Search results for "matter [quantum chromodynamics]"

showing 10 items of 162 documents

A White Paper on keV sterile neutrino Dark Matter

2017

We present a comprehensive review of keV-scale sterile neutrino Dark Matter, collecting views and insights from all disciplines involved - cosmology, astrophysics, nuclear, and particle physics - in each case viewed from both theoretical and experimental/observational perspectives. After reviewing the role of active neutrinos in particle physics, astrophysics, and cosmology, we focus on sterile neutrinos in the context of the Dark Matter puzzle. Here, we first review the physics motivation for sterile neutrino Dark Matter, based on challenges and tensions in purely cold Dark Matter scenarios. We then round out the discussion by critically summarizing all known constraints on sterile neutrin…

AstrofísicaSterile neutrinocosmological modelCold dark mattercosmological neutrinosPhysics beyond the Standard Model[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]Dark matter theory01 natural sciencesCosmologyHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)White paperHigh Energy Physics - Phenomenology (hep-ph)X-RAY-EMISSIONMETALLIC MAGNETIC CALORIMETERSQUANTUM-FIELD THEORY[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]neutrino: dark matterCosmological neutrinos; Dark matter experiments; Dark matter theory; Particle physics - cosmology connection010303 astronomy & astrophysicsPhysicsdark matter theorynew physicsDOUBLE-BETA-DECAYhep-phneutrino: sterileCosmological neutrinos; Dark matter experiments; Dark matter theory; Particle physics - cosmology connection; Astronomy and AstrophysicsNuclear & Particles PhysicsHigh Energy Physics - Phenomenologyneutrino: detectorDark matter experimentsparticle physics - cosmology connectionastro-ph.COMILKY-WAY SATELLITESCosmological neutrinos3.5 KEV LINENeutrinoParticle Physics - ExperimentAstrophysics - Cosmology and Nongalactic AstrophysicsParticle physicsAstrophysics and AstronomyCosmology and Nongalactic Astrophysics (astro-ph.CO)astro-ph.GADark matterLY-ALPHA FORESTreviewFOS: Physical sciencesContext (language use)neutrino: productionX-raySettore FIS/05 - Astronomia e Astrofisica[ PHYS.HEXP ] Physics [physics]/High Energy Physics - Experiment [hep-ex]RIGHT-HANDED NEUTRINOS0103 physical sciencesAstronomical And Space Sciencesnumerical calculationsDark matter experimentXMM-NEWTON OBSERVATIONSneutrino: modelParticle Physics - PhenomenologyDWARF SPHEROIDAL GALAXYCosmologia010308 nuclear & particles physicshep-exdark matter experimentsHigh Energy Physics::PhenomenologyAstronomy and AstrophysicsAtomic Molecular Nuclear Particle And Plasma PhysicsCosmological neutrinoAstrophysics - Astrophysics of Galaxies13. Climate actionAstrophysics of Galaxies (astro-ph.GA)[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]Particle physics - cosmology connection[ PHYS.HPHE ] Physics [physics]/High Energy Physics - Phenomenology [hep-ph]High Energy Physics::Experimentneutrino: oscillation[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Journal of Cosmology and Astroparticle Physics
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Thinking outside the box: effects of modes larger than the survey on matter power spectrum covariance

2012

Considering the matter power spectrum covariance matrix, it has recently been found that there is a potentially dominant effect on mildly non-linear scales due to power in modes of size equal to and larger than the survey volume. This {\it beat coupling} effect has been derived analytically in perturbation theory and while it has been tested with simulations, some questions remain unanswered. Moreover, there is an additional effect of these large modes, which has so far not been included in analytic studies, namely the effect on the estimated {\it average} density which enters the power spectrum estimate. In this article, we work out analytic, perturbation theory based expressions including…

Astrofísicadark matter simulationsCosmology and GravitationCosmology and Nongalactic Astrophysics (astro-ph.CO)FOS: Physical sciencesBeat (acoustics)Astrophysicspower spectrumAstrophysics01 natural sciences0103 physical sciencesStatistical physics010303 astronomy & astrophysics/dk/atira/pure/core/subjects/cosmologyPhysicsCosmologia010308 nuclear & particles physicsCovariance matrixMatter power spectrumcosmological simulationsSpectral densityFísicaAstronomy and AstrophysicsCovarianceRedshiftGalaxyCosmologyStepping stonegalaxy clusteringAstrophysics - Cosmology and Nongalactic Astrophysics
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High redshift galaxies in the ALHAMBRA survey. II. Strengthening the evidence of bright-end excess in UV luminosity functions at 2.5 <= z<= 4.5 by PD…

2018

Context. Knowing the exact shape of the ultraviolet (UV) luminosity function (LF) of high-redshift galaxies is important to understand the star formation history of the early Universe. However, the uncertainties, especially at the faint and bright ends of the LFs, remain significant. Aims. In this paper, we study the UV LF of redshift z = 2:5 4.5 galaxies in 2.38 deg of ALHAMBRA data with I ≤ 24. Thanks to the large area covered by ALHAMBRA, we particularly constrain the bright end of the LF. We also calculate the cosmic variance and the corresponding bias values for our sample and derive their host dark matter halo masses. Methods.We have used a novel methodology based on redshift and magn…

Astrophysics::High Energy Astrophysical PhenomenaContext (language use)AstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesLuminosityhigh-redshift [Galaxies]galaxies: high-redshift0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsLuminosity function (astronomy)Physics[PHYS]Physics [physics]010308 nuclear & particles physicsStar formationAstronomy and AstrophysicsCosmic varianceevolution [Galaxies]Astrophysics - Astrophysics of Galaxiesluminosity function [Galaxies]RedshiftGalaxyDark matter halogalaxies: luminosity functionSpace and Planetary Sciencemass functionMass functiongalaxies: evolution[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Algunas reflexiones acerca de la stjue de 9 de julio de 2020 sobre los pactos novatorios en materia de cláusulas suelo

2021

The Sentence of the Court of Justice of the European Union of July 9, 2020 comes to answer the five questions that, in its preliminary question, the Court of First Instance and Instruction No. 3 of Teruel asks about the validity of the new agreements in the context of the floor clauses, establishing jurisprudential doctrine on this matter about which our Supreme Court had previously ruled in its Judgments of October 16, 2017, in the sense of considering the agreed floor clause null as a consequence of the novation agreement and, subsequently, those of April 11, 2018 and September 13, 2018 in the opposite direction, declaring that the novation agreement was valid. It is a long-awaited and in…

Carolina del Carmen The Sentence of the Court of Justice of the European Union of July 9and its economic repercussion - as well as its procedural significance. -by the consequence of the lifting of procedural suspensions that its dictation supposes2018 in the opposite direction2017consumidorin its preliminary question2018 and September 13cláusula suelothe Court of First Instance and Instruction No. 3 of Teruel asks about the validity of the new agreements in the context of the floor clausesno doubtpacto novatorioagreed as a result of the ruling of the Luxembourg Court-. In this paper I will review the doctrine contained in the STJUE in its comparison with the one previously declared by our Supreme Courtremunerative interestMortgage:CIENCIAS JURÍDICAS [UNESCO]in attentioninterest variability 132 159consumerestablishing jurisprudential doctrine on this matter about which our Supreme Court had previously ruled in its Judgments of October 16new agreementsubsequentlyboth to its well-founded substantive relevance - due to the legal doctrine that it consolidates and which results from unquestionable applicationvariabilidad del interés.2070-8157 22082 Revista Boliviana de Derecho 565487 2021 31 7730055 Algunas reflexiones acerca de la stjue de 9 de julio de 2020 sobre los pactos novatorios en materia de cláusulas suelo Castillo Martínezdeclaring that the novation agreement was valid. It is a long-awaited and insistently commented resolution after its publication2020 comes to answer the five questions thatthose of April 11in the sense of considering the agreed floor clause null as a consequence of the novation agreement andin order to conclude what its incidence is with respect to the criterion maintained by our High Court in its Judgments of April 11UNESCO::CIENCIAS JURÍDICASfloor clauseinterés remuneratorio2018. Hipoteca
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Soil Carbon, Nitrogen and Phosphorus Dynamics as Affected by Solarization Alone or Combined with Organic Amendment

2006

Soil solarization, alone or combined with organic amendment, is an increasingly attractive approach for managing soil-borne plant pathogens in agricultural soils. Even though it consists in a relatively mild heating treatment, the increased soil temperature may strongly affect soil microbial processes and nutrients dynamics. This study aimed to investigate the impact of solarization, either with or without addition of farmyard manure, in soil dynamics of various C, N and P pools. Changes in total C, N and P contents and in some functionally-related labile pools (soil microbial biomass C and N, K2SO4-extractable C and N, basal respiration, KCl-exchangeable ammonium and nitrate, and water-sol…

ChemistrySoil organic matterSoil biologySettore AGR/13 - Chimica AgrariaBulk soilfood and beveragesSoil ScienceSoil solarizationPlant Sciencecomplex mixturesManureHumusSoil managementAgronomySoil fertilitychloroform fumigation–extraction labile N microbial biomass organic amendment soil organic matter soil solarization water-soluble PPlant and Soil
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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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Controlling Exciton Propagation in Organic Crystals through Strong Coupling to Plasmonic Nanoparticle Arrays.

2022

Exciton transport in most organic materials is based on an incoherent hopping process between neighboring molecules. This process is very slow, setting a limit to the performance of organic optoelectronic devices. In this Article, we overcome the incoherent exciton transport by strongly coupling localized singlet excitations in a tetracene crystal to confined light modes in an array of plasmonic nanoparticles. We image the transport of the resulting exciton–polaritons in Fourier space at various distances from the excitation to directly probe their propagation length as a function of the exciton to photon fraction. Exciton–polaritons with an exciton fraction of 50% show a propagation length…

Condensed Matter::Quantum GasesCondensed Matter::OtherPhysics::Opticsmolecular dynamics simulationspolariton transportfysikaalinen kemiaCondensed Matter::Mesoscopic Systems and Quantum Hall EffectelektronitkvasihiukkasetplasmonicsAtomic and Molecular Physics and Opticsnanoparticle arraytetraceneElectronic Optical and Magnetic MaterialsCondensed Matter::Materials Sciencemolekyylifysiikkaplasmoniikkastrong light-matter couplingeksitonitnanohiukkasetmolekyylidynamiikkaElectrical and Electronic EngineeringBiotechnologyACS photonics
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Elections ordinaires et aménagements constitutionnels

2001

It is widely held that voting in the course of ordinary elections has no significant influence on the constitutional regime or order of a country. At least three powerful arguments are provided in support of that view. First, to claim that, at the same time as they play, players can change the rules is, to say the least, logically puzzling. A second argument refers to the motivations and possibilities of voters : voters, this argument says, are not really interested in constitutional issues and, even if they were, are particularly ill-equiped to understand their implications. The third argument rests on the observation of what obtains in practice : as a matter of fact, constitutional issues…

Constitutional economicsElectionmedia_common.quotation_subjectConstitutionalismDecentralizationEtudes générales. Idéologies.ArgumentPolitical scienceVoting[ SHS.ECO ] Humanities and Social Sciences/Economies and financesTreaty[SHS.ECO] Humanities and Social Sciences/Economics and Financemedia_commonLaw and economicsSociology daily lifePolitical sociology of International RelationsVoterConstitution[SHS.ECO]Humanities and Social Sciences/Economics and FinanceMatter of factConstitutionLawSociologieGeneral Studies. Ideologies.ElecteurSociologie politique
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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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Primordial dark matter from curvature induced symmetry breaking

2020

We demonstrate that adiabatic dark matter can be generated by gravity induced symmetry breaking during inflation. We study a $Z_2$ symmetric scalar singlet that couples to other fields only through gravity and for which the symmetry is broken by the spacetime curvature during inflation when the non-minimal coupling $\xi$ is negative. We find that the symmetry breaking leads to the formation of adiabatic dark matter with the observed abundance for the singlet mass $m\sim{\rm MeV}$ and $|\xi|\sim 1$.

Cosmology and Nongalactic Astrophysics (astro-ph.CO)Dark matterScalar (mathematics)FOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsCurvature01 natural sciences114 Physical sciencessymmetry breakingGeneral Relativity and Quantum Cosmologypimeä aineGeneral Relativity and Quantum CosmologyHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesprimordial dark matterSymmetry breakinginflationAdiabatic processMathematical physicsPhysicsInflation (cosmology)symmetriadark matter theory010308 nuclear & particles physicsAstronomy and AstrophysicsCoupling (probability)Symmetry (physics)quantum field theory on curved spaceHigh Energy Physics - PhenomenologyAstrophysics - Cosmology and Nongalactic Astrophysics
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