Search results for " Cosmology"

showing 10 items of 1486 documents

The history of chemical enrichment in the intracluster medium from cosmological simulations

2017

The distribution of metals in the intracluster medium (ICM) of galaxy clusters provides valuable information on their formation and evolution, on the connection with the cosmic star formation and on the effects of different gas processes. By analyzing a sample of simulated galaxy clusters, we study the chemical enrichment of the ICM, its evolution, and its relation with the physical processes included in the simulation and with the thermal properties of the core. These simulations, consisting of re-simulations of 29 Lagrangian regions performed with an upgraded version of the SPH GADGET-3 code, have been run including two different sets of baryonic physics: one accounts for radiative coolin…

Active galactic nucleusCosmology and Nongalactic Astrophysics (astro-ph.CO)Radiative coolingGalaxies:clusters:general; Galaxies:clusters:Intracluster medium; Methods: numerical; Astronomy and Astrophysics; Space and Planetary ScienceMetallicityFOS: Physical sciencesclusters:Intracluster medium [Galaxies]AstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesSmoothed-particle hydrodynamicsclusters:general [Galaxies]Intracluster medium0103 physical sciencesGalaxies:clusters:Intracluster medium010303 astronomy & astrophysicsGalaxy clusterAstrophysics::Galaxy AstrophysicsPhysicsnumerical [Methods]Methods: numerical010308 nuclear & particles physicsStar formationAstronomyAstronomy and AstrophysicsAstronomy and AstrophysicAstrophysics - Astrophysics of GalaxiesGalaxies:clusters:generalSupernova13. Climate actionSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)Astrophysics - Cosmology and Nongalactic Astrophysics
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VLBI detection of the HST-1 feature in the M87 jet at 2 cm

2010

A bright feature 80 pc away from the core in the powerful jet of M87 shows highly unusual properties. Earlier radio, optical and X-ray observations have shown that this feature, labeled HST-1, is superluminal, and is possibly connected with the TeV flare detected by HESS in 2005. It has been claimed that this feature might have a blazar nature, due to these properties. To examine the possible blazar-like nature of HST-1, we analyzed lambda 2 cm VLBA archival data from dedicated full-track observations and the 2 cm survey/MOJAVE VLBI monitoring programs obtained between 2000 and 2009. Applying VLBI wide-field imaging techniques, the HST-1 region was imaged at milliarcsecond resolution. Here …

Active galactic nucleusCosmology and Nongalactic Astrophysics (astro-ph.CO)active [Galaxies]010504 meteorology & atmospheric sciencesRadio galaxyFluxFOS: Physical sciencesgalaxies [Radio continuum]Astrophysics01 natural scienceslaw.inventionlaw0103 physical sciencesVery-long-baseline interferometryUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Otras especialidades astronómicasBlazar010303 astronomy & astrophysicsUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia::Galaxias0105 earth and related environmental sciencesPhysicsSuperluminal motionAstronomy and Astrophysics:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia::Galaxias [UNESCO]Radio continuum : galaxies; Techniques : high angular resolution; Techniques : interferometric; Galaxies : active; Galaxies : jetshigh angular resolution [Techniques]InterferometrySpace and Planetary Scienceinterferometric [Techniques]jets [Galaxies]:ASTRONOMÍA Y ASTROFÍSICA::Otras especialidades astronómicas [UNESCO]FlareAstrophysics - Cosmology and Nongalactic Astrophysics
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Jet-torus connection in radio galaxies

2017

High-resolution Very-Long-Baseline Interferometry observations of active galactic nuclei have revealed asymmetric structures in the jets of radio galaxies. These asymmetric structures may be due to internal asymmetries in the jet, could be induced by the different conditions in the surrounding ambient medium including the obscuring torus, or a combination of the two. In this paper we investigate the influence of the ambient medium (including the obscuring torus) on the observed properties of jets from radio galaxies. We performed special-relativistic hydrodynamic (RHD) simulations of over-pressured and pressure-matched jets using the special-relativistic hydrodynamics code \texttt{Ratpenat}…

Active galactic nucleusRadio galaxyAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciencesElectromagnetic radiationGeneral Relativity and Quantum Cosmology0103 physical sciencesVery-long-baseline interferometryRadiative transfer010303 astronomy & astrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsJet (fluid)Spectral index010308 nuclear & particles physicsAstronomy and AstrophysicsTorusAstrophysics - Astrophysics of Galaxies13. Climate actionSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)Astrophysics - High Energy Astrophysical PhenomenaAstronomy & Astrophysics
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A study of the effect of molecular and aerosol conditions in the atmosphere on air fluorescence measurements at the Pierre Auger Observatory

2010

The air fluorescence detector of the Pierre Auger Observatory is designed to perforin calorimetric measurements of extensive air showers created by Cosmic rays of above 10(18) eV. To correct these measurements for the effects introduced by atmospheric fluctuations, the Observatory contains a group Of monitoring instruments to record atmospheric conditions across the detector site, ail area exceeding 3000 km(2). The atmospheric data are used extensively in the reconstruction of air showers, and are particularly important for the correct determination of shower energies and the depths of shower maxima. This paper contains a summary of the molecular and aerosol conditions measured at the Pierr…

Angstrom exponentAstronomyAstrophysics01 natural sciencesAugerCROSS-SECTIONSCOSMIC-RAY SHOWERSObservatoryDEPENDENCEHigh-Energy Cosmic Ray010303 astronomy & astrophysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Lidar[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]ANGSTROM EXPONENTPierre Auger ObservatoryBi-static lidarELECTRONSComputingMethodologies_DOCUMENTANDTEXTPROCESSINGMULTIPLE-SCATTERINGLight emissionFísica nuclearAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaLIGHT-EMISSIONAstrophysics - Cosmology and Nongalactic Astrophysics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Cosmology and Nongalactic Astrophysics (astro-ph.CO)Extensive air showerFOS: Physical sciencesCosmic raySURFACE DETECTORAir fluorescence method0103 physical sciencesExtensive air showersRECONSTRUCTIONAerosolInstrumentation and Methods for Astrophysics (astro-ph.IM)Cosmic raysPierre Auger ObservatoryAerosolsCalorimeter (particle physics)Atmospheric effect010308 nuclear & particles physicsAtmosphereFísicaAstronomy and AstrophysicsCosmic rays; Extensive air showers; Air fluorescence method; Atmosphere; Aerosols; Lidar; Bi-static lidarCosmic rayNITROGENAir showerFluorescence Telescopes13. Climate actionExperimental High Energy PhysicsAEROSSOL
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Dynamics of thick discs around Schwarzschild-de Sitter black holes

2003

We consider the effects of a cosmological constant on the dynamics of constant angular momentum discs orbiting Schwarzschild-de Sitter black holes. The motivation behind this study is to investigate whether the presence of a radial force contrasting the black hole's gravitational attraction can influence the occurrence of the runaway instability, a robust feature of the dynamics of constant angular momentum tori in Schwarzschild and Kerr spacetimes. In addition to the inner cusp near the black hole horizon through which matter can accrete onto the black hole, in fact, a positive cosmological constant introduces also an outer cusp through which matter can leave the torus without accreting on…

Angular momentumAstrophysics::High Energy Astrophysical PhenomenaAccretion discs ; Black holes ; Relativity ; Hydrodynamics ; Cosmological constantFOS: Physical sciencesCosmological constantGeneral Relativity and Quantum Cosmology (gr-qc)UNESCO::ASTRONOMÍA Y ASTROFÍSICAAstrophysicsInstabilityGeneral Relativity and Quantum CosmologyRelativityGravitationGeneral Relativity and Quantum CosmologyDe Sitter universeCosmological constantPhysicsBlack holesHorizonAstrophysics (astro-ph)Astronomy and AstrophysicsTorus:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia [UNESCO]Classical mechanicsSpace and Planetary ScienceHydrodynamicsUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogoniaSchwarzschild radiusAccretion discs:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]
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Relativistic simulations of rotational core collapse : I. Methods, initial models, and code tests

2002

We describe an axisymmetric general relativistic code for rotational core collapse. The code evolves the coupled system of metric and fluid equations using the ADM 3+1 formalism and a conformally flat metric approximation of the Einstein equations. The relativistic hydrodynamics equations are formulated as a first-order flux-conservative hyperbolic system and are integrated using high-resolution shock-capturing schemes based on Riemann solvers. We assess the quality of the conformally flat metric approximation for relativistic core collapse and present a comprehensive set of tests which the code successfully passed. The tests include relativistic shock tubes, the preservation of the rotatio…

Angular momentumAstrophysics::High Energy Astrophysical PhenomenaRotational symmetryFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)AstrophysicsNumerical methodAstrophysicsUNESCO::ASTRONOMÍA Y ASTROFÍSICAGeneral Relativity and Quantum CosmologyGravitational wavesGravitationRelativitysymbols.namesakeWaveformPhysicsAstrophysics (astro-ph)Astronomy and Astrophysics:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia [UNESCO]Hyperbolic systemsNeutron starRiemann hypothesisClassical mechanicsSpace and Planetary ScienceGravitational waves ; Hydrodynamics ; Numerical method ; RelativitysymbolsHydrodynamicsFluid equationUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]
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Gravity Probe Spin: Prospects for measuring general-relativistic precession of intrinsic spin using a ferromagnetic gyroscope

2020

An experimental test at the intersection of quantum physics and general relativity is proposed: measurement of relativistic frame dragging and geodetic precession using intrinsic spin of electrons. The behavior of intrinsic spin in spacetime dragged and warped by a massive rotating body is an experimentally open question, hence the results of such a measurement could have important theoretical consequences. Such a measurement is possible by using mm-scale ferromagnetic gyroscopes in orbit around the Earth. Under conditions where the rotational angular momentum of a ferromagnet is sufficiently small, a ferromagnet's angular momentum is dominated by atomic electron spins and is predicted to e…

Angular momentumGeneral relativityFOS: Physical sciencesElectronFrame-draggingGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciences7. Clean energyGeneral Relativity and Quantum Cosmologylaw.inventionPhysics::Geophysicslaw0103 physical sciencesddc:530010306 general physicsSpin (physics)Geodetic effectPhysicsQuantum Physics010308 nuclear & particles physicsGyroscopeQuantum electrodynamicsPhysics::Space PhysicsPrecessionCondensed Matter::Strongly Correlated ElectronsQuantum Physics (quant-ph)
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Minidisk dynamics in accreting, spinning black hole binaries: Simulations in full general relativity

2021

We perform magnetohydrodynamic simulations of accreting, equal-mass binary black holes in full general relativity focusing on the impact of black hole spin on the dynamical formation and evolution of minidisks. We find that during the late inspiral the sizes of minidisks are primarily determined by the interplay between the tidal field and the effective innermost stable orbit around each black hole. Our calculations support that a minidisk forms when the Hill sphere around each black hole is significantly larger than the black hole's effective innermost stable orbit. As the binary inspirals, the radius of the Hill sphere decreases, and minidisk sconsequently shrink in size. As a result, ele…

Astrofísica010504 meteorology & atmospheric sciencesGeneral relativityastro-ph.GAgr-qcAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologyLuminosityGravitationGeneral Relativity and Quantum CosmologyBinary black hole0103 physical sciences010303 astronomy & astrophysics0105 earth and related environmental sciencesPhysicsastro-ph.HEHigh Energy Astrophysical Phenomena (astro-ph.HE)Accretion (meteorology)Astronomy and AstrophysicsMass ratioAstrophysics - Astrophysics of Galaxies3. Good healthBlack holeSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)Hill sphereAstronomiaAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical Phenomena
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Astrophysics with the Laser Interferometer Space Antenna

2023

Full list of authors: Amaro-Seoane, Pau; Andrews, Jeff; Sedda, Manuel Arca; Askar, Abbas.; Baghi, Quentin; Balasov, Razvan; Bartos, Imre; Bavera, Simone S.; Bellovary, Jillian; Berry, Christopher P. L.; Berti, Emanuele; Bianchi, Stefano; Blecha, Laura; Blondin, Stephane; Bogdanovic, Tamara; Boissier, Samuel; Bonetti, Matteo; Bonoli, Silvia; Bortolas, Elisa; Breivik, Katelyn; Capelo, Pedro R.; Caramete, Laurentiu; Cattorini, Federico; Charisi, Maria; Chaty, Sylvain; Chen, Xian; Chruslinska, Martyna; Chua, Alvin J. K.; Church, Ross; Colpi, Monica; D'Orazio, Daniel; Danielski, Camilla; Davies, Melvyn B.; Dayal, Pratika; De Rosa, Alessandra; Derdzinski, Andrea; Destounis, Kyriakos; Dotti, Massi…

AstrofísicaACTIVE GALACTIC NUCLEICosmology and Nongalactic Astrophysics (astro-ph.CO)Physics and Astronomy (miscellaneous)Black holeAstronomyStellar remnantFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)TIDAL DISRUPTION EVENTSGeneral Relativity and Quantum CosmologyGravitational wavesMOCCA-SURVEY DATABASESettore FIS/05 - Astronomia e AstrofisicaStellar remnantsSoftware ScienceMulti-messengerGRAVITATIONAL-WAVE SOURCESInstrumentation and Methods for Astrophysics (astro-ph.IM)Extreme mass ratio in-spiralsSolar and Stellar Astrophysics (astro-ph.SR)High Energy Astrophysical Phenomena (astro-ph.HE)Black holes; Extreme mass ratio in-spirals; Gravitational waves; Multi-messenger; Stellar remnantsBlack holesData ScienceAstrophysics::Instrumentation and Methods for AstrophysicsExtreme mass ratio in-spiralAM-CVN STARSAstrophysics - Astrophysics of GalaxiesWHITE-DWARF BINARIESDOUBLE NEUTRON-STARSAstrophysics - Solar and Stellar Astrophysics[SDU]Sciences of the Universe [physics]Astrophysics of Galaxies (astro-ph.GA)AstronomiaMASSIVE BLACK-HOLEAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for AstrophysicsX-RAY BINARIESCOMMON-ENVELOPE EVOLUTIONGravitational waveAstrophysics - Cosmology and Nongalactic Astrophysics
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LeMMINGs III. The e-MERLIN legacy survey of the Palomar sample: exploring the origin of nuclear radio emission in active and inactive galaxies throug…

2021

Full list of authors: Baldi, R. D.; Williams, D. R. A.; Beswick, R. J.; McHardy, I.; Dullo, B. T.; Knapen, J. H.; Zanisi, L.; Argo, M. K.; Aalto, S.; Alberdi, A.; Baan, W. A.; Bendo, G. J.; Fenech, D. M.; Green, D. A.; Klöckner, H. -R.; Körding, E.; Maccarone, T. J.; Marcaide, J. M.; Mutie, I.; Panessa, F.; Pérez-Torres, M. A.; Romero-Cañizales, C.; Saikia, D. J.; Saikia, P.; Shankar, F.; Spencer, R. E.; Stevens, I. R.; Uttley, P.; Brinks, E.; Corbel, S.; Martí-Vidal, I.; Mundell, C. G.; Pahari, M.; Ward, M. J.

AstrofísicaActive galactic nucleusAstronomyAstrophysics::High Energy Astrophysical Phenomenanuclei [galaxies]jets [galaxies]Doubly ionized oxygenFOS: Physical sciencesAstrophysicsF500Astrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesRadio continuum: galaxiesLuminosityAstrophysical jetSubatomic Physics0103 physical sciencesAstronomy Astrophysics and CosmologyAstrophysics::Solar and Stellar AstrophysicsConnection (algebraic framework)010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsGalaxies: nucleiAstronomia ObservacionsHigh Energy Astrophysical Phenomena (astro-ph.HE)Physics[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]Galaxies: star formation010308 nuclear & particles physicsAstronomy and AstrophysicsGalaxies: activeAstrophysics - Astrophysics of Galaxiesgalaxies [radio continuum]Accretion (astrophysics)Galaxy[SDU]Sciences of the Universe [physics]Meteorology and Atmospheric SciencesSpace and Planetary ScienceGalaxies: jetsAstrophysics of Galaxies (astro-ph.GA)active [galaxies]Production (computer science)star formation [galaxies]Astrophysics - High Energy Astrophysical Phenomena
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