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000760645 019__ $$a908090185
000760645 020__ $$a9783319095400$$q(electronic book)
000760645 020__ $$a3319095404$$q(electronic book)
000760645 020__ $$z9783319095394
000760645 0247_ $$a10.1007/978-3-319-09540-0$$2doi
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000760645 050_4 $$aQB843.B55
000760645 08204 $$a523.8/875$$223
000760645 1001_ $$aGiri, Kinsuk,$$eauthor.
000760645 24510 $$aNumerical simulation of viscous shocked accretion flows around black holes /$$cKinsuk Giri.
000760645 264_1 $$aCham :$$bSpringer,$$c[2014]
000760645 264_4 $$c©2015
000760645 300__ $$a1 online resource (xxii, 129 pages) :$$billustrations.
000760645 336__ $$atext$$btxt$$2rdacontent
000760645 337__ $$acomputer$$bc$$2rdamedia
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000760645 4901_ $$aSpringer Theses,$$x2190-5053
000760645 500__ $$a"Doctoral thesis accepted by the Jadavpur University, India."
000760645 500__ $$a"Title has beem modified from 'Numerical simulation of viscous accretion flows around black holes which include shocks"."
000760645 504__ $$aIncludes bibliographical references.
000760645 5050_ $$aIntroduction -- Overview of Numerical Simulations on Accretion Processes and Our Objectives -- Governing Equations and Computational Methods -- Simulation Procedure and the Test of the Code -- Simulation for Inviscid Sub-Keplerian Flows and Shocks -- Simulation of Viscous Accretion Flows -- Effects of Powerlaw Cooling in Viscous Flows -- Conclusions and Future Plans.
000760645 506__ $$aAccess limited to authorized users.
000760645 520__ $$aThe work developed in this thesis addresses very important and relevant issues of accretion processes around black holes. Beginning by studying the time variation of the evolution of inviscid accretion discs around black holes, and their properties, the author investigates the change of the pattern of the flows when the strength of the shear viscosity is varied and cooling is introduced. He succeeds to verify theoretical predictions of the so called Two Component Advective Flow (TCAF) solution of the accretion problem onto black holes through numerical simulations under different input parameters. TCAF solutions are found to be stable. And thus explanations of spectral and timing properties (including Quasi-Period Oscillations, QPOs) of galactic and extra-galactic black holes based on shocked TCAF models appear to have a firm foundation.
000760645 588__ $$aOnline resource; title from PDF title page (SpringerLink, viewed September 12, 2014).
000760645 650_0 $$aBlack holes (Astronomy)$$xMathematical models.
000760645 650_0 $$aViscous flow.
000760645 77608 $$iPrint version:$$aGiri, Kinsuk.$$tNumerical Simulation of Viscous Shocked Accretion Flows Around Black Holes.$$dCham : Springer International Publishing, ©2014$$z9783319095394
000760645 830_0 $$aSpringer theses.
000760645 852__ $$bebk
000760645 85640 $$3SpringerLink$$uhttps://univsouthin.idm.oclc.org/login?url=http://link.springer.com/10.1007/978-3-319-09540-0$$zOnline Access$$91397441.1
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