0000000000582925

AUTHOR

M. Kümmel

showing 5 related works from this author

Euclid preparation XV. Forecasting cosmological constraints for the Euclid and CMB joint analysis

2022

The combination and cross-correlation of the upcoming $Euclid$ data with cosmic microwave background (CMB) measurements is a source of great expectation since it will provide the largest lever arm of epochs, ranging from recombination to structure formation across the entire past light cone. In this work, we present forecasts for the joint analysis of $Euclid$ and CMB data on the cosmological parameters of the standard cosmological model and some of its extensions. This work expands and complements the recently published forecasts based on $Euclid$-specific probes, namely galaxy clustering, weak lensing, and their cross-correlation. With some assumptions on the specifications of current and…

Cosmology and Nongalactic Astrophysics (astro-ph.CO)Cosmic microwave backgroundstatistical [methods]FOS: Physical sciencesAstrophysicscosmic background radiationAstrophysics::Cosmology and Extragalactic AstrophysicsJoint analysiskosmologia01 natural sciencesmethodsNOpimeä aine[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]mikroaallotSettore FIS/05 - Astronomia e Astrofisicasurveys0103 physical sciencestszsurvey010303 astronomy & astrophysicsPhysicsmethods: statistical010308 nuclear & particles physicsComputer Science::Information RetrievalmaailmankaikkeusAstrophysics::Instrumentation and Methods for AstrophysicsAstronomy and Astrophysicscross-correlation115 Astronomy Space scienceCosmic background radiation; Large-scale structure of Universe; Methods: statistical; Surveyskosminen taustasäteilySpace and Planetary Sciencemethodlarge-scale structure of Universepimeä energia[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]statisticalAstrophysics - Cosmology and Nongalactic Astrophysics
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Feasibility study for the measurement of πN transition distribution amplitudes at P¯ANDA in p¯p→J/ψπ0

2017

The exclusive charmonium production process in (P) over barp annihilation with an associated pi 0 meson (p) over barp -> J/psi pi(0) is studied in the framework of QCD collinear factorization. The feasibility of measuring this reaction through the J/psi -> e(+) e(-) decay channel with the AntiProton ANnihilation at DArmstadt ((P) over bar ANDA) experiment is investigated. Simulations on signal reconstruction efficiency as well as the background rejection from various sources including the (P) over barp -> pi(+)pi(-)pi(0) and (p) over barp -> J/psi pi(0)pi(0) reactions are performed with PANDAROOT, the simulation and analysis software framework of the (P) over bar ANDA experiment. It is show…

Quantum chromodynamicsPhysicsParticle physicsLuminosity (scattering theory)AnnihilationMeson010308 nuclear & particles physics7. Clean energy01 natural sciencesParticle identificationNuclear physicsFactorizationAntiproton0103 physical sciencesHigh Energy Physics::Experiment010306 general physicsBar (unit)Physical Review D
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Study of doubly strange systems using stored antiprotons

2016

Bound nuclear systems with two units of strangeness are still poorly known despite their importance for many strong interaction phenomena. Stored antiprotons beams in the GeV range represent an unparalleled factory for various hyperon-antihyperon pairs. Their outstanding large production probability in antiproton collisions will open the floodgates for a series of new studies of systems which contain two or even more units of strangeness at the PANDA experiment at FAIR. For the first time, high resolution gamma-spectroscopy of doubly strange Lambda Lambda-hypernuclei will be performed, thus complementing measurements of ground state decays of Lambda Lambda-hypernuclei at J-PARC or possible …

Particle physicsNuclear and High Energy PhysicsCOLLISIONSStrong interactionNuclear TheoryhyperatomsAntiprotons; Hyperatoms; Hypernuclei; Strangeness; Nuclear and High Energy PhysicsEXCHANGE CURRENTSAntiprotonsStrangeness01 natural sciencesPartícules (Física nuclear)NONuclear physicsSubatomär fysikHypemucleistrangenessDECUPLET BARYONSELECTRIC QUADRUPOLE-MOMENTSHyperatoms0103 physical sciencesSubatomic PhysicsHypernuclei010306 general physicsNuclear ExperimentPhysicshypernucleiNUCLEI010308 nuclear & particles physicsHyperonStrangenessTransport theoryDOUBLE-LAMBDA-HYPERNUCLEIMODELOMEGAAntiprotonPhysics::Accelerator PhysicsHeavy ionHigh Energy Physics::ExperimentantiprotonsINTERMEDIATE ENERGIESEMULSIONNuclear Physics A
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Euclid Preparation. XIV. The Complete Calibration of the Color–Redshift Relation (C3R2) Survey: Data Release 3

2021

Stanford, S. A., et al.

Cosmology and Nongalactic Astrophysics (astro-ph.CO)[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Calibration (statistics)FOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsColor space217101 natural sciencesCosmologyLarge-scale structure010309 optics[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]galaxy spectroscopySettore FIS/05 - Astronomia e AstrofisicaSpitzer Space Telescope0103 physical sciencesDISTRIBUTIONSAstrophysics::Solar and Stellar AstrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)PHOTOMETRIC REDSHIFTS010303 astronomy & astrophysicsWeak gravitational lensingAstrophysics::Galaxy AstrophysicsPhysicsHardware_MEMORYSTRUCTURESAstrophysics::Instrumentation and Methods for AstrophysicsEuclidAstronomy and AstrophysicsRedshiftGalaxyCosmologySpace and Planetary ScienceGalaxy spectroscopyDark energyAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - Cosmology and Nongalactic Astrophysics
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Euclid preparation - XVII. Cosmic Dawn Survey: Spitzer Space Telescope observations of the Euclid deep fields and calibration fields

2022

Artículo escrito por un elevado núnmero de autores, sólo se referencian el qque aparece en primer lugar, los autores pertenecientes a la UAM y el nombre del grupo de colaboración, si lo hubiere

SAMPLELarge-scale structure of UniverseDATA RELEASEFormationSurveysobservations Dark energy Dark matter Galaxy: formation Large-scale structure of Universe Surveys [Cosmology]kosmologiaAstrophysicsCosmology: observationdark mattergalaksijoukotpimeä ainesurveysDark energyDark matterobservations [Cosmology]dark energyObservationsLEGACY SURVEYAstrophysics of GalaxiesFísicaAstronomy and Astrophysics115 Astronomy Space scienceEVOLUTIONCosmologygalaksitGALAXIESCosmology: observations; Dark energy; Dark matter; Galaxy: formation; Large-scale structure of Universe; SurveysGalaxyformation [Galaxy]Space and Planetary ScienceGalaxy: formationcosmology: observationslarge-scale structure of Universepimeä energiaCosmology and Nongalactic Astrophysics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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