Search results for "scattering"

showing 10 items of 8332 documents

"Table 13" of "A glimpse of gluons through deeply virtual compton scattering on the proton"

2017

Beam helicity independent cross sections. The first systematic uncertainty is the combined correlated systematic uncertainty, the second is the point-to-point systematic uncertainty to add quadratically to the statistical uncertainty.

D4SIG/DQ**2/DX/DT/DPHIDeeply Virtual Compton ScatteringE- P --> E- GAMMA PBeam helicity independent cross sectionExclusive
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"Table 27" of "A glimpse of gluons through deeply virtual compton scattering on the proton"

2017

Beam helicity independent cross sections. The first systematic uncertainty is the combined correlated systematic uncertainty, the second is the point-to-point systematic uncertainty to add quadratically to the statistical uncertainty.

D4SIG/DQ**2/DX/DT/DPHIDeeply Virtual Compton ScatteringE- P --> E- GAMMA PBeam helicity independent cross sectionExclusive
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"Table 38" of "A glimpse of gluons through deeply virtual compton scattering on the proton"

2017

Beam helicity independent cross sections. The first systematic uncertainty is the combined correlated systematic uncertainty, the second is the point-to-point systematic uncertainty to add quadratically to the statistical uncertainty.

D4SIG/DQ**2/DX/DT/DPHIDeeply Virtual Compton ScatteringE- P --> E- GAMMA PBeam helicity independent cross sectionExclusive
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"Table 35" of "A glimpse of gluons through deeply virtual compton scattering on the proton"

2017

Beam helicity independent cross sections. The first systematic uncertainty is the combined correlated systematic uncertainty, the second is the point-to-point systematic uncertainty to add quadratically to the statistical uncertainty.

D4SIG/DQ**2/DX/DT/DPHIDeeply Virtual Compton ScatteringE- P --> E- GAMMA PBeam helicity independent cross sectionExclusive
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"Table 15" of "A glimpse of gluons through deeply virtual compton scattering on the proton"

2017

Beam helicity independent cross sections. The first systematic uncertainty is the combined correlated systematic uncertainty, the second is the point-to-point systematic uncertainty to add quadratically to the statistical uncertainty.

D4SIG/DQ**2/DX/DT/DPHIDeeply Virtual Compton ScatteringE- P --> E- GAMMA PBeam helicity independent cross sectionExclusive
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"Table 19" of "A glimpse of gluons through deeply virtual compton scattering on the proton"

2017

Beam helicity independent cross sections. The first systematic uncertainty is the combined correlated systematic uncertainty, the second is the point-to-point systematic uncertainty to add quadratically to the statistical uncertainty.

D4SIG/DQ**2/DX/DT/DPHIDeeply Virtual Compton ScatteringE- P --> E- GAMMA PBeam helicity independent cross sectionExclusive
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"Table 3" of "A glimpse of gluons through deeply virtual compton scattering on the proton"

2017

Beam helicity independent cross sections. The first systematic uncertainty is the combined correlated systematic uncertainty, the second is the point-to-point systematic uncertainty to add quadratically to the statistical uncertainty.

D4SIG/DQ**2/DX/DT/DPHIDeeply Virtual Compton ScatteringE- P --> E- GAMMA PBeam helicity independent cross sectionExclusive
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"Table 7" of "A glimpse of gluons through deeply virtual compton scattering on the proton"

2017

Beam helicity independent cross sections. The first systematic uncertainty is the combined correlated systematic uncertainty, the second is the point-to-point systematic uncertainty to add quadratically to the statistical uncertainty.

D4SIG/DQ**2/DX/DT/DPHIDeeply Virtual Compton ScatteringE- P --> E- GAMMA PBeam helicity independent cross sectionExclusive
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"Table 47" of "Energy dependence of event shapes and of alpha(s) at LEP-2."

1999

Measured value of the logarithmic energy slope of the inverse coupling constant.

DALPHAS/DLOGEE+ E- --> HADRONSE+ E- --> JETSE+ E- ScatteringExclusive91.2Astrophysics::Cosmology and Extragalactic AstrophysicsJet Production
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Electron-interacting dark matter: Implications from DAMA/LIBRA-phase2 and prospects for liquid xenon detectors and NaI detectors

2019

We investigate the possibility for the direct detection of low-mass (GeV scale) weakly interacting massive particles (WIMP) dark matter in scintillation experiments. Such WIMPs are typically too light to leave appreciable nuclear recoils but may be detected via their scattering off atomic electrons. In particular, the DAMA Collaboration [R. Bernabei et al., Nucl. Phys. At. Energy 19, 307 (2018)] has recently presented strong evidence of an annual modulation in the scintillation rate observed at energies as low as 1 keV. Despite a strong enhancement in the calculated event rate at low energies, we find that an interpretation in terms of electron-interacting WIMPs cannot be consistent with ex…

DAMA/LIBRACosmology and Nongalactic Astrophysics (astro-ph.CO)detector: performancePhysics::Instrumentation and DetectorsDark matterFOS: Physical scienceschemistry.chemical_elementElectron01 natural sciencesWIMP: dark matterNuclear physicsHigh Energy Physics - Phenomenology (hep-ph)XenonWIMP0103 physical sciences010306 general physicsenhancementscintillation counterenergy: lowPhysicsScintillationxenon: liquid010308 nuclear & particles physicsatom: wave functionDAMAmodulationHigh Energy Physics - Phenomenologychemistryelectron: scatteringWeakly interacting massive particles[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]direct detection[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Event (particle physics)Astrophysics and astroparticle physicsAstrophysics - Cosmology and Nongalactic AstrophysicsPhysical Review
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