Search results for "High Energy Physics::Phenomenology"

showing 10 items of 5791 documents

Search for resonances decaying into top-quark pairs using fully hadronic decays in pp collisions with ATLAS at root s=7 TeV

2013

A search for resonances produced in 7 TeV proton-proton collisions and decaying into top-quark pairs is described. In this Letter events where the top-quark decay produces two massive jets with large transverse momenta recorded with the ATLAS detector at the Large Hadron Collider are considered. Two techniques that rely on jet substructure are used to separate top-quark jets from those arising from light quarks and gluons. In addition, each massive jet is required to have evidence of an associated bottom-quark decay. The data are consistent with the Standard Model, and limits can be set on the production cross section times branching fraction of a Z' boson and a Kaluza-Klein gluon resonance…

Astrophysics::High Energy Astrophysical PhenomenaNuclear TheoryHigh Energy Physics::PhenomenologyFísicaHigh Energy Physics::ExperimentNuclear Experiment
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Production of J/psi and Y mesons in pp collisions at root s=8 TeV

2013

The production of J/psi and gamma mesons in pp collisions at root s = 8 TeV is studied with the LHCb detector. The J/psi and gamma mesons are reconstructed in the mu(+)mu(-) decay mode and the signal yields are determined with a fit to the mu(+)mu(-) invariant mass distributions. The analysis is performed in the rapidity range 2.0 < y < 4.5 and transverse momentum range 0 < PT < 14 (15) GeV/c of the J/psi (gamma) mesons. The J/psi and gamma production cross-sections and the fraction of J/psi mesons from b-hadron decays are measured as a function of the meson P-T and y.

Astrophysics::High Energy Astrophysical PhenomenaNuclear TheoryHigh Energy Physics::PhenomenologyHigh Energy Physics::ExperimentFísica nuclearNuclear ExperimentPartícules (Física nuclear)
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"Table 12" 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 reconstructed photons originating from the decay $a\rightarrow 2\gamma$ with $m_a$ = 2 GeV.

Astrophysics::High Energy Astrophysical PhenomenaPhysics::Space PhysicsHigh Energy Physics::PhenomenologySelection efficiencyHigh Energy Physics::Experiment$pp\rightarrow X \rightarrow aa \rightarrow 4\gamma$Nuclear Experiment13000Photon-jet
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"Table 9" 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 reconstructed photons originating from the decay $a\rightarrow 2\gamma$ with $m_a$ = 0.5 GeV.

Astrophysics::High Energy Astrophysical PhenomenaPhysics::Space PhysicsHigh Energy Physics::PhenomenologySelection efficiencyHigh Energy Physics::Experiment$pp\rightarrow X \rightarrow aa \rightarrow 4\gamma$Nuclear Experiment13000Photon-jet
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"Table 11" 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 reconstructed photons originating from the decay $a\rightarrow 2\gamma$ with $m_a$ = 1 GeV.

Astrophysics::High Energy Astrophysical PhenomenaPhysics::Space PhysicsHigh Energy Physics::PhenomenologySelection efficiencyHigh Energy Physics::Experiment$pp\rightarrow X \rightarrow aa \rightarrow 4\gamma$Nuclear Experiment13000Photon-jet
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"Table 10" 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 reconstructed photons originating from the decay $a\rightarrow 2\gamma$ with $m_a$ = 0.7 GeV.

Astrophysics::High Energy Astrophysical PhenomenaPhysics::Space PhysicsHigh Energy Physics::PhenomenologySelection efficiencyHigh Energy Physics::Experiment$pp\rightarrow X \rightarrow aa \rightarrow 4\gamma$Nuclear Experiment13000Photon-jet
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"Table 8" 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 reconstructed photons originating from the decay $a\rightarrow 2\gamma$ with $m_a$ = 0.1 GeV.

Astrophysics::High Energy Astrophysical PhenomenaPhysics::Space PhysicsHigh Energy Physics::PhenomenologySelection efficiencyHigh Energy Physics::Experiment$pp\rightarrow X \rightarrow aa \rightarrow 4\gamma$Nuclear Experiment13000Photon-jet
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"Table 14" 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 reconstructed photons originating from the decay $a\rightarrow 2\gamma$ with $m_a$ = 10 GeV.

Astrophysics::High Energy Astrophysical PhenomenaPhysics::Space PhysicsHigh Energy Physics::PhenomenologySelection efficiencyHigh Energy Physics::Experiment$pp\rightarrow X \rightarrow aa \rightarrow 4\gamma$Nuclear Experiment13000Photon-jet
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"Table 13" 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 reconstructed photons originating from the decay $a\rightarrow 2\gamma$ with $m_a$ = 5 GeV.

Astrophysics::High Energy Astrophysical PhenomenaPhysics::Space PhysicsHigh Energy Physics::PhenomenologySelection efficiencyHigh Energy Physics::Experiment$pp\rightarrow X \rightarrow aa \rightarrow 4\gamma$Nuclear Experiment13000Photon-jet
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Measurement of day and night neutrino energy spectra at SNO and constraints on neutrino mixing parameters

2002

The Sudbury Neutrino Observatory (SNO) has measured day and night solar neutrino energy spectra and rates. For charged current events, assuming an undistorted $^8$B spectrum, the night minus day rate is $14.0% \pm 6.3% ^{+1.5}_{-1.4}%$ of the average rate. If the total flux of active neutrinos is additionally constrained to have no asymmetry, the $\nu_e$ asymmetry is found to be $7.0% \pm 4.9% ^{+1.3}_{-1.2}%$. A global solar neutrino analysis in terms of matter-enhanced oscillations of two active flavors strongly favors the Large Mixing Angle (LMA) solution.

Astrophysics::High Energy Astrophysical PhenomenaSolar neutrinoFOS: Physical sciencesGeneral Physics and AstronomyFluxCosmic rayAstrophysics7. Clean energy01 natural sciencesHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)0103 physical sciencesNuclear astrophysicsNuclear Experiment (nucl-ex)010306 general physicsNeutrino oscillationNuclear ExperimentAstrophysics::Galaxy AstrophysicsCharged currentPhysicsSudbury Neutrino Observatory010308 nuclear & particles physicsAstrophysics (astro-ph)High Energy Physics::Phenomenology13. Climate actionHigh Energy Physics::ExperimentAstrophysics::Earth and Planetary AstrophysicsNeutrino
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