Search results for " dar"

showing 10 items of 1907 documents

Sensitivity of the Cherenkov Telescope Array to a dark matter signal from the Galactic centre

2021

Full list of authors: Acharyya, A.; Adam, R.; Adams, C.; Agudo, I.; Aguirre-Santaella, A.; Alfaro, R.; Alfaro, J.; Alispach, C.; Aloisio, R.; Alves Batista, R.; Amati, L.; Ambrosi, G.; Angüner, E. O.; Antonelli, L. A.; Aramo, C.; Araudo, A.; Armstrong, T.; Arqueros, F.; Asano, K.; Ascasíbar, Y. Ashley, M.; Balazs, C.; Ballester, O.; Baquero Larriva, A.; Barbosa Martins, V.; Barkov, M.; Barres de Almeida, U.; Barrio, J. A.; Bastieri, D.; Becerra, J.; Beck, G.; Becker Tjus, J.; Benbow, W.; Benito, M.; Berge, D.; Bernardini, E.; Bernlöhr, K.; Berti, A.; Bertucci, B.; Beshley, V.; Biasuzzi, B.; Biland, A.; Bissaldi, E.; Biteau, J.; Blanch, O.; Blazek, J.; Bocchino, F.; Boisson, C.; Bonneau Arbe…

Cherenkov Telescope ArrayMATÉRIA ESCURAscale: TeVAstronomyatmosphere [Cherenkov counter]dark matter experimentDark matter theoryenergy resolutionGamma ray experimentsParticleAstrophysicscosmic background radiation01 natural sciences7. Clean energyHigh Energy Physics - Phenomenology (hep-ph)benchmarkWIMPHESSenergy: fluxTeV [scale]relativistic [charged particle]gamma ray experimentMAGIC (telescope)Monte CarloEvent reconstructionPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Contractionspatial distributiontrack data analysisPhysicsdensity [dark matter]ClumpyAstrophysics::Instrumentation and Methods for AstrophysicsimagingHigh Energy Physics - Phenomenologydark matter experiments; dark matter theory; gamma ray experiments; galaxy morphologyDark matter experimentsFísica nuclearVERITASAstrophysics - High Energy Astrophysical PhenomenaSimulationsnoiseWIMPAstrophysics::High Energy Astrophysical PhenomenaDark mattersatelliteCosmic background radiationFOS: Physical sciencesAnnihilationdark matter: densityAstrophysics::Cosmology and Extragalactic AstrophysicsCherenkov counter: atmosphereheavy [dark matter]530annihilation [dark matter]GLASTDark matter experiments; Dark matter theory; Galaxy morphology; Gamma ray experimentscosmic radiation [p]0103 physical sciencesCherenkov [radiation]Candidatesddc:530AGNCherenkov radiationRadiative Processesthermal [cross section]010308 nuclear & particles physicsFísicadark matter: annihilationGamma-Ray SignalsCherenkov Telescope Array ; dark matter ; Galactic Center ; TeV gamma-ray astronomyAstronomy and AstrophysicsMassCherenkov Telescope Arrayradiation: CherenkovsensitivityMAGICGalaxyAstronomíadark matter: heavygamma rayp: cosmic radiation[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]correlationcharged particle: relativisticflux [energy]Galaxy morphology/dk/atira/pure/subjectarea/asjc/3100/3103galaxysupersymmetry[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]cross section: thermal
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Piedziņas vēršana uz darba samaksu un tai pielīdzinātiem maksājumiem.

2018

Bakalaura darbs veltīts piedziņas vēršanas uz darba samaksu un tai pielīdzināmiem maksājumiem izvērtēšanai. Bakalaura darba mērķis ir pētīt piedziņas būtību, piedziņas vēršanas uz mantu vispārīgo kārtību, piedziņas vēršanas uz personas naudas līdzekļiem īpatnības, kā arī piedziņas vēršanu pret nepilngadīgas personas darba samaksu un citiem naudas līdzekļiem. Lai sasniegtu bakalaura darba mērķi, autors ir aplūkojis Latvijas un ārvalstu normatīvos aktus, juridisko literatūru, publikācijas, kā arī Latvijas tiesu praksi. Bakalaura darba pētījuma rezultātā izstrādāti secinājumi un priekšlikumi sprieduma izpildes institūta uzlabošanai, kā arī Civilprocesa likuma un Darba likuma grozījumiem. Atslē…

Civilprocesa likumssprieduma izpildepiedziņa uz darba samaksupiedziņaJuridiskā zinātnecivilprocess
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Contradicciones y paradojas de la restauración monumental en España en el siglo XX: las intervenciones del arquitecto manuel Lorente Junquera en la I…

2014

Contradicciones y paradojas de la restauración monumental en España en el siglo XX: las intervenciones del arquitecto manuel Lorente Junquera en la Iglesia de San Miguel Daroca (Zaragoza 1961-1968) Artículolas intervenciones del arquitecto manuel Lorente Junquera en la Iglesia de San Miguel Daroca (Zaragoza 1961-1968) Artículo [Contradicciones y paradojas de la restauración monumental en España en el siglo XX]UNESCO::HISTORIA::Historia por especialidades::Historia del arte:HISTORIA::Historia por especialidades::Historia del arte [UNESCO]
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A three-dimensional study of the onset of convection in a horizontal, rectangular porous channel heated from below

2012

Author's version of an article published in the journal: International Journal of Thermal Sciences. Also available from the publisher at: http://dx.doi.org/10.1016/j.ijthermalsci.2011.12.012 The onset of convection is studied in a rectangular channel filled with a fluid saturated porous medium, bounded above and below by impermeable isothermal walls at unequal temperatures and laterally by partially conducting walls. A three-dimensional linear stability analysis is carried out under the assumption of an infinite longitudinal channel length. Then, this assumption is relaxed in order to determine the threshold length for the three-dimensional convection to be the preferred mode at onset. Sens…

ConvectionMaterials scienceBiot number Darcy-Bénard problem lateral confinement linear stability method of weighted residuals rectangular channelAspect ratioBiot numberLINEAR STABILITYBIOT NUMBERGeneral EngineeringThermodynamicsMechanicsCondensed Matter PhysicsInstabilityVDP::Mathematics and natural science: 400::Mathematics: 410Physics::Fluid DynamicsTransverse planeDARCY-BÉNARD PROBLEMHeat transferMETHOD OF WEIGHTED RESIDUALSRECTANGULAR CHANNELLongitudinal waveLinear stability
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Per una critica dell’art. 319-quater c.p. Una terza via tra concussione e corruzione

2013

L’introduzione dell’art. 319-quater mira a risolvere i problemi storicamente po-sti dalla distinzione tra corruzione e concussione. Pur sorretta da uno spunto condivisibile, quella disposizione, per il modo in cui è concretamente concepita, finisce tuttavia per solle-vare un novero di questioni fors’anche superiore rispetto a quelle che contribuisce a risolve-re. Gli stessi problemi si sarebbero potuti assai più agevolmente risolvere, già in vigenza del precedente sistema, sol che si fosse accettato di superare il dogma della mutua esclusività di quelle due fattispecie.

CorruptionInduzione indebita a dare o a promettere utilità (art. 319-quater c.p.)ExtortionBribery in the public sectorConcussioneCorruzioneSettore IUS/17 - Diritto PenaleL. 6 novembre 2012 n. 190
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Search for topological defect dark matter with a global network of optical magnetometers

2021

Ultralight bosons such as axion-like particles are viable candidates for dark matter. They can form stable, macroscopic field configurations in the form of topological defects that could concentrate the dark matter density into many distinct, compact spatial regions that are small compared with the Galaxy but much larger than the Earth. Here we report the results of the search for transient signals from the domain walls of axion-like particles by using the global network of optical magnetometers for exotic (GNOME) physics searches. We search the data, consisting of correlated measurements from optical atomic magnetometers located in laboratories all over the world, for patterns of signals p…

Cosmology and Nongalactic Astrophysics (astro-ph.CO)010308 nuclear & particles physicsAtomic Physics (physics.atom-ph)Particle physicsGeneral Physics and AstronomyFOS: Physical sciences53001 natural sciencesArticleHigh Energy Physics - ExperimentPhysics - Atomic PhysicsHigh Energy Physics - Experiment (hep-ex)0103 physical sciencesDark energy and dark matterddc:530Atomic and molecular physics010306 general physicsAstrophysics - Cosmology and Nongalactic Astrophysics
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Radio data and synchrotron emission in consistent cosmic ray models

2011

It is well established that phenomenological two-zone diffusion models of the galactic halo can very well reproduce cosmic-ray nuclear data and the observed antiproton flux. Here, we consider lepton propagation in such models and compute the expected galactic population of electrons, as well as the diffuse synchrotron emission that results from their interaction with galactic magnetic fields. We find models in agreement not only with cosmic ray data but also with radio surveys at essentially all frequencies. Requiring such a globally consistent description strongly disfavors very large ($L\gtrsim 15$ kpc) and, even stronger, small ($L\lesssim 1$ kpc) effective diffusive halo sizes. This has…

Cosmology and Nongalactic Astrophysics (astro-ph.CO)Astrophysics::High Energy Astrophysical PhenomenaPopulationDark matterFOS: Physical sciencesSynchrotron radiationCosmic rayAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciencesGalactic haloHigh Energy Physics - Phenomenology (hep-ph)0103 physical scienceseducation010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsPhysicseducation.field_of_studydark matter theorycosmic ray theory; dark matter theory010308 nuclear & particles physicsAstronomy and Astrophysicscosmic ray theoryAstrophysics - Astrophysics of GalaxiesHigh Energy Physics - PhenomenologyAntiprotonAstrophysics of Galaxies (astro-ph.GA)HaloAstrophysics - Cosmology and Nongalactic AstrophysicsRadio waveJournal of Cosmology and Astroparticle Physics
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Stochastic fluctuations of bosonic dark matter

2021

Numerous theories extending beyond the standard model of particle physics predict the existence of bosons that could constitute the dark matter (DM) permeating the universe. In the standard halo model (SHM) of galactic dark matter the velocity distribution of the bosonic DM field defines a characteristic coherence time $\tau_c$. Until recently, laboratory experiments searching for bosonic DM fields have been in the regime where the measurement time $T$ significantly exceeds $\tau_c$, so null results have been interpreted as constraints on the coupling of bosonic DM to standard model particles with a bosonic DM field amplitude $\Phi_0$ fixed by the average local DM density. However, motivate…

Cosmology and Nongalactic Astrophysics (astro-ph.CO)Atomic Physics (physics.atom-ph)530 PhysicsScienceQFOS: Physical sciences500Astrophysics::Cosmology and Extragalactic Astrophysics530 PhysikCharacterization and analytical techniquesArticlePhysics - Atomic PhysicsHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Dark energy and dark matterddc:500Astrophysics - Cosmology and Nongalactic AstrophysicsNature Communications
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Real- and redshift-space halo clustering in $f(R)$ cosmologies

2016

We present two-point correlation function statistics of the mass and the halos in the chameleon $f(R)$ modified gravity scenario using a series of large volume N-body simulations. Three distinct variations of $f(R)$ are considered (F4, F5 and F6) and compared to a fiducial $\Lambda$CDM model in the redshift range $z \in [0,1]$. We find that the matter clustering is indistinguishable for all models except for F4, which shows a significantly steeper slope. The ratio of the redshift- to real-space correlation function at scales $> 20 h^{-1} \mathrm{Mpc}$ agrees with the linear General Relativity (GR) Kaiser formula for the viable $f(R)$ models considered. We consider three halo populations cha…

Cosmology and Nongalactic Astrophysics (astro-ph.CO)Cold dark matterDark matterFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysicsdark energy [cosmology]Correlation function (astronomy)ST/K00042X/101 natural sciencesST/H008519/10103 physical sciencesHalo effectdata analysis [methods]010303 astronomy & astrophysicsSTFCGalaxy clusterAstrophysics::Galaxy Astrophysicslarge-scale structure of Universe [cosmology]Physicstheory [cosmology]010308 nuclear & particles physicsRCUKAstronomyAstronomy and AstrophysicsST/K003267/1RedshiftGalaxygravitationSpace and Planetary ScienceHaloST/L00075X/1Astrophysics - Cosmology and Nongalactic Astrophysics
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Cold dark matter plus not-so-clumpy dark relics

2017

Various particle physics models suggest that, besides the (nearly) cold dark matter that accounts for current observations, additional but sub-dominant dark relics might exist. These could be warm, hot, or even contribute as dark radiation. We present here a comprehensive study of two-component dark matter scenarios, where the first component is assumed to be cold, and the second is a non-cold thermal relic. Considering the cases where the non-cold dark matter species could be either a fermion or a boson, we derive consistent upper limits on the non-cold dark relic energy density for a very large range of velocity dispersions, covering the entire range from dark radiation to cold dark matte…

Cosmology and Nongalactic Astrophysics (astro-ph.CO)Cold dark matterMilky WayCosmic microwave backgroundDark matterFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics7. Clean energy01 natural sciencessymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesPlanck010303 astronomy & astrophysicsCondensed Matter::Quantum GasesPhysics010308 nuclear & particles physicsMatter power spectrumAstronomy and AstrophysicsBaryonHigh Energy Physics - Phenomenology13. Climate actionDark radiationsymbolsAstrophysics - Cosmology and Nongalactic Astrophysics
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