Search results for "Matter"

showing 10 items of 16762 documents

Crystal structure of bis-(allyl-ammonium) oxalate.

2014

The title salt, 2C3H8N+·C2O42−, crystallized with six independent allylammonium cations and three independent oxalate dianions in the asymmetric unit. One of the oxalate dianions is nearly planar [dihedral angle between CO2planes = 1.91 (19)°], while the other two are twisted with angles of 11.3 (3) and 26.09 (13)°. One cation has a synperiplanar (cis) conformation with an N—C—C—C torsion angle of 0.9 (3)°, whereas the five remaining cations are characterized bygauchearrangements, with the N—C—C—C torsion angles ranging from 115.9 (12) to 128.8 (3)°. One of the allylammonium cations is positionally disordered (fixed occupancy ratio = 0.45:0.55). In the crystal, the cations and anions are co…

crystal structureoxalateallylammoniumHydrogen bondGeneral ChemistryCrystal structureAmmonium oxalateDihedral angleCondensed Matter PhysicsBioinformaticshydrogen bondingOxalateData ReportsDicationlcsh:Chemistrychemistry.chemical_compoundCrystallographydicationchemistrylcsh:QD1-999allyl­ammoniumGeneral Materials ScienceActa crystallographica. Section E, Structure reports online
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A second solvatomorph of poly[[μ4-N,N′-(1,3,5-oxadiazinane-3,5-diyl)bis(carbamoylmethanoato)]nickel(II)dipotassium] : crystal structure, Hirshfeld su…

2021

The title compound, poly[triaquabis[μ4-N,N′-(1,3,5-oxadiazinane-3,5-diyl)bis(carbamoylmethanoato)]dinickel(II)tetrapotassium], [K4Ni2(C7H6N4O7)2(H2O)3] n , is a second solvatomorph of poly[(μ4-N,N′-(1,3,5-oxadiazinane-3,5-diyl)bis(carbamoylmethanoato)nickel(II)dipotassium] reported previously [Plutenko et al. (2021). Acta Cryst. E77, 298–304]. The asymmetric unit of the title compound includes two structurally independent complex anions [Ni(C7H6N4O7)]2−, which exhibit an L-shaped geometry and consist of two almost flat fragments perpendicular to one another: the 1,3,5-oxadiazinane fragment and the fragment including other atoms of the anion. The central Ni atom is in a square-planar N2O2 co…

crystal structureshape analysischemistry.chemical_elementCrystal structureEnergy minimizationIonpseudomacrocyclic ligandCrystalchemistry.chemical_compoundtemplate reactionSHAPE analysisAmidehirshfeld surface analysisAtomHirshfeld surface analysisGeneral Materials Sciencesemi-empirical geometry optimizationCrystallographynickel(ii) complexGeneral ChemistrykompleksiyhdisteetCondensed Matter Physicsnickel(II) complexkiteetTemplate reactionNickelCrystallographychemistryQD901-999nikkelihydrazide-based ligand
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Crystal structure, spectroscopic characterization and Hirshfeld surface analysis of trans-di­aqua­[2,5-bis­(pyridin-4-yl)-1,3,4-oxa­diazole]di­thio­c…

2019

The NiII atom in the mononuclear title complex has an almost regular octa­hedral N4O2 coordination geometry. In the crystal, the complex mol­ecules are linked in a three-dimensional network through strong O—H⋯N hydrogen bonds.

crystal structurespectroscopyThio-chemistry.chemical_elementcoordination complexCrystal structure010403 inorganic & nuclear chemistry01 natural sciencesCoordination complexResearch CommunicationsCrystalchemistry.chemical_compound134-oxadiazoleGeneral Materials Sciencethio­cyanatechemistry.chemical_classificationthiocyanateCrystallographyThiocyanate010405 organic chemistryHydrogen bondGeneral ChemistryHirshfeld analysisCondensed Matter Physics0104 chemical sciencesCrystallographyNickel134-oxa­diazolechemistryQD901-999hydrogen bondsDiazoleActa Crystallographica Section E: Crystallographic Communications
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Crystal structure of two N′-(1-phenyl­benzyl­idene)-2-(thio­phen-3-yl)acetohydrazides

2019

Two N′-(1-(phenyl­ethyl­idene)-2-(thio­phen-3-yl)acetohydrazides containing –OH and –OCH3 at the para-position of the phenyl ring have been synthesized and their mol­ecular and crystal structures are reported.

crystal structurethiopheneSubstituentThio-Crystal structureDihedral angle010402 general chemistry010403 inorganic & nuclear chemistryRing (chemistry)01 natural sciencesResearch CommunicationsCrystalchemistry.chemical_compoundThiopheneGeneral Materials ScienceHirshield analysisScience & TechnologyCrystallographyHydrogen bondGeneral Chemistrythio­pheneHirshfeld analysisCondensed Matter Physics0104 chemical sciencesCrystallographychemistryQD901-999Physical SciencesacetohydrazidesActa Crystallographica Section E: Crystallographic Communications
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Crystal structure of 5′′-benzylidene-1′-methyl-4′-phenyltrispiro[acenaphthylene-1,2′-pyrrolidine-3′,1′′-cyclohexane-3′′,2′′′-[1,3]dioxane]-2,6′′-dione

2016

In the title tris­piro compound, both the methyl-substituted pyrrolidine and dioxalane rings adopt a twist conformation. The cyclo­penta­none ring of the acenapthylen-1-one system adopts flattened envelope conformation, and the cyclo­hexa­none attached to the dioxalane ring adopts boat conformation. In the crystal, centrosymmetrically related mol­ecules are linked into dimers forming rings of (10) graph-set motif, which are further connected into chains parallel to the b axis by C—H⋯O contacts forming rings of (8) graph-set motif.

crystal structuretrispiropyrrolidinesStereochemistryCyclohexane conformationCrystal structurespiro­cyclo­hexa­nones010402 general chemistryRing (chemistry)01 natural sciencesPyrrolidineResearch Communicationslcsh:ChemistryCrystalchemistry.chemical_compoundacenaphthyleneGeneral Materials SciencedioxalaneEne reaction010405 organic chemistryChemistryHydrogen bondtris­piropyrrolidinesGeneral ChemistryCondensed Matter Physicsace­naphthyl­eneAcenaphthylene0104 chemical scienceslcsh:QD1-999spirocyclohexanonesActa Crystallographica Section E Crystallographic Communications
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Estimating QCD uncertainties in Monte Carlo event generators for gamma-ray dark matter searches

2018

Motivated by the recent galactic center gamma-ray excess identified in the Fermi-LAT data, we perform a detailed study of QCD fragmentation uncertainties in the modeling of the energy spectra of gamma-rays from Dark-Matter (DM) annihilation. When Dark-Matter particles annihilate to coloured final states, either directly or via decays such as $W^{(*)}\to q\bar{q}'$, photons are produced from a complex sequence of shower, hadronisation and hadron decays. In phenomenological studies, their energy spectra are typically computed using Monte Carlo event generators. These results have however intrinsic uncertainties due to the specific model used and the choice of model parameters, which are diffi…

dark matter simulationsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)PhotonAstrophysics::High Energy Astrophysical Phenomenamodel [hadronization]SLDgamma ray theoryDark matterMonte Carlo methodHadronFOS: Physical sciencesmass [dark matter]01 natural sciencesHigh Energy Physics - Phenomenology (hep-ph)fragmentationquantum chromodynamics0103 physical sciencesconservation lawddc:530High Energy PhysicsMonte Carloenergy spectrum [gamma ray]Quantum chromodynamicsPhysicsdark matter theoryAnnihilation010308 nuclear & particles physicsphotonGamma rayCERN LEP StorAstronomy and AstrophysicsshowersGalaxyHigh Energy Physics - PhenomenologyannihilationExperimental High Energy PhysicsHigh Energy Physics::Experimentgalaxydecay [hadron]GLAST [interpretation of experiments]Astrophysics - Cosmology and Nongalactic Astrophysics
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Physics reach of the XENON1T dark matter experiment.

2016

The XENON1T experiment is currently in the commissioning phase at the Laboratori Nazionali del Gran Sasso, Italy. In this article we study the experiment's expected sensitivity to the spin-independent WIMP-nucleon interaction cross section, based on Monte Carlo predictions of the electronic and nuclear recoil backgrounds. The total electronic recoil background in $1$ tonne fiducial volume and ($1$, $12$) keV electronic recoil equivalent energy region, before applying any selection to discriminate between electronic and nuclear recoils, is $(1.80 \pm 0.15) \cdot 10^{-4}$ ($\rm{kg} \cdot day \cdot keV)^{-1}$, mainly due to the decay of $^{222}\rm{Rn}$ daughters inside the xenon target. The nu…

dark matter simulationsPhysics - Instrumentation and DetectorsCosmology and Nongalactic Astrophysics (astro-ph.CO)Physics::Instrumentation and Detectorsdark matter experimentFOS: Physical scienceschemistry.chemical_elementCosmic ray7. Clean energy01 natural sciencesdark matter simulationNuclear physicsRecoilXenonIonization0103 physical sciencesNeutronNuclear Experiment010306 general physicsPhysicsMuon010308 nuclear & particles physicsdark matter experimentsAstronomy and AstrophysicsInstrumentation and Detectors (physics.ins-det)dark matter experiments; dark matter simulationschemistryNeutrinoNucleonAstrophysics - Cosmology and Nongalactic AstrophysicsJournal of Cosmology and Astroparticle Physics
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Measurement of the cosmic ray proton spectrum from 40 GeV to 100 TeV with the DAMPE satellite

2019

DAMPE satellite has directly measured the cosmic ray proton spectrum from 40 GeV to 100 TeV and revealed a new feature at about 13.6 TeV.

dark matter cosmic rays spaceProtonMilky WayAstrophysics::High Energy Astrophysical PhenomenaDark matterFOS: Physical sciencesCosmic rayAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsKinetic energy01 natural sciences0103 physical sciences010306 general physicsNuclear ExperimentResearch ArticlesPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Spectral indexMultidisciplinary010308 nuclear & particles physicsPhysicsHigh Energy Physics::PhenomenologySettore FIS/01 - Fisica SperimentaleSciAdv r-articlesPhysics::Accelerator PhysicsHigh Energy Physics::ExperimentAstrophysics - High Energy Astrophysical PhenomenaResearch Article
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Edges and Endpoints in 21-cm Observations from Resonant Photon Production

2020

Physical review letters 127(1), 011102 (1-7) (2021). doi:10.1103/PhysRevLett.127.011102

dark matter: interactionPhotonCosmology and Nongalactic Astrophysics (astro-ph.CO)Physics beyond the Standard ModelbrightnesskineticGeneral Physics and AstronomyFOS: Physical sciencesContext (language use)AstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics53001 natural sciencesDark photonHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesddc:530010306 general physicsPhysicsphoton: productionCOSMIC cancer databasenew physicsproduction [photon]temperatureHigh Energy Physics - PhenomenologyBrightness temperatureDark Agesspectralinteraction [dark matter]signatureAstrophysics - Cosmology and Nongalactic Astrophysics
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Computational Techniques for the Analysis of Small Signals in High-Statistics Neutrino Oscillation Experiments

2020

The current and upcoming generation of Very Large Volume Neutrino Telescopes – collecting unprecedented quantities of neutrino events – can be used to explore subtle effects in oscillation physics, such as (but not restricted to) the neutrino mass ordering. The sensitivity of an experiment to these effects can be estimated from Monte Carlo simulations. With the high number of events that will be collected, there is a trade-off between the computational expense of running such simulations and the inherent statistical uncertainty in the determined values. In such a scenario, it becomes impractical to produce and use adequately-sized sets of simulated events with traditional methods, such as M…

data analysis methodNuclear and High Energy PhysicsMonte Carlo methodFVLV nu TData analysis; Detector; KDE; MC; Monte Carlo; Neutrino; Neutrino mass ordering; Smoothing; Statistics; VLVνTData analysisKDEFOS: Physical sciences01 natural sciencesIceCubeHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)statistical analysisnumerical methods0103 physical sciencesStatisticsNeutrinoddc:530Sensitivity (control systems)MC010306 general physicsNeutrino oscillationInstrumentation and Methods for Astrophysics (astro-ph.IM)InstrumentationMonte CarloPhysicsVLVνT010308 nuclear & particles physicsOscillationStatisticsoscillation [neutrino]ObservableDetectorMonte Carlo [numerical calculations]WeightingNeutrino mass orderingPhysics and AstronomyPhysics - Data Analysis Statistics and ProbabilityPhysique des particules élémentairesNeutrinoAstrophysics - Instrumentation and Methods for AstrophysicsMATTERData Analysis Statistics and Probability (physics.data-an)SmoothingSmoothing
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