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=Solving the Poisson Equation=
=Common Theme: Determining the Gravitational Potential for Axisymmetric Mass Distributions=
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When constructing rotating equilibrium configurations that obey a [[SR#Time-Independent_Problems|barotropic equation of state]], keep in mind that certain physical variable profiles should be avoided because they will lead to structures that are unstable toward the dynamical development of shape-distorting or ''convective''-type motions.  Here are a few well-known examples.
 
You have arrived at this page from our [[H_BookTiledMenu#Axisymmetric_Equilibrium_Structures|''Tiled Menu'']] by clicking on the chapter title that is also identified, below, by the light-blue-colored icon.  You may proceed directly to that chapter by clicking (again) on that highlighted chapter icon.  However, we have brought you to this intermediate page in order to bring to your attention that there are a number of additional chapters that have a strong thematic connection to the chapter you have selected.  The common thread is the "Key Equation" titled, ''Gravitational Potential of an Axisymmetric Mass Distribution'', that appears at the top of the following set of chapter synopses.
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Revision as of 13:07, 10 September 2021

Common Theme: Determining the Gravitational Potential for Axisymmetric Mass Distributions

Solving the
Poisson Equation

You have arrived at this page from our Tiled Menu by clicking on the chapter title that is also identified, below, by the light-blue-colored icon. You may proceed directly to that chapter by clicking (again) on that highlighted chapter icon. However, we have brought you to this intermediate page in order to bring to your attention that there are a number of additional chapters that have a strong thematic connection to the chapter you have selected. The common thread is the "Key Equation" titled, Gravitational Potential of an Axisymmetric Mass Distribution, that appears at the top of the following set of chapter synopses.  
 
 
 
 

See Also

  1. Shortly after their equation (3.2), Marcus, Press & Teukolsky make the following statement: "… we know that an equilibrium incompressible configuration must rotate uniformly on cylinders (the famous "Poincaré-Wavre" theorem, cf. Tassoul 1977, &Sect;4.3) …"


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