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=PGE for Spherically Symmetric Configurations=
=PGE for Spherically Symmetric Configurations=
If the self-gravitating configuration that we wish to construct is spherically symmetric, then the coupled set of multidimensional, partial differential equations that serve as our [[PGE#Principal_Governing_Equations|principal governing equations]] can be simplified to a coupled set of one-dimensional, ordinary differential equations.  This is accomplished by expressing each of the multidimensional spatial operators &#8212; gradient, divergence, and Laplacian &#8212; in spherical coordinates<sup>&dagger;</sup> <math>(r, \theta, \varphi)</math> then setting to zero all derivatives that are taken with respect to the angular coordinates <math>~\theta</math> and <math>\varphi</math>.  After making this simplification, our governing equations become,
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<font size="-1">[[H_BookTiledMenu#Spherically_Symmetric_Configurations|One-Dimensional<br />PGEs]]</font>
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If the self-gravitating configuration that we wish to construct is spherically symmetric, then the coupled set of multidimensional, partial differential equations that serve as our [[PGE#Principal_Governing_Equations|principal governing equations]] can be simplified to a coupled set of one-dimensional, ordinary differential equations.  This is accomplished by expressing each of the multidimensional spatial operators &#8212; gradient, divergence, and Laplacian &#8212; in spherical coordinates<sup>&dagger;</sup> <math>(r, \theta, \varphi)</math> then setting to zero all derivatives that are taken with respect to the angular coordinates <math>\theta</math> and <math>\varphi</math>.  After making this simplification, our governing equations become,
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Part 2 of ''Spherically Symmetric Configurations'':  Structure &#8212; [[User:Tohline/SphericallySymmetricConfigurations/SolutionStrategies#Spherically_Symmetric_Configurations_.28Part_II.29|Solution Strategies]]
Part 2 of ''Spherically Symmetric Configurations'':  Structure &#8212; [[SSCpt2/SolutionStrategies#Spherically_Symmetric_Configurations_.28Part_II.29|Solution Strategies]]
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Part 2 of ''Spherically Symmetric Configurations'':  Stability &#8212; [[User:Tohline/SSC/Perturbations#Spherically_Symmetric_Configurations_.28Stability_.E2.80.94_Part_II.29|Linearization of Governing Equations]]
Part 2 of ''Spherically Symmetric Configurations'':  Stability &#8212; [[SSC/Perturbations#Spherically_Symmetric_Configurations_.28Stability_.E2.80.94_Part_II.29|Linearization of Governing Equations]]
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<li>[[SphericallySymmetricConfigurations/IndexFreeEnergy#Index_to_Free-Energy_Analyses|Index to a Variety of Free-Energy and/or Virial Analyses]]</li>
<li>[[SSC/Index|Spherically Symmetric Configurations (SSC) Index]]</li>
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Latest revision as of 16:34, 1 August 2021


PGE for Spherically Symmetric Configurations

One-Dimensional
PGEs

If the self-gravitating configuration that we wish to construct is spherically symmetric, then the coupled set of multidimensional, partial differential equations that serve as our principal governing equations can be simplified to a coupled set of one-dimensional, ordinary differential equations. This is accomplished by expressing each of the multidimensional spatial operators — gradient, divergence, and Laplacian — in spherical coordinates (r,θ,φ) then setting to zero all derivatives that are taken with respect to the angular coordinates θ and φ. After making this simplification, our governing equations become,  
 
 

Equation of Continuity

dρdt+ρ[1r2d(r2vr)dr]=0


Euler Equation

dvrdt=1ρdPdrdΦdr


Adiabatic Form of the
First Law of Thermodynamics

dϵdt+Pddt(1ρ)=0


Poisson Equation

1r2[ddr(r2dΦdr)]=4πGρ

Footnotes

See, for example, the Wikipedia discussion of integration and differentiation in spherical coordinates.

See Also


Tiled Menu

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