Search results for "Astrophysics::High Energy Astrophysical Phenomena"

showing 10 items of 4757 documents

"Table 18" 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 $a\rightarrow 3\pi^0\rightarrow 6\gamma$ with $m_a$ = 2 GeV.

$pp\rightarrow X \rightarrow aa \rightarrow 6\pi^0$Astrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::PhenomenologySelection efficiencyHigh Energy Physics::Experiment13000Photon-jet
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"Table 17" 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 $a\rightarrow 3\pi^0\rightarrow 6\gamma$ with $m_a$ = 1 GeV.

$pp\rightarrow X \rightarrow aa \rightarrow 6\pi^0$Astrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::PhenomenologySelection efficiencyHigh Energy Physics::Experiment13000Photon-jet
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"Table 16" 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 $a\rightarrow 3\pi^0\rightarrow 6\gamma$ with $m_a$ = 0.7 GeV.

$pp\rightarrow X \rightarrow aa \rightarrow 6\pi^0$Astrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::PhenomenologySelection efficiencyHigh Energy Physics::Experiment13000Photon-jet
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"Table 15" 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 $a\rightarrow 3\pi^0\rightarrow 6\gamma$ with $m_a$ = 0.5 GeV.

$pp\rightarrow X \rightarrow aa \rightarrow 6\pi^0$Astrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::PhenomenologySelection efficiencyHigh Energy Physics::Experiment13000Photon-jet
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"Table 20" 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 $a\rightarrow 3\pi^0\rightarrow 6\gamma$ with $m_a$ = 10 GeV.

$pp\rightarrow X \rightarrow aa \rightarrow 6\pi^0$Astrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::PhenomenologySelection efficiencyHigh Energy Physics::Experiment13000Photon-jet
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"Table 19" 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 $a\rightarrow 3\pi^0\rightarrow 6\gamma$ with $m_a$ = 5 GeV.

$pp\rightarrow X \rightarrow aa \rightarrow 6\pi^0$Astrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::PhenomenologySelection efficiencyHigh Energy Physics::Experiment13000Photon-jet
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Formation of dislocations and hardening of LiF under high-dose irradiation with 5–21 MeV 12C ions

2017

R. Zabels, I. Manika, J. Maniks, and R.Grants acknowledge the national project IMIS2, and A. Dauletbekova, M. Baizhumanov, and M. Zdorovets the Ministry of Education and Science of the Republic of Kazakhstan for the financial support.

010302 applied physicsEnergy lossMaterials sciencePhysics::Instrumentation and DetectorsAtomic force microscopyAstrophysics::High Energy Astrophysical PhenomenaPhysics::Medical Physicsmacromolecular substances02 engineering and technologyGeneral ChemistryNanoindentation021001 nanoscience & nanotechnology01 natural sciencesMolecular physicsIsotropic etchingElastic collisionIonPhysics::Plasma Physics0103 physical sciences:NATURAL SCIENCES:Physics [Research Subject Categories]Hardening (metallurgy)General Materials ScienceIrradiationAtomic physics0210 nano-technologyApplied Physics A
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Low-temperature luminescence of ScF3 single crystals under excitation by VUV synchrotron radiation

2020

The work was supported by the Latvian Science Council grant LZP-2018/2-0358. The research leading to this result has also been supported by the project CALIPSO plus under the Grant Agreement 730872 from the EU Framework Programme for Research and Innovation HORIZON 2020. The author is grateful to K. Chernenko (MAX IV Laboratory, Lund University) for his assistance during beamtime experiments and to A. I. Popov for the fruitful discussions. V.P. also acknowledges Valsts pētījumu programma “Augstas enerģijas fizika un paātrinātāju tehnoloģijas” (Projekta Nr. VPP-IZM-CERN-2020/1-0002). REFERENCES

010302 applied physicsMaterials sciencePhotoluminescencePhysics and Astronomy (miscellaneous)synchrotron radiationAstrophysics::High Energy Astrophysical PhenomenaExcitonGeneral Physics and AstronomySynchrotron radiationUndulator7. Clean energy01 natural sciencesSynchrotronlaw.inventionlawAbsorption band0103 physical sciences:NATURAL SCIENCES:Physics [Research Subject Categories]VUV luminescence spectroscopyAtomic physics010306 general physicsLuminescenceExcitationScF3
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Low-temperature luminescence of catangasite single crystals under excitation by vacuum ultraviolet synchrotron radiation

2020

The luminescent properties of Ca3TaGa3Si2O14 (CTGS, catangasite) single crystals have been studied by means of the vacuum ultraviolet excitation spectroscopy utilizing synchrotron radiation from 1.5 GeV storage ring of MAX IV synchrotron facility. Two emission bands at 320 nm (3.87 eV) and 445 nm (2.78 eV) have been detected. Examining excitation spectra in vacuum ultraviolet spectral range, the 320 nm emission band was explained as the emission band of self-trapped exciton in CTGS single crystal. Its atomic structure is discussed. It is also proposed that the 445 nm (2.78 eV) emission in the CTGS is due to the F centers, which have shown a well-resolved excitation (absorption) band at 5.1 …

010302 applied physicsMaterials sciencePhysics and Astronomy (miscellaneous)Astrophysics::High Energy Astrophysical PhenomenaExcitonGeneral Physics and AstronomySynchrotron radiation01 natural sciencesSynchrotronlaw.inventionlaw0103 physical sciencesAtomic physics010306 general physicsAbsorption (electromagnetic radiation)LuminescenceSingle crystalStorage ringExcitation
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Photoelectron Emission from Metal Surfaces Induced by Radiation Emitted by a 14 GHz Electron Cyclotron Resonance Ion Source

2015

Photoelectron emission measurements have been performed using a room-temperature 14 GHz ECR ion source. It is shown that the photoelectron emission from Al, Cu, and stainless steel (SAE 304) surfaces, which are common plasma chamber materials, is predominantly caused by radiation emitted from plasma with energies between 8 eV and 1 keV. Characteristic X-ray emission and bremsstrahlung from plasma have a negligible contribution to the photoelectron emission. It is estimated from the measured data that the maximum conceivable photoelectron flux from plasma chamber walls is on the order of 10% of the estimated total electron losses from the plasma. peerReviewed

010302 applied physicsMaterials scienceta114Physics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaCyclotron resonanceBremsstrahlungFOS: Physical sciencesPlasmaElectronphotoelectron emissionRadiation01 natural sciences7. Clean energyElectron cyclotron resonanceIon sourcePhysics - Plasma Physics010305 fluids & plasmasPlasma Physics (physics.plasm-ph)Physics::Plasma Physics0103 physical scienceselectron cyclotron resonance ion sourcesPlasma diagnosticsAtomic physicsInstrumentation
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