0000000001325712

AUTHOR

A. B. Balantekin

showing 7 related works from this author

Snowmass Neutrino Frontier: Neutrino Interaction Cross Sections (NF06) Topical Group Report

2022

A thorough understanding of neutrino cross sections in a wide range of energies is crucial for the successful execution of the entire neutrino physics program. In order to extract neutrino properties, long-baseline experiments need an accurate determination of neutrino cross sections within their detector(s). Since very few of the needed neutrino cross sections across the energy spectrum are directly measured, we emphasize the need for theoretical input and indirect measurements such as electron scattering, which would complement direct measurements. In this report we briefly summarize the current status of our knowledge of the neutrino cross sections and articulate needs of the experiments…

neutrino: detectorneutrino: energyDUNEelectron: scatteringneutrino: atmosphereneutrino: energy spectrumfar detectorneutrino: scatteringneutrino: supernovachannel cross section: energy dependenceneutrino: interactiondeep underground detectoractivity report
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Optimization of the JUNO liquid scintillator composition using a Daya Bay antineutrino detector

2021

To maximize the light yield of the liquid scintillator (LS) for the Jiangmen Underground Neutrino Observatory (JUNO), a 20 t LS sample was produced in a pilot plant at Daya Bay. The optical properties of the new LS in various compositions were studied by replacing the gadolinium-loaded LS in one antineutrino detector. The concentrations of the fluor, PPO, and the wavelength shifter, bis-MSB, were increased in 12 steps from 0.5 g/L and <0.01 mg/L to 4 g/L and 13 mg/L, respectively. The numbers of total detected photoelectrons suggest that, with the optically purified solvent, the bis-MSB concentration does not need to be more than 4 mg/L. To bridge the one order of magnitude in the detect…

organic compounds: admixtureNuclear and High Energy PhysicsPhysics - Instrumentation and DetectorsLiquid scintillatorscintillation counter: liquidAnalytical chemistryFOS: Physical sciencesmodel: opticalScintillatorWavelength shifterantineutrino: detector01 natural sciencesNOHigh Energy Physics - Experimentwavelength shifterHigh Energy Physics - Experiment (hep-ex)PE2_2Daya BayNeutrino0103 physical sciencesfluorine: admixture[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]ddc:530neutrino oscillation[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsInstrumentationJiangmen Underground Neutrino ObservatoryPhysicsJUNO010308 nuclear & particles physicsSettore FIS/01 - Fisica SperimentaleDetectorLight yield; Liquid scintillator; NeutrinoInstrumentation and Detectors (physics.ins-det)Yield (chemistry)Scintillation counterComposition (visual arts)photon: yieldNeutrinoLight yieldNuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
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Mott scattering as a probe of long range QCD effects

1994

We investigate the possibility of using the Mott scattering between identical nuclei to assess the existence of long range QCD effects, e.g., a color van der Waals interaction, as suggested recently. We show that the inclusion of atomic effects is very important and should be considered in order to extract limits on the strength of the color van der Waals force. We compare our calculations with the analysis of a recent heavy ion experiment.

PhysicsQuantum chromodynamicsElastic scatteringNuclear reactionNuclear and High Energy PhysicsCondensed matter physicsScatteringMott scatteringCharged particleColor modelsymbols.namesakesymbolsPhysics::Atomic PhysicsAtomic physicsvan der Waals forcePhysical Review C
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Spectroscopy of the neutron-deficient isobars 163 Re and 163 W using tagging techniques

2008

Bozok University;Erciyes University;et al.;Istanbul University;Nigde University;The Turkish Atomic Energy Authority (TAEK)

PhysicsNuclear Reactions 60 Ni+ 106 Cd at 270 MeV beam energy enriched targetsSpectrometerProtonYrastNuclear TheorySegmented Si and Ge detectorsNeutron spectroscopyNuclear physicsMeasured E ?IsobarNeutronGasfilled recoil separatorNuclear ExperimentGround stateRadioactive decay
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Decays of new nuclides and isomers beyond the proton drip line - The influence of neutron configurations

2008

Bozok University;Erciyes University;et al.;Istanbul University;Nigde University;The Turkish Atomic Energy Authority (TAEK)

PhysicsProtonGamma rayAlpha particleSegmented Si and Ge detectors. Measured E ? E proton E ? T 1/2Nuclear physicsNuclear Reactions 58 Ni+ 106 Cd at 290300310 MeV beam energyBeta particleNeutronEnriched targetsNuclideAlpha decayGas-filled recoil separatorAtomic physicsNuclear ExperimentGround state
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FRIB and the GW170817 Kilonova

2018

In July 2018 an FRIB Theory Alliance program was held on the implications of GW170817 and its associated kilonova for r-process nucleosynthesis. Topics of discussion included the astrophysical and nuclear physics uncertainties in the interpretation of the GW170817 kilonova, what we can learn about the astrophysical site or sites of the r process from this event, and the advances in nuclear experiment and theory most crucial to pursue in light of the new data. Here we compile a selection of scientific contributions to the workshop, broadly representative of progress in r-process studies since the GW170817 event.

High Energy Astrophysical Phenomena (astro-ph.HE)Nuclear Theory (nucl-th)Astrophysics - Solar and Stellar AstrophysicsNuclear TheoryFOS: Physical sciencesAstrophysics - High Energy Astrophysical PhenomenaSolar and Stellar Astrophysics (astro-ph.SR)
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FRIB and the GW170817 Kilonova

2018

In July 2018 an FRIB Theory Alliance program was held on the implications of GW170817 and its associated kilonova for r-process nucleosynthesis. Topics of discussion included the astrophysical and nuclear physics uncertainties in the interpretation of the GW170817 kilonova, what we can learn about the astrophysical site or sites of the r process from this event, and the advances in nuclear experiment and theory most crucial to pursue in light of the new data. Here we compile a selection of scientific contributions to the workshop, broadly representative of progress in r-process studies since the GW170817 event.

High Energy Astrophysical Phenomena (astro-ph.HE)Nuclear Theory (nucl-th)FOS: Physical sciencesSolar and Stellar Astrophysics (astro-ph.SR)
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