Search results for "Cosmology"

showing 10 items of 2905 documents

"Table 20" of "Search for heavy Higgs bosons decaying into two tau leptons with the ATLAS detector using $pp$ collisions at $\sqrt{s}=13$ TeV"

2020

Acceptance times efficiency for a scalar boson produced by b-associated production as a function of the scalar boson mass.

Condensed Matter::Quantum GasesInclusiveGeneral Relativity and Quantum CosmologyP P --> TAU+ TAU- X13000.0Proton-Proton ScatteringHigh Energy Physics::PhenomenologyEFFACCHiggs
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"Table 20" of "Search for heavy Higgs bosons decaying into two tau leptons with the ATLAS detector using $pp$ collisions at $\sqrt{s}=13$ TeV"

2020

Acceptance times efficiency for a scalar boson produced by b-associated production as a function of the scalar boson mass.

Condensed Matter::Quantum GasesInclusiveGeneral Relativity and Quantum CosmologyP P --> TAU+ TAU- X13000.0Proton-Proton ScatteringHigh Energy Physics::PhenomenologyEFFACCHiggs
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"Table 20" of "Search for heavy Higgs bosons decaying into two tau leptons with the ATLAS detector using $pp$ collisions at $\sqrt{s}=13$ TeV"

2020

Acceptance times efficiency for a scalar boson produced by b-associated production as a function of the scalar boson mass.

Condensed Matter::Quantum GasesInclusiveGeneral Relativity and Quantum CosmologyP P --> TAU+ TAU- X13000.0Proton-Proton ScatteringHigh Energy Physics::PhenomenologyEFFACCHiggs
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"Table 2" of "Measurement of the shape of the boson transverse momentum distribution in p anti-p ---> Z / gamma* ---> e+ e- + X events produced…

2008

Correlation matrix for all rapidity Z bosons for the 12 bins used for PT < 30.

Condensed Matter::Quantum GasesInclusiveZ ProductionElectron productionPBAR P --> E+ E- XCORRHigh Energy Physics::PhenomenologyPBAR P --> GAMMA* XAstrophysics::Cosmology and Extragalactic AstrophysicsPhysics::Data Analysis; Statistics and ProbabilityPBAR P --> Z0 X
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Dynamically stabilized spin superfluidity in frustrated magnets

2020

We study the onset of spin superfluidity, namely coherent spin transport mediated by a topological spin texture, in frustrated exchange-dominated magnetic systems, engendered by an external magnetic field. We show that for typical device geometries used in nonlocal magnetotransport experiments, the magnetic field stabilizes a spin superflow against fluctuations, up to a critical current. For a given current, the critical field depends on the precessional frequency of the texture, which can be separately controlled. We contrast such dynamic stabilization of a spin superfluid to the conventional approaches based on topological stabilization.

Condensed Matter::Quantum GasesPhysicsCondensed Matter - Mesoscale and Nanoscale PhysicsCondensed matter physicsTexture (cosmology)FOS: Physical sciences02 engineering and technology021001 nanoscience & nanotechnology01 natural sciencesMagnetic fieldSuperfluidityMagnetMesoscale and Nanoscale Physics (cond-mat.mes-hall)0103 physical sciencesCondensed Matter::Strongly Correlated ElectronsCritical currentCurrent (fluid)010306 general physics0210 nano-technologyCritical fieldSpin-½Physical Review B
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Zero-point excitation of a circularly moving detector in an atomic condensate and phonon laser dynamical instabilities

2020

We study a circularly moving impurity in an atomic condensate for the realisation of superradiance phenomena in tabletop experiments. The impurity is coupled to the density fluctuations of the condensate and, in a quantum field theory language, it serves as an analog of a detector for the quantum phonon field. For sufficiently large rotation speeds, the zero-point fluctuations of the phonon field induce a sizeable excitation rate of the detector even when the condensate is initially at rest in its ground state. For spatially confined condensates and harmonic detectors, such a superradiant emission of sound waves provides a dynamical instability mechanism leading to a new concept of phonon l…

Condensed Matter::Quantum GasesPhysicsQuantum PhysicsCondensed Matter::Other010308 nuclear & particles physicsPhononAstrophysics::High Energy Astrophysical PhenomenaDetectorFOS: Physical sciencesZero-point energySuperradianceCondensed Matter::Mesoscopic Systems and Quantum Hall EffectLaser01 natural scienceslaw.inventionGeneral Relativity and Quantum CosmologyQuantum Gases (cond-mat.quant-gas)Impuritylaw0103 physical sciencesAtomic physicsCondensed Matter - Quantum GasesQuantum Physics (quant-ph)010306 general physicsExcitationPhysical Review Research
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Effects of a uniform acceleration on atom–field interactions

2014

We review some quantum electrodynamical effects related to the uniform acceleration of atoms in vacuum. After discussing the energy level shifts of a uniformly accelerated atom in vacuum, we investigate the atom-wall Casimir-Polder force for accelerated atoms, and the van der Waals/Casimir-Polder interaction between two accelerated atoms. The possibility of detecting the Unruh effect through these phenomena is also discussed in detail.

Condensed Matter::Quantum GasesPhysicsQuantum PhysicsField (physics)FOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Condensed Matter PhysicsGeneral Relativity and Quantum CosmologyAtomic and Molecular Physics and OpticsCasimir effectGeneral Relativity and Quantum Cosmologysymbols.namesakeAccelerationUnruh effectUnruh effect Casimir–Polder forces vacuum fluctuationsAtomPhysics::Atomic and Molecular ClusterssymbolsPhysics::Accelerator PhysicsPhysics::Atomic Physicsvan der Waals forceAtomic physicsQuantum Physics (quant-ph)QuantumMathematical PhysicsPhysica Scripta
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An optical pulse modulator based on an all-fibre mirror

1996

In this article we present an all-fiber Sagnac interferometer modulated in a pulsed regime.

Condensed Matter::Quantum GasesPhysics::General PhysicsGeneral Relativity and Quantum CosmologyAstrophysics::Instrumentation and Methods for AstrophysicsPhysics::OpticsFísica
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Non-circular rotating beams and CMB experiments

2002

This paper is concerned with small angular scale experiments for the observation of cosmic microwave background anisotropies. In the absence of beam, the effects of partial coverage and pixelisation are disentangled and analyzed (using simulations). Then, appropriate maps involving the CMB signal plus the synchrotron and dust emissions from the Milky Way are simulated, and an asymmetric beam --which turns following different strategies-- is used to smooth the simulated maps. An associated circular beam is defined to estimate the deviations in the angular power spectrum produced by beam asymmetry without rotation and, afterwards, the deviations due to beam rotation are calculated. For a cert…

Cosmic microwave background ; Cosmology theory ; Large-scale structure of the universe ; Numerical method ; Data analysis methodmedia_common.quotation_subjectCosmic microwave backgroundFOS: Physical sciencesAstrophysicsNumerical methodUNESCO::ASTRONOMÍA Y ASTROFÍSICAAstrophysicsRotationAsymmetryCosmic microwave backgroundlaw.inventionsymbols.namesakelawCosmology theoryLarge-scale structure of the universePlanckAnisotropymedia_commonPhysicsData analysis methodAstrophysics (astro-ph)Spectral densityAstronomy and Astrophysics:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia [UNESCO]SynchrotronComputational physicsSpace and Planetary SciencesymbolsUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]Beam (structure)Astronomy & Astrophysics
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The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Measuring D_A and H at z=0.57 from the Baryon Acoustic Peak in th…

2014

We present measurements of the angular diameter distance to and Hubble parameter at z = 0.57 from the measurement of the baryon acoustic peak in the correlation of galaxies from the Sloan Digital Sky Survey III Baryon Oscillation Spectroscopic Survey. Our analysis is based on a sample from Data Release 9 of 264 283 galaxies over 3275 square degrees in the redshift range 0.43 z DA(0.57) = 1408 ± 45 Mpc and H(0.57) = 92.9 ± 7.8 km s-1 Mpc-1 for our fiducial value of the sound horizon. These results from the anisotropic fitting are fully consistent with the analysis of the spherically averaged acoustic peak position presented in Anderson et al. Our distance measurements are a close match to th…

Cosmology and GravitationCosmology and Nongalactic Astrophysics (astro-ph.CO)Cosmological parametersDark matterLarge scale structure of UniverseFOS: Physical sciencesLambda-CDM modelAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsExpanding universesymbols.namesakeExpansió de l'universObservacions astronòmiquesDark energyQB Astronomyobservations [Cosmology]QCComputingMilieux_MISCELLANEOUSAstrophysics::Galaxy AstrophysicsQB/dk/atira/pure/core/subjects/cosmologyPhysics[PHYS]Physics [physics]Distance scaleCosmologiaAngular diameter distanceFísicaAstronomy and AstrophysicsRedshiftGalaxyCosmologyBaryonQC PhysicsSpace and Planetary ScienceDark energysymbols[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astrophysics - Cosmology and Nongalactic AstrophysicsHubble's lawAstronomical observations
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