Search results for "EINSTEIN"

showing 10 items of 246 documents

Outer boundary conditions for Einstein's field equations in harmonic coordinates

2007

We analyze Einstein's vacuum field equations in generalized harmonic coordinates on a compact spatial domain with boundaries. We specify a class of boundary conditions which is constraint-preserving and sufficiently general to include recent proposals for reducing the amount of spurious reflections of gravitational radiation. In particular, our class comprises the boundary conditions recently proposed by Kreiss and Winicour, a geometric modification thereof, the freezing-Psi0 boundary condition and the hierarchy of absorbing boundary conditions introduced by Buchman and Sarbach. Using the recent technique developed by Kreiss and Winicour based on an appropriate reduction to a pseudo-differe…

AstrofísicaWell-posed problemPhysicsHarmonic coordinatesPhysics and Astronomy (miscellaneous)010308 nuclear & particles physicsGravitational waveMathematical analysisFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologyNonlinear systemsymbols.namesake0103 physical sciencesAstronomiaSchwarzschild metricsymbolsBoundary value problemEinstein010306 general physicsReduction (mathematics)Caltech Library ServicesClassical and Quantum Gravity
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GRAVITATIONAL WAVE SIGNATURES IN BLACK HOLE FORMING CORE COLLAPSE

2013

We present numerical simulations in general relativity of collapsing stellar cores. Our initial model consists of a low metallicity rapidly-rotating progenitor which is evolved in axisymmetry with the latest version of our general relativistic code CoCoNuT, which allows for black hole formation and includes the effects of a microphysical equation of state (LS220) and a neutrino leakage scheme to account for radiative losses. The motivation of our study is to analyze in detail the emission of gravitational waves in the collapsar scenario of long gamma-ray bursts. Our simulations show that the phase during which the proto-neutron star (PNS) survives before ultimately collapsing to a black hol…

Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics01 natural sciencesInstabilityGeneral Relativity and Quantum Cosmology0103 physical sciencesRadiative transferAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy AstrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsEinstein Telescope010308 nuclear & particles physicsGravitational waveAstronomy and AstrophysicsVirgo ClusterBlack holeSupernovaNeutron starAstrophysics - Solar and Stellar Astrophysics13. Climate actionSpace and Planetary ScienceAstrophysics - High Energy Astrophysical PhenomenaThe Astrophysical Journal
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Gravitational Lensing: the Structure of Quasars and Galaxies

2016

We use gravitational lens systems in which a galaxy produces multiple images of a distant quasar to study the properties of both the unresolved structure of the lensed quasar and the mass distribution in the gravitational lens. First, we estimate the size and the logarithmic slope of the temperature profile in the accretion disk of the lensed quasar Q2237+0305 using a method that is independent of the component velocities, based on six epochs of multi-wavelength narrowband images from the Nordic Optical Telescope. A statistical comparison of the observed microlensing with simulations based on microlensing magnification maps gives Bayesian estimates for the half-light radius of ~8 light-days…

Astrophysics::High Energy Astrophysical Phenomenaaccretion disksgravitational lensingquasarsmid-infraredAstrophysics::Cosmology and Extragalactic AstrophysicsUNESCO::ASTRONOMÍA Y ASTROFÍSICAmicrolensingdark matterradioEinstein Crossaccretiongalaxiesstrong lensingAstrophysics::Earth and Planetary AstrophysicsQ2237+0305Astrophysics::Galaxy Astrophysics:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]
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Quantum localization and bound state formation in Bose-Einstein condensates

2010

We discuss the possibility of exponential quantum localization in systems of ultracold bosonic atoms with repulsive interactions in open optical lattices without disorder. We show that exponential localization occurs in the maximally excited state of the lowest energy band. We establish the conditions under which the presence of the upper energy bands can be neglected, determine the successive stages and the quantum phase boundaries at which localization occurs, and discuss schemes to detect it experimentally by visibility measurements. The discussed mechanism is a particular type of quantum localization that is intuitively understood in terms of the interplay between nonlinearity and a bou…

Atomic Physics (physics.atom-ph)FOS: Physical sciences01 natural sciencesSpectral linelocalization010305 fluids & plasmaslaw.inventionPhysics - Atomic PhysicslawQuantum mechanics0103 physical sciencesBound state010306 general physicsElectronic band structureQuantumPhysicsQuantum PhysicsAtomic and Molecular Physics and Optics3. Good healthExponential functionWeak localizationQuantum Gases (cond-mat.quant-gas)Excited stateQuantum electrodynamicsQuantum Physics (quant-ph)Condensed Matter - Quantum GasesBose–Einstein condensate
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Space-borne Bose–Einstein condensation for precision interferometry

2018

Space offers virtually unlimited free-fall in gravity. Bose-Einstein condensation (BEC) enables ineffable low kinetic energies corresponding to pico- or even femtokelvins. The combination of both features makes atom interferometers with unprecedented sensitivity for inertial forces possible and opens a new era for quantum gas experiments. On January 23, 2017, we created Bose-Einstein condensates in space on the sounding rocket mission MAIUS-1 and conducted 110 experiments central to matter-wave interferometry. In particular, we have explored laser cooling and trapping in the presence of large accelerations as experienced during launch, and have studied the evolution, manipulation and interf…

Atomic Physics (physics.atom-ph)FOS: Physical sciencesSpace (mathematics)01 natural sciencesPhysics - Atomic Physicslaw.invention010309 opticslawLaser cooling0103 physical sciencesAstronomical interferometer010306 general physicsQuantumCondensed Matter::Quantum GasesPhysicsMultidisciplinaryBragg's lawinterferometryBose-EinsteinComputational physicsInterferometryQuantum Gases (cond-mat.quant-gas)QuasiparticleAtomic physicsCondensed Matter - Quantum GasesBose–Einstein condensateNature
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Excision technique in constrained formulations of Einstein equations: collapse scenario

2015

We present a new excision technique used in constrained formulations of Einstein equations to deal with black hole in numerical simulations. We show the applicability of this scheme in several scenarios. In particular, we present the dynamical evolution of the collapse of a neutron star to a black hole, using the CoCoNuT code and this excision technique.

Black holePhysicsGeneral Relativity and Quantum CosmologyHistoryNeutron starCode (set theory)Classical mechanicsAstrophysics::High Energy Astrophysical PhenomenaEinstein equationsCollapse (topology)Computer Science ApplicationsEducationJournal of Physics: Conference Series
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The e-ASTROGAM gamma-ray space observatory for the multimessenger astronomy of the 2030s

2018

e-ASTROGAM is a concept for a breakthrough observatory space mission carrying a gamma-ray telescope dedicated to the study of the non-thermal Universe in the photon energy range from 0.15 MeV to 3 GeV. The lower energy limit can be pushed down to energies as low as 30 keV for gamma-ray burst detection with the calorimeter. The mission is based on an advanced space-proven detector technology, with unprecedented sensitivity, angular and energy resolution, combined with remarkable polarimetric capability. Thanks to its performance in the MeV-GeV domain, substantially improving its predecessors, e-ASTROGAM will open a new window on the non-thermal Universe, making pioneering observations of the…

Cherenkov Telescope ArrayHigh-energy astrophysical phenomenaCompton and pair creation telescope; Gamma-ray astronomy; gamma-ray polarization; high-energy astrophysical phenomena; space mission; time-domain astronomyenergy resolution7. Clean energy01 natural sciencesSpace missionlaw.inventionIceCubeEinstein TelescopelawObservatoryLIGO010303 astronomy & astrophysicsKM3NeTPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Applied MathematicsAstrophysics::Instrumentation and Methods for AstrophysicsComputer Science Applications1707 Computer Vision and Pattern RecognitionGamma-ray astronomyGamma-ray polarizationCondensed Matter Physicsphoton: energyobservatoryNuclear astrophysicsApace missionAstrophysics - High Energy Astrophysical Phenomenaperformancedetector: technologyAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysicsgamma ray: burstspace missionCompton and pair creation telescopeTelescope0103 physical sciencessupernovaElectroniccalorimetergamma ray: detectorOptical and Magnetic MaterialsKAGRAElectrical and Electronic Engineering010306 general physicsTime domain astronomyLISAGamma-ray astronomyEinstein TelescopeAstronomyInstitut für Physik und AstronomieTime-domain astronomyCherenkov Telescope ArraysensitivityLIGOmessengerKM3NeTVIRGO13. Climate actionCompton and pair creation telescope; Gamma-ray astronomy; gamma-ray polarization; high-energy astrophysical phenomena; space mission; time-domain astronomy; Electronic Optical and Magnetic Materials; Condensed Matter Physics; Computer Science Applications1707 Computer Vision and Pattern Recognition; Applied Mathematics; Electrical and Electronic Engineeringddc:520galaxyCompton and pair creation telescope; Gamma-ray astronomy; gamma-ray polarization; high-energy astrophysical phenomena; space mission; time-domain astronomy; Electronic Optical and Magnetic Materials; Condensed Matter Physics; Applied Mathematics; Electrical and Electronic Engineering[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Design of a compact diode laser system for dual-species atom interferometry with rubidium and potassium in space

2017

We report on a micro-integrated high power diode laser based system for the MAIUS II/III missions. The laser system features fiber coupled and frequency stabilized external cavity diode lasers (ECDL) for laser cooling, Bose-Einstein condensate (BEC) generation and dual species atom interferometry with rubidium and potassium on board a sounding rocket.

Condensed Matter::Quantum GasesAtom interferometerMaterials scienceSounding rocketbusiness.industryPotassiumPhysics::Opticschemistry.chemical_elementLaser01 natural scienceslaw.inventionRubidium010309 opticschemistrylawLaser cooling0103 physical sciencesOptoelectronicsPhysics::Atomic Physics010306 general physicsbusinessBose–Einstein condensateDiode2017 Conference on Lasers and Electro-Optics Pacific Rim (CLEO-PR)
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The effect of interactions on Bose-Einstein condensation in a quasi two-dimensional harmonic trap

1999

A dilute bose gas in a quasi two-dimensional harmonic trap and interacting with a repulsive two-body zero-range potential of fixed coupling constant is considered. Using the Thomas-Fermi method, it is shown to remain in the same uncondensed phase as the temperature is lowered. Its density profile and energy are identical to that of an ideal gas obeying the fractional exclusion statistics of Haldane. PACS: ~03.75.Fi, 05.30.Jp, 67.40.Db, 05.30.-d

Condensed Matter::Quantum GasesCoupling constantPhysicsStatistical Mechanics (cond-mat.stat-mech)Condensed Matter - Mesoscale and Nanoscale PhysicsBose gasFOS: Physical sciencesCondensed Matter Physics01 natural sciencesAtomic and Molecular Physics and OpticsIdeal gas010305 fluids & plasmaslaw.inventionTrap (computing)lawPhase (matter)Mesoscale and Nanoscale Physics (cond-mat.mes-hall)0103 physical sciencesHarmonicAtomic physics010306 general physicsCondensed Matter - Statistical MechanicsBose–Einstein condensateJournal of Physics B: Atomic, Molecular and Optical Physics
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Vortices in rotating two-component boson and fermion traps

2010

Quantum liquids may carry angular momentum by the formation of vortex states. This is well known for Bose-Einstein condensates in rotating traps, and was even found to occur in quantum dots at strong magnetic fields. Here we consider a two-component quantum liquid, where coreless vortices and interlaced lattices of coreless vortices appear in a very similar way for fermions and bosons with repulsive two-body interactions. The ground states at given angular momentum, as well as the pair correlations for equal and different numbers of atoms in the two components, are studied. (C) 2009 Elsevier B.V. All rights reserved.

Condensed Matter::Quantum GasesPhysicsAngular momentumta214Condensed matter physicsta114ta221vorticesquantum dotsFermionCondensed Matter PhysicsAtomic and Molecular Physics and OpticsElectronic Optical and Magnetic Materialslaw.inventionVortexlawQuantum dotTotal angular momentum quantum numberQuantum mechanicsAngular momentum couplingBose–Einstein condensateta218BosonPHYSICA E: LOW: DIMENSIONAL SYSTEMS AND NANOSTRUCTURES
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