Bourbaki

§ 2. Asymptotic expansions

1. Scales of comparison

Let E be a set filtered by a filter with base F\mathfrak{F}, and K a non-discrete valued field (most often K=RK = \mathbf{R} or K=CK = \mathbf{C}). In the set of functions in H(F,K)\mathscr{H}(\mathfrak{F}, K) not equivalent to 0 modulo R∞R_\infty (that is, those for which in every set in F\mathfrak{F} there is at least one point where the function does not vanish), the relation " f≪gf \ll g or f=gf = g" is an order relation.

Definition 1

One says that a subset E\mathscr{E} of H(F,K)\mathscr{H}(\mathfrak{F}, K) formed of functions not equivalent to 0 modulo R∞R_\infty is a comparison scale when E\mathscr{E} is totally ordered by the relation " f≪gf \ll g or f=gf = g".

In other words, if ff and gg are functions in E\mathscr{E} then one (and only one) of the relations f≪gf \ll g, g≪fg \ll f, f=gf = g always holds. It follows that on E\mathscr{E} the relation f≍gf \asymp g (and a fortiori ∣f∣∼a ∣g∣|f| \sim a\,|g|, where aa is a number >0> 0) implies f=gf = g.

Every subset of a comparison scale is clearly also a comparison scale.

Example 1

For xx real and tending to +∞+\infty the set of functions xαx^\alpha (α\alpha an arbitrary real number) is a comparison scale. The same is true for the functions (x−a)α(x-a)^\alpha when F\mathfrak{F} is the set of open intervals with left-hand endpoint aa.

Example 2

For zz complex tending to ∞\infty the set of functions znz^n (nn a rational integer) is a comparison scale; so are the functions (z−a)n(z-a)^n when F\mathfrak{F} is the trace on the complement of the point a∈Ca \in \mathbf{C} of the filter of neighbourhoods of this point.

Cited by 1

Cited by Example 5

Example 3

Let F be normed space; the family of functions ∥x−a∥α\|x-\mathbf{a}\|^\alpha (α\alpha an arbitrary real number) is a comparison scale when F\mathfrak{F} is the trace on the complement of a\mathbf{a} of the filter of neighbourhoods of this point. Note that if pp and qq are two distinct norms on F, the union of the two comparison scales (p(x−a))α(p(x-\mathbf{a}))^\alpha and (q(x−a))α(q(x-\mathbf{a}))^\alpha is not in general a comparison scale.

Example 4

For xx real tending to +∞+\infty the family E\mathscr{E} of functions of the form exp⁡(p(x))\exp(p(x)), where pp runs through the set of polynomials without constant term (with real coefficients), is a comparison scale: it suffices to remark that the quotient of two functions in E\mathscr{E} is again in E\mathscr{E}, and that a function exp⁡(p(x))\exp(p(x)) must tend either to 0 or +∞+\infty if p≠0p \neq 0; indeed, p(x)∼αxnp(x) \sim \alpha x^n where n>0n > 0 and α≠0\alpha \neq 0; if α>0\alpha > 0 then p(x)>12αxnp(x) > \frac{1}{2} \alpha x^n for xx sufficiently large; if α<0\alpha < 0 then p(x)<12αxnp(x) < \frac{1}{2} \alpha x^n for xx sufficiently large; in the first case exp⁡(p(x))\exp(p(x)) tends to +∞+\infty, in the second to 0.

Example 5

For xx real tending to +∞+\infty the set E\mathscr{E} of functions of the form xα(log⁡x)βx^\alpha (\log x)^\beta (defined for x>1x > 1), where α\alpha and β\beta are arbitrary real numbers, is a comparison scale. Indeed, here again the quotient of two functions in E\mathscr{E} is a function in E\mathscr{E}; it is enough to show that if α\alpha and β\beta are not both zero then xα(log⁡x)βx^\alpha (\log x)^\beta tends to 0 or +∞+\infty; this is clear if α=0,β≠0\alpha = 0, \beta \neq 0; if α>0\alpha > 0 one has (log⁡x)−β≪xα(\log x)^{-\beta} \ll x^\alpha, and if α<0\alpha < 0 one has (log⁡x)β≪x−α(\log x)^\beta \ll x^{-\alpha} for any β\beta, whence the proposition.

Note that this last comparison scale is a totally ordered set (for the relation "f ≪\ll g" or f=gf = g") whose order structure is isomorphic to the lexicographic order on R2\mathbf{R}^2 (Set Theory, III, p. 157); recall that in this structure the relation (α,β)<(γ,δ)(\alpha, \beta) < (\gamma, \delta) means "α<γ\alpha < \gamma, or α=γ\alpha = \gamma and β<δ\beta < \delta").

Similarly, the scale formed by the functions exp⁡(p(x))\exp(p(x)), where pp runs through the set P0P_0 of polynomials with no constant term, has order structure isomorphic to the order structure of P0P_0, in which the relation p<qp < q implies that the dominant term of the polynomial q−pq - p has a coefficient >0> 0 (cf. Alg., VI. 19, Example 2).

Let φ\varphi be a map from a set F into E, such that φ−1(F)\varphi^{-1}(\mathfrak{F}) is a filter base on F. If E\mathscr{E} is a comparison scale on E (for the filter base F\mathfrak{F}) then the functions f∘φf \circ \varphi, as ff runs through E\mathscr{E}, form a comparison scale on F (for the filter base φ−1(F)\varphi^{-1}(\mathfrak{F})).

Cites 1

Cites Example 2

2. Principal parts and asymptotic expansions

Let E\mathscr{E} be a comparison scale formed by functions with values in a non-discrete valued field K. Let V be a normed space over K, and let f\mathbf{f} be a function in H(F,V)\mathscr{H}(\mathfrak{F}, V); if there are a function g∈Eg \in \mathscr{E} and an element a≠0\mathbf{a} \neq 0 in V such that f∼ag\mathbf{f} \sim \mathbf{a}g, one says that ag\mathbf{a}g is a principal part of f\mathbf{f} relative to the scale E\mathscr{E}. From def. 1 of V, p. 10, f\mathbf{f} can have only one principal part relative to E\mathscr{E}, for if g1, g2g_1,\ g_2 are two functions in E\mathscr{E} and a1, a2\mathbf{a}_1,\ \mathbf{a}_2 are two ≠0\neq 0 elements of V, then the relation a1g1∼a2g2\mathbf{a}_1 g_1 \sim \mathbf{a}_2 g_2 implies ∣g1∣≍∣g2∣|g_1| \asymp |g_2| and consequently g1=g2g_1 = g_2, whence (a2−a1)g1≪g1(\mathbf{a}_2 - \mathbf{a}_1)g_1 \ll g_1, and since g1g_1 is not identically zero on any set in E\mathscr{E} this implies a2=a1\mathbf{a}_2 = \mathbf{a}_1.

If f\mathbf{f} has a principal part relative to a comparison scale E\mathscr{E} it has the same principal part relative to every comparison scale E′⊃E\mathscr{E}' \supset \mathscr{E}.

Example 1

For xx real (resp. complex) tending to +∞+\infty (resp. ∞\infty), every polynomial a0xn+a1xn−1+…+ana_0 x^n + a_1 x^{n-1} + \ldots + a_n with coefficients in V, such that a0≠0a_0 \neq 0, has principal part a0xna_0 x^n with respect to the scale xnx^n (or any scale containing the xnx^n). It follows that every rational fraction a0xn+⋯+amb0xn+⋯+bn\frac{a_0 x^n + \cdots + a_m}{b_0 x^n + \cdots + b_n} with real or complex coefficients such that a0b0≠0a_0 b_0 \neq 0 has principal part a0b0xn\frac{a_0}{b_0} x^n with respect to the same scale.

Example 2

A function may be comparable to all the functions of a scale and yet not admit a principal part with respect to this scale. For example, for xx real tending to +∞+\infty, x\sqrt{x} has no principal part with respect to the scale xnx^n where nn is a rational integer; log⁡x\log x has no principal part with respect to the scale of xαx^\alpha (α\alpha arbitrary real); exp⁡(log⁡x)\exp(\sqrt{\log x}) and x′=exlog⁡xx' = e^{x \log x} have no principal part with respect to the scale of the xα(log⁡x)βx^\alpha (\log x)^\beta, nor with respect to the scale of the exp⁡(p(x))\exp(p(x)) (pp a polynomial with no constant term).

The concept of principal part admits extensive generalization. Suppose that a function f∈H(F,V)f \in \mathscr{H}(\mathfrak{F}, V) has a principal part a1g1a_1 g_1 with respect to a scale E\mathscr{E}; the relation f∼a1g1f \sim a_1 g_1 is equivalent to f−a1g1≪g1f - a_1 g_1 \ll g_1 (V, p. 216, def. 4); to study the function ff more closely one is thus led to consider the function f−a1g1f - a_1 g_1. If this function has a principal part a2g2a_2 g_2 with respect to E\mathscr{E} one must have g2≪g1g_2 \ll g_1 and f−a1g1−a2g2≪g2f - a_1 g_1 - a_2 g_2 \ll g_2.

More generally, suppose that the scale E\mathscr{E} is written parametrically in the form (gα)(g_\alpha) where α\alpha runs through a set of indices AA endowed with a totally ordered structure isomorphic to the opposite of the order structure of E\mathscr{E}: the relation α<β\alpha < \beta is thus equivalent to gβ≪gαg_\beta \ll g_\alpha. In these circumstances:

Cites 1

Cites V § 1. Comparison of functions on a filtered set

Definition 2

One says that a function* f∈H(F,V)f \in \mathscr{H}(\mathfrak{F}, V) admits an asymptotic expansion to precision gαg_\alpha (relative to the scale E\mathscr{E}*) if there exists a family (aλ)λ≤α(a_\lambda)_{\lambda \leq \alpha} of elements of VV, all but a finite number of them being 00, such that f−∑λ≤αaλgλ≪gαf - \sum_{\lambda \leq \alpha} a_\lambda g_\lambda \ll g_\alpha. One says that ∑λ≤αaλgλ\sum_{\lambda \leq \alpha} a_\lambda g_\lambda is an asymptotic expansion of ff to precision gαg_\alpha, that the aλgλa_\lambda g_\lambda (λ≤α\lambda \leq \alpha) are its terms, the aλa_\lambda its coefficients, and the function rα=f−∑λ≤αaλgλr_\alpha = f - \sum_{\lambda \leq \alpha} a_\lambda g_\lambda the remainder of this expansion.

Cites 2

Cites V § 1. Comparison of functions on a filtered set, I § 3. Derivatives of higher order

To express the fact that ∑λ≤αaλgλ\sum_{\lambda \leq \alpha} a_\lambda g_\lambda is an asymptotic expansion of ff to precision gαg_\alpha one most often restricts oneself to writing

f=∑λ≤αaλgλ+o(gα)(or f=∑λ≤αaλgλ+ok(gα) f = \sum_{\lambda \leq \alpha} a_\lambda g_\lambda + o(g_\alpha) \quad \text{(or } f = \sum_{\lambda \leq \alpha} a_\lambda g_\lambda + o_k(g_\alpha)

if there are several functions in the proof) following the notation of V, p. 219 and 220.

Of two asymptotic expansions (of two functions, distinct or not) relative to the same scale E\mathscr{E}, one says that the one with precision of greater index is the more precise.

If ∑λ≤αaλgλ\sum_{\lambda \leq \alpha} a_\lambda g_\lambda is an asymptotic expansion of ff to precision gαg_\alpha, then, for every β<α\beta < \alpha, ∑λ≤βaλgλ\sum_{\lambda \leq \beta} a_\lambda g_\lambda is an asymptotic expansion of ff to precision gβg_\beta (V, p. 215, prop. 5): one says that it is obtained by reducing the precision of the given expansion ∑λ≤αaλgλ\sum_{\lambda \leq \alpha} a_\lambda g_\lambda of ff to gβg_\beta.

If ∑λ≤αaλgλ\sum_{\lambda \leq \alpha} a_\lambda g_\lambda and ∑λ≤αbλgλ\sum_{\lambda \leq \alpha} b_\lambda g_\lambda are asymptotic expansions to the same precision gαg_\alpha of two functions f1,f2f_1, f_2, then ∑λ≤α(aλ+bλ)gλ\sum_{\lambda \leq \alpha} (a_\lambda + b_\lambda) g_\lambda is an asymptotic expansion of f1+f2f_1 + f_2 to precision gαg_\alpha (V, p. 215, prop. 5); and for every scalar cc, ∑λ≤αaλcgλ\sum_{\lambda \leq \alpha} a_\lambda c g_\lambda is an asymptotic expansion of f1cf_1 c to precision gαg_\alpha. It follows that if a function admits an asymptotic expansion to precision gαg_\alpha then this expansion is unique: it is sufficient to see that the function 0 does not admit an asymptotic expansion with precision gαg_\alpha having coefficients ≠0\neq 0. For, if 0=∑λ≤αaλgλ+rα0 = \sum_{\lambda \leq \alpha} a_\lambda g_\lambda + r_\alpha, and if γ\gamma were the least of the indices λ≤α\lambda \leq \alpha such that aλ≠0a_\lambda \neq 0, one would have aγgγ=−∑γ<λ≤αaλgλ−rα≪gγa_\gamma g_\gamma = - \sum_{\gamma < \lambda \leq \alpha} a_\lambda g_\lambda - r_\alpha \ll g_\gamma, which is absurd.

To say that a function ff admits an asymptotic expansion to precision gαg_\alpha, all of whose coefficients are zero, is equivalent to saying that f≪gαf \ll g_\alpha. If ff admits an asymptotic expansion ∑λ≤αaλgλ\sum_{\lambda \leq \alpha} a_\lambda g_\lambda to precision gαg_\alpha whose coefficients are not all zero, and if γ\gamma is the smallest of the indices λ\lambda such that aλ≠0a_\lambda \neq 0, then aγgγa_\gamma g_\gamma is the principal part of ff relative to the scale E\mathscr{E}, for one has f−aγgγ=∑γ<λ≤αaλgλ+rα≪gγf - a_\gamma g_\gamma = \sum_{\gamma < \lambda \leq \alpha} a_\lambda g_\lambda + r_\alpha \ll g_\gamma; similarly, if μ≤α\mu \leq \alpha is an index such that aμ≠0a_\mu \neq 0, then aμgμa_\mu g_\mu is the principal part of f−∑λ<μaλgλf - \sum_{\lambda < \mu} a_\lambda g_\lambda.

The most important asymptotic expansions in applications are those relative to the scale of the x−nx^{-n} (resp. of the z−nz^{-n}), where nn is a positive or negative integer, as xx tends to +∞+\infty or to −∞-\infty (resp. when the complex number zz tends to ∞\infty), or relative to the scale of the (x−c)n(x - c)^n (resp. (z−c)n(z - c)^n) when the real number xx tends to cc from the right or left (resp. when the complex number zz tends to cc). We saw in I, p. 21 that every vector function of a real variable xx which is kk times differentiable at a point c∈Rc \in \mathbf{R} admits a Taylor expansion of order kk at this point, that is, an asymptotic expansion to precision (x−c)k(x - c)^k with respect to the scale of the (x−c)n(x - c)^n.

3. Sums and products of asymptotic expansions

If f1,f2f_1, f_2 admit asymptotic expansions to precision gαg_\alpha and gβg_\beta respectively, relative to a comparison scale E\mathscr{E}, one deduces expansions to precision gmin⁡(α,β)g_{\min(\alpha, \beta)} by limiting the two expansions to this precision; we have seen in V, p. 222 how one obtains an asymptotic expansion for f1+f2f_1 + f_2 to precision gmin⁡(α,β)g_{\min(\alpha, \beta)}.

Let V1,V2V_1, V_2 and VV be three normed spaces over the field KK, and let (x,y)↦[x.y](\mathbf{x}, \mathbf{y}) \mapsto [\mathbf{x}. \mathbf{y}] be a continuous bilinear map from V1×V2V_1 \times V_2 into VV; we suppose further, for the rest of this section, that the scale E\mathscr{E} is such that the product of any two functions in E\mathscr{E} is again in E\mathscr{E} (which is true for all the comparison scales given as examples (in V, p. 220)).

Now let f1,f2f_1, f_2 be two functions in H(F,V1)\mathscr{H}(\mathfrak{F}, V_1) and H(F,V2)\mathscr{H}(\mathfrak{F}, V_2) respectively, having asymptotic expansions f1=∑λ≤αaλgλ+rαf_1 = \sum_{\lambda \leq \alpha} a_\lambda g_\lambda + r_\alpha and f2=∑μ≤βbμgμ+rβf_2 = \sum_{\mu \leq \beta} b_\mu g_\mu + r_\beta to precision gαg_\alpha and gβg_\beta respectively, with respect to the scale E\mathscr{E}. Suppose further that neither the aλa_\lambda nor the bμb_\mu are all zero, and let aγgγa_\gamma g_\gamma and bδgδb_\delta g_\delta be the principal parts of f1f_1 and f2f_2. By hypothesis, one can write gγgβ=gρg_\gamma g_\beta = g_\rho and gδgα=gσg_\delta g_\alpha = g_\sigma; let us show that the sum ∑[aλ.bμ]gλgμ\sum [\mathbf{a}_\lambda . \mathbf{b}_\mu] g_\lambda g_\mu taken over all pairs (λ,μ)(\lambda, \mu) such that gmin⁡(ρ,σ)≪gλgμg_{\min(\rho, \sigma)} \ll g_\lambda g_\mu, is an asymptotic expansion of [f1.f2][f_1.f_2] to precision gmin⁡(ρ,σ)g_{\min(\rho, \sigma)}. Now the difference between [f1.f2][f_1.f_2] and this sum is the sum of a finite number of terms, each of which is either of the form [aλ.bμ]gλgμ[\mathbf{a}_\lambda . \mathbf{b}_\mu] g_\lambda g_\mu with gλgμ≪gmin⁡(ρ,σ)g_\lambda g_\mu \ll g_{\min(\rho, \sigma)}, or of the form [aλ.rβ]gλ[\mathbf{a}_\lambda . \mathbf{r}_\beta] g_\lambda where λ≥γ\lambda \geq \gamma, or of the form [rα.bμ]gμ[\mathbf{r}_\alpha . \mathbf{b}_\mu] g_\mu where μ≥δ\mu \geq \delta; but since [x.y][\mathbf{x}. \mathbf{y}] is continuous, one has from (V, p. 213, prop. 3 and V, p. 215, prop. 6) that [aλ.rβ]gλ≼rβgλ≪gβgγ=gρ[\mathbf{a}_\lambda . \mathbf{r}_\beta] g_\lambda \preccurlyeq \mathbf{r}_\beta g_\lambda \ll g_\beta g_\gamma = g_\rho for λ≥γ\lambda \geq \gamma, and similarly [rα.bμ]gμ≼rαgμ≪gαgδ=gσ[\mathbf{r}_\alpha . \mathbf{b}_\mu] g_\mu \preccurlyeq \mathbf{r}_\alpha g_\mu \ll g_\alpha g_\delta = g_\sigma for μ≥δ\mu \geq \delta, whence the proposition (V, p. 215, prop. 5).

If all the aλ\mathbf{a}_\lambda are zero one has [f1.f2]≪gαgδ[f_1.f_2] \ll g_\alpha g_\delta: in other words, one has an asymptotic expansion of [f1.f2][f_1.f_2] with zero terms, to precision gαgδg_\alpha g_\delta; similarly if all the aλ\mathbf{a}_\lambda and bμ\mathbf{b}_\mu are zero one has an asymptotic expansion of [f1.f2][f_1.f_2] with zero terms to precision gαgβg_\alpha g_\beta.

We shall apply the preceding result principally to the case where V is a normed algebra over K and the bilinear function [x.y][\mathbf{x}. \mathbf{y}] is the product xy in this algebra; the most important cases are those where V is equal to R\mathbf{R} or to C\mathbf{C}.

In particular, if fif_i (1≤i≤n1 \leq i \leq n) are n functions in H(F,K)\mathscr{H}(\mathfrak{F}, K) each of which admits an asymptotic expansion with respect to E\mathscr{E} one can obtain an asymptotic expansion with respect to E\mathscr{E} for every polynomial ∑(vi)av1v2vnf1v1…fnvn\sum_{(v_i)} \mathbf{a}_{v_1 v_2} v_n f_1^{v_1} \ldots f_n^{v_n} in the fif_i with coefficients in a normed space V; furthermore, the preceding rules allow one to determine the precision of the expansion obtained, if one knows those of the expansions of the functions fif_i.

4. Composition of asymptotic expansions

Let ff be a function in H(F,R)\mathscr{H}(\mathfrak{F}, \mathbf{R}) (resp. H(F,C)\mathscr{H}(\mathfrak{F}, \mathbf{C})), admitting an asymptotic expansion to precision gαg_\alpha with respect to a scale E\mathscr{E}, and having limit 0 along the filter with base F~\widetilde{\mathfrak{F}}. On the other hand let h\mathbf{h} be a function with values in a normed space V over R\mathbf{R} (resp. C\mathbf{C}), defined on a neighbourhood of the point 0 in R\mathbf{R} (resp. C\mathbf{C}), and n times differentiable on this neighbourhood; then

h(t)=c0+c1t+⋯+cntn+o(tn) \mathbf{h}(t) = c_0 + c_1 t + \cdots + c_n t^n + o(t^n)

on this neighbourhood (I, p. 21), whence, on a suitable set in F~\widetilde{\mathfrak{F}}

h∘f=c0+c1f+⋯+cnfn+o(fn). \mathbf{h} \circ f = c_0 + c_1 f + \cdots + c_n f^n + o(f^n).

We have seen, in n 3, how to form an asymptotic expansion for c0+c1f+⋯+cnfnc_0 + c_1 f + \cdots + c_n f^n to a precision gρg_\rho determined by the precision of the expansion of ff; moreover, suppose that the coefficients of the asymptotic expansion of ff are not all zero, and that aγgγa_\gamma g_\gamma is the principal part of ff, and let gσ=gγng_\sigma = g_\gamma^n; if σ<ρ\sigma < \rho one will have an expansion of h∘f\mathbf{h} \circ f to precision gσg_\sigma on limiting the expansion of ∑k=0nckfk\sum_{k=0}^n c_k f^k to this precision; if, on the contrary, ρ≤σ\rho \leq \sigma, then the expansion of ∑k=0nckfk\sum_{k=0}^n c_k f^k is also an expansion of h∘f\mathbf{h} \circ f to precision gρg_\rho.

If all the terms of the asymptotic expansion of ff are zero, and if gα≪1g_\alpha \ll 1, then f≪gαf \ll g_\alpha and so fk≪gαk≪gαf^k \ll g_\alpha^k \ll g_\alpha for every integer k>0k > 0; if cmc_m is the first coefficient of index >0> 0 which is not zero (assuming that the ckc_k for indices k>0k > 0 are not all 0), then c0c_0 is an asymptotic expansion of h∘fh \circ f to precision gαmg_\alpha^m.

In the remainder of this section we shall restrict ourselves to the case where the functions in E\mathscr{E} have real values and are strictly positive on a set in F\mathfrak{F}, and we shall consider asymptotic expansions only of functions in H(F,R)\mathscr{H}(\mathfrak{F}, \mathbf{R}). Suppose first that for every function g∈Eg \in \mathscr{E} and every real number ν\nu, gνg^\nu again belongs to E\mathscr{E}: this condition is fulfilled, for example, by the scale of the xαx^\alpha or by that of the xα∣log⁡x∣βx^\alpha |\log x|^\beta (α\alpha and β\beta being arbitrary real numbers) on a neighbourhood of +∞+\infty or a neighbourhood of 0 in R\mathbf{R}. This property implies that the quotient of two functions in E\mathscr{E} again belongs to E\mathscr{E}. This being so, from an asymptotic expansion relative to E\mathscr{E} of a function f∈H(F,R)f \in \mathscr{H}(\mathfrak{F}, \mathbf{R}), to precision gαg_\alpha, one can derive an expansion for ∣f∣ν|f|^\nu for every real number ν\nu. Let us restrict ourselves to the case where the coefficients of the expansion of ff are not all zero, and let aγgγa_\gamma g_\gamma be the principal part of ff; one can write ∣f∣ν=∣aγ∣νgγν(1+h)ν|f|^\nu = |a_\gamma|^\nu g_\gamma^\nu (1 + h)^\nu, with

h=∑γ<λ≤αaλaγgλgγ+o(gαgγ). h = \sum_{\gamma < \lambda \leq \alpha} \frac{a_\lambda}{a_\gamma} \frac{g_\lambda}{g_\gamma} + o \left( \frac{g_\alpha}{g_\gamma} \right).
Under our hypotheses ∑γ<λ≤αaλaγgλgγ\sum_{\gamma < \lambda \leq \alpha} \frac{a_\lambda}{a_\gamma} \frac{g_\lambda}{g_\gamma} is an asymptotic expansion of hh, to precision gα/gγg_\alpha / g_\gamma; since hh tends to 0 along F\mathfrak{F} the method described above gives an asymptotic expansion of (1+h)ν(1 + h)^\nu, then an expansion of ∣f∣ν|f|^\nu on multiplying by ∣aγ∣νgγν|a_\gamma|^\nu g_\gamma^\nu.

With the same hypotheses on ff one can write

log⁡∣f∣=log⁡∣aγgγ∣+log⁡(1+h) \log |f| = \log |a_\gamma g_\gamma| + \log (1 + h)
and log⁡(1+h)\log (1 + h) can be expanded, as has been said above, the function log⁡(1+t)\log (1 + t) being indefinitely differentiable on a neighbourhood of 0; if, further, log⁡gγ\log g_\gamma admits an asymptotic expansion with respect to E\mathscr{E}, or with respect to a scale E1⊃E\mathscr{E}_1 \supset \mathscr{E}, one obtains an asymptotic expansion for log⁡∣f∣\log |f| on adding the two asymptotic expansions.

Example

We have (1+x)1/x=exp⁡(1xlog⁡(1+x))(1 + x)^{1/x} = \exp \left( \frac{1}{x} \log (1 + x) \right): when xx tends to +∞+\infty we have log⁡(1+x)=log⁡x+log⁡(1+1x)\log (1 + x) = \log x + \log \left( 1 + \frac{1}{x} \right), whence the asymptotic expansion of 1xlog⁡(1+x)\frac{1}{x} \log (1 + x) with respect to the scale of the xα(log⁡x)βx^\alpha (\log x)^\beta:

1xlog⁡(1+x)=log⁡xx+1x2−12x3+o1(1x3). \frac{1}{x} \log (1 + x) = \frac{\log x}{x} + \frac{1}{x^2} - \frac{1}{2x^3} + o_1 \left( \frac{1}{x^3} \right).
From this expansion, and from the Taylor expansion
eu=1+u+u22+u36+o(u3) e^u = 1 + u + \frac{u^2}{2} + \frac{u^3}{6} + o(u^3)

on a neighbourhood of u=0u = 0, one deduces the asymptotic expansion

(1+x)1/x=1+log⁡xx+12(log⁡x)2x2+1x2+16(log⁡x)3x3+log⁡xx3−12x3+o2(1x3) (1 + x)^{1/x} = 1 + \frac{\log x}{x} + \frac{1}{2} \frac{(\log x)^2}{x^2} + \frac{1}{x^2} + \frac{1}{6} \frac{(\log x)^3}{x^3} + \frac{\log x}{x^3} - \frac{1}{2x^3} + o_2 \left( \frac{1}{x^3} \right)

with respect to the scale xα(log⁡x)βx^\alpha (\log x)^\beta by the methods explained above.

Keeping the same hypotheses and notation, the asymptotic expansion of efe^f does not pose new problems except when f≫1f \gg 1; one must then distinguish two cases, as gα≫1g_\alpha \gg 1 or gα≪1g_\alpha \ll 1. In the first case, giving an expansion for ff does not allow one to obtain a principal part for efe^f relative to E\mathscr{E}, because one does not know in general whether the remainder rαr_\alpha tends to 0, that is, whether erαe^{r_\alpha} tends to 1. On the contrary, if gα≪1g_\alpha \ll 1 then rσ≪1r_\sigma \ll 1 and so ef∼exp⁡(∑λ≤αaλgλ)e^f \sim \exp \left( \sum_{\lambda \leq \alpha} a_\lambda g_\lambda \right). One can make this result more precise: let aγgγa_\gamma g_\gamma be the principal part of ff and let δ\delta be the index (such that γ<δ≤α\gamma < \delta \leq \alpha) for which gδ=1g_\delta = 1; we put f1=∑λ≤δaλgλf_1 = \sum_{\lambda \leq \delta} a_\lambda g_\lambda, f2=∑δ<λ≤αaλgλ+rαf_2 = \sum_{\delta < \lambda \leq \alpha} a_\lambda g_\lambda + r_\alpha; we have f=f1+f2f = f_1 + f_2, so ef=ef1ef2e^f = e^{f_1} e^{f_2}, and the general method explained at the start of this subsection allows one to form an asymptotic expansion of ef2e^{f_2} (starting from the Taylor expansion of ete^t at the point t=0t = 0). One will then have an asymptotic expansion for efe^f if ef1=∏λ≤δexp⁡(aλgλ)e^{f_1} = \prod_{\lambda \leq \delta} \exp(a_\lambda g_\lambda) belongs to E\mathscr{E}, or to a scale E1\mathscr{E}_1 containing E\mathscr{E}.

Example

We have x1/1=exp⁡(log⁡x⋅exp⁡(1xlog⁡x))x^{1/1} = \exp \left( \log x \cdot \exp \left( \frac{1}{x} \log x \right) \right); when xx tends to +∞+\infty one has log⁡x≪x\log x \ll x, whence the asymptotic expansion of log⁡x⋅exp⁡(1xlog⁡x)\log x \cdot \exp \left( \frac{1}{x} \log x \right) with respect to the scale xα(log⁡x)βx^\alpha (\log x)^\beta:

log⁡x⋅exp⁡(1xlog⁡x)=log⁡x+(log⁡x)2x+12(log⁡x)3x2+o((log⁡x)3x2). \log x \cdot \exp \left( \frac{1}{x} \log x \right) = \log x + \frac{(\log x)^2}{x} + \frac{1}{2} \frac{(\log x)^3}{x^2} + o \left( \frac{(\log x)^3}{x^2} \right).

All the terms of this expansion, starting from the second, tend to 0; from this expansion and from the Taylor expansion eu=1+u+u2/2+o(u2)e^u = 1 + u + u^2/2 + o(u^2) on a neighbourhood of u=0u = 0 one deduces

x1/1=1+(log⁡x)2+12(log⁡x)4x+12(log⁡x)3x+o((log⁡x)3x). x^{1/1} = 1 + (\log x)^2 + \frac{1}{2} \frac{(\log x)^4}{x} + \frac{1}{2} \frac{(\log x)^3}{x} + o \left( \frac{(\log x)^3}{x} \right).

5. Asymptotic expansions with variable coefficients

One can generalize the concept of principal part, and that of an asymptotic expansion, in the following way. Let E\mathscr{E} be a comparison scale formed of real (resp. complex) functions such that, for each of them, there is a set in F\mathfrak{F} on which the function does not vanish at any point. Further, let CC be a set of functions in H(F,V)\mathscr{H}(\mathfrak{F}, V) satisfying the following three conditions:

(CO₁) For every function a∈Ca \in C one has a≼1a \preccurlyeq 1. (CO₂) The relation a≪1a \ll 1 for a function a∈Ca \in C implies a=0a = 0. (CO₃) CC is a vector space over R\mathbf{R} (resp. C\mathbf{C}).

Now let ff be any function in H(F,V)\mathscr{H}(\mathfrak{F}, V); if there exist a function g∈Eg \in \mathscr{E} and a nonzero function a∈Ca \in C such that f−ag≪gf - ag \ll g one will say that agag is a principal part of ff, relative to the comparison scale E\mathscr{E} and to the domain of coefficients CC. If such a principal part exists, it is unique: for suppose that there are two principal parts a1g1a_1 g_1 and a2g2a_2 g_2; one cannot have g1≪g2g_1 \ll g_2 since from (CO₁) one could deduce that a1g1≪g2a_1 g_1 \ll g_2 and f−a1g1≪g1≪g2f - a_1 g_1 \ll g_1 \ll g_2, so f≪g2f \ll g_2; but one would also have a2g2≪g2a_2 g_2 \ll g_2 and consequently a2≪1a_2 \ll 1 contradicting the hypothesis a2≠0a_2 \neq 0 and (CO₂). So one must have g1=g2g_1 = g_2; from the relations f−a1g1≪g1,f−a2g1≪g1f - a_1 g_1 \ll g_1, f - a_2 g_1 \ll g_1 one deduces that (a2−a1)g1≪g1(a_2 - a_1)g_1 \ll g_1 whence a2−a1≪1a_2 - a_1 \ll 1, and consequently a2=a1a_2 = a_1, by (CO₂) and (CO₃).

Example

For xx real tending to +∞+\infty the periodic bounded functions on R\mathbf{R}, having the same period τ\tau, satisfy conditions (CO₁), (CO₂) and (CO₃): if lim⁡x→+∞a(x)=0\lim_{x \to +\infty} a(x) = 0 then for every ε>0\varepsilon > 0 there is an x0x_0 such that ∣a(x)∣≤ε|a(x)| \leq \varepsilon for every x≥x0x \geq x_0; one deduces that ∣a(x)∣≤ε|a(x)| \leq \varepsilon for 0≤x≤τ0 \leq x \leq \tau too, since there exists an integer nn such that x+nτ≥x0x + n\tau \geq x_0, and such that a(x)=a(x+nτ)a(x) = a(x + n\tau); since ε\varepsilon is arbitrary one has a(x)=0a(x) = 0 on [0,τ][0, \tau], hence everywhere.

With the notation of V, p. 222, we will say that ∑λ≤αaλgλ\sum_{\lambda \leq \alpha} a_\lambda g_\lambda, where the aλa_\lambda belong to CC and all but a finite number of them are zero, is an asymptotic expansion of ff with coefficients in CC, to precision gαg_\alpha, if f−∑λ≤αaλgλ≪gαf - \sum_{\lambda \leq \alpha} a_\lambda g_\lambda \ll g_\alpha; for every index μ\mu such that aμ≠0a_\mu \neq 0 then aμgμa_\mu g_\mu is the principal part of f−∑λ<μaλgλf - \sum_{\lambda < \mu} a_\lambda g_\lambda, relative to E\mathscr{E} and to C′C', which proves the uniqueness of the asymptotic expansion of ff (to precision gαg_\alpha) when it exists.

The methods given in n 3 (V, p. 223) for forming an asymptotic expansion for f1+f2f_1 + f_2 or for [f1.f2][f_1 . f_2], starting from given asymptotic expansions for f1f_1 and f2f_2, can again be applied to expansions with variable coefficients, so long as the [aλ.bμ][a_\lambda . b_\mu] belong to the domain of coefficients CC corresponding to the normed space VV or admit an asymptotic expansion with coefficients in CC.

Cites 1

Cites § 2. Asymptotic expansions

Transcribed from the printed volume. Not translated.