Titlebook: Rechnergestützte Optimierung statischer und dynamischer Systeme; Beispiele mit FORTRA Heinrich G. Jacob Book 1982 Springer-Verlag Berlin, H

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Heinrich G. Jacobed to be rotating, however be the magnitude of angular speed. The generalized astrophysical black hole is the rotating one (the Kerr black hole) which often accretes matter from its surrounding (e.g. from its binary companion) forming an accretion disk (namely X-ray binary). This accretion disk is t

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Heinrich G. Jacob those having their roots in our specialties of archaeology and geology. The average reader probably is unfamiliar with the earth sciences or the archaeological history of man. Nor does the average reader have the time and literary resources to verify all he or she reads. Our aim is to lend a helpin

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Heinrich G. Jacob those having their roots in our specialties of archaeology and geology. The average reader probably is unfamiliar with the earth sciences or the archaeological history of man. Nor does the average reader have the time and literary resources to verify all he or she reads. Our aim is to lend a helpin

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Heinrich G. Jacobing their roots in our specialties of archaeology and geology. The average reader probably is unfamiliar with the earth sciences or the archaeological history of man. Nor does the average reader have the time and literary resources to verify all he or she reads. Our aim is to lend a helping hand by

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ing their roots in our specialties of archaeology and geology. The average reader probably is unfamiliar with the earth sciences or the archaeological history of man. Nor does the average reader have the time and literary resources to verify all he or she reads. Our aim is to lend a helping hand by

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and only a parametric viscosity of unknown origin, it is necessary to rely on a promising physical solution. In a Two Component Advective Flow solution, a high-viscosity Keplerian disk is flanked by a low angular momentum and low-viscosity flow that forms a centrifugal pressure-supported shock. The

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Heinrich G. Jacobly, we calculate the critical values of both viscosity and accretion rate that cater shocks. We continue the search of shocked accretion solutions for two-temperature flow and obtain such solutions for the first time in the literature. Finally, we discuss the possible origin of mass loss from the ac

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Heinrich G. Jacob for magnetically driven outflows. We show that the flow geometry close to a black hole is quite different from a neutron star because of the strong magnetic field around the latter, which has implication on the radiative processes dominant nearby. We also obtained shock solutions for lepton dominat