Search results for "Cosmology"

showing 10 items of 2905 documents

Black hole lightning due to particle acceleration at subhorizon scales

2015

Supermassive black holes with masses of millions to billions of solar masses are commonly found in the centers of galaxies. Astronomers seek to image jet formation using radio interferometry, but still suffer from insufficient angular resolution. An alternative method to resolve small structures is to measure the time variability of their emission. Here, we report on gamma-ray observations of the radio galaxy IC 310 obtained with the MAGIC telescopes revealing variability with doubling time scales faster than 4.8 min. Causality constrains the size of the emission region to be smaller than 20\% of the gravitational radius of its central black hole. We suggest that the emission is associated …

Black HolesRadio galaxyAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsVery High Energy Gamma AstronomyBlack Holes Very High Energy Gamma Astronomy Active Galactic NucleiX-shaped radio galaxysupermassive black hole ; jet formation ; IC 310 ; MAGIC telescopesAstrophysics::Galaxy AstrophysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)astro-ph.HESupermassive black holeta115MultidisciplinaryPhysicsActive Galactic NucleiAstronomy and AstrophysicsGalaxyIntermediate-mass black holeStellar black holeElectrónicaFísica nuclearddc:500Spin-flipElectricidadAstrophysics - High Energy Astrophysical PhenomenaSchwarzschild radius
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Black Holes in Extended Gravity Theories in Palatini Formalism

2013

We consider several physical scenarios where black holes within classical gravity theories including R 2 and Ricci-squared corrections and formulated a la Palatini can be analytically studied.

Black holePhysicsGeneral Relativity and Quantum CosmologyFormalism (philosophy of mathematics)Classical mechanicsAstrophysics::High Energy Astrophysical PhenomenaField equation
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Non-supersymmetric Extremal Black Holes: First-Order Flows and Stabilisation Equations

2013

We review the results of [1, 2] on reducing the second-order equations of motion for stationary extremal black holes in four-dimensional \({\textit{N}}\,=\,2\) supergravity to first-order flow equations and further to non-differential stabilisation equations.

Black holePhysicsGeneral Relativity and Quantum CosmologyHarmonic functionFlow (mathematics)SupergravityExtremal black holeEquations of motionFirst orderMathematical physics
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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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Numerical Simulations of Relativistic Wind Accretion onto Black Holes Using Godunov-Type Methods

2001

We have studied numerically the so-called Bondi-Hoyle (wind) accretion onto a rotating black hole in general relativity. We have used the Kerr-Schild form of the Kerr metric, free of coordinate singularities at the black hole horizon. The ‘test-fluid’ approximation has been adopted, assuming no dynamical evolution of the gravitational field. We have used a formulation of the relativistic hydrodynamic equations which casts them into a first-order hyperbolic system of conservation laws. Our studies were performed using a Godunov-type scheme based on Marquina’s flux-formula.

Black holePhysicsGeneral Relativity and Quantum CosmologyNumerical relativityClassical mechanicsRotating black holeBinary black holeEvent horizonAstrophysics::High Energy Astrophysical PhenomenaWhite holeExtremal black holeAstrophysicsCharged black hole
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NONSINGULAR BLACK HOLES IN PALATINI EXTENSIONS OF GENERAL RELATIVITY

2015

An introduction to extended theories of gravity formulated in metric-affine (or Palatini) spaces is presented. Focusing on spherically symmetric configurations with electric fields, we will see that in these theories the central singularity present in General Relativity is generically replaced by a wormhole structure. The resulting space-time becomes geodesically complete and, therefore, can be regarded as non-singular. We illustrate these properties considering two different models, namely, a quadratic f(R) theory and a Born-Infeld like gravity theory.

Black holePhysicsGeneral Relativity and Quantum CosmologyNumerical relativityGravity (chemistry)SingularityGeneral relativityStructure (category theory)WormholeRicci curvatureMathematical physicsThe Thirteenth Marcel Grossmann Meeting
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The NHXM observatory

2011

Exploration of the X-ray sky has established X-ray astronomy as a fundamental astrophysical discipline. While our knowledge of the sky below 10 keV has increased dramatically (∼8 orders of magnitude) by use of grazing incidence optics, we still await a similar improvement above 10 keV, where to date only collimated instruments have been used. Also ripe for exploration is the field of X-ray polarimetry, an unused fundamental tool to understand the physics and morphology of X-ray sources. Here we present a novel mission, the New Hard X-ray Mission (NHXM) that brings together for the first time simultaneous high-sensitivity, hard-X-ray imaging, broadband spectroscopy and polarimetry. NHXM will…

Black-holesAcceleration mechanismCosmic Visionmedia_common.quotation_subjectPolarimetry7. Clean energy01 natural sciencesMissionsCosmologyPhysical cosmologyNon-thermal emissionAcceleration mechanism; Accretion physics; Black-holes; Compact objects; Cosmology; Missions; Non-thermal emission; X-ray imaging; X-ray polarimetry; Astronomy and Astrophysics; Space and Planetary ScienceObservatory0103 physical sciencesBroadbandX-ray polarimetry010303 astronomy & astrophysicsCompact objectsmedia_commonPhysics010308 nuclear & particles physicsX-ray imagingVegaAstronomyAstronomy and AstrophysicsAccretion physicsCosmologySkySpace and Planetary ScienceExperimental Astronomy
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ARES I: WASP-76 b, A Tale of Two HST Spectra

2020

We analyse the transmission and emission spectra of the ultra-hot Jupiter WASP-76b, observed with the G141 grism of the Hubble Space Telescope's Wide Field Camera 3 (WFC3). We reduce and fit the raw data for each observation using the open-source software Iraclis before performing a fully Bayesian retrieval using the publicly available analysis suite TauRex 3. Previous studies of the WFC3 transmission spectra of WASP-76 b found hints of titanium oxide (TiO) and vanadium oxide (VO) or non-grey clouds. Accounting for a fainter stellar companion to WASP-76, we reanalyse this data and show that removing the effects of this background star changes the slope of the spectrum, resulting in these vi…

Brightness010504 meteorology & atmospheric sciencesExoplanet atmospheres; Exoplanet atmospheric composition; Hubble Space Telescope; Astrophysics - Earth and Planetary AstrophysicsFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsAstronomy & AstrophysicsExoplanet atmospheres; Exoplanet atmospheric composition; Hubble Space Telescope01 natural sciencesSpectral lineAtmosphereJupiterHAT-P-7B0103 physical sciencesHubble Space TelescopeAstrophysics::Solar and Stellar AstrophysicsEmission spectrumMOLECULAR LINE LISTS010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesHOTPhysicsEarth and Planetary Astrophysics (astro-ph.EP)Science & TechnologyAstronomy and AstrophysicsATMOSPHEREGIANT EXOPLANETGrismRESOLUTIONTransmission (telecommunications)Exoplanet atmospheric composition13. Climate actionSpace and Planetary Science[SDU]Sciences of the Universe [physics]Physical SciencesINFERENCEAstrophysics::Earth and Planetary Astrophysics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Wide Field Camera 3STARSExoplanet atmospheresAstrophysics - Earth and Planetary Astrophysics
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First M87 Event Horizon Telescope Results. IV. Imaging the Central Supermassive Black Hole

2019

We present the first Event Horizon Telescope (EHT) images of M87, using observations from April 2017 at 1.3 mm wavelength. These images show a prominent ring with a diameter of ~40 μas, consistent with the size and shape of the lensed photon orbit encircling the "shadow" of a supermassive black hole. The ring is persistent across four observing nights and shows enhanced brightness in the south. To assess the reliability of these results, we implemented a two-stage imaging procedure. In the first stage, four teams, each blind to the others' work, produced images of M87 using both an established method (CLEAN) and a newer technique (regularized maximum likelihood). This stage allowed us to av…

Brightness010504 meteorology & atmospheric sciencesgalaxies: jetAstronomyblack hole physicsFOS: Physical sciencesgalaxies: individualtechniques: image processingAstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)galaxies: individual: M8701 natural sciencesSynthetic dataGeneral Relativity and Quantum Cosmologygalaxies: individual (M87)0103 physical sciencesimage processing [Techniques]010303 astronomy & astrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)0105 earth and related environmental sciencesEvent Horizon TelescopePhysicsGround truthSupermassive black holetechniques: high angular resolutionAstronomy and AstrophysicsBlack hole physicsgalaxies: jetsindividual (M87) [Galaxies]Astrophysics - Astrophysics of Galaxiesblack hole physic3. Good healthOrbitInterferometryhigh angular resolution [Techniques]Space and Planetary Sciencetechniques: interferometricAstrophysics of Galaxies (astro-ph.GA)interferometric [Techniques]jets [Galaxies]Deconvolution[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astrophysics - Instrumentation and Methods for Astrophysics
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Monitoring the Morphology of M87* in 2009-2017 with the Event Horizon Telescope

2020

All authors: Wielgus, Maciek; Akiyama, Kazunori; Blackburn, Lindy; Chan, Chi-kwan; Dexter, Jason; Doeleman, Sheperd S.; Fish, Vincent L.; Issaoun, Sara; Johnson, Michael D.; Krichbaum, Thomas P.; Lu, Ru-Sen; Pesce, Dominic W.; Wong, George N.; Bower, Geoffrey C.; Broderick, Avery E.; Chael, Andrew; Chatterjee, Koushik; Gammie, Charles F.; Georgiev, Boris; Hada, Kazuhiro Loinard, Laurent; Markoff, Sera; Marrone, Daniel P.; Plambeck, Richard; Weintroub, Jonathan; Dexter, Matthew; MacMahon, David H. E.; Wright, Melvyn; Alberdi, Antxon; Alef, Walter; Asada, Keiichi; Azulay, Rebecca; Baczko, Anne-Kathrin; Ball, David; Baloković, Mislav; Barausse, Enrico; Barrett, John; Bintley, Dan; Boland, Wilf…

Brightness1663Active galactic nucleus010504 meteorology & atmospheric sciences1346Event horizonAstronomyAstrophysics::High Energy Astrophysical PhenomenaGalaxy accretion disksFOS: Physical sciencesAstrophysicsF500Astrophysics::Cosmology and Extragalactic Astrophysics01 natural sciences5752033Settore FIS/05 - Astronomia e AstrofisicaSupermassive black holes0103 physical sciencesVery-long-baseline interferometryAstronomy Astrophysics and Cosmology1769010303 astronomy & astrophysicsComputer Vision and Robotics (Autonomous Systems)Astronomy data modelingVery long baseline interferometry0105 earth and related environmental sciences162Black holes; Galaxy accretion disks; Galaxy accretion; Supermassive black holes; Active galactic nuclei; Low-luminosity active galactic nuclei; Very long baseline interferometry; Astronomy data modeling; Radio interferometryEvent Horizon TelescopePhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Active galactic nucleiSupermassive black holeBlack holesAstronomy and Astrophysics16Galaxy accretion562Position angleGalaxyLow-luminosity active galactic nucleiMedical Image ProcessingSpace and Planetary ScienceRadio interferometryAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]1859
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