrive at the final multiplicity given in the table, $M^{h^{-}}$, as follows: $M^{h^{-}}$ = $M_{raw}^{h^{-}}$ * $\frac{\eta^{h^{-}}} {\eta^{DIS}}$ * $\frac{ DVM^{h^{-}} } {DVM^{DIS} }$.

$\mu^{+}$ d --> $\mu'^{+}$ $h^{-}$ XHigh Energy Physics::ExperimentNuclear ExperimentMULT
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"Table 2" of "Multiplicities of charged pions and unidentified charged hadrons from deep-inelastic scattering of muons off an isoscalar target"

2017

Multiplicities of negatively charged pions from semi-inclusive deep-inelastic scattering of muons off an isoscalar target, $M^{\pi^{-}}$, in bins of $x$, $y$, and $z$. Also given are the diffractive vector meson correction to the pion count, $DVM^{\pi^{-}}$, and DIS count, $DVM^{DIS}$, as well as the radiative correction factors to the pion count, $\eta^{\pi^{-}}$, and DIS count, $\eta^{DIS}$. The correction factors were applied to the raw multiplicity to arrive at the final multiplicity given in the table, $M^{\pi^{-}}$, as follows: $M^{\pi^{-}}$ = $M_{raw}^{\pi^{-}}$ * $\frac{\eta^{\pi^{-}}} {\eta^{DIS}}$ * $\frac{ DVM^{\pi^{-}} } {DVM^{DIS} }$.

$\mu^{+}$ d --> $\mu^{+}$ $\pi^{-}$ XNuclear TheoryHigh Energy Physics::ExperimentNuclear ExperimentMULT
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"Table 2" of "Multiplicities of charged kaons from deep-inelastic muon scattering off an isoscalar target"

2017

Multiplicities of negatively charged kaons from semi-inclusive deep-inelastic scattering of muons off an isoscalar target, $M^{K^{-}}$, in bins of $x$, $y$, and $z$. Also given are the diffractive vector meson correction to the kaon count, $DVM^{K^{-}}$, and DIS count, $DVM^{DIS}$, as well as the radiative correction factors to the kaon count, $\eta^{K^{-}}$, and DIS count, $\eta^{DIS}$. The correction factors were applied to the raw multiplicity to arrive at the final multiplicity given in the table, $M^{K^{-}}$, as follows: $M^{K^{-}}$ = $M_{raw}^{K^{-}}$ * $\frac{\eta^{K^{-}}} {\eta^{DIS}}$ * $\frac{ DVM^{K^{-}} } {DVM^{DIS} }$.

$\mu^{+}$d-->\mu^{+}$K^{-}$XNuclear TheoryHigh Energy Physics::ExperimentNuclear ExperimentMULT
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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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