Search results for "accelerator"

showing 10 items of 1507 documents

La città di Alphabet. Architettura per prosumers.

2021

Attraverso alcuni aspetti salienti dell’ideazione, della produzione e dell’opposizione al progetto del Toronto Quayside di Sidewalk labs, l’articolo discute l’influenza delle infrastrutture digitali per l’informazione sul progetto della casa e del quartiere. L’ampliamento delle attività svolte da remoto nello spazio domestico, enfatizzato dal quotidiano della pandemia da Covid 19, costituisce per gli oligopolisti planetari degli urban data come Alphabet un utile volano pubblicitario e un acceleratore. La fusione dei nuovi vessilli della tecnoemancipazione e della sostenibilità in ipotesi sperimentali che mirano a costruirsi sia per intero che per parti realizza un nuovo orizzonte in cui lo …

Settore ICAR/14 - Composizione Architettonica E UrbanaTaking into account some salient aspects of the conception production and opposition to the Toronto Quayside project by Sidewalk labs the article discusses the influence of urban data-digital infrastructures on the architectural design of the house and the neighbourhood. The extension of remote control on the practices of everyday life in the domestic space emphasized by the daily Covid 19 pandemic constitutes a useful advertising reference and an accelerator for the planetary oligopolists of urban data such as Alphabet. The fusion of the new emblems of techno-emancipation and sustainability in experimental hypotheses that can be built both in whole or in parts draws a new horizon in which the domestic space generates a technological profit and the inhabitants are transformed into producers. From a historical perspective our reality eclipses the idea of technology as an anonymous contribution to collective progress demonstrated by Giedion in Mechanization takes command and subverts the allegorical value assigned by the Architecture of the Seventies to the relational utopias of the Web Stem and Cluster.
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Observation of a $\gamma$-decaying millisecond isomeric state in $^{128}$Cd$_{80}$

2017

A. Jungclaus et al. -- 6 pags., 5 figs., 2 tabs. -- Open Access funded by Creative Commons Atribution Licence 4.0

Shell model calculationNuclear and High Energy PhysicsFissionSHELL modelNuclear TheoryShell model calculationsTransition strengths[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]01 natural sciences7. Clean energy0103 physical sciencesmedicineddc:530010306 general physicsNuclear ExperimentPhysicsMillisecondRadionuclideIsomeric decay010308 nuclear & particles physicsProjectileParity (physics)lcsh:QC1-999medicine.anatomical_structureIsomeric decaysPhysics::Accelerator PhysicsTransition strengthAtomic physicsNucleuslcsh:Physics
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Modeling particle acceleration and non-thermal emission in supernova remnants

2021

According to the most popular model for the origin of cosmic rays (CRs), supernova remnants (SNRs) are the site where CRs are accelerated. Observations across the electromagnetic spectrum support this picture through the detection of non-thermal emission that is compatible with being synchrotron or inverse Compton radiation from high energy electrons, or pion decay due to proton-proton interactions. These observations of growing quantity and quality promise to unveil many aspects of CRs acceleration and require more and more accurate tools for their interpretation. Here, we show how multi-dimensional MHD models of SNRs, including the effects on shock dynamics due to back-reaction of acceler…

Shock waveMagnetohydrodynamics (MHD)Radiation mechanisms: non-thermalElectromagnetic spectrumAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayAstrophysicsElectronRadiation01 natural sciencesShock wavesAcceleration0103 physical sciencesCosmic rays010303 astronomy & astrophysicsInstrumentationAstrophysics::Galaxy AstrophysicsISM: supernova remnantsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsAstronomy and AstrophysicsParticle accelerationSupernovaSpace and Planetary SciencePhysics::Accelerator PhysicsAstrophysics - High Energy Astrophysical Phenomena
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Laboratory evidence for proton energization by collisionless shock surfing

2021

Charged particles can be accelerated to high energies by collisionless shock waves in astrophysical environments, such as supernova remnants. By interacting with the magnetized ambient medium, these shocks can transfer energy to particles. Despite increasing efforts in the characterization of these shocks from satellite measurements at Earth’s bow shock as well as powerful numerical simulations, the underlying acceleration mechanism or a combination thereof is still widely debated. Here we show that astrophysically relevant super-critical quasi-perpendicular magnetized collisionless shocks can be produced and characterized in the laboratory. We observe the characteristics of super-criticali…

Shock waveProtonAstrophysics::High Energy Astrophysical PhenomenaGeneral Physics and AstronomyFOS: Physical sciences01 natural sciencesAccelerationSettore FIS/05 - Astronomia E Astrofisica0103 physical sciencesBow shock (aerodynamics)010306 general physics010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsPhysicsMechanicsplasmasPhysics - Plasma PhysicsCharged particleComputer Science::Computers and Society[PHYS.PHYS.PHYS-GEN-PH]Physics [physics]/Physics [physics]/General Physics [physics.gen-ph]Magnetic fieldShock (mechanics)Plasma Physics (physics.plasm-ph)Supernova13. Climate actionPhysics::Space PhysicsPhysics::Accelerator Physics
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Signal integrity studies at optical multiplexer board for TileCal system

2007

6 pages.-- ISI Article Identifier: 000253651800006

Signal delayOptical fiberComputer sciencebusiness.industryElectrical engineeringHardware and accelerator control systemsMultiplexerlaw.inventionData acquisitionElectric power transmissionCoupling (computer programming)lawDistortionSignal integritybusinessInstrumentationInstrumentation for particle accelerators and storage rings - high energy (linear accelerators synchrotrons)Mathematical PhysicsComputer hardware
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Search for Isovector Valence-Shell Excitations in 140 Nd and 142 Sm via Coulomb excitation reactions of radioactive ion beams

2018

Projectile Coulomb excitation experiments were performed at HIE-ISOLDE at CERN with the radioactive ion beams of 140Nd and 142Sm. Ions with an energy of 4:62 MeV/A were impinging on a 1.45 mg/cm2 thick 208Pb target. The γ-rays depopulating the Coulomb-excited states were recorded by the HPGe-array MINIBALL and scattered particles were detected by a double-sided silicon strip detector. Experimental intensities were used for the determination of electromagnetic transition matrix elements. A preliminary result of the B(M1; 2+3 → 2+1) of 140Nd and an upper limit for the case of 142Sm are revealing the main fragments of the proton-neutron mixed-symmetry 2+1;ms states.

SiliconPhysics::Instrumentation and DetectorsQC1-999chemistry.chemical_elementCoulomb excitation01 natural sciencesIon0103 physical sciencesNuclear Physics - ExperimentNuclear Experiment010306 general physicsCoulomb excitation experimentsPhysicsLarge Hadron ColliderIsovectorta114010308 nuclear & particles physicsProjectilePhysicsDetectorchemistryPhysics::Accelerator PhysicsAtomic physicsValence electronydinfysiikkaEPJ Web of Conferences
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"Table 2" of "Quasi-free Compton Scattering and the Polarizabilities of the Neutron"

2003

Energy dependence of the quasi-free proton differential cross section.

Single Differential Cross SectionPhotoproduction1.146-1.266ElasticNuclear TheoryPhysics::Accelerator PhysicsGAMMA P --> GAMMA PNuclear ExperimentDSIG/DOMEGA
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"Table 1" of "Quasi-free Compton Scattering and the Polarizabilities of the Neutron"

2003

Energy dependence of the free-proton differential cross section.

Single Differential Cross SectionPhotoproductionElasticNuclear TheoryPhysics::Accelerator PhysicsGAMMA P --> GAMMA P1.13-1.327Nuclear ExperimentDSIG/DOMEGA
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A reservoir trap for antiprotons

2015

We have developed techniques to extract arbitrary fractions of antiprotons from an accumulated reservoir, and to inject them into a Penning-trap system for high-precision measurements. In our trap-system antiproton storage times > 1.08 years are estimated. The device is fail-safe against power-cuts of up to 10 hours. This makes our planned comparisons of the fundamental properties of protons and antiprotons independent from accelerator cycles, and will enable us to perform experiments during long accelerator shutdown periods when background magnetic noise is low. The demonstrated scheme has the potential to be applied in many other precision Penning trap experiments dealing with exotic p…

Speichertechnik - Abteilung BlaumPhysics - Instrumentation and DetectorsMagnetic noiseAtomic Physics (physics.atom-ph)Other Fields of PhysicsFOS: Physical sciences7. Clean energy01 natural sciencesIon trappingphysics.atom-ph010305 fluids & plasmasPhysics - Atomic PhysicsNuclear physicsTrap (computing)0103 physical sciencesPhysics::Atomic PhysicsPhysical and Theoretical ChemistryDetectors and Experimental Techniques010306 general physicsNuclear ExperimentInstrumentationphysics.ins-detSpectroscopyPhysicsInstrumentation and Detectors (physics.ins-det)Condensed Matter PhysicsPenning trapAntiprotonPhysics::Accelerator Physics
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Measurement of the single-top-quark production cross section at CDF.

2008

We report a measurement of the single top quark production cross section in 2.2 ~fb-1 of p-pbar collision data collected by the Collider Detector at Fermilab at sqrt{s}=1.96 TeV. Candidate events are classified as signal-like by three parallel analyses which use likelihood, matrix element, and neural network discriminants. These results are combined in order to improve the sensitivity. We observe a signal consistent with the standard model prediction, but inconsistent with the background-only model by 3.7 standard deviations with a median expected sensitivity of 4.9 standard deviations. We measure a cross section of 2.2 +0.7 -0.6(stat+sys) pb, extract the CKM matrix element value |V_{tb}|=0…

StandardsTop quarkParticle physicsFOS: Physical sciencesGeneral Physics and Astronomyddc:500.2Astrophysics::Cosmology and Extragalactic Astrophysics114 Physical sciences01 natural sciencesStandard ModelHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)Tellurium compoundsMatrix elementsCross section (physics)Colliding beam acceleratorsStandard deviations0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Sensitivity (control systems)010306 general physicsStandard models14.65.Ha 13.85Qk 12.15Hh 12.15.JiPhysicshep-ex010308 nuclear & particles physicsCabibbo–Kobayashi–Maskawa matrixPhysicsStatisticsHigh Energy Physics::PhenomenologyOrder (ring theory)Collider Detector at FermilabCross sections_Parallel analysisProduction (computer science)High Energy Physics::ExperimentCollider Detector at FermilabNeural networksQuark productions
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