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pro vyhledávání: '"Humi, Mayer"'
Autor:
Humi, Mayer
The paper considers Euler-Poisson equations which govern the steady state of a self gravitating, rotating, axi-symmetric fluid under the additional assumption that it is incompressible and stratified. In this setting we show that the original system
Externí odkaz:
http://arxiv.org/abs/2204.14221
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Autor:
Humi, Mayer
Many papers and monographs were written about the modeling the Earth climate and its variability. However there is still an obvious need for a module that presents the fundamentals of climate modeling to students at the undergraduate level. The prese
Externí odkaz:
http://arxiv.org/abs/1907.11067
Autor:
Humi, Mayer
The paper considers Euler-Poisson equations which govern the steady state of a self gravitating, rotating, axi-symmetric stars under the additional assumption that it is composed of incompressible stratified fluid. The original system of six nonlinea
Externí odkaz:
http://arxiv.org/abs/1807.06482
Autor:
Humi, Mayer, Roumas, John
The inner structure of a star or a primordial interstellar cloud is a major topic in classical and relativistic physics. The impact that General Relativistic principles have on this structure has been the subject of many research papers. In this pape
Externí odkaz:
http://arxiv.org/abs/1806.05719
Autor:
Humi, Mayer, Roumas, John
In the process of protostar formation, astrophysical gas clouds undergo thermodynamically irreversible processes and emit heat and radiation to their surroundings. Due the emission of this energy one can envision an idealized situation in which the g
Externí odkaz:
http://arxiv.org/abs/1605.08650
Autor:
Humi, Mayer
In this paper we consider satellite trajectories in central force field with quadratic drag using two formalisms. The first using polar coordinates in which the angular momentum plays a dominant role. The second is in Levi-Civita coordinates in which
Externí odkaz:
http://arxiv.org/abs/1507.07245
Autor:
Humi, Mayer, Tian, Zilu
In this paper we develop two models for the steady states and evolution of two dimensional isothermal self gravitating and rotating incompressible gas which are based on the hydrodynamic equations for stratified fluid. The first model is for the stea
Externí odkaz:
http://arxiv.org/abs/1504.02798