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000293562 0247_ $$2arXiv$$aarXiv:1512.03624
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000293562 0247_ $$2inspire$$ainspire:1409297
000293562 037__ $$aPUBDB-2016-00631
000293562 041__ $$aEnglish
000293562 0881_ $$aDESY-15-241; arXiv:1512.03624
000293562 088__ $$2DESY$$aDESY-15-241
000293562 088__ $$2arXiv$$aarXiv:1512.03624
000293562 1001_ $$0P:(DE-H253)PIP1002698$$aGeiser, Achim$$b0$$eCorresponding author$$udesy
000293562 1112_ $$aWorkshop on Future Physics with HERA Data for Current and Planned Experiments$$cHamburg$$d2014-11-11 - 2014-11-13$$wGermany
000293562 245__ $$aPossible future HERA analyses
000293562 260__ $$c2015
000293562 300__ $$a14
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000293562 520__ $$aA variety of possible future analyses of HERA data in the context of the HERA data preservation programme is collected, motivated, and commented. The focus is placed on possible future analyses of the existing $ep$ collider data and their physics scope. Comparisons to the original scope of the HERA programme are made, and cross references to topics also covered by other participants of the workshop are given. This includes topics on QCD, proton structure, diffraction, jets, hadronic final states, heavy flavours, electroweak physics, and the application of related theory and phenomenology topics like NNLO QCD calculations, low-x related models, nonperturbative QCD aspects, and electroweak radiative corrections. Synergies with other collider programmes are also addressed. In summary, the range of physics topics which can still be uniquely covered using the existing data is very broad and of considerable physics interest, often matching the interest of results from colliders currently in operation. Due to well-established data and MC sets, calibrations, and analysis procedures the manpower and expertise needed for a particular analysis is often very much smaller than that needed for an ongoing experiment. Since centrally funded manpower to carry out such analyses is not available any longer, this contribution not only targets experienced self-funded experimentalists, but also theorists and master-level students who might wish to carry out such an analysis.
000293562 536__ $$0G:(DE-HGF)POF3-611$$a611 - Fundamental Particles and Forces (POF3-611)$$cPOF3-611$$fPOF III$$x0
000293562 588__ $$aDataset connected to INSPIRE
000293562 650_7 $$2INSPIRE$$apositron p: interaction
000293562 650_7 $$2INSPIRE$$aelectron p: interaction
000293562 650_7 $$2INSPIRE$$aquantum chromodynamics: nonperturbative
000293562 650_7 $$2INSPIRE$$aelectroweak interaction: radiative correction
000293562 650_7 $$2INSPIRE$$afinal state: hadronic
000293562 650_7 $$2INSPIRE$$aDESY HERA Stor
000293562 650_7 $$2INSPIRE$$adata preservation
000293562 650_7 $$2INSPIRE$$aheavy quark
000293562 650_7 $$2INSPIRE$$acalibration
000293562 650_7 $$2INSPIRE$$adiffraction
000293562 650_7 $$2INSPIRE$$astructure
000293562 650_7 $$2INSPIRE$$asmall-x
000293562 650_7 $$2INSPIRE$$aexperimental results
000293562 693__ $$0EXP:(DE-588)4276505-5$$1EXP:(DE-588)4159571-3$$5EXP:(DE-588)4276505-5$$aHERA$$eHERA: ZEUS$$x0
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