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581 - 590 of 1885 for Einstein Field EquationsSearch Results
The second-order ordinary differential equation (x^2y^')^'+x^2y^n=0.
The third-order ordinary differential equation y^(''')+alphayy^('')+beta(1-y^('2))=0.
The solution to the differential equation [D^(2v)+alphaD^v+betaD^0]y(t)=0 (1) is y(t)={e_alpha(t)-e_beta(t) for alpha!=beta; ...
A system of linear differential equations (dy)/(dz)=A(z)y, (1) with A(z) an analytic n×n matrix, for which the matrix A(z) is analytic in C^_\{a_1,...,a_N} and has a pole of ...
Gives a lower bound for the inner product (Lu,u), where L is a linear elliptic real differential operator of order m, and u has compact support.
The partial differential equation w_t-6(w+epsilon^2w^2)w_x+w_(xxx)=0, which can also be rewritten (w)_t+(-3w^2-2epsilon^2w^3+w_(xx))_x=0.
The second-order ordinary differential equation (Moon and Spencer 1961, p. 157; Zwillinger 1997, p. 166).
In bipolar coordinates, the Helmholtz differential equation is not separable, but Laplace's equation is.
The Helmholtz differential equation is not separable in bispherical coordinates.
The Helmholtz differential equation is not separable in toroidal coordinates
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