- Lane-Emden equation
In
astrophysics , the Lane-Emden equation isPoisson's equation for the gravitational potential of a self-gravitating, spherically symmetricpolytropic fluid. It is named after the astrophysicistsJonathan Homer Lane andRobert Emden . Its solution provides the run of pressure and density with radius "r"::
where
:
and
:
where the subscripts "c" refer to the values of pressure and density at the center of the sphere. Here is the polytropic index in which the pressure and density of the gas are related by the polytropic equation
:
Note that solutions to the Lane-Emden equation for a given polytropic index are known as
polytrope s of index . Physically, hydrostatic equilibrium connects the gradient of the potential, the density, and the gradient of the pressure, whereas Poisson's equation connects the potential with the density. It should be clear then if we know nothing about the gas other than the way pressure and density vary with respect to one another, we can reach a solution, in principle. The particular choice of a polytropic gas as given above makes the mathematical statement of the problem particularly succinct, resulting in the Lane-Emden equation. This is a useful "zeroth order" solution for self-gravitating gaseous spheres such as stars. It is still a useful approximation in certain situations, but typically it is a rather limiting assumption.olutions of equation
It is known that the equation can be solved analytically when "n" = 0, 1 or 5:
The equation reduces to a
Spherical Bessel differential equation when "n" = 1 which gives asinc function .References
*.
External links
*MathWorld | urlname=Lane-EmdenDifferentialEquation | title=Lane-Emden Differential Equation
* Horedt, George Paul ( 1986 ) PDFlink| [http://articles.adsabs.harvard.edu/cgi-bin/nph-iarticle_query?1986Ap%26SS.126..357H&data_typePDF_HIGH&whole_paperYES&typePRINTER&filetype.pdf 'Seven-digit tables of Lane-Emden functions'] | 5.9MB , "Astrophysics and Space Science" vol. 126, no. 2, Oct. 1986, p. 357-408. ( ISSN 0004-640X ). Collected at the Smithsonian/NASA Astrophysical Data System.
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