Search results for "TEIL"

showing 10 items of 437 documents

Isovector and isoscalar spin-multipole giant resonances in the parent and daughter nuclei of double-β-decay triplets

2022

The strength distributions, including giant resonances, of isovector and isoscalar spin-multipole transitions in the commonly studied double-β-decay triplets are computed in the framework of the quasiparticle random-phase approximation (QRPA) using the Bonn-A two-body interaction in no-core single-particle valence spaces. The studied nuclei include the double-β parent and daughter pairs (76Ge, 76Se), (82Se, 82Kr), (96Zr, 96Mo), (100Mo, 100Ru), (116Cd, 116Sn), (128Te, 128Xe), (130Te, 130Xe), and (136Xe, 136Ba). The studied transitions proceed from the ground states to the Jπ=0−,1−,2− (spin-dipole transitions) and Jπ=1+,2+,3+ (spin-quadrupole transitions) excited states in these nuclei. Compa…

59 ≤ A ≤ 8990 ≤ A ≤ 149nuclear physicsbeetasäteilyneutriinotdouble beta decaynuclear structure & decayscollective modelshiukkasfysiikkaydinfysiikkakvasihiukkaset
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New exotic beams from the SPIRAL 1 upgrade

2018

Since 2001, the SPIRAL 1 facility has been one of the pioneering facilities in ISOL techniques for reaccelerating radioactive ion beams: the fragmentation of the heavy ion beams of GANIL on graphite targets and subsequent ionization in the Nanogan ECR ion source has permitted to deliver beams of gaseous elements (He, N, O, F, Ne, Ar, Kr) to numerous experiments. Thanks to the CIME cyclotron, energies up to 20 AMeV could be obtained. In 2014, the facility was stopped to undertake a major upgrade, with the aim to extend the production capabilities of SPIRAL 1 to a number of new elements. This upgrade, which is presently under commissioning, consists in the integration of an ECR booster in the…

Accelerator Physics (physics.acc-ph)Nuclear and High Energy PhysicsNuclear engineering[PHYS.PHYS.PHYS-ACC-PH]Physics [physics]/Physics [physics]/Accelerator Physics [physics.acc-ph]tutkimuslaitteetCyclotronFOS: Physical scienceshiukkaskiihdyttimet[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]nucl-ex7. Clean energy01 natural sciencesIonlaw.inventionion sourceslawIonization0103 physical sciencesIon sourcesNuclear Physics - ExperimentNuclear Experiment (nucl-ex)radioactive ion beams010306 general physicsNuclear ExperimentInstrumentationRadioactive ion beamsphysics.acc-ph[PHYS]Physics [physics]Physics010308 nuclear & particles physicsAccelerators and Storage RingsIon sourceUpgradesäteilyfysiikkaBeamlinePhysics - Accelerator PhysicsAGATABeam (structure)
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Broadband Multi-wavelength Properties of M87 during the 2017 Event Horizon Telescope Campaign

2021

Full list of authors: EHT MWL Science Working Group; Algaba, J. C.; Anczarski, J.; Asada, K.; Baloković, M.; Chandra, S.; Cui, Y. -Z.; Falcone, A. D.; Giroletti, M.; Goddi, C.; Hada, K.; Haggard, D.; Jorstad, S.; Kaur, A.; Kawashima, T.; Keating, G.; Kim, J. -Y.; Kino, M.; Komossa, S.; Kravchenko, E. V.; Krichbaum, T. P.; Lee, S. -S.; Lu, R. -S.; Lucchini, M.; Markoff, S.; Neilsen, J.; Nowak, M. A.; Park, J.; Principe, G.; Ramakrishnan, V.; Reynolds, M. T.; Sasada, M.; Savchenko, S. S.; Williamson, K. E.; Event Horizon Telescope Collaboration; Akiyama, Kazunori; Alberdi, Antxon; Alef, Walter; Anantua, Richard; Azulay, Rebecca; Baczko, Anne-Kathrin; Ball, David; Barrett, John; Bintley, Dan; …

Accretion010504 meteorology & atmospheric sciencesAstronomyFluxAstrophysics7. Clean energy01 natural sciencesActive galactic nuclei; Radio cores; Low-luminosity active galactic nuclei; High energy astrophysics; Astrophysical black holes; Accretion; Astrophysics - High Energy Astrophysical Phenomena; Astrophysics - Cosmology and Nongalactic Astrophysics; Astrophysics - Astrophysics of Galaxies010303 astronomy & astrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicsastro-ph.HERadio coreAccretion (meteorology)PhysicsAstrophysical black holes520 Astronomie und zugeordnete WissenschaftenActive galactic nuclei ; Radio cores ; Low-luminosity ; active galactic nuclei ; High energy astrophysics ; Astrophysical black holes ; AccretionAstrophysical black holeLow-luminosity active galactic nucleiastro-ph.COAstrophysics - High Energy Astrophysical PhenomenaAccretion; Active galactic nuclei; Astrophysical black holes; High energy astrophysics; Low-luminosity active galactic nuclei; Radio coresHigh energy astrophysicsRadio coresAstrophysics - Cosmology and Nongalactic AstrophysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Active galactic nucleusHigh-energy astronomyastro-ph.GAAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesF500Astrophysics::Cosmology and Extragalactic AstrophysicsHigh energy astrophysic0103 physical sciencesVery-long-baseline interferometryddc:530Astrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesEvent Horizon TelescopeSupermassive black holeActive galactic nucleiAstronomy and Astrophysics530 PhysikAstrophysics - Astrophysics of GalaxiesGalaxySpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)ddc:520Active galactic nuclei; Radio cores; Low-luminosity active galactic nuclei; High energy astrophysics; Astrophysical black holes; AccretionHESS - Abteilung Hinton[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Mitä mieltä, professorit?

2006

25 vuoden ikään ehtinyt Aikuiskasvatus kysyi kaikilta aikuiskasvatuksen professoreiltamme heidän näkemyksiään neljässä asiassa. Kaikkiin ei tarvinnut vastata. Tällaista kysyttiin ja näin vastasivat Yrjö Engeström ja Reijo Miettinen Helsingin yliopistosta, Anneli Eteläpelto Jyväskylän yliopistosta, Jukka Tuomisto ja Juha Suoranta Tampereen yliopistosta, Risto Rinne Turun yliopistosta, Kari E. Nurmi Lapin yliopistosta sekä vt:nä virkaa hoitava Leena Ahteenmäki-Pelkonen Joensuun yliopistosta. Vastausjärjestys on arvottu.

Ahteenmäki-Pelkonen LeenaEngeström Yrjökasvatustieteilijät [http://www.yso.fi/onto/yso/p20573]Rinne RistoMiettinen ReijoGeneral MedicineGeneral Chemistrytiede [http://www.yso.fi/onto/yso/p2240]Eteläpelto Annelitiedelehdet [http://www.yso.fi/onto/yso/p10315]Nurmi Kari E.Tuomisto JukkaSuoranta Juhatutkimus [http://www.yso.fi/onto/yso/p183]aikuiskoulutus [http://www.yso.fi/onto/yso/p300][Aikuiskasvatus]aikuiskasvatus [http://www.yso.fi/onto/yso/p10754]professorit [http://www.yso.fi/onto/yso/p17044]Aikuiskasvatus
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Luonto ja eläimet Eija-Liisa Ahtilan teoksessa Tänään

2014

Sivuttukielmassa käsitellään taiteilija Eija-Liisa Ahtilan kolmikanavaista videoinstallaatiota Tänään (1996–1997). Erityisesti pohditaan teoksesta avautuvia käsityksiä luonnosta ja eläimistä. Taustaksi tutkimukselle esitellään videoinstallaatioiden kehitystä taidemuotona 1990-luvun lopulla sekä erityisesti Eija-Liisa Ahtilan tapoja käyttää monikuvainstaalaatiota taiteensa välineenä. Myös Ahtiloan tuotannossa olennaiset käsitteet aika, paikka ja subjekti tulevat myös kytketyiksi tutkimukseen.

Ahtila Eija-Liisavideotaiteilijateläimetvideotaideluonto
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Asiantuntevien lukijoiden jäljillä : Alara-lehden lukemistutkimus

2008

Alara (aikakauslehti)lukijatvastaanottolukemistutkimusSäteilyturvakeskuslukeminensurvey-tutkimus
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Sixfold improved single particle measurement of the magnetic moment of the antiproton

2017

Our current understanding of the Universe comes, among others, from particle physics and cosmology. In particle physics an almost perfect symmetry between matter and antimatter exists. On cosmological scales, however, a striking matter/antimatter imbalance is observed. This contradiction inspires comparisons of the fundamental properties of particles and antiparticles with high precision. Here we report on a measurement of the g-factor of the antiproton with a fractional precision of 0.8 parts per million at 95% confidence level. Our value /2=2.7928465(23) outperforms the previous best measurement by a factor of 6. The result is consistent with our proton g-factor measurement gp/2=2.7928473…

AntiparticleParticle physicsLorentz transformationSciencelorentzGeneral Physics and Astronomysystem01 natural sciencesArticleGeneral Biochemistry Genetics and Molecular BiologyCosmologyNuclear physicssymbols.namesakeStandard-Model Extension0103 physical sciencesNuclear Physics - Experimentcpt010306 general physicsNuclear ExperimentPhysicsMultidisciplinary010308 nuclear & particles physicsQpenning trapParity (physics)General ChemistryPenning trapAntiprotonAntimattersymbolstestsddc:500Präzisionsexperimente - Abteilung Blaum
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Investigating the Impact of Radiation-Induced Soft Errors on the Reliability of Approximate Computing Systems

2020

International audience; Approximate Computing (AxC) is a well-known paradigm able to reduce the computational and power overheads of a multitude of applications, at the cost of a decreased accuracy. Convolutional Neural Networks (CNNs) have proven to be particularly suited for AxC because of their inherent resilience to errors. However, the implementation of AxC techniques may affect the intrinsic resilience of the application to errors induced by Single Events in a harsh environment. This work introduces an experimental study of the impact of neutron irradiation on approximate computing techniques applied on the data representation of a CNN.

Approximate computingComputer scienceReliability (computer networking)Radiation effectsRadiation induced02 engineering and technologyneuroverkotExternal Data Representation01 natural sciencesConvolutional neural networkSoftwareHardware020204 information systems0103 physical sciences0202 electrical engineering electronic engineering information engineering[SPI.NANO]Engineering Sciences [physics]/Micro and nanotechnologies/MicroelectronicsResilience (network)mikroprosessoritNeutronsResilience010308 nuclear & particles physicsbusiness.industryReliabilityApproximate computingPower (physics)[SPI.TRON]Engineering Sciences [physics]/ElectronicsComputer engineeringsäteilyfysiikka[INFO.INFO-ES]Computer Science [cs]/Embedded SystemsbusinessSoftware
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Constraints on the Coupling between Axionlike Dark Matter and Photons Using an Antiproton Superconducting Tuned Detection Circuit in a Cryogenic Penn…

2021

We constrain the coupling between axionlike particles (ALPs) and photons, measured with the superconducting resonant detection circuit of a cryogenic Penning trap. By searching the noise spectrum of our fixed-frequency resonant circuit for peaks caused by dark matter ALPs converting into photons in the strong magnetic field of the Penning-trap magnet, we are able to constrain the coupling of ALPs with masses around $2.7906-2.7914\,\textrm{neV/c}^2$ to $g_{a\gamma}< 1 \times 10^{-11}\,\textrm{GeV}^{-1}$. This is more than one order of magnitude lower than the best laboratory haloscope and approximately 5 times lower than the CERN axion solar telescope (CAST), setting limits in a mass and cou…

Astrophysics and AstronomyCosmology and Nongalactic Astrophysics (astro-ph.CO)PhotonAtomic Physics (physics.atom-ph)Dark matterOther Fields of PhysicsFOS: Physical sciencesGeneral Physics and Astronomyphysics.atom-ph01 natural sciences7. Clean energyPhysics - Atomic PhysicsNuclear physicsHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesddc:530Physics::Atomic Physics010306 general physicsParticle Physics - PhenomenologySuperconductivityPhysicshep-phPenning trapCoupling (probability)Magnetic fieldHigh Energy Physics - PhenomenologyAntiprotonastro-ph.COPräzisionsexperimente - Abteilung BlaumCERN Axion Solar TelescopeAstrophysics - Cosmology and Nongalactic AstrophysicsPhysical Review Letters
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In-situ observations of young contrails – overview and selected results from the CONCERT campaign

2010

Lineshaped contrails were detected with the research aircraft Falcon during the CONCERT – CONtrail and Cirrus ExpeRimenT – campaign in October/November 2008. The Falcon was equipped with a set of instruments to measure the particle size distribution, shape, extinction and chemical composition as well as trace gas mixing ratios of sulfur dioxide (SO&lt;sub&gt;2&lt;/sub&gt;), reactive nitrogen and halogen species (NO, NO&lt;sub&gt;y&lt;/sub&gt;, HNO&lt;sub&gt;3&lt;/sub&gt;, HONO, HCl), ozone (O&lt;sub&gt;3&lt;/sub&gt;) and carbon monoxide (CO). During 12 mission flights over Europe, numerous contrails, cirrus clouds and a volcanic aerosol layer were probed at altitudes between 8.5 and 11.6 km…

Atmospheric ScienceOzoneMeteorologyicecirrusSO2medicine.disease_causeAtmospheric scienceslcsh:Chemistrychemistry.chemical_compoundAltitudetrace gasesddc:550medicineLife ScienceFlugabteilung OberpfaffenhofenStratosphereIce crystalsInstitut für AntriebstechnikAtmosphärische SpurenstoffecontrailSootlcsh:QC1-999JTrace gaschemistrylcsh:QD1-999Extinction (optical mineralogy)Cirruslcsh:PhysicsAtmospheric Chemistry and Physics
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