अवकल समीकरण
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हल की विधि
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सामान्य हल
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चर अलग करने योग्य समीकरण (Separable equations)
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First-order, separable in x and y (general case, see below for special cases)[1]
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Separation of variables (divide by P2Q1).
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First-order, separable in x[2]
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Direct integration.
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First-order, autonomous, separable in y[2]
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Separation of variables (divide by F).
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First-order, separable in x and y[2]
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Integrate throughout.
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General first-order equations
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First-order, homogeneous[2]
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Set y = ux, then solve by separation of variables in u and x.
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First-order, separable[1]
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Separation of variables (divide by xy).
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If N = M, the solution is xy = C.
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Exact differential, first-order[2]
where
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Integrate throughout.
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where Y(y) and X(x) are functions from the integrals rather than constant values, which are set to make the final function F(x, y) satisfy the initial equation.
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Inexact differential, first-order[2]
where
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Integration factor μ(x, y) satisfying
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If μ(x, y) can be found:
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General second-order equations
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Second-order, autonomous[3]
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Multiply equation by 2dy/dx, substitute , then integrate twice.
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Linear equations (up to nth order)
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First-order, linear, inhomogeneous, function coefficients[2]
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Integrating factor: .
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Second-order, linear, inhomogeneous, constant coefficients[4]
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Complementary function yc: assume yc = eαx, substitute and solve polynomial in α, to find the linearly independent functions .
Particular integral yp: in general the method of variation of parameters, though for very simple r(x) inspection may work.[2]
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If b2 > 4c, then:
If b2 = 4c, then:
If b2 < 4c, then:
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nth-order, linear, inhomogeneous, constant coefficients[4]
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Complementary function yc: assume yc = eαx, substitute and solve polynomial in α, to find the linearly independent functions .
Particular integral yp: in general the method of variation of parameters, though for very simple r(x) inspection may work.[2]
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Since αj are the solutions of the polynomial of degree n: , then:
for αj all different,
for each root αj repeated kj times,
for some αj complex, then setting α = χj + iγj, and using Euler's formula, allows some terms in the previous results to be written in the form
where ϕj is an arbitrary constant (phase shift).
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