Search results for "Cosmology"

showing 10 items of 2905 documents

Status of the EDELWEISS experiment

1999

The Edelweiss Dark Matter Experiment is installed in the Modane Underground Laboratory since 1994. In 1997 the first detector of a 70 g heat and ionization Ge low-temperature detector built by the collaboration showed its discrimination capabilities. During the last two years the installation was upgraded, and a new generation of 70 g Ge detectors is operational. The detector environment is drastically controlled to avoid radioactive contamination. A test run with two new 70 g detectors shows a reduction by a factor of ten in the background level before 7-ray rejection which is now around 2 events/kg/keV/day. Three 320 g Ge cryogenic detectors have been constructed and are now being tested …

CryostatPhysicsNuclear and High Energy Physics[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]Dark matterBolometerDetectorCosmic rayEDELWEISSAtomic and Molecular Physics and OpticsParticle detectorlaw.invention[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Nuclear physicsWIMPlaw[SDU]Sciences of the Universe [physics]Measuring instrumentInstrumentationEvent (probability theory)
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BART: The Czech Autonomous Observatory

2010

The High Energy Astrophysics group of the stellar department of the Astronomical Institute in Ondřejov operates two small aperture robotic telescopes called BART and D50. Both telescopes are capable of making automatic followup observation of gamma-ray burst optical counterparts. This paper deals with the smaller telescope BART.

CzechPhysicsHigh-energy astronomylcsh:AstronomyAstrophysics::High Energy Astrophysical PhenomenaAstrophysics::Instrumentation and Methods for AstrophysicsAstronomyAstronomy and AstrophysicsAstrophysicsLarge apertureAstrophysics::Cosmology and Extragalactic Astrophysicslanguage.human_languagelaw.inventionTelescopelcsh:QB1-991Space and Planetary ScienceObservatorylawlanguageAstrophysics::Earth and Planetary AstrophysicsAstrophysics::Galaxy AstrophysicsAdvances in Astronomy
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"Table 47" of "Energy dependence of event shapes and of alpha(s) at LEP-2."

1999

Measured value of the logarithmic energy slope of the inverse coupling constant.

DALPHAS/DLOGEE+ E- --> HADRONSE+ E- --> JETSE+ E- ScatteringExclusive91.2Astrophysics::Cosmology and Extragalactic AstrophysicsJet Production
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Electron-interacting dark matter: Implications from DAMA/LIBRA-phase2 and prospects for liquid xenon detectors and NaI detectors

2019

We investigate the possibility for the direct detection of low-mass (GeV scale) weakly interacting massive particles (WIMP) dark matter in scintillation experiments. Such WIMPs are typically too light to leave appreciable nuclear recoils but may be detected via their scattering off atomic electrons. In particular, the DAMA Collaboration [R. Bernabei et al., Nucl. Phys. At. Energy 19, 307 (2018)] has recently presented strong evidence of an annual modulation in the scintillation rate observed at energies as low as 1 keV. Despite a strong enhancement in the calculated event rate at low energies, we find that an interpretation in terms of electron-interacting WIMPs cannot be consistent with ex…

DAMA/LIBRACosmology and Nongalactic Astrophysics (astro-ph.CO)detector: performancePhysics::Instrumentation and DetectorsDark matterFOS: Physical scienceschemistry.chemical_elementElectron01 natural sciencesWIMP: dark matterNuclear physicsHigh Energy Physics - Phenomenology (hep-ph)XenonWIMP0103 physical sciences010306 general physicsenhancementscintillation counterenergy: lowPhysicsScintillationxenon: liquid010308 nuclear & particles physicsatom: wave functionDAMAmodulationHigh Energy Physics - Phenomenologychemistryelectron: scatteringWeakly interacting massive particles[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]direct detection[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Event (particle physics)Astrophysics and astroparticle physicsAstrophysics - Cosmology and Nongalactic AstrophysicsPhysical Review
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Two Remarkably Luminous Galaxy Candidates at z ≈ 10-12 Revealed by JWST

2022

The first few 100 Myr at z > 10 mark the last major uncharted epoch in the history of the universe, where only a single galaxy (GN-z11 at z ≈ 11) is currently spectroscopically confirmed. Here we present a search for luminous z > 10 galaxies with JWST/NIRCam photometry spanning ≈1–5 μm and covering 49 arcmin2 from the public JWST Early Release Science programs (CEERS and GLASS). Our most secure candidates are two MUV ≈ −21 systems: GLASS-z12 and GLASS-z10. These galaxies display abrupt ≳1.8 mag breaks in their spectral energy distributions (SEDs), consistent with complete absorption of flux bluewards of Lyα that is redshifted to =+z12.40.3 0.1and=+z10.40.5 0.4. Lower redshift interlopers su…

DECOMPOSITIONII.594Early universeFOS: Physical sciences2291435PROPAGATION734595310Galaxies and CosmologyUNCERTAINTIESGalaxy evolutionGalaxy formationTO 8REIONIZATIONMASSIVE GALAXIESAstronomy and AstrophysicsBRIGHT ENDAstrophysics - Astrophysics of GalaxiesEVOLUTIONSTELLARSpace and Planetary Science5101 Astronomical SciencesAstrophysics of Galaxies (astro-ph.GA)High-redshift galaxiesJames Webb Space Telescope51 Physical Sciences
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"Table 2" of "Study of ordered hadron chains with the ATLAS detector"

2017

The Delta(3h), for 3-hadron chains with mass below 0.59 GeV, as a function of $Q$, in the interval 0.02 GeV < Q < 0.36 GeV.

DELTA(3H)CorrelationsAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::ExperimentAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics::Earth and Planetary AstrophysicsNuclear Experimentpp --> X
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"Table 1" of "Measurements of the charge asymmetry in top-quark pair production in the dilepton final state at $\sqrt{s}=8$ TeV with the ATLAS detect…

2017

Unfolded distribution for the inclusive $\Delta|\eta|$ observable in the fiducial volume.

DELTA(ABS(ETA))Quantitative Biology::Biomolecules8000.0Proton-Proton ScatteringP P --> top + antitopAstrophysics::Instrumentation and Methods for AstrophysicsExclusiveTopTop ProductionHigh Energy Physics::ExperimentAstrophysics::Cosmology and Extragalactic AstrophysicsNuclear Experiment
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"Table 23" of "Measurement of the production cross section for Z/gamma* in association with jets in pp collisions at sqrt(s) = 7 TeV with the ATLAS d…

2014

Measured normalized differential cross section as a function of dijet azimuthal separation 1/sigma_DY dsigma/dDeltaPhijj (1/rad.) for the electron channel and the muon channel in the individual lepton fiducial regions and uncorrected for QED effects.

DSIG/DPHIZ ProductionPhysics::Instrumentation and DetectorsHigh Energy Physics::PhenomenologyAstrophysics::Cosmology and Extragalactic AstrophysicsJet ProductionAzimuthal Angular DependenceInclusiveSingle Differential Cross SectionP P --> Z0 JET XP P --> GAMMA* JET XProton-Proton ScatteringHigh Energy Physics::ExperimentNuclear Experiment
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"Table 14" of "Measurement of the inclusive jet cross-section in p anti-p collisions at s**(1/2) =1.96-TeV"

1970

Detailed systematic errors for the absolute value of the jet rapidity in the range 0.4 to 0.8: (1st) Luminosity (2nd) eta-intercalibration (3rd) eta-intercalibration (4th) eta-intercalibration (5th) JES resolution bias (6th) Resolution method.

DSYSInclusive20477612047761PBAR P --> JET XHigh Energy Physics::ExperimentAstrophysics::Cosmology and Extragalactic AstrophysicsJet ProductionNuclear Experiment
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"Table 9" of "Measurement of the inclusive jet cross-section in p anti-p collisions at s**(1/2) =1.96-TeV"

1970

Detailed systematic errors for the absolute value of the jet rapidity in the range 0.0 to 0.4: (1st) Luminosity (2nd) eta-intercalibration (3rd) eta-intercalibration (4th) eta-intercalibration (5th) JES resolution bias (6th) Resolution method.

DSYSInclusive20477612047761PBAR P --> JET XHigh Energy Physics::ExperimentAstrophysics::Cosmology and Extragalactic AstrophysicsJet ProductionNuclear ExperimentAstrophysics::Galaxy Astrophysics
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