Search results for "background"

showing 10 items of 556 documents

Search for Tensor, Vector, and Scalar Polarizations in the Stochastic Gravitational-Wave Background

2018

The detection of gravitational waves with Advanced LIGO and Advanced Virgo has enabled novel tests of general relativity, including direct study of the polarization of gravitational waves. While general relativity allows for only two tensor gravitational-wave polarizations, general metric theories can additionally predict two vector and two scalar polarizations. The polarization of gravitational waves is encoded in the spectral shape of the stochastic gravitational-wave background, formed by the superposition of cosmological and individually-unresolved astrophysical sources. Using data recorded by Advanced LIGO during its first observing run, we search for a stochastic background of generic…

AstronomyTestingdetectionGeneral Physics and AstronomyEFFICIENTTESTING RELATIVISTIC GRAVITYTensorsSpectral shapes01 natural sciencesGeneral Relativity and Quantum CosmologyGravitational wave backgroundEnergy densityTOOLQCComputingMilieux_MISCELLANEOUSstochastic modelMathematical physicsQBPhysics[PHYS]Physics [physics]Stochastic systemsGravitational effectsarticleVectorsPolarization (waves)gravitational wavesastro-ph.CO[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Astrophysics - Cosmology and Nongalactic AstrophysicsGeneral RelativityCosmology and Nongalactic Astrophysics (astro-ph.CO)General relativitygr-qcFOS: Physical sciencesexperimental studies of gravityGeneral Relativity and Quantum Cosmology (gr-qc)Gravity wavesRelativityReference frequencyPhysics and Astronomy (all)General Relativity and Quantum CosmologyTheory of relativityScalar modesTests of general relativity0103 physical sciencesAdvanced LIGOddc:530Tensor010306 general physicsSTFCGravitational Wavespolarization010308 nuclear & particles physicsGravitational waveRCUKAstrophysical sourcesLIGOPhysics and AstronomygravitationRADIATIONStochastic BackgroundDewey Decimal Classification::500 | Naturwissenschaften::530 | Physik[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]cosmologyGravitational Waves Stochastic Background Advanced LIGO
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Coupled dark matter-dark energy in light of near Universe observations

2010

Cosmological analysis based on currently available observations are unable to rule out a sizeable coupling among the dark energy and dark matter fluids. We explore a variety of coupled dark matter-dark energy models, which satisfy cosmic microwave background constraints, in light of low redshift and near universe observations. We illustrate the phenomenology of different classes of dark coupling models, paying particular attention in distinguishing between effects that appear only on the expansion history and those that appear in the growth of structure. We find that while a broad class of dark coupling models are effectively models where general relativity (GR) is modified - and thus can b…

Astrophysics and AstronomyCosmology and Nongalactic Astrophysics (astro-ph.CO)General relativityCosmic microwave backgroundDark matterFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsEnergia fosca (Astronomia)01 natural sciencesRedshift-space distortionssymbols.namesake0103 physical sciencesDark energy (Astronomy)010303 astronomy & astrophysicsPhysicsCosmologia010308 nuclear & particles physicsAstronomy and AstrophysicsGalaxyRedshiftCosmologyDark matter (Astronomy)symbolsDark energyMatèria fosca (Astronomia)Astrophysics - Cosmology and Nongalactic AstrophysicsHubble's law
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Cosmological lepton asymmetry with a nonzero mixing angle \theta13

2012

While the baryon asymmetry of the Universe is nowadays well measured by cosmological observations, the bounds on the lepton asymmetry in the form of neutrinos are still significantly weaker. We place limits on the relic neutrino asymmetries using some of the latest cosmological data, taking into account the effect of flavor oscillations. We present our results for two different values of the neutrino mixing angle \theta_{13}, and show that for large \theta_{13} the limits on the total neutrino asymmetry become more stringent, diluting even large initial flavor asymmetries. In particular, we find that the present bounds are still dominated by the limits coming from Big Bang Nucleosynthesis, …

Astrophysics and AstronomyNuclear and High Energy PhysicsParticle physicsmedia_common.quotation_subjectCosmic microwave backgroundCosmic background radiationAstrophysics::Cosmology and Extragalactic AstrophysicsEarly Universe7. Clean energy01 natural sciencesAsymmetryPartícules (Física nuclear)CosmologyBaryon asymmetryBig Bang nucleosynthesisPower Spectrum0103 physical sciences010306 general physicsTelescopemedia_commonPhysicsFlavor Oscillations010308 nuclear & particles physicsHigh Energy Physics::Phenomenology[PHYS.HPHE] Physics [physics]/High Energy Physics - Phenomenology [hep-ph]High Energy Physics - Phenomenology[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]ConstraintsParametersNeutrino DegeneracyHigh Energy Physics::ExperimentNeutrinoAstrophysics - Cosmology and Nongalactic AstrophysicsLepton
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Cosmological analogies in the search for new physics in high-energy collisions

2020

In this paper, analogies between multiparticle production in high-energy collisions and the time evolution of the early universe are discussed. A common explanation is put forward under the assumption of an unconventional early state: a rapidly expanding universe before recombination (last scattering surface), followed by the CMB, later evolving up to present days, versus the formation of hidden/dark states in hadronic collisions followed by a conventional QCD parton shower yielding final-state particles. In particular, long-range angular correlations are considered pointing out deep connections between the two physical cases potentially useful for the discovery of new physics.

Astrophysics and AstronomyParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Physics beyond the Standard Modelmedia_common.quotation_subjectCosmic microwave backgroundFOS: Physical sciences01 natural sciencesMetric expansion of spaceHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesNuclear Experiment010306 general physicsParton showerParticle Physics - Phenomenologymedia_commonPhysicsQuantum chromodynamics010308 nuclear & particles physicsScatteringTime evolutionhep-phUniverseHigh Energy Physics - Phenomenologyastro-ph.COAstrophysics - Cosmology and Nongalactic Astrophysics
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Comparison of gamma-ray coincidence and low-background gamma-ray singles spectrometry

2011

Aerosol samples have been studied under different background conditions using gamma-ray coincidence and low-background gamma-ray singles spectrometric techniques with High-Purity Germanium detectors. Conventional low-background gamma-ray singles counting is a competitive technique when compared to the gamma-gamma coincidence approach in elevated background conditions. However, measurement of gamma-gamma coincidences can clearly make the identification of different nuclides more reliable and efficient than using singles spectrometry alone. The optimum solution would be a low-background counting station capable of both singles and gamma-gamma coincidence spectrometry.

Astrophysics::High Energy Astrophysical Phenomena[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]010403 inorganic & nuclear chemistryMass spectrometry01 natural sciencesComprehensive Nuclear-Test-Ban TreatyCoincidence030218 nuclear medicine & medical imagingNuclear physics03 medical and health sciences0302 clinical medicineBackground RadiationAir Pollution RadioactiveNuclideGamma ray spectrometryBackground radiationNuclear PhysicsPhysicsAerosolsRadiation surveillanceRadiationta114GermaniumGamma rayGamma-ray spectrometry0104 chemical sciencesSpectrometry GammaGamma Rays22Na
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TeV gamma-ray survey of the Northern sky using the ARGO-YBJ detector

2013

The ARGO-YBJ detector is an extensive air shower array that has been used to monitor the northern $\gamma$-ray sky at energies above 0.3 TeV from 2007 November to 2013 January. In this paper, we present the results of a sky survey in the declination band from $-10^{\circ}$ to $70^{\circ}$, using data recorded over the past five years. With an integrated sensitivity ranging from 0.24 to $\sim$1 Crab units depending on the declination, six sources have been detected with a statistical significance greater than 5 standard deviations. Several excesses are also reported as potential $\gamma$-ray emitters. The features of each source are presented and discussed. Additionally, $95\%$ confidence le…

Astrophysics::High Energy Astrophysical Phenomenamedia_common.quotation_subjectFOS: Physical sciencesFluxField of viewAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsGamma rays: general – surveys01 natural sciencesDeclination0103 physical sciencesAbsorption (logic)010303 astronomy & astrophysicsmedia_commonHigh Energy Astrophysical Phenomena (astro-ph.HE)Physics010308 nuclear & particles physicsSettore FIS/01 - Fisica SperimentaleAstrophysics::Instrumentation and Methods for AstrophysicsGamma rayAstronomy and Astrophysicsgeneral – su [gamma rays]Air showerExtragalactic background light13. Climate actionSpace and Planetary ScienceSkygeneral – surveys [Gamma rays]Astrophysics - High Energy Astrophysical Phenomena
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Long-term (1995-2018) aerosol optical depth derived using ground based AERONET and SKYNET measurements from aerosol aged-background sites

2019

Abstract We examined long-term aerosol optical depth (AOD) trends over 53 sites across the globe which comprise 49 sites from the Aerosol Robotic Network (AERONET) and 4 sites from the Sky radiometer Network (SKYNET) during 1995–2018. Most of these sites are located in remote and isolated aged-background regions, and few are in urban/semi-urban sites having averaged AOD ∼0.1 at 500 nm. These selected sites have a global distribution including tropical, mid-latitudes, high-latitudes and Polar regions. Among them, there are 14 high-altitude stations (∼1028–5050 m amsl), including Himalayan and Polar regions. The main objective of the present work is to evaluate the AOD trends over the aged-ba…

Atmospheric ScienceSKYNETRadiometer010504 meteorology & atmospheric sciencesSKYNETClimate changeAged-background010501 environmental sciences01 natural sciencesPollutionAerosol optical depthAnthropogenicAerosolAERONETArctic13. Climate actionGlobal distributionClimatologyEnvironmental scienceSatelliteWaste Management and DisposalAERONET0105 earth and related environmental sciences
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Fluorescence-Based Screening of Cytochrome P450 Activities in Intact Cells

2013

Fluorimetric methods to assess cytochrome P450 (P450) activities that do not require metabolite separation have been developed. These methods make use of non- or low-fluorescent P450 substrates that produce highly fluorescent metabolites in aqueous solutions. The assays are based on the direct incubation of intact cells in culture with appropriate fluorogenic probe substrates, followed by fluorimetric quantification of the product formed and released into incubation medium. We describe a battery of fluorescence assays for rapid measurement of the activity of nine P450s involved in drug metabolism. For each individual P450 activity the probe showing the best properties (highest metabolic rat…

Background fluorescencechemistry.chemical_compoundChromatographychemistrybiologyMetabolitebiology.proteinCytochrome P450IncubationFluorescenceDrug metabolismHighly sensitive
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Coupled-cluster techniques for computational chemistry: The CFOUR program package

2020

An up-to-date overview of the CFOUR program system is given. After providing a brief outline of the evolution of the program since its inception in 1989, a comprehensive presentation is given of its well-known capabilities for high-level coupled-cluster theory and its application to molecular properties. Subsequent to this generally well-known background information, much of the remaining content focuses on lesser-known capabilities of CFOUR, most of which have become available to the public only recently or will become available in the near future. Each of these new features is illustrated by a representative example, with additional discussion targeted to educating users as to classes of …

Background information010304 chemical physicsComputer sciencemedia_common.quotation_subjectGeneral Physics and Astronomy010402 general chemistry01 natural sciencesData science0104 chemical sciencesPresentationCoupled cluster0103 physical sciencesPhysical and Theoretical ChemistrySpeculationmedia_common
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Consumer texture preferences: Effect of age, gender and previous experience

2000

Four different strawberry candies with varying thickening agents (pectin, gelatin, starch, and gelatin + starch) were rated by three consumer age groups: teenagers (13–14 years), young adults (19–23 years) and the middle-aged (40–63 years) (n = 60 in each group). Age, gender, use frequencies and hedonic ratings often commercial candy types were collected as background information. Four preference groups were found by using preference mapping. The most important factor predicting preference of a sample were hedonic evaluations of commercial candies whose texture was similar to that of the test sample. If the consumers gave high hedonic ratings to one sample they also tended to report liking …

Background information0303 health sciences030309 nutrition & dietetics[SDV]Life Sciences [q-bio]Preference mappingPharmaceutical Science04 agricultural and veterinary sciencesTexture (music)040401 food sciencePreferenceAge and gender[SDV] Life Sciences [q-bio]03 medical and health sciences0404 agricultural biotechnologyAge groupsThickeningPsychologyTest sampleComputingMilieux_MISCELLANEOUSFood ScienceDemography
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