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单词 difference equation
释义
difference equation

Mathematics
  • Let u0, u1, u2,…, un,… be a sequence. If the terms satisfy the first‐order difference equation un + 1 + aun = 0, it is easy to see that un = A(−a)n, where A( = u0) is arbitrary.

    Suppose that the terms satisfy the second‐order difference equation un + 2 + aun + 1 + bun = 0. Let α‎ and β‎ be the roots of the quadratic ‘auxiliary equation’ x2 + ax + b = 0. If α‎ ≠ β‎, then un = Aα‎n + Bβ‎n, and if α‎ = β‎ ≠ 0, then un = (A + Bn)α‎n, where A and B are arbitrary constants. For example, the Fibonacci sequence is given by the difference equation un + 2 = un + 1 + un, with u0 = 1 and u1 = 1, and the above method gives Binet’s formula

    un=12(1+52)n12(152)n.

    The above theory generalizes to linear constant coefficient difference equations (see linear equation) of higher orders, with the solutions forming a vector space with dimension equalling the order. The solutions to an inhomogeneous linear difference equation are a particular solution added to the homogeneous solutions. Difference equations, also called recurrence relations, do not necessarily have constant coefficients like those considered above. Such difference equations may be approached using generating functions.


Electronics and Electrical Engineering
  • 1. An equation that defines an indexed sequence of numbers by giving some initial values and describing how subsequent members of the sequence are related to immediate neighbours. For example, the Fibonacci sequence defines f0 and f1 as 1 and then recursively defines fn = fn−1 + fn−2 for n > 1.

    2. A discrete form of differentiation applied to sequences of real numbers. For example, given the ordered sequence r1, r2, r3, … we can define the first difference as the sequence Δ(r1),Δ(r2),Δ(r3), … defined by

    Δ(rn)=rn+1rn

    See also differential equation.


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