Math 2.0

Integral equations Wiener-Hopf equations Example

Chandrasekhar's X- and Y-functions

Builds on Chandrasekhar's H-functionRadiative transfer equationNonlinear integral equation

Example

Let τ1>0\tau_1 > 0 be the optical thickness of a plane-parallel slab. Let Ψ\Psi be an even polynomial, the characteristic function, with Ψ≥0\Psi \ge 0 on [0,1][0, 1] and ∫01Ψ dμ≤12\int_0^1 \Psi\, d\mu \le \frac{1}{2}. Chandrasekhar's X- and Y-functions are the functions XX and YY on [0,1][0, 1] that solve the system X(μ)=1+μ∫01Ψ(μ′)μ+μ′[X(μ)X(μ′)−Y(μ)Y(μ′)] dμ′,X(\mu) = 1 + \mu \int_0^1 \frac{\Psi(\mu')}{\mu + \mu'} \bigl[X(\mu) X(\mu') - Y(\mu) Y(\mu')\bigr]\, d\mu', Y(μ)=e−τ1/μ+μ∫01Ψ(μ′)μ−μ′[Y(μ)X(μ′)−X(μ)Y(μ′)] dμ′.Y(\mu) = e^{-\tau_1/\mu} + \mu \int_0^1 \frac{\Psi(\mu')}{\mu - \mu'} \bigl[Y(\mu) X(\mu') - X(\mu) Y(\mu')\bigr]\, d\mu'. In the second equation the bracket vanishes at μ′=μ\mu' = \mu, so the integrand has no singularity there. This is a system of two coupled nonlinear integral equations for the two unknowns.

Check of two limits. For τ1=0\tau_1 = 0, the constant functions X=1X = 1 and Y=1Y = 1 solve the system: both brackets vanish and e0=1e^{0} = 1. This is a slab of thickness 00, which lets all light through. As τ1→∞\tau_1 \to \infty, the term e−τ1/μe^{-\tau_1/\mu} tends to 00; with Y=0Y = 0 the first equation becomes the equation of Chandrasekhar's H-function, X=HX = H.

Remarks

The functions XX and YY give the light reflected and transmitted by a slab of finite thickness in the radiative transfer equation, while HH handles a half-space. In the conservative case ∫01Ψ dμ=12\int_0^1 \Psi\, d\mu = \frac{1}{2} the system does not determine XX and YY uniquely, and an extra condition selects the physical solution.

Reading path

To understand this page from the ground up, read these 8 pages in order. The foundations come first.

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  1. Exponential integral concept
  2. Nonlinear integral equation concept
  3. Radiative transfer equation example
  4. Wiener–Hopf equation concept
  5. Wiener–Hopf method concept
  6. Milne problem example
  7. Chandrasekhar's H-function example
  8. Chandrasekhar's X- and Y-functions example

Further reading

  1. Web https://en.wikipedia.org/wiki/Chandrasekhar%27s_X-_and_Y-function
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MSC45G15, 85A25
Instance ofNonlinear integral equation
UsesChandrasekhar's H-function, Radiative transfer equation, Nonlinear integral equation
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