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An arbitrarily small seed perturbation flips a later Bessel sign

Statement

At x=1, every Jn(1) is positive and tends to zero as n→∞, whereas the complementary recurrence solution Dn(1) defined in Complementary solution for the integer Bessel recurrence is positive and unbounded for n≥1. Hence, for every ε>0, the perturbed seed pair J~0=J0(1)−εD0(1),J~1=J1(1)−εD1(1) can be arbitrarily close to the exact seeds, yet its forward recurrence solution J~n=Jn(1)−εDn(1) is negative for some index where the exact Jn(1) is positive. This is a recurrence-sensitivity example, not a claim that every floating-point implementation follows this particular error direction.

Facts & Assumptions

Given: The Bessel series at x=1, the order recurrence, and the complementary solution D.

[F1]

Integer-order Bessel series: at x=1, Jn(1)=∑k≥0(−1)k(1/2)2k+n/(k!(k+n)!).

[F2]

Convergence and geometric tails for integer-order Bessel series: these series converge absolutely, and their successive absolute term ratio is 1/[4(k+1)(k+n+1)] at x=1.

[F3]

Bessel differential equations and order recurrences from the series: Jn+1(1)=2nJn(1)−Jn−1(1) for n≥1.

[F4]

Complementary solution for the integer Bessel recurrence: D0=−J1, D1=J0, and Dn+1=2nDn−Dn−1 at x=1.

Proof

1.1F1F2algebra

Let ak=(1/2)2k+n/(k!(k+n)!). By [F2], the positive terms ak decrease strictly to zero. Grouping the alternating series in consecutive pairs gives Jn(1)=(a0−a1)+(a2−a3)+⋯>0. Also (k+n)!≥n!, so 0<Jn(1)≤∑k≥0ak≤2−nn!∑k≥0(1/4)kk!=2−ne1/4n!⟶0. In particular, J0(1)≥1−1/4=3/4 and J1(1)≥1/2−1/16=7/16.

2.1F1F3F4step 1.1induction

By [F4], D0(1)=−J1(1)<0 and D1(1)=J0(1)>0; hence D2=2D1−D0>D1>0. If n≥2 and Dn≥Dn−1>0, then Dn+1=2nDn−Dn−1≥(2n−1)Dn≥3Dn. Induction gives Dn≥3n−2D2 for n≥2, so Dn→∞.

3.1F1F3F4step 1.1step 2.1algebra∎

The exact sequence Jn−εDn obeys the same linear recurrence by [F3] and [F4], so it is the forward-recurrence solution from the displayed perturbed seeds. Since Jn→0 and Dn→∞ by steps 1.1 and 2.1, some finite n satisfies εDn>Jn. At that index J~n<0<Jn. The seed differences have magnitudes ε∣D0∣ and ε∣D1∣, which tend to zero with ε.

Depends on

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