Search results for "methods [Gene Expression Profiling]"

showing 10 items of 838 documents

First-principles modelling for time-resolved ARPES under different pump-probe conditions

2021

First-principles methods for time-resolved angular resolved photoelectron spectroscopy play a pivotal role in providing interpretation and microscopic understanding of the complex experimental data and in exploring novel observables or observation conditions that may be achieved in future experiments. Here we describe an efficient, reliable and scalable first-principles method for tr-ARPES based on time-dependent density functional theory including propagation and surface effects usually discarded in the widely used many-body techniques based on computing the non-equilibrium spectral function and discuss its application to a variety of pump–probe conditions. We identify four conditions, dep…

Time-resolved angular resolved photoelectron spectroscopy (ARPES)Condensed Matter - Materials ScienceRadiationMaterials Science (cond-mat.mtrl-sci)FOS: Physical sciences02 engineering and technologyTheoretical spectroscopy021001 nanoscience & nanotechnologyCondensed Matter Physics01 natural sciencesAtomic and Molecular Physics and OpticsSettore FIS/03 - Fisica Della MateriaElectronic Optical and Magnetic MaterialsComputational methods for excitation in solids0103 physical sciencesTime-dependent density functional theoryPhysical and Theoretical Chemistry010306 general physics0210 nano-technologySpectroscopy
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Search for lepton flavour violation in the e mu continuum with the ATLAS detector in root s=7 TeV pp collisions at the LHC

2012

This paper presents a search for the t-channel exchange of an R-parity violating scalar top quark ([~ over t] ) in the e[superscript ±]μ[superscript ∓] continuum using 2.1 fb[superscript −1] of data collected by the ATLAS detector in s√=7 TeV pp collisions at the Large Hadron Collider. Data are found to be consistent with the expectation from the Standard Model backgrounds. Limits on R-parity-violating couplings at 95 % C.L. are calculated as a function of the scalar top mass ( m[subscript bar over t]). The upper limits on the production cross section for pp→eμX, through the t-channel exchange of a scalar top quark, ranges from 170 fb for m[subscript ~ over t]=95 GeV to 30 fb for m[subscrip…

Top quarkPhysics and Astronomy (miscellaneous)Hadron01 natural sciencesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Nuclear ExperimentSUPERSYMMETRYPair ProductionPhysicsddc:539eμ continuumLarge Hadron ColliderSettore FIS/01 - Fisica SperimentaleScalar LeptoquarksSupersymmetryHERAATLASComputer Science::Computers and SocietyPhysical SciencesComputingMethodologies_DOCUMENTANDTEXTPROCESSINGFísica nuclearLHCParticle Physics - ExperimentParticle physics[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]leptonsCiências Naturais::Ciências FísicasScalar (mathematics):Ciências Físicas [Ciências Naturais]FOS: Physical sciencesddc:500.2530Partícules (Física nuclear)Nuclear physicsViolació CP (Física nuclear)0103 physical sciencesFysikddc:530High Energy Physics010306 general physicsEngineering (miscellaneous)lepton flavour violation; eμ continuum; ATLAS detector; LHCCiencias ExactasHeraScience & TechnologyATLAS detector010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyFísica[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Pair productionHADRON-HADRON COLLISIONSCol·lisions (Física nuclear)Experimental High Energy PhysicsHigh Energy Physics::ExperimentLeptonEuropean Physical Journal C
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Option Pricing and Hedging in the Presence of Transaction Costs and Nonlinear Partial Differential Equations

2008

In the presence of transaction costs the perfect option replication is impossible which invalidates the celebrated Black and Scholes (1973) model. In this chapter we consider some approaches to option pricing and hedging in the presence of transaction costs. The distinguishing feature of all these approaches is that the solution for the option price and hedging strategy is given by a nonlinear partial differential equation (PDE). We start with a review of the Leland (1985) approach which yields a nonlinear parabolic PDE for the option price, one of the first such in finance. Since the Leland's approach to option pricing has been criticized on different grounds, we present a justification of…

Transaction costAsymptotic analysisMathematical optimizationActuarial scienceValuation of optionsEconomicsPortfolioAsian optionBlack–Scholes modelFinite difference methods for option pricingFutures contractSSRN Electronic Journal
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A method for genome-wide analysis of DNA helical tension by means of psoralen-DNA photobinding

2010

The helical tension of chromosomal DNA is one of the epigenetic landmarks most difficult to examine experimentally. The occurrence of DNA crosslinks mediated by psoralen photobinding (PB) stands as the only suitable probe for assessing this problem. PB is affected by chromatin structure when is done to saturation; but it is mainly determined by DNA helical tension when it is done to very low hit conditions. Hence, we developed a method for genome-wide analysis of DNA helical tension based on PB. We adjusted in vitro PB conditions that discern DNA helical tension and applied them to Saccharomyces cerevisiae cells. We selected the in vivo cross-linked DNA sequences and identified them on DNA …

Transcription GeneticUltraviolet RaysSaccharomyces cerevisiaeMutantADNSaccharomyces cerevisiaeBiologyDNA sequencingGenètica molecularchemistry.chemical_compoundGeneticsTrioxsalenDNA FungalOligonucleotide Array Sequence AnalysisProbabilityTopoisomeraseChromosomeDNAGenomicsbiology.organism_classificationMolecular biologyChromatinNucleosomesChromatinDNA-Binding ProteinsGenòmicaCross-Linking ReagentschemistryNaked DNAbiology.proteinBiophysicsNucleic Acid ConformationMethods OnlineChromosomes FungalDNA TopoisomerasesDNA
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Advanced Virgo Status

2015

Abstract The detection of a gravitational wave signal in September 2015 by LIGO interferometers, announced jointly by LIGO collaboration and Virgo collaboration in February 2016, opened a new era in Astrophysics and brought to the whole community a new way to look at - or “listen” to - the Universe. In this regard, the next big step was the joint observation with at least three detectors at the same time. This configuration provides a twofold benefit: it increases the signal-to-noise ratio of the events by means of triple coincidence and allows a narrower pinpointing of GW sources, and, in turn, the search for Electromagnetic counterparts to GW signals. Advanced Virgo (AdV) is the second ge…

Triple coincidenceHistoryComputer sciencePhysics::Instrumentation and DetectorsAstronomy01 natural sciencesLIGO010303 astronomy & astrophysicsmedia_commonSettore FIS/01Detector/dk/atira/pure/sustainabledevelopmentgoals/partnershipsAstrophysics::Instrumentation and Methods for AstrophysicsDetectorsdetector: upgradeComputer Science ApplicationsInterferometryUpgrade[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]upgradeDetection rateAdvanced VirgoGWOrders of magnitude (power)Nuclear and High Energy PhysicsnoiseVIRGO: sensitivitydetector: performancemedia_common.quotation_subjectinterferometerJoint observationgravitational radiation: direct detectionAdvanced Virgo; GW; detectorsEducationelectromagnetic field: production[ PHYS.GRQC ] Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Gravitational wavesSDG 17 - Partnerships for the Goals0103 physical sciencesAerospace engineeringdetector: design010308 nuclear & particles physicsGravitational wavebusiness.industrygravitational radiationAstronomy and AstrophysicsLIGOUniversegravitational radiation detector* Automatic Keywords *VIRGODetectors; Gravitational waves; Nuclear and High Energy Physics; Astronomy and Astrophysicsgravitational radiation: emissionHigh Energy Physics::ExperimentTelecommunicationsbusiness[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Trigger and aperture of the surface detector array of the Pierre Auger Observatory

2010

The surface detector array of the Pierre Auger Observatory consists of 1600 water-Cherenkov detectors, for the study of extensive airshowers (EAS) generated by ultra-high-energy cosmic rays. We describe the trigger hierarchy, from the identification of candidates howers at the level of a single detector, amongst a large background (mainly random single cosmic ray muons), up to the selection of real events and the rejection of random coincidences. Such trigger makes the surface detector array fully efficient for the detection of EAS with energy above 3 x 1018 eV, for all zenith angles between 03 and 603, independently of the position of the impact point and of the mass of the primary particl…

Ultra high energy cosmic rays; Auger Observatory; Extensive air showers; Trigger; ExposurePhysics::Instrumentation and DetectorsAstronomyHigh-Energy Cosmi Ray7. Clean energy01 natural sciencesAugerAcceptance and Trigger Efficiency010303 astronomy & astrophysicsInstrumentationComputingMilieux_MISCELLANEOUSPhysicsRange (particle radiation)PhysicsDetectorAstrophysics::Instrumentation and Methods for AstrophysicsPierre Auger ObservatoryHigh energyFísica nuclearAstrophysics - Instrumentation and Methods for AstrophysicsNuclear and High Energy Physics[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]AIR SHOWERSApertureInstrumentationAstrophysics::High Energy Astrophysical PhenomenaExtensive air showerFOS: Physical sciencesCosmic rayENERGIACosmic RayUltra high energy cosmic rayExposureOpticsultra high energy cosmic rays Auger Observatory extensive airshowers trigger exposure0103 physical sciencesPARTICLESExtensive air showersSurface DetectorInstrumentation and Methods for Astrophysics (astro-ph.IM)ZenithCiencias ExactasNuclear and High Energy PhysicPierre Auger Observatory010308 nuclear & particles physicsbusiness.industryFísicaUltra high energy cosmic raysUltra-high energy cosmic rays[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]TriggerAuger ObservatoryExperimental High Energy PhysicsHigh Energy Physics::Experimentbusiness
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Zināšanu vadīšanas metožu pilnveidošana organizācijās

2013

Elektroniskā versija nesatur pielikumus

VadībzinātneZināšanu vadīšanas sistēmaBusiness managementUzņēmējdarbības vadībapersonāla attīstībaknowledge management systempersonnel developmentinovatīvās mācību metodesinnovative methods of teachingVadība un administrēšana un nekustamo īpašumu pārvaldība
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The Voyage of Metals in the Universe from Cosmological to Planetary Scales: the need for a Very High-Resolution, High Throughput Soft X-ray Spectrome…

2019

Metals form an essential part of the Universe at all scales. Without metals we would not exist, and the Cosmos would look completely different. Metals are primarily born through nuclear processes in stars. They leave their cradles through winds or explosions, and then start their journey through space. This can lead them in and out of astronomical objects on all scales, ranging from comets, planets, stars, entire galaxies, groups and clusters of galaxies to the largest structures of the Universe. Their wanderings are fundamental in determining how these objects, and the entire universe, evolve. In addition, their bare presence can be used to trace what these structures look like. The scope …

Very high resolutionAstronomical ObjectsCosmology and Nongalactic Astrophysics (astro-ph.CO)010504 meteorology & atmospheric sciencesGalaxy-ISM-CGM-IGM feedbackFOS: Physical sciencesSpace (mathematics)Cycle of baryons and metals7. Clean energy01 natural sciencesCycle of baryons and metals; Galaxy-ISM-CGM-IGM feedback; High-resolution X-ray spectrometer; X-ray gratingsSettore FIS/05 - Astronomia E Astrofisica0103 physical sciences[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]X-ray gratingsInstrumentation and Methods for Astrophysics (astro-ph.IM)010303 astronomy & astrophysicsThroughput (business)0105 earth and related environmental sciencesCycle of baryons and metalHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsSoft x rayCOSMIC cancer databaseSpectrometerSettore FIS/05AstronomyAstronomy and AstrophysicsHigh-resolution X-ray spectrometerAstrophysics - Astrophysics of GalaxiesStars13. Climate actionSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)Astrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astrophysics - Cosmology and Nongalactic Astrophysics
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EDGE: explorer of diffuse emission and gamma-ray burst explosions

2009

How structures on various scales formed and evolved from the early Universe up to present time is a fundamental question of astrophysical cosmology. EDGE will trace the cosmic history of the baryons from the early generations of massive star by Gamma-Ray Burst (GRB) explosions, through the period of cluster formation, down to very low redshifts, when between a third and one half of the baryons are expected to reside in cosmic filaments undergoing gravitational collapse by dark matter (Warm Hot Intragalactic Medium: WHIM). In addition EDGE, with its unprecedented observational capabilities, will provide key results on several other topics. The science is feasible with a medium class mission …

Vision[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Warm–hot intergalactic mediumAstrophysicsAstrophysics7. Clean energy01 natural sciencesCosmologySettore FIS/05 - Astronomia E AstrofisicaIntergalactic MediumWarm-Hot Intergalactic MediumX-rays Cosmology Clusters Gamma-ray bursts Warm-hot intergalactic medium Missions010303 astronomy & astrophysicsX-ray telescopesX-rays; Cosmology; Clusters; Gamma-ray bursts; Warm– hot intergalactic medium; MissionsPhysicsEquipment and servicesSatellite MissionSpectrometersAstrophysics (astro-ph)X-rays Cosmology Clusters Gamma-ray bursts Warm– hot intergalactic medium MissionsTemperatureAstrophysics::Instrumentation and Methods for AstrophysicsCosmologyGamma-ray burstsCosmic VisionSpectral resolutionGalaxy ClustersAstrophysics::High Energy Astrophysical PhenomenaDark matterFOS: Physical sciencesWarm&ndashAstrophysics::Cosmology and Extragalactic AstrophysicsMissionshot intergalactic mediumAbsorptionNO010309 opticsX-rayClustersWarm–hot intergalactic mediumGalaxy groups and clusters0103 physical sciencesX-raysGalaxy groups and clustersImaging systems010306 general physicsGamma-ray burstWarm&ndashGalaxy clusterSpatial resolutionSensorsAstronomyX-rays clusters Gamma-Ray Bursts Warm-Hot Intergalactic Medium missionsAstronomy and AstrophysicsGalaxyRedshiftCluster13. Climate actionSpace and Planetary ScienceGamma-ray burstOptics for EUV, X-Ray, and Gamma-Ray Astronomy III. Edited by O'Dell, Stephen L.; Pareschi, Giovanni. Proceedings of the SPIE
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Effective field theory search for high-energy nuclear recoils using the XENON100 dark matter detector

2017

International audience; We report on weakly interacting massive particles (WIMPs) search results in the XENON100 detector using a nonrelativistic effective field theory approach. The data from science run II (34  kg×224.6 live days) were reanalyzed, with an increased recoil energy interval compared to previous analyses, ranging from (6.6–240)  keVnr. The data are found to be compatible with the background-only hypothesis. We present 90% confidence level exclusion limits on the coupling constants of WIMP-nucleon effective operators using a binned profile likelihood method. We also consider the case of inelastic WIMP scattering, where incident WIMPs may up-scatter to a higher mass state, and …

WIMP nucleon: scatteringParticle physicsdata analysis methodCosmology and Nongalactic Astrophysics (astro-ph.CO)Physics and Astronomy (miscellaneous)Physics::Instrumentation and DetectorsWIMP[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]Dark matterchemistry.chemical_elementFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesNuclear physicsXENONXenonWIMPstatistical analysis0103 physical sciencesEffective field theoryDark Matter010306 general physicsS030UDMnucleus: recoilPhysicsCoupling constanteffective field theory: nonrelativistic010308 nuclear & particles physicsScatteringDetectorAstrophysics::Instrumentation and Methods for Astrophysicsdark matter: detectorchemistryWeakly interacting massive particlesDirect SearchHigh Energy Physics::ExperimentTPC[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]recoil: energyAstrophysics - Cosmology and Nongalactic Astrophysics
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