00899nam0-22002771i-450 99000403262040332120180622105648.02-222-03188-500040326219990530d1984----km-y0itay50------bafrey 001yy<<La >>martyrologe d'Adonses deux familles, ses trois recensiontexte et commentaire[publié par] Jacques Dubois et Geneviève RenaudPariséditions du Centre Nationalde la Recherche Scientifique1984484 p.24 cmSources d'Histoire Médiévale272Dubois,Jacques<1933- >153638Renaud,GenevièveITUNINARICAUNIMARCBK990004032620403321200/3 0616DIP.D.S.536FLFBCFLFBCMartyrologe d'Adon470966UNINA03708nam 22006375 450 991030040960332120200629115930.03-319-09540-410.1007/978-3-319-09540-0(CKB)3710000000227360(EBL)1968643(OCoLC)908090185(SSID)ssj0001338807(PQKBManifestationID)11704407(PQKBTitleCode)TC0001338807(PQKBWorkID)11345035(PQKB)10140195(DE-He213)978-3-319-09540-0(MiAaPQ)EBC1968643(PPN)180628178(EXLCZ)99371000000022736020140830d2015 u| 0engur|n|---|||||txtccrNumerical Simulation of Viscous Shocked Accretion Flows Around Black Holes /by Kinsuk Giri1st ed. 2015.Cham :Springer International Publishing :Imprint: Springer,2015.1 online resource (148 p.)Springer Theses, Recognizing Outstanding Ph.D. Research,2190-5053Description based upon print version of record.3-319-09539-0 Includes bibliographical references.Introduction -- Overview of Numerical Simulations on Accretion Processes and Our Objectives -- Governing Equations and Computational Methods -- Simulation Procedure and the Test of the Code -- Simulation for Inviscid Sub-Keplerian Flows and Shocks -- Simulation of Viscous Accretion Flows -- Effects of Power-law Cooling in Viscous Flows -- Conclusions and Future Plans.The work developed in this thesis addresses very important and relevant issues of accretion processes around black holes. Beginning by studying the time variation of the evolution of inviscid accretion discs around black holes, and their properties, the author investigates the change of the pattern of the flows when the strength of the shear viscosity is varied and cooling is introduced. He succeeds to verify theoretical predictions of the so called Two Component Advective Flow (TCAF) solution of the accretion problem onto black holes through numerical simulations under different input parameters. TCAF solutions are found to be stable. And thus explanations of spectral and timing properties (including Quasi-Period Oscillations, QPOs) of galactic and extra-galactic black holes based on shocked TCAF models appear to have a firm foundation.Springer Theses, Recognizing Outstanding Ph.D. Research,2190-5053AstrophysicsMathematical physicsComputer scienceMathematicsAstrophysics and Astroparticleshttps://scigraph.springernature.com/ontologies/product-market-codes/P22022Theoretical, Mathematical and Computational Physicshttps://scigraph.springernature.com/ontologies/product-market-codes/P19005Computational Mathematics and Numerical Analysishttps://scigraph.springernature.com/ontologies/product-market-codes/M1400XAstrophysics.Mathematical physics.Computer scienceMathematics.Astrophysics and Astroparticles.Theoretical, Mathematical and Computational Physics.Computational Mathematics and Numerical Analysis.523.8875015118Giri Kinsukauthttp://id.loc.gov/vocabulary/relators/aut792328BOOK9910300409603321Numerical Simulation of Viscous Shocked Accretion Flows Around Black Holes1771650UNINA