Mingarelli identity

In the field of ordinary differential equations, the Mingarelli identity (coined by Philip Hartman[1]) is a theorem that provides criteria for the oscillation and non-oscillation of solutions of some linear differential equations in the real domain. It extends the Picone identity from two to three or more differential equations of the second order. Its most basic form appears here.

The identity

Consider the n solutions of the following (uncoupled) system of second order linear differential equations over the t-interval [a, b]. (p_{i}(t)x_{i}^{\prime })^{\prime }+q_{i}(t)x_{i}=0,\,\,\,\,\,\,\,\,\,\,x_{i}(a)=1,\,\,x_{i}^{\prime }(a)=R_{i}\, where i=1,2,\ldots ,n. Let \Delta denote the forward difference operator, i.e., \Delta x_{i}=x_{i+1}-x_{i}. The second order difference operator is found by iterating the first order operator as in \Delta ^{2}(x_{i})=\Delta (\Delta x_{i})=x_{i+2}-2x_{i+1}+x_{i}, with a similar definition for the higher iterates.

Leaving out the independent variable t for convenience, and assuming the x_{i}(t)\neq 0 on (a, b], there holds the identity,[2]

{\begin{aligned}x_{n-1}^{2}\Delta ^{n-1}(p_{1}r_{1})]_{a}^{b}&=\int _{a}^{b}(x_{n-1}^{\prime })^{2}\Delta ^{n-1}(p_{1})-\int _{a}^{b}x_{n-1}^{2}\Delta ^{n-1}(q_{1})-\sum _{k=0}^{n-1}C(n-1,k)(-1)^{n-k-1}\int _{a}^{b}p_{k+1}W^{2}(x_{k+1},x_{n-1})/x_{k+1}^{2},\end{aligned}}

where r_{i}=x_{i}^{\prime }/x_{i} is a logarithmic derivative, W(x_{i},x_{j})=x_{i}^{\prime }x_{j}-x_{i}x_{j}^{\prime }, is a Wronskian and the C(n-1,k) are binomial coefficients. When n=2 this reduces to the Picone identity.

The above identity leads quickly to the following comparison theorem for three linear differential equations,[2] extending the Sturm–Picone comparison theorem.

Let p_{i},\,q_{i},\, i = 1, 2, 3 be real-valued continuous functions on the interval [a, b] and let

  1. (p_{1}(t)x_{1}^{\prime })^{\prime }+q_{1}(t)x_{1}=0,\,\,\,\,\,\,\,\,\,\,x_{1}(a)=1,\,\,x_{1}^{\prime }(a)=R_{1}\,
  2. (p_{2}(t)x_{2}^{\prime })^{\prime }+q_{2}(t)x_{2}=0,\,\,\,\,\,\,\,\,\,\,x_{2}(a)=1,\,\,x_{2}^{\prime }(a)=R_{2}\,
  3. (p_{3}(t)x_{3}^{\prime })^{\prime }+q_{3}(t)x_{3}=0,\,\,\,\,\,\,\,\,\,\,x_{3}(a)=1,\,\,x_{3}^{\prime }(a)=R_{3}\,

be three homogeneous linear second order differential equations in self-adjoint form with

p_{i}(t)>0\, for each i and for all t in [a, b], and where the R_{i} are arbitrary real numbers.

Assume that for all t in [a, b] we have,

\Delta ^{2}(q_{1})\geq 0,
\Delta ^{2}(p_{1})\leq 0,
\Delta ^{2}(p_{1}(a)R_{1})\leq 0.

If x_{1}(t)>0 on [a, b], and x_{2}(b)=0, then any solution x_{3}(t) has at least one zero in [a, b].

References

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