Search results for "Cosmology"

showing 10 items of 2905 documents

"Table 1" of "Study of Dimuon Production in Photon-Photon Collisions and Measurement of QED Photon Structure Functions at LEP"

2001

The measured QED photon structure function at Q**2 = 12.5 GeV for the combine SAT and STIC data.

GAMMA GAMMA --> MU+ MU-Electron productionE+ E- --> E+ E- MU+ MU-91.2Astrophysics::Cosmology and Extragalactic AstrophysicsMuon productionF2PhotoproductionE+ E- ScatteringTwo-PhotonStructure FunctionExclusiveHigh Energy Physics::ExperimentPhysics::Atomic PhysicsNuclear ExperimentAstrophysics::Galaxy Astrophysics
researchProduct

The ALHAMBRA survey: reliable morphological catalogue of 22 051 early- and late-type galaxies

2013

Advanced Large Homogeneous Area Medium Band Redshift Astronomical (ALHAMBRA) is photometric survey designed to trace the cosmic evolution and cosmic variance. It covers a large area of ~4 deg2 in eight fields, where seven fields overlap with other surveys, allowing us to have complementary data in other wavelengths. All observations were carried out in 20 continuous, medium band (30 nm width) optical and 3 near-infrared (JHK) bands, providing the precise measurements of photometric redshifts. In addition, morphological classification of galaxies is crucial for any kind of galaxy formation and cosmic evolution studies, providing the information about star formation histories, their environme…

Galaxies: fundamental parametersCosmology and Nongalactic Astrophysics (astro-ph.CO)Galaxies: statisticsFOS: Physical sciencesLibrary scienceAstrophysics::Cosmology and Extragalactic AstrophysicsEuropean Social FundSurveys01 natural sciencesstatistics [Galaxies]0103 physical sciences10. No inequality010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsComputingMilieux_MISCELLANEOUSPhysics[PHYS]Physics [physics]010308 nuclear & particles physicsLate typeAstronomyAstronomy and AstrophysicsSpace and Planetary ScienceResearch councilfundamental parameters [Galaxies]Christian ministry[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Data releaseAstrophysics - Cosmology and Nongalactic AstrophysicsMonthly Notices of the Royal Astronomical Society
researchProduct

The ALHAMBRA survey: An empirical estimation of the cosmic variance for merger fraction studies based on close pairs

2014

[Aims]: Our goal is to estimate empirically the cosmic variance that affects merger fraction studies based on close pairs for the first time. [Methods]: We compute the merger fraction from photometric redshift close pairs with 10 h−1 kpc ≤ rp ≤ 50 h−1 kpc and Δv ≤ 500 km s−1 and measure it in the 48 sub-fields of the ALHAMBRA survey. We study the distribution of the measured merger fractions that follow a log-normal function and estimate the cosmic variance σv as the intrinsic dispersion of the observed distribution. We develop a maximum likelihood estimator to measure a reliable σv and avoid the dispersion due to the observational errors (including the Poisson shot noise term). [Results]: …

Galaxies: fundamental parametersCosmology and Nongalactic Astrophysics (astro-ph.CO)Stellar massGalaxies: statisticsFOS: Physical sciencesAstrophysicsinteractions [Galaxies]Astrophysics::Cosmology and Extragalactic AstrophysicsPoisson distribution01 natural sciencesLuminositysymbols.namesakestatistics [Galaxies]0103 physical sciences010303 astronomy & astrophysicsComputingMilieux_MISCELLANEOUSAstrophysics::Galaxy AstrophysicsPhotometric redshiftPhysics[PHYS]Physics [physics]COSMIC cancer database010308 nuclear & particles physicsAstronomy and AstrophysicsCosmic varianceRedshiftGalaxyGalaxies: interactionsSpace and Planetary Sciencefundamental parameters [Galaxies]symbols[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astrophysics - Cosmology and Nongalactic Astrophysics
researchProduct

SHARDS: A global view of the star formation activity at z~0.84 and z~1.23

2015

et al.

Galaxies: generalAstrofísicaStellar massFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysicsstar formation [Galaxies]Luminosityhigh-redshift [Galaxies]emission lines [Quasars]Stellar evolutionAstrophysics::Galaxy AstrophysicsCosmic dustPhysicsQuasars: emission linesGalaxies: star formationStar formationphotometry [Galaxies]Galaxies: high-redshiftGalaxies: evolutiongeneral [Galaxies]Astronomy and AstrophysicsQuasarGalaxies: photometryevolution [Galaxies]Astrophysics - Astrophysics of GalaxiesRedshiftGalaxyAstronomíaSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)
researchProduct

Evolution of Balmer jump selected galaxies in the ALHAMBRA survey

2016

Extragalactic astronomy.-- et al.

Galaxies: generalAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesevolution [Galaxy]high-redshift [Galaxies]Galactic haloBalmer jump0103 physical sciencesGalaxy formation and evolutionAstrophysics::Solar and Stellar Astrophysicshalo [Galaxy]010303 astronomy & astrophysicsComputingMilieux_MISCELLANEOUSAstrophysics::Galaxy Astrophysics[PHYS]Physics [physics]PhysicsGalaxy: evolution010308 nuclear & particles physicsphotometry [Galaxies]Astrophysics::Instrumentation and Methods for AstrophysicsGalaxies: high-redshiftGalaxies: evolutiongeneral [Galaxies]Astronomy and AstrophysicsGalaxies: photometryevolution [Galaxies]Astrophysics - Astrophysics of GalaxiesGalaxyPhysics::History of PhysicsGalaxy: haloSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astronomy & Astrophysics
researchProduct

The ALHAMBRA survey: accurate merger fractions derived by PDF analysis of photometrically close pairs

2015

[Aims]: Our goal is to develop and test a novel methodology to compute accurate close-pair fractions with photometric redshifts. [Methods]: We improved the currently used methodologies to estimate the merger fraction fm from photometric redshifts by (i) using the full probability distribution functions (PDFs) of the sources in redshift space; (ii) including the variation in the luminosity of the sources with z in both the sample selection and the luminosity ratio constrain; and (iii) splitting individual PDFs into red and blue spectral templates to reliably work with colour selections.We tested the performance of our new methodology with the PDFs provided by the ALHAMBRA photometric survey.…

Galaxies: statisticsmedia_common.quotation_subjectAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsEuropean Social Fundinteractions [Galaxies]Public administration01 natural sciencesstatistics [Galaxies]Excellence0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsComputingMilieux_MISCELLANEOUSmedia_commonPhysics[PHYS]Physics [physics]Government010308 nuclear & particles physicsGalaxies: evolutionAstronomy and Astrophysicsevolution [Galaxies]Galaxies: interactionsWork (electrical)Space and Planetary ScienceResearch council[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
researchProduct

Sensitivity of the Cherenkov Telescope Array for probing cosmology and fundamental physics with gamma-ray propagation

2021

Full list of authors: Abdalla, H.; Abe, H.; Acero, F.; Acharyya, A.; Adam, R.; Agudo, I; Aguirre-Santaella, A.; Alfaro, R.; Alfaro, J.; Alispach, C.; Aloisio, R.; Batista, R. Alves; Amati, L.; Amato, E.; Ambrosi, G.; Anguner, E. O.; Araudo, A.; Armstrong, T.; Arqueros, F.; Arrabito, L.; Asano, K.; Ascasibar, Y.; Ashley, M.; Backes, M.; Balazs, C.; Balbo, M.; Balmaverde, B.; Baquero Larriva, A.; Martins, V. Barbosa; Barkov, M.; Baroncelli, L.; de Almeida, U. Barres; Barrio, J. A.; Batista, P-, I; Becerra Gonzalez, J.; Becherini, Y.; Beck, G.; Tjus, J. Becker; Belmont, R.; Benbow, W.; Bernardini, E.; Berti, A.; Berton, M.; Bertucci, B.; Beshley, V; Bi, B.; Biasuzzi, B.; Biland, A.; Bissaldi, …

Gamma ray AstronomyCherenkov Telescope ArrayaxionsMATÉRIA ESCURAredshift: dependenceAstronomyGamma ray experimentsgamma ray experimentsAstrophysics01 natural sciencesCosmologyObservatorycosmological model: parameter spacegamma ray experimentHigh Energy Astrophysical Phenomena (astro-ph.HE)astro-ph.HEPhysicsCherenkov telescopes ; IACT technique ; Gamma rays ; Cosmic raysnew physics4. EducationSettore FIS/01 - Fisica SperimentaleAstrophysics::Instrumentation and Methods for AstrophysicsGamma-ray astronomyviolation: Lorentz3. Good healthobservatoryExtragalactic background lightastro-ph.COaxion-like particlesFísica nuclearAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Cosmology and Nongalactic Astrophysicsgamma ray: propagationCosmology and Nongalactic Astrophysics (astro-ph.CO)Active galactic nucleusAxionsAstrophysics::High Energy Astrophysical PhenomenaDark matterFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysicsinvariance: Lorentzjet: relativisticdark matter: halo0103 physical sciencesactive galactic nuclei; gamma ray experiments; axions; extragalactic magnetic fieldsAGNBlazarbackground010308 nuclear & particles physicsFísicaAstronomy and AstrophysicssensitivityCherenkov Telescope Arrayaxionextragalactic magnetic fieldsactive galactic nuclei[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]absorptionstatisticalBlazarsTelescopes
researchProduct

Approximation Algorithms for Multicoloring Planar Graphs and Powers of Square and Triangular Meshes

2006

A multicoloring of a weighted graph G is an assignment of sets of colors to the vertices of G so that two adjacent vertices receive two disjoint sets of colors. A multicoloring problem on G is to find a multicoloring of G. In particular, we are interested in a minimum multicoloring that uses the least total number of colors. The main focus of this work is to obtain upper bounds on the weighted chromatic number of some classes of graphs in terms of the weighted clique number. We first propose an 11/6-approximation algorithm for multicoloring any weighted planar graph. We then study the multicoloring problem on powers of square and triangular meshes. Among other results, we show that the infi…

General Computer SciencePower graphAstrophysics::High Energy Astrophysical PhenomenaInduced subgraphDisjoint setsAstrophysics::Cosmology and Extragalactic Astrophysics[INFO.INFO-DM]Computer Science [cs]/Discrete Mathematics [cs.DM]Theoretical Computer ScienceCombinatoricssymbols.namesakeTriangle meshGreedy algorithmDiscrete Mathematics and CombinatoricsAstrophysics::Solar and Stellar AstrophysicsColoringPolygon meshProduct graphMathematicsComputingMethodologies_COMPUTERGRAPHICSDiscrete mathematicsGreedy algorithm.lcsh:MathematicsApproximation algorithmGraph theory[ INFO.INFO-DM ] Computer Science [cs]/Discrete Mathematics [cs.DM]Cartesian productlcsh:QA1-939Approximation algorithmPlanar graphGraph theory[INFO.INFO-DM] Computer Science [cs]/Discrete Mathematics [cs.DM]symbolsMulticoloring
researchProduct

Spacetime curvature and Higgs stability after inflation

2015

We investigate the dynamics of the Higgs field at the end of inflation in the minimal scenario consisting of an inflaton field coupled to the Standard Model only through the non-minimal gravitational coupling $\xi$ of the Higgs field. Such a coupling is required by renormalisation of the Standard Model in curved space, and in the current scenario also by vacuum stability during high-scale inflation. We find that for $\xi\gtrsim 1$, rapidly changing spacetime curvature at the end of inflation leads to significant production of Higgs particles, potentially triggering a transition to a negative-energy Planck scale vacuum state and causing an immediate collapse of the Universe.

General PhysicsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)spacetime curvaturePhysics MultidisciplinaryVacuum stateFOS: Physical sciencesGeneral Physics and Astronomy01 natural sciences09 Engineeringrenormalizationvacuum stateStandard ModelGravitationGeneral Relativity and Quantum CosmologyHigh Energy Physics - Phenomenology (hep-ph)vacuum stability0103 physical sciencesPARTICLE-PRODUCTIONELECTROWEAK VACUUMHiggs fieldHiggs particles010306 general physics01 Mathematical SciencesPlanck scalePhysicsInflation (cosmology)Science & Technology02 Physical SciencesQuantum field theory in curved spacetimeta114010308 nuclear & particles physicsPhysicsHigh Energy Physics::Phenomenologyhep-phInflatonFIELDSThe Standard ModelCREATIONHiggs fieldHigh Energy Physics - PhenomenologyPhysical Sciencesastro-ph.COHiggs bosonAstrophysics - Cosmology and Nongalactic Astrophysics
researchProduct

Weak-field regime of the generalized hybrid metric-Palatini gravity

2021

In this work we explore the dynamics of the generalized hybrid metric-Palatini theory of gravity in the weak-field, slow-motion regime. We start by introducing the equivalent scalar-tensor representation of the theory, which contains two scalar degrees of freedom, and perform a conformal transformation to the Einstein frame. Linear perturbations of the metric in a Minkowskian background are then studied for the metric and both scalar fields. The effective Newton constant and the PPN parameter $\gamma$ of the theory are extracted after transforming back to the (original) Jordan frame. Two particular cases where the general method ceases to be applicable are approached separately. A compariso…

General Relativity and Quantum Cosmology010308 nuclear & particles physics0103 physical sciencesFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)16. Peace & justice010306 general physics01 natural sciencesGeneral Relativity and Quantum Cosmology
researchProduct