Search results for "background"

showing 10 items of 556 documents

Cosmic microwave background constraints on secret interactions among sterile neutrinos

2017

Secret contact interactions among eV sterile neutrinos, mediated by a massive gauge boson $X$ (with $M_X \ll M_W$), and characterized by a gauge coupling $g_X$, have been proposed as a mean to reconcile cosmological observations and short-baseline laboratory anomalies. We constrain this scenario using the latest Planck data on Cosmic Microwave Background anisotropies, and measurements of baryon acoustic oscillations (BAO). We consistently include the effect of secret interactions on cosmological perturbations, namely the increased density and pressure fluctuations in the neutrino fluid, and still find a severe tension between the secret interaction framework and cosmology. In fact, taking i…

Sterile neutrinoParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)cosmological neutrinosDark matterCosmic microwave backgroundFOS: Physical sciencescosmological neutrinos; cosmological parameters from CMBR; neutrino masses from cosmology; neutrino properties; Astronomy and AstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesNOsymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesPlanck010303 astronomy & astrophysicsneutrino propertiesPhysicsGauge bosoncosmological neutrino010308 nuclear & particles physicsHigh Energy Physics::Phenomenologycosmological parameters from CMBRAstronomy and Astrophysicsneutrino masses from cosmologyCoupling (probability)3. Good healthHigh Energy Physics - Phenomenology13. Climate actionsymbolsHigh Energy Physics::ExperimentBaryon acoustic oscillationsNeutrinoAstrophysics - Cosmology and Nongalactic Astrophysics
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Revisiting cosmological bounds on sterile neutrinos

2014

We employ state-of-the art cosmological observables including supernova surveys and BAO information to provide constraints on the mass and mixing angle of a non-resonantly produced sterile neutrino species, showing that cosmology can effectively rule out sterile neutrinos which decay between BBN and the present day. The decoupling of an additional heavy neutrino species can modify the time dependence of the Universe's expansion between BBN and recombination and, in extreme cases, lead to an additional matter-dominated period; while this could naively lead to a younger Universe with a larger Hubble parameter, it could later be compensated by the extra radiation expected in the form of neutri…

Sterile neutrinoParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)media_common.quotation_subjectCosmic microwave backgroundCosmic background radiationFOS: Physical sciencesNeutrino decouplingAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencessymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciences010306 general physicsmedia_commonPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyFísicaAstronomy and Astrophysicshep-phUniverseHigh Energy Physics - Phenomenology13. Climate actionsymbolsastro-ph.COHigh Energy Physics::ExperimentBaryon acoustic oscillationsNeutrinoHubble's lawAstrophysics - Cosmology and Nongalactic Astrophysics
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Recent Borexino results and prospects for the near future

2015

The Borexino experiment, located in the Gran Sasso National Laboratory, is an organic liquid scintillator detector conceived for the real time spectroscopy of low energy solar neutrinos. The data taking campaign phase I (2007 - 2010) has allowed the first independent measurements of 7Be, 8B and pep fluxes as well as the first measurement of anti-neutrinos from the earth. After a purification of the scintillator, Borexino is now in phase II since 2011. We review here the recent results achieved during 2013, concerning the seasonal modulation in the 7Be signal, the study of cosmogenic backgrounds and the updated measurement of geo-neutrinos. We also review the upcoming measurements from phase…

Sterile neutrinoPhysics - Instrumentation and Detectorsneutrino: solarPhysics::Instrumentation and DetectorsSolar neutrinoQC1-999Astrophysics::High Energy Astrophysical Phenomenascintillation counter: liquidFOS: Physical sciencesScintillator53001 natural sciences7. Clean energyHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)Physics and Astronomy (all)Low energy[ PHYS.HEXP ] Physics [physics]/High Energy Physics - Experiment [hep-ex]0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]ddc:530[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physics[ PHYS.PHYS.PHYS-INS-DET ] Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]BorexinoPhysics010308 nuclear & particles physicsneutrino: energy: lowgeophysicsbackgroundPhysicsDetectorneutrino: flux: measuredHigh Energy Physics::PhenomenologyInstrumentation and Detectors (physics.ins-det)neutrino: particle sourceneutrino: sterileantineutrinoGran SassoNEUTRINOS13. Climate actionBorexinoHigh Energy Physics::ExperimentNeutrinoNational laboratory
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Cosmological origin of anomalous radio background

2012

The ARCADE 2 collaboration has reported a significant excess in the isotropic radio background, whose homogeneity cannot be reconciled with clustered sources. This suggests a cosmological origin prior to structure formation. We investigate several potential mechanisms and show that injection of relativistic electrons through late decays of a metastable particle can give rise to the observed excess radio spectrum through synchrotron emission. However, constraints from the cosmic microwave background (CMB) anisotropy, on injection of charged particles and on the primordial magnetic field, present a challenge. The simplest scenario is with a greater than or similar to 9 GeV particle decaying i…

Structure formationCosmology and Nongalactic Astrophysics (astro-ph.CO)Astrophysics::High Energy Astrophysical PhenomenaDark matterCosmic microwave backgroundCosmic background radiationFOS: Physical sciencesAstrophysicsElectronAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesParticle decayHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciences010303 astronomy & astrophysicsPhysicsdark matter theory010308 nuclear & particles physicsFísicaAstronomy and AstrophysicsCosmology of Theories beyond the SMRedshiftCharged particleHigh Energy Physics - Phenomenologyextragalactic magnetic fieldsAstrophysics - Cosmology and Nongalactic Astrophysics
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Late decaying 2-component dark matter scenario as an explanation of the AMS-02 positron excess

2016

The long standing anomaly in the positron flux as measured by the PAMELA and AMS-02 experiments could potentially be explained by dark matter (DM) annihilations. This scenario typically requires a large "boost factor" to be consistent with a thermal relic dark matter candidate produced via freeze-out. However, such an explanation is disfavored by constraints from CMB observations on energy deposition during the epoch of recombination. We discuss a scenario called late-decaying two-component dark matter (LD2DM), where the entire DM consists of two semi-degenerate species. Within this framework, the heavier species is produced as a thermal relic in the early universe and decays to the lighter…

Structure formationCosmology and Nongalactic Astrophysics (astro-ph.CO)Satellitesmedia_common.quotation_subjectPhysics beyond the Standard ModelCosmic microwave backgroundDark matterCosmic background radiationFOS: Physical sciencesAnnihilationAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsDark Matter TheoryGalactic Cosmic-Rays01 natural sciencesCosmic Ray ExperimentsParticle Physics - Cosmology ConnectionHigh Energy Physics - Phenomenology (hep-ph)AbundanceReionization0103 physical sciencesGamma010303 astronomy & astrophysicsmedia_commonPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Annihilation010308 nuclear & particles physicsAstronomy and AstrophysicsGalaxiesUniverseHaloesHigh Energy Physics - PhenomenologySolar ModulationConstraintsDark AgesMinimumAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Cosmology and Nongalactic AstrophysicsIndraStra Global
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Some past and present challenges of econophysics

2016

We discuss the cultural background that was shared by some of the first econophysicists when they started to work on economic and financial problems with methods and tools of statistical physics. In particular we discuss about the role of stylized facts and statistical physical laws in economics and statistical physics respectively. As an example of the problems and potentials associated with the interaction of different communities of scholars dealing with problems observed in economic and financial systems we briefly discuss the development and the perspectives of the use of tools and concepts of networks in econophysics, economics and finance.

Stylized factEconophysicsGeneral Physics and AstronomyStatistical finance01 natural sciences010305 fluids & plasmasCultural backgroundPhysics and Astronomy (all)Work (electrical)0103 physical sciencesEconomicsGeneral Materials ScienceMaterials Science (all)Positive economicsPhysical and Theoretical Chemistry010306 general physicsPhysical law
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La Llegenda del cor menjat al Decameró de Boccaccio: Estratègies de traducció al català

2013

Resum: El grau d’intervencio del traductor determina l’acostament del text al lector. Amb la comparacio de les quatre traduccions catalanes de La llegenda del cor menjat , el conte nove de la quarta jornada del Decamero de Giovanni Boccaccio, es pot comprovar que cada traductor utilitza estrategies diferents per mirar de resoldre un mateix problema de traduccio. A mes del bagatge cultural i la subjectivitat de cada un d’ells, cal tenir en compte un seguit de factors (temporals, historics, referencials, lingu?istics, socials, etc.) que determinen el resultat final. Paraules clau: llegenda; cor; menjat; Decamero ; Boccaccio; estrategia de traduccio Abstract: The extent to which translators in…

SubjectivityHistoryLiterature and Literary Theorymedia_common.quotation_subjectlcsh:Literature (General)lcsh:D111-203lcsh:Medieval historyBoccacciomenjatArtlcsh:PN1-6790LegendLanguage and Linguisticslanguage.human_languageCultural backgroundestratègia de traduccióllegendadecameronlcsh:D204-475languagecorCatalanHumanitieslcsh:Modern history 1453-media_common
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The Social Background of Treasure Hunters

2012

We have already referred to the treasure hunt in Westminster Abbey. The organizer and initiator of this venture was Davey Ramsey, the clock- maker of King James I and his successor. Some of his works are now in the British Museum. Ramsey had some financial difficulties but he was well-connected at court. We mentioned in Chapter 6 that he managed to receive royal permits to search for treasure in 1628 and in 1635. Nothing seems to have come of these enterprises. In the winter of 1632/33, he received a permit from the Dean of Westminster to search for treasure in the cloister of the abbey. Ramsey did not undertake the hunt alone. He mustered the support of William Lilly, the renowned London a…

Successor cardinalSocial backgroundEvil spiritNothingmedia_common.quotation_subjectCloisterCuriosityGender studiesArtTreasureClassicsmedia_common
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Fast simulation of muons produced at the SHiP experiment using Generative Adversarial Networks

2019

This paper presents a fast approach to simulating muons produced in interactions of the SPS proton beams with the target of the SHiP experiment. The SHiP experiment will be able to search for new long-lived particles produced in a 400~GeV$/c$ SPS proton beam dump and which travel distances between fifty metres and tens of kilometers. The SHiP detector needs to operate under ultra-low background conditions and requires large simulated samples of muon induced background processes. Through the use of Generative Adversarial Networks it is possible to emulate the simulation of the interaction of 400~GeV$/c$ proton beams with the SHiP target, an otherwise computationally intensive process. For th…

TechnologyPhysics - Instrumentation and DetectorsProtonPhysics::Instrumentation and DetectorsComputer sciencebackground: inducedNuclear TheoryDetector modelling and simulations I (interaction of radiation with matter interaction of photons with matter interaction of hadrons with matter etc); Simulation methods and programs01 natural sciences09 EngineeringHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]muon: momentumDetectors and Experimental TechniquesNuclear Experimentphysics.ins-detGeneralLiterature_REFERENCE(e.g.dictionariesencyclopediasglossaries)InstrumentationInstruments & InstrumentationMathematical PhysicsDetector modelling and simulations I (interaction of radiation with matter interaction of photons with matter interaction of hadrons with matter etc)02 Physical Sciencesinteraction of photons with matterInstrumentation and Detectors (physics.ins-det)p: beammuon: productionDetector modelling and simulations INuclear & Particles Physicsinteraction of hadrons with matterParticle Physics - Experimentperformancedata analysis methodDetector modelling and simulations I (interaction of radiation with matterFOS: Physical sciencesAccelerator Physics and Instrumentation0103 physical sciencesnumerical methodsddc:610[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Aerospace engineering010306 general physicsnumerical calculationsetc)MuonScience & Technologyhep-ex010308 nuclear & particles physicsbusiness.industryNumerical analysisAcceleratorfysik och instrumenteringCERN SPSPhysics::Accelerator PhysicsHigh Energy Physics::ExperimentSimulation methods and programsbusinessGenerative grammar
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The experimental facility for the Search for Hidden Particles at the CERN SPS

2019

The Search for Hidden Particles (SHiP) Collaboration has shown that the CERN SPS accelerator with its 400 $\mathrm{\small GeV/c}$ proton beam offers a unique opportunity to explore the Hidden Sector. The proposed experiment is an intensity frontier experiment which is capable of searching for hidden particles through both visible decays and through scattering signatures from recoil of electrons or nuclei. The high-intensity experimental facility developed by the SHiP collaboration is based on a number of key features and developments which provide the possibility of probing a large part of the parameter space for a wide range of models with light long-lived superweakly interacting particles…

TechnologyPhysics - Instrumentation and Detectorsbackground: inducedlarge detector systems for particle and astroparticle physicsSPSbeam transportElectron7. Clean energy01 natural sciences09 Engineeringdark matter detectors (wimps axions etc.)High Energy Physics - Experiment030218 nuclear medicine & medical imaginglaw.inventionNeutrino detectorHigh Energy Physics - Experiment (hep-ex)0302 clinical medicineRecoillawetc.)[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Neutrino detectorsDetectors and Experimental TechniquesNuclear Experimentphysics.ins-detInstruments & InstrumentationInstrumentationbackground: suppressionMathematical Physicsnucleus: recoilPhysicsRange (particle radiation)tau neutrino02 Physical SciencesLarge Hadron Colliderbeam lossInstrumentation and Detectors (physics.ins-det)p: beamNuclear & Particles Physicsvacuum systemparticle: interactionDark Matter detectors (WIMPbeam opticsNeutrino detectorp: beam dumpPhysics - Instrumentation and Detectorproposed experimentParticle Physics - Experimentzirconium: admixtureFOS: Physical sciencesAccelerator Physics and Instrumentationbeam: ejectionp: targetHidden SectorNuclear physicsKKKK: SHiP03 medical and health sciences0103 physical sciences[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Beam dumpnumerical calculationsmuon: shieldingdetector: designactivity reportDark Matter detectors (WIMPsScience & Technologyhep-ex010308 nuclear & particles physicsLarge detector systems for particle and astroparticle physicsbeam-dump facilityAcceleratorfysik och instrumenteringCERN SPSHidden sectoraxionaxions etc.)Large detector systems for particle and astroparticle physicmolybdenum: alloyPhysics::Accelerator Physicstarget: designtitanium: admixtureBeam (structure)neutrino detectors
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