Search results for "Proton"

showing 10 items of 5886 documents

α decay of the πh11/2 isomer in Ir164

2014

The α -decay branch of the πh 11 / 2 isomer in 164 Ir has been identified using the GREAT spectrometer. The 164 Ir nuclei were produced using the 92 Mo( 78 Kr ,p 5 n ) 164 Ir reaction and separated in flight using the recoil ion transport unit (RITU) gas-filled separator. The measured α -decay energy of 6880 ± 10 keV allowed the excitation of the πh 11 / 2 state in 160 Re to be deduced as 166 ± 14 keV. The half-life of 164 Ir was measured with improved precision to be 70 ± 10 μ sandan α -decay branching ratio of 4 ± 2% was determined. Improved half-life and branching ratio measurements were also obtained for 165 Ir, but no evidence was found for the ground-state decays of either 164 Ir or 1…

neutron-deficent isotopesenergianuclear-structuremodeltotal data readout. proton drip-lineemissionrituosmiumvolframi
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Acidity and basicity of primaryN-phenylnitramines: catalytic effect of protons on the nitramine rearrangement

2002

Para-substituted N-phenylnitramines were prepared either by oxidation of diazonium salts or by nitration under alkaline or acidic conditions. Isotopic [15N-NO2] labelling indicated that the bands characteristic of the N-nitro group appear in the 1318–1323 and 1585–1607 cm−1 regions. In the nitrogen NMR spectra, the nitramino group gives two resonances at −193 ± 3 (NH) and −32 ± 3 ppm (NO2). The chemical shifts in proton and carbon NMR spectra are predictable, based on increments and the additivity rule. The spectral data indicate the lack of conjugation between the nitramino group and another substituent bound to the ring. It seems to contradict the well-known fact that substituents strongl…

nitraminesReaction mechanismChemical shiftrearrangementOrganic ChemistryInorganic chemistrySubstituentProtonationNuclear magnetic resonance spectroscopyCarbon-13 NMRMedicinal chemistryNMR spectra databasechemistry.chemical_compoundNMR spectroscopychemistryNitrationamphiprotic compoundsreaction mechanismPhysical and Theoretical ChemistryJournal of Physical Organic Chemistry
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Inference of proto-neutron star properties from gravitational-wave data in core-collapse supernovae

2021

The eventual detection of gravitational waves from core-collapse supernovae (CCSN) will help improve our current understanding of the explosion mechanism of massive stars. The stochastic nature of the late post-bounce gravitational wave signal due to the non-linear dynamics of the matter involved and the large number of degrees of freedom of the phenomenon make the source parameter inference problem very challenging. In this paper we take a step towards that goal and present a parameter estimation approach which is based on the gravitational waves associated with oscillations of proto-neutron stars (PNS). Numerical simulations of CCSN have shown that buoyancy-driven g-modes are responsible …

noiseGravitational-wave observatorygravitational radiation: stochasticAstrophysics::High Energy Astrophysical Phenomenaprotoneutron starDegrees of freedom (physics and chemistry)FOS: Physical sciencesAstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciences7. Clean energyGeneral Relativity and Quantum CosmologyEinstein Telescopeeffect: nonlinearsupernova0103 physical sciences[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]LIGOnumerical calculations010306 general physicsInstrumentation and Methods for Astrophysics (astro-ph.IM)equation of statePhysicsSolar massmass: solarEinstein Telescope010308 nuclear & particles physicsGravitational wavegravitational radiationoscillationgravitational radiation detectorLIGOgravitation: collapsedetector: sensitivitystar: massiveSupernovaStarswave: modelVIRGO13. Climate actiongravitational radiation: emission[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]galaxyAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics and astroparticle physics
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Direct Visualization of Molecule Deprotonation on an Insulating Surface

2012

Elucidating molecular-scale details of basic reaction steps on surfaces is decisive for a fundamental understanding of molecular reactivity within many fields, including catalysis and on-surface synthesis. Here, the deprotonation of 2,5-dihydroxybenzoic acid (DHBA) deposited onto calcite (101;4) held at room temperature is followed in situ by noncontact atomic force microscopy. After deposition, the molecules form two coexisting phases, a transient striped phase and a stable dense phase. A detailed analysis of high-resolution noncontact atomic force microscopy images indicates the transient striped phase being a bulk-like phase, which requires hydrogen bonds between the carboxylic acid moie…

noncontact atomic force microscopyCarboxylic acidCatecholsGeneral Physics and AstronomyMicroscopy Atomic ForceKelvin probe force microscopy530Calcium Carbonatechemistry.chemical_compoundDeprotonationPhase (matter)Materials TestingHydroxybenzoatesMoleculeGeneral Materials ScienceReactivity (chemistry)CarboxylateParticle Sizechemistry.chemical_classificationKelvin probe force microscopeHydrogen bondinsulating surfaceGeneral EngineeringElectric ConductivityMolecular ImagingNanostructuresCrystallographychemistrydeprotonationProtons
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The beta-delayed proton and gamma decay of 27P for nuclear astrophysics

2013

The creation site of 26Al is still under debate. It is thought to be produced in hydrogen burning and in explosive helium burning in novae and supernovae, and possibly also in the H-burning in outer shells of red giant stars. Also, the reactions for its creation or destruction are not completely known. When 26Al is created in novae, the reaction chain is: 24Mg(p, γ) 25Al(β +ν) 25Mg(p, γ) 26Al, but this chain can be by-passed by another chain, 25Al(p, γ) 26Si(p, γ) 27P and it can also be destroyed directly. The reaction 26mAl(p, γ) 27Si∗ is another avenue to bypass the production of 26Al and it is dominated by resonant capture. We find and study these resonances by an indirect method, throug…

nuclear astro-physicsindirect methodsdaughter nucleusproduction ofresonant capturehelium-burningreaction chainslow-energy protons
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Proton Exchange Membrane Fuel Cells (PEMFCs): Advances and Challenges

2021

The study of the electrochemical catalyst conversion of renewable electricity and carbon oxides into chemical fuels attracts a great deal of attention by different researchers. The main role of this process is in mitigating the worldwide energy crisis through a closed technological carbon cycle, where chemical fuels, such as hydrogen, are stored and reconverted to electricity via electrochemical reaction processes in fuel cells. The scientific community focuses its efforts on the development of high-performance polymeric membranes together with nanomaterials with high catalytic activity and stability in order to reduce the platinum group metal applied as a cathode to build stacks of proton …

organic polymersMaterials sciencePolymers and PlasticsHydrogenMembrane electrode assemblymembrane–electrode assemblyNanoparticleProton exchange membrane fuel cellchemistry.chemical_elementOrganic chemistryNanotechnologyGeneral ChemistryReviewElectrochemistryNanomaterialsCatalysisElectroquímicafuel cellMembraneQD241-441chemistryproton conductivityMaterialsproton exchange membranePolymers
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"Table 1" of "Jet-like correlations with neutral pion triggers in pp and central Pb-Pb collisions at 2.76 TeV"

2016

Charged-particle associated yields relative to $\pi^{0}$ trigger particles versus $\Delta\varphi$ in pp collisions at $\sqrt{s_{NN}}$=2.76 TeV. The $\pi^{0}$ trigger momentum range is $8< p_{T}^{trig} < 16~GeV/c$, and associated charged particle ranges are $0.5 < p_{T}^{assoc} < 1$, $1 < p_{T}^{assoc} < 2$, $2 < p_{T}^{assoc} < 4$ and $4 < p_{T}^{assoc} < 6~GeV/c$.

p p --> CHARGED XInclusiveProton-Proton Scattering2760.0
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"Table 2" of "Search for Higgs boson decays into a $Z$ boson and a light hadronically decaying resonance using 13 TeV $pp$ collision data from the AT…

2020

Efficiencies of the MLP selection, complete selection and total expected signal yields for each signal sample, assuming B$(H\to Z(Q/a))=100\%$ and $\sigma(pp\to H) = \sigma_\text{SM}(pp\to H)$. Pythia 8 branching fractions of $a$ are assumed using a $\tan\beta$ value of 1. The MLP efficiencies, total efficiencies, and expected yields are determined using MC samples, with uncertainties due to MC sample statistics, except for the expected background yield. The expected background yield and its uncertainty is calculated as described in the main text of the paper.

p p ---> t tbarYields13000.0p p ---> Z Zp p ---> H ---> Z JpsiHiggs bosonp p ---> H ---> Z etac2HDM(+S)p p ---> H ---> Z aATLASp p ---> Z jetEfficienciesProton-Proton ScatteringLHCp p ---> W Z
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"Table 1" of "Search for Higgs boson decays into a $Z$ boson and a light hadronically decaying resonance using 13 TeV $pp$ collision data from the AT…

2020

Observed number of data events and expected number of background events in the signal region.

p p ---> t tbarp p ---> e e jet13000.0p p ---> Z ZProton-Proton ScatteringHiggs bosonEvents2HDM(+S)p p ---> mu mu jetLHCATLASp p ---> W Zp p ---> Z jet
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The PANDA Endcap Disc DIRC

2018

Journal of Instrumentation 13(02), C02002 - C02002 (2018). doi:10.1088/1748-0221/13/02/C02002

particle identification [K]Physics::Instrumentation and Detectors61001 natural sciencesDIRCK: particle identificationOpticsPionDetection of internally reflected Cherenkov light0103 physical sciencesparticle identification [pi]ddc:610010306 general physicsNuclear ExperimentInstrumentationMathematical PhysicsCherenkov radiationPhysicsCherenkov counter: designRange (particle radiation)010308 nuclear & particles physicsbusiness.industryPANDADetectorSolid angleDESYLight guideTest beamdesign [Cherenkov counter]Radiator (engine cooling)Facility for Antiproton and Ion ResearchHigh Energy Physics::ExperimentPhotonicsbusinesspi: particle identificationperformance
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