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  • Open Daily: 10am - 10pm
    Alley-side Pickup: 10am - 7pm

    3038 Hennepin Ave Minneapolis, MN
    612-822-4611

Open Daily: 10am - 10pm | Alley-side Pickup: 10am - 7pm
3038 Hennepin Ave Minneapolis, MN
612-822-4611
Non-rotating Spherically-symmetric Blackhole Spacetimes

Non-rotating Spherically-symmetric Blackhole Spacetimes

Lecian, Orchidea Maria

Paperback

Physics

ISBN10: 6208118670
ISBN13: 9786208118679
Publisher: LAP Lambert Academic Publishing
Published: Sep 28 2024
Pages: 128
Weight: 0.44
Height: 0.30 Width: 6.00 Depth: 9.00
Language: English
The book is aimed at describing spherically-symmetric non-rotating blackkhole spacetimes surrounded of media; the media considered are the Relativistic dusts, the Relativistic plasmas and the Relativistic gaseous materials. The General-Relativistic implementation established after the definition of the positions and of the velocities of the generic observer; the configurations are analytically calculated after the stress-energy tensor. The Relativistic-Astrophysical implementation is provided with after the description of the investigation of the phenomena which characterize the several blackhole environments: for these purposes, the Relativistic Jeans gas, the adiabatic perturbations of the perfect fluids and the 3-velocities perturbations of the gas are considered. The new behaviors are analytically written of the velocities. Furthermore, the paradigms of temperature-descending fluid, which characterize some of the events taking place in the corona of the AGN region of the supermassive blackholes are fixed: the new Landau-Lifshitz-Pitaevskii Magneto-Hydrodynamics of the pressure fluid is newly analytically found.

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