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5.3. The case j k ≠ 0 : uniform estimates and asymptotics [053W]

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5.3. The case jk≠0j_{k}\neq 0: uniform estimates and asymptotics

In this subsection, we consider the case jk≠0j_{k}\neq 0 of the homogeneous equation

(5.76) d2​uk​(z)d​z2−(jk2​n24⋅zn+n​λk)​zn−2​uk​(z)=0.z≥1,\frac{d^{2}u_{k}(z)}{dz^{2}}-(\frac{j_{k}^{2}n^{2}}{4}\cdot z^{n}+n\lambda_{k})z^{n-2}u_{k}(z)=0.\ z\geq 1,

Under the change of variables given by (5.21) and (5.25), the above equation is transformed into the confluent hypergeometric equation,

(5.77) y⋅d2​𝒥​(y)d​y2+(α−y)⋅d​𝒥​(y)dy−β⋅𝒥⁡(y)=0,y<0,y\cdot\frac{d^{2}\mathcal{J}(y)}{dy^{2}}+(\fa-y)\cdot\frac{d\mathcal{J}(y)}{dy}-\fb\cdot\mathcal{J}(y)=0,\ y<0,

where

(5.78) {α=1−1nβ=12​(1−1n)−λkjk⋅n.\displaystyle\begin{cases}\fa=1-\frac{1}{n}\\ \fb=\frac{1}{2}(1-\frac{1}{n})-\frac{\lambda_{k}}{j_{k}\cdot n}.\end{cases}

Since we have shown in Section 5.1 that λk≥jk​(n−1)2\lambda_{k}\geq\frac{j_{k}(n-1)}{2}, we have that

(5.79) β≤0​andα−β≥1−1n>0.\beta\leq 0\ \text{and}\ \ \alpha-\beta\geq 1-\frac{1}{n}>0.

According to the discussion in Appendix A, in our case y<0y<0, the confluent hypergeometric equation (5.77) has two linearly independent solutions

(5.80) Φ♯⁡(β,α,y)≡∑k=0∞(β)k(α)k⋅ykk!\Ku(\beta,\alpha,y)\equiv\sum\limits_{k=0}^{\infty}\frac{(\beta)_{k}}{(\alpha)_{k}}\cdot\frac{y^{k}}{k!}

and

(5.81) Ψ♭⁡(β,α,y)≡eyΓ⁡(α−β)​∫0∞eyt​tα−β−1​(1+t)β−1​dt.\Tri(\beta,\alpha,y)\equiv\frac{e^{y}}{\Gamma(\fa-\fb)}\int_{0}^{\infty}e^{yt}t^{\fa-\fb-1}(1+t)^{\fb-1}dt.

By Item (3) of Lemma A.3, as y→−∞y\to-\infty, Ψ♭⁡(y)\Tri(y) is a decaying solution to (5.77) for every α>β\alpha>\beta, while Lemma A.5 shows that, in the case β<0\beta<0, the solution Φ♯⁡(y)\Ku(y) is growing of certain polynomial rate as y→−∞y\to-\infty. These then yield two linearly independent solutions to the homogeneous equation (5.76),

(5.82) {𝒢k​(z)=ejk​zn2⋅Φ♯⁡(β,α,−jk​zn),𝒟k​(z)=ejk​zn2⋅Ψ♭⁡(β,α,−jk​zn).\begin{cases}\mathcal{G}_{k}(z)=e^{\frac{j_{k}z^{n}}{2}}\cdot\Ku(\beta,\alpha,-j_{k}z^{n}),\\ \mathcal{D}_{k}(z)=e^{\frac{j_{k}z^{n}}{2}}\cdot\Tri(\beta,\alpha,-j_{k}z^{n}).\end{cases}

First we can compute the Wronskian

Proposition 5.6.

For every k∈ℕk\in\mathbb{N}, the Wronskian of 𝒢k​(z)\mathcal{G}_{k}(z) and 𝒟k​(z)\mathcal{D}_{k}(z) is a constant given by

(5.83) 𝒲⁡(𝒢k​(z),𝒟k​(z))=Γ⁡(α−1)Γ⁡(α−β)⋅jk1n.\mathcal{W}(\mathcal{G}_{k}(z),\mathcal{D}_{k}(z))=\frac{\Gamma(\alpha-1)}{\Gamma(\alpha-\beta)}\cdot j_{k}^{\frac{1}{n}}.
Proof.

Since 𝒢k​(z)\mathcal{G}_{k}(z) and 𝒟k​(z)\mathcal{D}_{k}(z) solve the homogeneous equation

(5.84) d2​uk​(z)d​z2−(jk2​n24⋅zn+n​λk)​zn−2​uk​(z)=0\frac{d^{2}u_{k}(z)}{dz^{2}}-(\frac{j_{k}^{2}n^{2}}{4}\cdot z^{n}+n\lambda_{k})z^{n-2}u_{k}(z)=0

which misses the first order term. Immediately, for all z≥0z\geq 0,

(5.85) dd​z​𝒲​(𝒢k​(z),𝒟k​(z))=0,\frac{d}{dz}\mathcal{W}(\mathcal{G}_{k}(z),\mathcal{D}_{k}(z))=0,

which implies that the Wronskian 𝒲⁡(𝒢k​(z),𝒟k​(z))\mathcal{W}(\mathcal{G}_{k}(z),\mathcal{D}_{k}(z)) is a constant. So it suffices to calculate it at z=0z=0. By the definition of the Wronskian,

𝒲⁡(𝒢k​(z),𝒟k​(z))=\displaystyle\mathcal{W}(\mathcal{G}_{k}(z),\mathcal{D}_{k}(z))= ejk​zn⋅(Φ♯⁡(β,α,−jk​zn)⋅ddz​Ψ♭⁡(β,α,−jk​zn)CLOSE\displaystyle e^{j_{k}z^{n}}\cdot\Big(\Ku(\beta,\alpha,-j_{k}z^{n})\cdot\frac{d}{dz}\Tri(\beta,\alpha,-j_{k}z^{n})
(5.86) −dd​zΦ♯(β,α,−jkzn)⋅Ψ♭(β,α,−jkzn)).\displaystyle-\frac{d}{dz}\Ku(\beta,\alpha,-j_{k}z^{n})\cdot\Tri(\beta,\alpha,-j_{k}z^{n})\Big).

To calculate dd​z​Ψ♭⁡(β,α,−jk​zn)\frac{d}{dz}\Tri(\beta,\alpha,-j_{k}z^{n}), we will apply Kummer’s transformation law to relate Ψ♭\Tri and Φ♯\Ku, that is,

(5.87) Ψ♭⁡(β,α,−jk​zn)\displaystyle\Tri(\beta,\alpha,-j_{k}z^{n})
=\displaystyle= e−jk​zn⋅𝒰⁡(α−β,α,jk​zn)\displaystyle e^{-{j_{k}}z^{n}}\cdot\mathcal{U}(\alpha-\beta,\alpha,{j_{k}}z^{n})
=\displaystyle= e−jk​zn⋅(Γ⁡(1−α)Γ⁡(1−β)⋅Φ♯⁡(α−β,α,jk​zn)+Γ⁡(α−1)Γ⁡(α−β)⋅(jk​zn)1−α​Φ♯⁡(1−β,2−α,jk​zn))\displaystyle e^{-{j_{k}}z^{n}}\cdot\Big(\frac{\Gamma(1-\alpha)}{\Gamma(1-\beta)}\cdot\Ku(\alpha-\beta,\alpha,{j_{k}}z^{n})+\frac{\Gamma(\alpha-1)}{\Gamma(\alpha-\beta)}\cdot({j_{k}}z^{n})^{1-\alpha}\Ku(1-\beta,2-\alpha,{j_{k}}z^{n})\Big)
=\displaystyle= e−jk​zn⋅(Γ⁡(1−α)Γ⁡(1−β)⋅Φ♯⁡(α−β,α,jk​zn)+Γ⁡(α−1)Γ⁡(α−β)⋅jk1n​z⋅Φ♯⁡(1−β,2−α,jk​zn))\displaystyle e^{-{j_{k}}z^{n}}\cdot\Big(\frac{\Gamma(1-\alpha)}{\Gamma(1-\beta)}\cdot\Ku(\alpha-\beta,\alpha,{j_{k}}z^{n})+\frac{\Gamma(\alpha-1)}{\Gamma(\alpha-\beta)}\cdot{j_{k}}^{\frac{1}{n}}z\cdot\Ku(1-\beta,2-\alpha,{j_{k}}z^{n})\Big)
=\displaystyle= Γ⁡(1−α)Γ⁡(1−β)⋅Φ♯⁡(β,α,−jk​zn)+Γ⁡(α−1)Γ⁡(α−β)⋅jk1n​z⋅Φ♯⁡(1−α+β,2−α,−jk​zn).\displaystyle\frac{\Gamma(1-\alpha)}{\Gamma(1-\beta)}\cdot\Ku(\beta,\alpha,-{j_{k}}z^{n})+\frac{\Gamma(\alpha-1)}{\Gamma(\alpha-\beta)}\cdot{j_{k}}^{\frac{1}{n}}z\cdot\Ku(1-\alpha+\beta,2-\alpha,-{j_{k}}z^{n}).

So it follows that

(5.88) dd​z​Ψ♭⁡(β,α,−jk​zn)\displaystyle\frac{d}{dz}\Tri(\beta,\alpha,-{j_{k}}z^{n})
=\displaystyle= Γ⁡(1−α)Γ⁡(1−β)⋅dd​z​Φ♯⁡(β,α,−jk​zn)+Γ⁡(α−1)Γ⁡(α−β)⋅jk1n⋅(Φ♯⁡(1−α+β,2−α,−jk​zn)CLOSE\displaystyle\frac{\Gamma(1-\alpha)}{\Gamma(1-\beta)}\cdot\frac{d}{dz}\Ku(\beta,\alpha,-{j_{k}}z^{n})+\frac{\Gamma(\alpha-1)}{\Gamma(\alpha-\beta)}\cdot{j_{k}}^{\frac{1}{n}}\cdot\Big(\Ku(1-\alpha+\beta,2-\alpha,-{j_{k}}z^{n})
+\displaystyle+ OPENz⋅dd​z​Φ♯⁡(1−α+β,2−α,−jk​zn)).\displaystyle z\cdot\frac{d}{dz}\Ku(1-\alpha+\beta,2-\alpha,-{j_{k}}z^{n})\Big).

Since n≥2n\geq 2, it directly follows from the definition of Φ♯\Ku that

(5.89) dd​z|z=0​Φ♯⁡(β,α,−jk​zn)=0,\displaystyle\frac{d}{dz}\Big|_{z=0}\Ku(\beta,\alpha,-{j_{k}}z^{n})=0,
(5.90) dd​z|z=0​Φ♯⁡(1−α+β,2−α,−jk​zn)=0.\displaystyle\frac{d}{dz}\Big|_{z=0}\Ku(1-\alpha+\beta,2-\alpha,-{j_{k}}z^{n})=0.

Therefore,

(5.91) dd​z|z=0​Ψ♭⁡(β,α,−jk​zn)\displaystyle\frac{d}{dz}\Big|_{z=0}\Tri(\beta,\alpha,-{j_{k}}z^{n}) =\displaystyle= Γ⁡(α−1)Γ⁡(α−β)⋅jk1n⋅Φ♯⁡(1−α+β,2−α,0)\displaystyle\frac{\Gamma(\alpha-1)}{\Gamma(\alpha-\beta)}\cdot{j_{k}}^{\frac{1}{n}}\cdot\Ku(1-\alpha+\beta,2-\alpha,0)
=\displaystyle= Γ⁡(α−1)⋅jk1nΓ⁡(α−β).\displaystyle\frac{\Gamma(\alpha-1)\cdot{j_{k}}^{\frac{1}{n}}}{\Gamma(\alpha-\beta)}.

Now evaluate (5.86) at z=0z=0, we have

(5.92) 𝒲⁡(𝒢k,𝒟k)​(z)=𝒲⁡(𝒢k,𝒟k)​(0)=dd​z|z=0​Ψ♭⁡(β,α,−jk​zn)=Γ⁡(α−1)⋅jk1nΓ⁡(α−β).\mathcal{W}(\mathcal{G}_{k},\mathcal{D}_{k})(z)=\mathcal{W}(\mathcal{G}_{k},\mathcal{D}_{k})(0)=\frac{d}{dz}\Big|_{z=0}\Tri(\beta,\alpha,-{j_{k}}z^{n})=\frac{\Gamma(\alpha-1)\cdot{j_{k}}^{\frac{1}{n}}}{\Gamma(\alpha-\beta)}.

∎

Applying Lemma A.3 and Lemma A.5, immediately we have the following asymptotics for the solutions 𝒢k​(z)\mathcal{G}_{k}(z) and 𝒟k​(z)\mathcal{D}_{k}(z) for fixed kk.

Lemma 5.7.

For each fixed kk, as z→+∞z\to+\infty, we have

(5.93) 𝒢k​(z)\displaystyle\mathcal{G}_{k}(z) ∼Γ⁡(α)Γ⁡(α−β)⋅(jk​zn)−β⋅ejk​zn2,\displaystyle\sim\frac{\Gamma(\alpha)}{\Gamma(\alpha-\beta)}\cdot(j_{k}z^{n})^{-\beta}\cdot e^{\frac{j_{k}z^{n}}{2}},
(5.94) 𝒟k​(z)\displaystyle\mathcal{D}_{k}(z) ∼(jk​zn)β−α⋅e−jk​zn2.\displaystyle\sim(j_{k}z^{n})^{\beta-\alpha}\cdot e^{-\frac{j_{k}z^{n}}{2}}.

Again we need to derive uniform estimates and asymptotic behavior for Φ♯\Ku and Ψ♭\Tri. The idea is to first estimate them in terms of certain integrals and then apply Laplace’s method. To start with, we need some preliminary calculations for Φ♯\Ku and Ψ♭\Tri.

By definition,

(5.95) Ψ♭⁡(β,α,y)\displaystyle\Tri(\fb,\fa,y) =\displaystyle= eyΓ⁡(α−β)​∫0∞ey​t+(α−β−1)​log⁡t+(β−1)​log⁡(t+1)​𝑑t\displaystyle\frac{e^{y}}{\Gamma(\alpha-\beta)}\int_{0}^{\infty}e^{yt+(\alpha-\beta-1)\log t+(\beta-1)\log(t+1)}dt
=\displaystyle= eyΓ⁡(α−β)​∫0∞ey​t+(α−β−1)​log⁡tt+1⋅1(1+t)1+1n​𝑑t.\displaystyle\frac{e^{y}}{\Gamma(\alpha-\beta)}\int_{0}^{\infty}e^{yt+(\alpha-\beta-1)\log\frac{t}{t+1}}\cdot\frac{1}{(1+t)^{1+\frac{1}{n}}}dt.

For simplicity, we denote

(5.96) F⁡(t)≡y​t+(α−β−1)​log⁡tt+1,F(t)\equiv yt+(\fa-\fb-1)\log\frac{t}{t+1},

then

(5.97) Ψ♭⁡(β,α,y)=eyΓ⁡(α−β)​∫0∞eF⁡(t)⋅1(1+t)1+1n​dt.\Tri(\fb,\fa,y)=\frac{e^{y}}{\Gamma(\alpha-\beta)}\int_{0}^{\infty}e^{F(t)}\cdot\frac{1}{(1+t)^{1+\frac{1}{n}}}dt.

Now we give both upper and lower bounds for Φ♯⁡(β,α,y)\Ku(\fb,\fa,y) by simpler exponential integrals.

Lemma 5.8.

Let y≤−1y\leq-1, then following holds,

(5.98) Cn−1⋅ey​(−y)1−2​α4Γ⁡(α−β)⋅∫1−y∞eG⁡(u)​𝑑u≤Φ♯⁡(β,α,y)≤Cn⋅ey​(−y)1−2​α4Γ⁡(α−β)⋅∫0∞eG⁡(u)​du,C_{n}^{-1}\cdot\frac{e^{y}(-y)^{\frac{1-2\alpha}{4}}}{\Gamma(\alpha-\beta)}\cdot\int_{\frac{1}{\sqrt{-y}}}^{\infty}e^{G(u)}du\leq\Ku(\fb,\fa,y)\leq C_{n}\cdot\frac{e^{y}(-y)^{\frac{1-2\alpha}{4}}}{\Gamma(\alpha-\beta)}\cdot\int_{0}^{\infty}e^{G(u)}du,

where

(5.99) G⁡(u)≡−u2+2​−y​u+(α−2​β−12)​log⁡u.G(u)\equiv-u^{2}+2\sqrt{-y}u+(\alpha-2\beta-\frac{1}{2})\log u.
Proof.

To prove this estimate, we need the following integral representation formula for Φ♯⁡(β,α,y)\Ku(\fb,\fa,y),

(5.100) Φ♯⁡(β,α,y)=Γ⁡(α)Γ⁡(α−β)⋅ey​(−y)1−α2⋅∫0∞e−t⋅tα−12−β⋅Iα−1​(2​−yt)​dt.\Ku(\fb,\fa,y)=\frac{\Gamma(\fa)}{\Gamma(\fa-\fb)}\cdot e^{y}(-y)^{\frac{1-\fa}{2}}\cdot\int_{0}^{\infty}e^{-t}\cdot t^{\frac{\fa-1}{2}-\fb}\cdot I_{\fa-1}(2\sqrt{-yt})dt.

The proof is included in Lemma A.2 of Appendix A.

The key point in the proof of (5.98) is to apply the estimate of Iα−1I_{\alpha-1} in Proposition 5.5. By definition, α=1−1n\alpha=1-\frac{1}{n} and hence α−1=−1n≥−12\alpha-1=-\frac{1}{n}\geq-\frac{1}{2}. Applying the upper bound estimate of Iα−1I_{\alpha-1} in (5.48) of Proposition 5.5,

(5.101) Iα−1​(2​−y​t)=I−1n​(2​−y​t)\displaystyle I_{\alpha-1}(2\sqrt{-yt})=I_{-\frac{1}{n}}(2\sqrt{-yt}) ≤\displaystyle\leq Cn⋅max⁡{(2​−y​t)−1n,(2​−y​t)−12⋅e2​−y​t}\displaystyle C_{n}\cdot\max\Big\{(2\sqrt{-yt})^{-\frac{1}{n}},(2\sqrt{-yt})^{-\frac{1}{2}}\cdot e^{2\sqrt{-yt}}\Big\}
≤\displaystyle\leq Cn⋅(−y​t)−14⋅e2​−y​t.\displaystyle C_{n}\cdot(-yt)^{-\frac{1}{4}}\cdot e^{2\sqrt{-yt}}.

Substituting the above in (5.100),

(5.102) ∫0∞e−t⋅tα−12−β⋅Iα−1​(2​−y​t)​𝑑t\displaystyle\int_{0}^{\infty}e^{-t}\cdot t^{\frac{\fa-1}{2}-\fb}\cdot I_{\fa-1}(2\sqrt{-yt})dt ≤\displaystyle\leq Cn⋅∫0∞e−t+2​−y​t⋅t2​α−34−β​𝑑t\displaystyle C_{n}\cdot\int_{0}^{\infty}e^{-t+2\sqrt{-yt}}\cdot t^{\frac{2\alpha-3}{4}-\beta}dt
=\displaystyle= Cn⋅∫0∞e−t+2​−y​t+(2​α−34−β)​log⁡t​𝑑t\displaystyle C_{n}\cdot\int_{0}^{\infty}e^{-t+2\sqrt{-yt}+(\frac{2\alpha-3}{4}-\beta)\log t}dt
=\displaystyle= Cn⋅∫0∞e−u2+2​−y​u+(α−2​β−12)​log⁡u​𝑑u.\displaystyle C_{n}\cdot\int_{0}^{\infty}e^{-u^{2}+2\sqrt{-y}u+(\alpha-2\beta-\frac{1}{2})\log u}du.

Therefore,

(5.103) Φ♯⁡(β,α,y)\displaystyle\Ku(\fb,\fa,y) ≤\displaystyle\leq Cn⋅ey​(−y)1−2​α4Γ⁡(α−β)⋅∫0∞e−u2+2​−y​u+(α−2​β−12)​log⁡u​𝑑u.\displaystyle C_{n}\cdot\frac{e^{y}(-y)^{\frac{1-2\alpha}{4}}}{\Gamma(\alpha-\beta)}\cdot\int_{0}^{\infty}e^{-u^{2}+2\sqrt{-y}u+(\alpha-2\beta-\frac{1}{2})\log u}du.

Next, Φ♯\Ku can be also bounded below in a similar way. In fact, we consider the integral domain t≥1−yt\geq\frac{1}{-y} with y≤−1y\leq-1, then

(5.104) Iα−1​(2​−y​t)≥Cn−1⋅e2​−y​t(−y​t)14,I_{\alpha-1}(2\sqrt{-yt})\geq C_{n}^{-1}\cdot\frac{e^{2\sqrt{-yt}}}{(-yt)^{\frac{1}{4}}},

and hence

∫0∞e−t⋅tα−12−β⋅Iα−1​(2​−y​t)​𝑑t\displaystyle\int_{0}^{\infty}e^{-t}\cdot t^{\frac{\fa-1}{2}-\fb}\cdot I_{\fa-1}(2\sqrt{-yt})dt ≥∫1−y∞e−t⋅tα−12−β⋅Iα−1​(2​−y​t)​𝑑t\displaystyle\geq\int_{\frac{1}{-y}}^{\infty}e^{-t}\cdot t^{\frac{\fa-1}{2}-\fb}\cdot I_{\fa-1}(2\sqrt{-yt})dt
≥Cn−1⋅∫1−y∞e−t+2​−y​t+(2​α−34−β)​log⁡t​𝑑t\displaystyle\geq C_{n}^{-1}\cdot\int_{\frac{1}{-y}}^{\infty}e^{-t+2\sqrt{-yt}+(\frac{2\alpha-3}{4}-\beta)\log t}dt
(5.105) =Cn−1⋅∫1−y∞e−u2+2​−y​u+(α−2​β−12)​log⁡u​𝑑u.\displaystyle=C_{n}^{-1}\cdot\int_{\frac{1}{\sqrt{-y}}}^{\infty}e^{-u^{2}+2\sqrt{-y}u+(\alpha-2\beta-\frac{1}{2})\log u}du.

Therefore,

(5.106) Φ♯⁡(β,α,y)≥Cn−1⋅ey​(−y)1−2​α4Γ⁡(α−β)⋅∫1−y∞e−u2+2​−y​u+(α−2​β−12)​log⁡u​du.\Ku(\fb,\fa,y)\geq C_{n}^{-1}\cdot\frac{e^{y}(-y)^{\frac{1-2\alpha}{4}}}{\Gamma(\alpha-\beta)}\cdot\int_{\frac{1}{\sqrt{-y}}}^{\infty}e^{-u^{2}+2\sqrt{-y}u+(\alpha-2\beta-\frac{1}{2})\log u}du.

∎

Now we set up a few notations for convenience. Let

(5.107) Q≡α−β−1≥−1n,γn≡12+1n,Q\equiv\alpha-\beta-1\geq-\frac{1}{n},\ \gamma_{n}\equiv\frac{1}{2}+\frac{1}{n},

and recall the notations (5.96) and (5.99),

(5.108) F⁡(t)\displaystyle F(t) =y​t+Q​log⁡tt+1,\displaystyle=yt+Q\log\frac{t}{t+1},
(5.109) G⁡(u)\displaystyle G(u) =−u2+2​(−y)12⋅u+(2​Q+γn)⋅log⁡u.\displaystyle=-u^{2}+2(-y)^{\frac{1}{2}}\cdot u+(2Q+\gamma_{n})\cdot\log u.

By direct calculation

(5.110) F′′​(t)\displaystyle F^{\prime\prime}(t) =Q⁡(−1t2+1(t+1)2),\displaystyle=Q(-\frac{1}{t^{2}}+\frac{1}{(t+1)^{2}}),
(5.111) G′′​(u)\displaystyle G^{\prime\prime}(u) =−2−2​Q+γnu.\displaystyle=-2-\frac{2Q+\gamma_{n}}{u}.

Notice that 2​Q+γn≥12−1n≥02Q+\gamma_{n}\geq\frac{1}{2}-\frac{1}{n}\geq 0. Therefore, G⁡(u)G(u) is strictly concave in ℝ+\mathbb{R}_{+}, and FF is strictly concave in ℝ\mathbb{R} if Q>0Q>0.

We will split our analysis in two different cases:

Case (A): Q≥1Q\geq 1.

Case (B): Q≤1Q\leq 1.

Our main focus is Case (A) which is more difficult. The upper bound estimates in Case (B) follows from elementary integral calculations (see Lemma 5.12).

Case (A)

Let t0>0t_{0}>0 be the unique critical point of F⁡(t)F(t) and let u0>0u_{0}>0 be the unique critical point of G⁡(u)G(u), then t0t_{0} and u0u_{0} satisfy the equations

(5.112) t02+t0+Qy=0,\displaystyle t_{0}^{2}+t_{0}+\frac{Q}{y}=0,
(5.113) u02−(−y)12⋅u0−2​Q+γn2=0.\displaystyle u_{0}^{2}-(-y)^{\frac{1}{2}}\cdot u_{0}-\frac{2Q+\gamma_{n}}{2}=0.

Immediately we have

(5.114) t0\displaystyle t_{0} =−1+1+4​Q−y2,\displaystyle=\frac{-1+\sqrt{1+\frac{4Q}{-y}}}{2},
(5.115) u0\displaystyle u_{0} =(−y)122⋅(1+1+4​Q−y+2​γn−y).\displaystyle=\frac{(-y)^{\frac{1}{2}}}{2}\cdot\Big(1+\sqrt{1+\frac{4Q}{-y}+\frac{2\gamma_{n}}{-y}}\Big).

Now prove the following effective estimates on Φ♯\Ku and Ψ♭\Tri. The difference from Lemma 5.7 is here the estimates holds uniformly for all β≤0\beta\leq 0 (recall α\alpha is the fixed number 1−1n1-\frac{1}{n}).

Proposition 5.9.

There exists some dimensional constant Cn>0C_{n}>0 such that for every y≤−1y\leq-1, the following estimates hold:

(5.116) Cn−1⋅Q−14−12​n⋅(−y)−1⋅ey+F⁡(t0)Γ⁡(Q+1)\displaystyle C_{n}^{-1}\cdot Q^{-\frac{1}{4}-\frac{1}{2n}}\cdot\frac{(-y)^{-1}\cdot e^{y+F(t_{0})}}{\Gamma(Q+1)} ≤Ψ♭⁡(β,α,y)≤Cn⋅Q14⋅ey+F⁡(t0)Γ⁡(Q+1),\displaystyle\leq\Tri(\beta,\alpha,y)\leq C_{n}\cdot Q^{\frac{1}{4}}\cdot\frac{e^{y+F(t_{0})}}{\Gamma(Q+1)},
(5.117) Cn−1⋅Q−14⋅(−y)1−2​α4⋅ey+G⁡(u0)Γ⁡(Q+1)\displaystyle C_{n}^{-1}\cdot Q^{-\frac{1}{4}}\cdot\frac{(-y)^{\frac{1-2\alpha}{4}}\cdot e^{y+G(u_{0})}}{\Gamma(Q+1)} ≤Φ♯⁡(β,α,y)≤Cn⋅(−y)1−2​α4⋅ey+G⁡(u0)Γ⁡(Q+1).\displaystyle\leq\Ku(\beta,\alpha,y)\leq C_{n}\cdot\frac{(-y)^{\frac{1-2\alpha}{4}}\cdot e^{y+G(u_{0})}}{\Gamma(Q+1)}.
Proof.

Our main strategy is to apply Laplace’s method. The basic idea is that the above exponential integrals are concentrated at the critical values t0t_{0} and u0u_{0}.

First, we prove the uniform estimate for Ψ♭⁡(β,α,y)\Tri(\fb,\fa,y). By (5.97),

(5.118) Ψ♭⁡(β,α,y)≤eyΓ⁡(α−β)​∫0∞eF⁡(t)​dt.\Tri(\fb,\fa,y)\leq\frac{e^{y}}{\Gamma(\fa-\fb)}\int_{0}^{\infty}e^{F(t)}dt.

Clearly, the upper bound of Ψ♭⁡(β,α,y)\Tri(\fb,\fa,y) follows from the upper bound estimate of ∫0∞eF⁡(t)​𝑑t\int_{0}^{\infty}e^{F(t)}dt. Write

(5.119) ∫0∞eF⁡(t)​𝑑t=∫02​t0eF⁡(t)​𝑑t+∫2​t0∞eF⁡(t)​𝑑t.\int_{0}^{\infty}e^{F(t)}dt=\int_{0}^{2t_{0}}e^{F(t)}dt+\int_{2t_{0}}^{\infty}e^{F(t)}dt.

We will estimate the two terms separately.

To estimate the first term in (5.119), we make a change of variable

(5.120) t=t0⋅(1+ξ),ξ∈(−1,1),t=t_{0}\cdot(1+\xi),\ \xi\in(-1,1),

then Taylor’s theorem gives that

(5.121) F⁡(t)−F⁡(t0)\displaystyle F(t)-F(t_{0}) =\displaystyle= F⁡(t0​(1+ξ))−F⁡(t0)\displaystyle F(t_{0}(1+\xi))-F(t_{0})
=\displaystyle= F′​(t0)⋅t0⋅ξ+F′′​(θ)2⋅t02⋅ξ2\displaystyle F^{\prime}(t_{0})\cdot t_{0}\cdot\xi+\frac{F^{\prime\prime}(\theta)}{2}\cdot t_{0}^{2}\cdot\xi^{2}
=\displaystyle= F′′​(θ)2⋅t02⋅ξ2,\displaystyle\frac{F^{\prime\prime}(\theta)}{2}\cdot t_{0}^{2}\cdot\xi^{2},

where θ\theta is between tt and t0t_{0}. Now we need to estimate the quadratic error term. It is straightforward calculation that

(5.122) F′′′​(t)\displaystyle F^{\prime\prime\prime}(t) =2​(Qt3−Q(t+1)3)>0,\displaystyle=2(\frac{Q}{t^{3}}-\frac{Q}{(t+1)^{3}})>0,

then F′′​(t)F^{\prime\prime}(t) is increasing in tt. Since θ\theta is between t0t_{0} and t∈[0,2​t0]t\in[0,2t_{0}], the above monotonicity of F′′F^{\prime\prime} implies F′′​(θ)≤F′′​(2​t0)<0F^{\prime\prime}(\theta)\leq F^{\prime\prime}(2t_{0})<0. So the first term of (5.119) becomes

(5.123) ∫02​t0eF⁡(t)​𝑑t\displaystyle\int_{0}^{2t_{0}}e^{F(t)}dt =\displaystyle= eF⁡(t0)​∫02​t0eF⁡(t)−F⁡(t0)​𝑑t\displaystyle e^{F(t_{0})}\int_{0}^{2t_{0}}e^{F(t)-F(t_{0})}dt
≤\displaystyle\leq eF⁡(t0)⋅t0⋅∫−11eF′′​(2​t0)2⋅t02⋅ξ2​𝑑ξ\displaystyle e^{F(t_{0})}\cdot t_{0}\cdot\int_{-1}^{1}e^{\frac{F^{\prime\prime}(2t_{0})}{2}\cdot t_{0}^{2}\cdot\xi^{2}}d\xi

By direct computations, F′′(2t0)=−(4​t0+1)4​t02​(2​t0+1)2⋅QF^{\prime\prime}(2t_{0})=-\frac{(4t_{0}+1)}{4t_{0}^{2}(2t_{0}+1)^{2}}\cdot Q. So we have,

(5.124) ∫02​t0eF⁡(t)​𝑑t\displaystyle\int_{0}^{2t_{0}}e^{F(t)}dt ≤\displaystyle\leq eF⁡(t0)⋅t0⋅∫−11e−4​t0+18​(2​t0+1)2⋅Q⋅ξ2dξ\displaystyle e^{F(t_{0})}\cdot t_{0}\cdot\int_{-1}^{1}e^{-\frac{4t_{0}+1}{8(2t_{0}+1)^{2}}\cdot Q\cdot\xi^{2}}d\xi
≤\displaystyle\leq Cn⋅t0​(2​t0+1)4​t0+1⋅Q⋅eF⁡(t0)\displaystyle C_{n}\cdot\frac{t_{0}(2t_{0}+1)}{\sqrt{4t_{0}+1}\cdot\sqrt{Q}}\cdot e^{F(t_{0})}
≤\displaystyle\leq Cn⋅Q14⋅eF⁡(t0),\displaystyle C_{n}\cdot Q^{\frac{1}{4}}\cdot e^{F(t_{0})},

where we used that t0≤Cn⋅Q1/2t_{0}\leq C_{n}\cdot Q^{1/2} (since y≤−1y\leq-1 and Q≥1Q\geq 1). Immediately, we have

(5.125) Ψ♭⁡(β,α,y)≤Cn⋅Q14⋅ey+F⁡(t0)Γ⁡(α−β).\Tri(\beta,\alpha,y)\leq C_{n}\cdot Q^{\frac{1}{4}}\cdot\frac{e^{y+F(t_{0})}}{\Gamma(\alpha-\beta)}.

Next, we estimate the second term in (5.119). Since we have proved F′′​(t)<0F^{\prime\prime}(t)<0, so this implies that F′​(t)F^{\prime}(t) is decreasing and hence F′​(t)≤F′​(2​t0)F^{\prime}(t)\leq F^{\prime}(2t_{0}) for any t≥2​t0t\geq 2t_{0}. Now Taylor’s theorem gives that

(5.126) F⁡(t)≤F⁡(2​t0)+F′​(2​t0)⋅(t−2​t0),F(t)\leq F(2t_{0})+F^{\prime}(2t_{0})\cdot(t-2t_{0}),

which implies that

(5.127) ∫2​t0∞eF⁡(t)​𝑑t≤eF⁡(2​t0)​∫2​t0∞eF′​(2​t0)⋅(t−2​t0)​𝑑t=eF⁡(2​t0)−F′​(2​t0).\int_{2t_{0}}^{\infty}e^{F(t)}dt\leq e^{F(2t_{0})}\int_{2t_{0}}^{\infty}e^{F^{\prime}(2t_{0})\cdot(t-2t_{0})}dt=\frac{e^{F(2t_{0})}}{-F^{\prime}(2t_{0})}.

One can check that F′​(2​t0)=y⁡(3​t0+1)2​(2​t0+1)<0F^{\prime}(2t_{0})=\frac{y(3t_{0}+1)}{2(2t_{0}+1)}<0 with 0<t0<+∞0<t_{0}<+\infty. Since F′​(t)<0F^{\prime}(t)<0 for all t>t0t>t_{0}, so F⁡(2​t0)≤F⁡(t0)F(2t_{0})\leq F(t_{0}) and hence for y≤−1y\leq-1 we have

(5.128) ∫2​t0∞eF⁡(t)​𝑑t≤Cn​eF⁡(t0).\int_{2t_{0}}^{\infty}e^{F(t)}dt\leq C_{n}e^{F(t_{0})}.

Combining the above, we have

(5.129) ∫0∞eF⁡(t)​𝑑t≤Cn⋅Q14⋅eF⁡(t0).\int_{0}^{\infty}e^{F(t)}dt\leq C_{n}\cdot Q^{\frac{1}{4}}\cdot e^{F(t_{0})}.

Therefore,

(5.130) Ψ♭⁡(β,α,y)\displaystyle\Tri(\beta,\alpha,y) ≤Cn⋅Q14⋅ey+F⁡(t0)Γ⁡(α−β).\displaystyle\leq C_{n}\cdot Q^{\frac{1}{4}}\cdot\frac{e^{y+F(t_{0})}}{\Gamma(\alpha-\beta)}.

The lower bound estimate for Ψ♭⁡(β,α,y)\Tri(\fb,\fa,y) also follows from Laplace’s method and we just sketch the computations.

Ψ♭⁡(β,α,y)\displaystyle\Tri(\fb,\fa,y) =eyΓ⁡(α−β)​∫0∞eF⁡(t)⋅1(t+1)1+1n​𝑑t\displaystyle=\frac{e^{y}}{\Gamma(\fa-\fb)}\int_{0}^{\infty}e^{F(t)}\cdot\frac{1}{(t+1)^{1+\frac{1}{n}}}dt
≥eyΓ⁡(α−β)​∫t0​(y)2​t0​(y)eF⁡(t)⋅1(t+1)1+1n​𝑑t\displaystyle\geq\frac{e^{y}}{\Gamma(\alpha-\beta)}\int_{t_{0}(y)}^{2t_{0}(y)}e^{F(t)}\cdot\frac{1}{(t+1)^{1+\frac{1}{n}}}dt
(5.131) ≥eyΓ⁡(α−β)⋅(1+2​t0)1+1n​∫t0​(y)2​t0​(y)eF⁡(t)​𝑑t.\displaystyle\geq\frac{e^{y}}{\Gamma(\alpha-\beta)\cdot(1+2t_{0})^{1+\frac{1}{n}}}\int_{t_{0}(y)}^{2t_{0}(y)}e^{F(t)}dt.

By the concavity of F⁡(t)F(t) and the monotonicity of F′′​(t)F^{\prime\prime}(t) in the domain t0≤t≤2​t0t_{0}\leq t\leq 2t_{0}, we have

(5.132) ∫t0​(y)2​t0​(y)eF⁡(t)​𝑑t≥eF⁡(t0)​∫t0​(y)2​t0​(y)eF′′​(t0)2​(t−t0)2​𝑑t≥Cn⋅eF⁡(t0)​t0​(t0+1)2​t0+1⋅Q\int_{t_{0}(y)}^{2t_{0}(y)}e^{F(t)}dt\geq e^{F(t_{0})}\int_{t_{0}(y)}^{2t_{0}(y)}e^{\frac{F^{\prime\prime}(t_{0})}{2}(t-t_{0})^{2}}dt\geq C_{n}\cdot e^{F(t_{0})}\frac{t_{0}(t_{0}+1)}{\sqrt{2t_{0}+1}\cdot\sqrt{Q}}

It is elementary to see that

(5.133) Cn​Q12​(−y)−1≤t0≤Cn⋅Q12C_{n}Q^{\frac{1}{2}}(-y)^{-1}\leq t_{0}\leq C_{n}\cdot{Q^{\frac{1}{2}}}

Therefore,

(5.134) Ψ♭⁡(β,α,y)≥Cn⋅Q−14−12​n⋅ey⋅(−y)−1Γ⁡(α−β)⋅eF⁡(t0).\Tri(\fb,\fa,y)\geq C_{n}\cdot Q^{-\frac{1}{4}-\frac{1}{2n}}\cdot\frac{e^{y}\cdot(-y)^{-1}}{\Gamma(\alpha-\beta)}\cdot e^{F(t_{0})}.

The uniform estimate for Φ♯⁡(β,α,y)\Ku(\fb,\fa,y) stated in (5.117) can be proved in the same way. One just needs to apply Laplace’s method to the integral estimate formula in Lemma 5.8. We can eventually obtain

(5.135) Cn−1⋅Q−14⋅eG⁡(u0)≤∫0∞eG⁡(u)​𝑑u≤Cn⋅eG⁡(u0).C_{n}^{-1}\cdot Q^{-\frac{1}{4}}\cdot e^{G(u_{0})}\leq\int_{0}^{\infty}e^{G(u)}du\leq C_{n}\cdot e^{G(u_{0})}.

We omit the computations here.

∎

Converting into the variables zz, we obtain

Corollary 5.9.1.

There exists Cn>0C_{n}>0 such that for all z≥1z\geq 1, we have

(5.136) Cn−1⋅Q−14−12​nΓ⁡(Q+1)⋅e−jk⋅zn2+F​(t0​(z))⋅(jk​zn)−1\displaystyle C_{n}^{-1}\cdot\frac{Q^{-\frac{1}{4}-\frac{1}{2n}}}{\Gamma(Q+1)}\cdot e^{-\frac{j_{k}\cdot z^{n}}{2}+F(t_{0}(z))}\cdot(j_{k}z^{n})^{-1} ≤𝒟k​(z)≤Cn⋅Q14Γ⁡(Q+1)⋅e−jk⋅zn2+F​(t0​(z)),\displaystyle\leq\mathcal{D}_{k}(z)\leq C_{n}\cdot\frac{Q^{\frac{1}{4}}}{\Gamma(Q+1)}\cdot e^{-\frac{j_{k}\cdot z^{n}}{2}+F(t_{0}(z))},
(5.137) Cn−1⋅Q−14⋅(jk⋅zn)1−2​α4Γ⁡(Q+1)⋅e−jk⋅zn2+G​(u0​(z))\displaystyle C_{n}^{-1}\cdot Q^{-\frac{1}{4}}\cdot\frac{(j_{k}\cdot z^{n})^{\frac{1-2\alpha}{4}}}{\Gamma(Q+1)}\cdot e^{-\frac{j_{k}\cdot z^{n}}{2}+G(u_{0}(z))} ≤𝒢k​(z)≤Cn⋅(jk⋅zn)1−2​α4Γ⁡(Q+1)⋅e−jk⋅zn2+G​(u0​(z)),\displaystyle\leq\mathcal{G}_{k}(z)\leq C_{n}\cdot\frac{(j_{k}\cdot z^{n})^{\frac{1-2\alpha}{4}}}{\Gamma(Q+1)}\cdot e^{-\frac{j_{k}\cdot z^{n}}{2}+G(u_{0}(z))},

where Q≡α−β−1≥1Q\equiv\alpha-\beta-1\geq 1.

The next Proposition essentially gives an estimate of the product of Φ♯\Ku and Ψ♭\Tri.

Proposition 5.10.

There exists some dimensional constant Cn>0C_{n}>0 such that for any y≤−1y\leq-1, we have

(5.138) eF⁡(t0)+G⁡(u0)≤Cn​(−y)γn2​e−y​e−Q​QQ+γn2.e^{F(t_{0})+G(u_{0})}\leq C_{n}(-y)^{\frac{\gamma_{n}}{2}}e^{-y}e^{-Q}Q^{Q+\frac{\gamma_{n}}{2}}.

In particular we have

(5.139) Ψ♭⋅Φ♯≤Cn⋅Γ⁡(α)Γ​(α−β)2(−y)1nQQe−Qey.\Tri\cdot\Ku\leq C_{n}\cdot\frac{\Gamma(\alpha)}{\Gamma(\alpha-\beta)^{2}}(-y)^{\frac{1}{n}}Q^{Q}e^{-Q}e^{y}.
Proof.

The calculation in the proof is purely elementary. The order estimate involving the parameter QQ will be used at crucial places for our later estimates, so we include the detailed proof. Plugging the critical points formulae (5.114) and (5.115) into the expression of FF and GG,

(5.140) F⁡(t0)+G⁡(u0)=y​t0+(−y)12​u0−2​Q+γn2+Q​log​t0t0+1+(2​Q+γn)​log​u0,F(t_{0})+G(u_{0})=yt_{0}+(-y)^{\frac{1}{2}}u_{0}-\frac{2Q+\gamma_{n}}{2}+Q\log\frac{t_{0}}{t_{0}+1}+(2Q+\gamma_{n})\log u_{0},

where Q≡α−β−1Q\equiv\alpha-\beta-1 and γn≡12+1n\gamma_{n}\equiv\frac{1}{2}+\frac{1}{n} as before.

First, it is straightforward that

(5.141) y​t0+(−y)12​u0≤(−y)+γn2.yt_{0}+(-y)^{\frac{1}{2}}u_{0}\leq(-y)+\frac{\gamma_{n}}{2}.

So this implies that

(5.142) eF⁡(t0)+G⁡(u0)\displaystyle e^{F(t_{0})+G(u_{0})} ≤\displaystyle\leq Cn⋅e−y⋅e−Q⋅(t01+t0)Q⋅u02​Q+γn\displaystyle C_{n}\cdot e^{-y}\cdot e^{-Q}\cdot\Big(\frac{t_{0}}{1+t_{0}}\Big)^{Q}\cdot u_{0}^{2Q+\gamma_{n}}
=\displaystyle= Cn⋅e−y⋅e−Q⋅(t02t0​(1+t0))Q⋅u02​Q+γn\displaystyle C_{n}\cdot e^{-y}\cdot e^{-Q}\cdot\Big(\frac{t_{0}^{2}}{t_{0}(1+t_{0})}\Big)^{Q}\cdot u_{0}^{2Q+\gamma_{n}}
=\displaystyle= Cn⋅e−y⋅u0γn⋅e−Q⋅(u0​t0)2​Q(Q−y)Q,\displaystyle C_{n}\cdot e^{-y}\cdot u_{0}^{\gamma_{n}}\cdot e^{-Q}\cdot\frac{(u_{0}t_{0})^{2Q}}{(\frac{Q}{-y})^{Q}},

where the last equality follows from (5.112).

Now we claim

(5.143) u0​t0≤(−y)−12⋅(Q+γn2).u_{0}t_{0}\leq(-y)^{-\frac{1}{2}}\cdot(Q+\frac{\gamma_{n}}{2}).

To prove this, we denote τ≡2​γn−y>0\tau\equiv\frac{2\gamma_{n}}{-y}>0 and Q^≡4​Q−y>0\widehat{Q}\equiv\frac{4Q}{-y}>0. Then using the critical point formulae of u0u_{0} and t0t_{0} given by (5.114) and (5.115), we obtain

(5.144) u0​t0\displaystyle u_{0}t_{0}
=\displaystyle= (−y)124⋅(1+1+Q^)⋅(−1+1+Q^+τ)\displaystyle\frac{(-y)^{\frac{1}{2}}}{4}\cdot\Big(1+\sqrt{1+\widehat{Q}}\Big)\cdot\Big(-1+\sqrt{1+\widehat{Q}+\tau}\Big)
=\displaystyle= (−y)124⋅(−1+1+Q^⋅1+Q^+τ+1+Q^−1+Q^+τ)\displaystyle\frac{(-y)^{\frac{1}{2}}}{4}\cdot\Big(-1+\sqrt{1+\widehat{Q}}\cdot\sqrt{1+\widehat{Q}+\tau}+\sqrt{1+\widehat{Q}}-\sqrt{1+\widehat{Q}+\tau}\Big)
≤\displaystyle\leq (−y)124⋅(−1+1+Q^+τ⋅1+Q^+τ+1+Q^+τ−1+Q^+τ)\displaystyle\frac{(-y)^{\frac{1}{2}}}{4}\cdot\Big(-1+\sqrt{1+\widehat{Q}+\tau}\cdot\sqrt{1+\widehat{Q}+\tau}+\sqrt{1+\widehat{Q}+\tau}-\sqrt{1+\widehat{Q}+\tau}\Big)
=\displaystyle= (−y)124⋅(Q^+τ)\displaystyle\frac{(-y)^{\frac{1}{2}}}{4}\cdot(\widehat{Q}+\tau)
=\displaystyle= (−y)−12⋅(Q+γn2).\displaystyle(-y)^{-\frac{1}{2}}\cdot(Q+\frac{\gamma_{n}}{2}).

Then it follows that

(5.145) (u0​t0)2​Q(Q−y)Q≤(Q+γn2)2​QQQ=QQ⋅(1+γn2​Q)2​Q≤eγn⋅QQ.\frac{(u_{0}t_{0})^{2Q}}{(\frac{Q}{-y})^{Q}}\leq\frac{(Q+\frac{\gamma_{n}}{2})^{2Q}}{Q^{Q}}=Q^{Q}\cdot(1+\frac{\gamma_{n}}{2Q})^{2Q}\leq e^{\gamma_{n}}\cdot Q^{Q}.

Moreover, we notice that

(5.146) u0γn≤Cn⋅Qγn2⋅(−y)γn2.u_{0}^{\gamma_{n}}\leq C_{n}\cdot Q^{\frac{\gamma_{n}}{2}}\cdot(-y)^{\frac{\gamma_{n}}{2}}.

Therefore, combining all the above, we have

(5.147) eF⁡(t0)+G⁡(u0)\displaystyle e^{F(t_{0})+G(u_{0})} ≤\displaystyle\leq Cn⋅e−y⋅u0γn⋅e−Q⋅(u0​t0)2​Q(Q−y)Q\displaystyle C_{n}\cdot e^{-y}\cdot u_{0}^{\gamma_{n}}\cdot e^{-Q}\cdot\frac{(u_{0}t_{0})^{2Q}}{(\frac{Q}{-y})^{Q}}
≤\displaystyle\leq Cn⋅(−y)γn2⋅e−y⋅e−Q⋅QQ+γn2.\displaystyle C_{n}\cdot(-y)^{\frac{\gamma_{n}}{2}}\cdot e^{-y}\cdot e^{-Q}\cdot Q^{Q+\frac{\gamma_{n}}{2}}.

∎

In the next subsections, we will also need the following monotonicity formula to study the integral estimates for the above fundamental solutions 𝒢k\mathcal{G}_{k} and 𝒟k\mathcal{D}_{k}.

Lemma 5.11.

Let

(5.148) F^​(z)\displaystyle\widehat{F}(z) ≡−j​zn2+F⁡(t0​(z)),\displaystyle\equiv-\frac{jz^{n}}{2}+F(t_{0}(z)),
(5.149) G^​(z)\displaystyle\widehat{G}(z) ≡−j​zn2+G⁡(u0​(z)),\displaystyle\equiv-\frac{jz^{n}}{2}+G(u_{0}(z)),

then for all η≥0\eta\geq 0, when z≥η2nz\geq\eta^{\frac{2}{n}}, F^​(z)+η⋅zn2\widehat{F}(z)+\eta\cdot z^{\frac{n}{2}} is decreasing and G^​(z)−η⋅zn2\widehat{G}(z)-\eta\cdot z^{\frac{n}{2}} is increasing.

Proof.

Let y=−j​zny=-jz^{n}, then it is straightforward that

(5.150) d​F^​(y)d​y=12+t0​(y)+F′​(t0​(y))⋅d​t0​(y)d​y=12+t0​(y)=12​1+4​Q−y≥12.\displaystyle\frac{d\widehat{F}(y)}{dy}=\frac{1}{2}+t_{0}(y)+F^{\prime}(t_{0}(y))\cdot\frac{dt_{0}(y)}{dy}=\frac{1}{2}+t_{0}(y)=\frac{1}{2}\sqrt{1+\frac{4Q}{-y}}\geq\frac{1}{2}.

This implies that, as z≥η2nz\geq\eta^{\frac{2}{n}},

(5.151) d​(F^​(z)+η​zn2)d​z=d​F^​(y)d​y⋅(−nj⋅zn−1)+n⋅η2⋅zn2−1≤−n2⋅zn2−1(j⋅zn2−η)≤0.\displaystyle\frac{d(\widehat{F}(z)+\eta z^{\frac{n}{2}})}{dz}=\frac{d\widehat{F}(y)}{dy}\cdot(-nj\cdot z^{n-1})+\frac{n\cdot\eta}{2}\cdot z^{\frac{n}{2}-1}\leq-\frac{n}{2}\cdot z^{\frac{n}{2}-1}(j\cdot z^{\frac{n}{2}}-\eta)\leq 0.

By similar calculations, one can also obtain that G^​(z)−η⋅zn2\widehat{G}(z)-\eta\cdot z^{\frac{n}{2}} is increasing as z≥η2nz\geq\eta^{\frac{2}{n}}.

∎

Case (B): Now we consider the case when Q≤1Q\leq 1. As mentioned in the above, this case is easier.

Lemma 5.12.

Let Q≤1Q\leq 1, then there is some dimensional constant Cn>0C_{n}>0 such that

(5.152) Cn−1⋅ey⋅(−y)β−α\displaystyle C_{n}^{-1}\cdot e^{y}\cdot(-y)^{\beta-\alpha} ≤Ψ♭⁡(β,α,y)≤ey⋅(−y)β−α,\displaystyle\leq\Tri(\fb,\fa,y)\leq e^{y}\cdot(-y)^{\beta-\alpha},
(5.153) Cn−1⋅(−y)−β\displaystyle C_{n}^{-1}\cdot(-y)^{-\beta} ≤Φ♯⁡(β,α,y)≤Cn⋅(−y)−β.\displaystyle\leq\Ku(\fb,\fa,y)\leq C_{n}\cdot(-y)^{-\beta}.

for all y≤−1y\leq-1.

Remark 5.12.1.

In the case Q≤1Q\leq 1, the estimate is optimal in the sense that it coincides with the asymptotic behavior of Ψ♭\Tri and Φ♯\Ku for fixed α\alpha and β\beta, as given in Lemma A.3 and Lemma A.5.

Proof.

First, we prove (5.152). Both the upper bound and lower bound estimates can be proved in the similar way:

Ψ♭⁡(β,α,y)\displaystyle\Tri(\beta,\alpha,y) =eyΓ⁡(α−β)​∫0∞ey​t​tα−β−1​(1+t)β−1​𝑑t\displaystyle=\frac{e^{y}}{\Gamma(\fa-\fb)}\int_{0}^{\infty}e^{yt}t^{\fa-\fb-1}(1+t)^{\fb-1}dt
≤eyΓ⁡(α−β)⋅∫0∞ey​t​tα−β−1​𝑑t\displaystyle\leq\frac{e^{y}}{\Gamma(\fa-\fb)}\cdot\int_{0}^{\infty}e^{yt}t^{\fa-\fb-1}dt
=ey⋅(−y)β−αΓ⁡(α−β)⋅∫0∞e−u​uα−β−1​𝑑u\displaystyle=\frac{e^{y}\cdot(-y)^{\beta-\alpha}}{\Gamma(\fa-\fb)}\cdot\int_{0}^{\infty}e^{-u}u^{\fa-\fb-1}du
(5.154) =ey⋅(−y)β−α.\displaystyle=e^{y}\cdot(-y)^{\beta-\alpha}.

Similarly,

Ψ♭⁡(β,α,y)\displaystyle\Tri(\fb,\fa,y) ≥eyΓ⁡(α−β)​∫01ey​t​tα−β−1​(1+t)β−1​𝑑t\displaystyle\geq\frac{e^{y}}{\Gamma(\fa-\fb)}\int_{0}^{1}e^{yt}t^{\fa-\fb-1}(1+t)^{\fb-1}dt
≥Cn⋅ey∫01ey​ttα−β−1dt\displaystyle\geq C_{n}\cdot e^{y}\int_{0}^{1}e^{yt}t^{\fa-\fb-1}dt
(5.155) ≥Cn⋅ey⋅(−y)β−α.\displaystyle\geq C_{n}\cdot e^{y}\cdot(-y)^{\fb-\fa}.

Next, we prove the upper bound estimate for Φ♯\Ku. Notice in the proof of Lemma 5.9 we do not need the condition Q≤1Q\leq 1 for the upper bound on Φ♯\Ku. So we have

(5.156) Φ♯⁡(β,α,y)≤Cn⋅Γ⁡(α)Γ⁡(α−β)⋅(−y)1−2​α4⋅ey+G⁡(u0).\Ku(\beta,\alpha,y)\leq C_{n}\cdot\frac{\Gamma(\alpha)}{\Gamma(\alpha-\beta)}\cdot(-y)^{\frac{1-2\alpha}{4}}\cdot e^{y+G(u_{0})}.

To prove (5.153), we need an upper bound estimate for ey+G⁡(u0)e^{y+G(u_{0})}. This follows from elementary computations. In fact,

ey+G⁡(u0)=ey−u02+2​−y​u0⋅(u0)2​Q+γn≤Cn⋅ey−u02+2​−y​u0⋅(−y)Q+γn2.e^{y+G(u_{0})}=e^{y-u_{0}^{2}+2\sqrt{-y}u_{0}}\cdot(u_{0})^{2Q+\gamma_{n}}\\ \leq C_{n}\cdot e^{y-u_{0}^{2}+2\sqrt{-y}u_{0}}\cdot(-y)^{Q+\frac{\gamma_{n}}{2}}.

Notice that u0u_{0} satisfies G′​(u0)=0G^{\prime}(u_{0})=0, i.e.,

(5.157) u02−−y⋅u0−2​Q+γn2=0,u_{0}^{2}-\sqrt{-y}\cdot u_{0}-\frac{2Q+\gamma_{n}}{2}=0,

so we have

(5.158) ey+G⁡(u0)≤Cn⋅ey+−y​u0⋅(−y)Q+γn2.e^{y+G(u_{0})}\leq C_{n}\cdot e^{y+\sqrt{-y}u_{0}}\cdot(-y)^{Q+\frac{\gamma_{n}}{2}}.

By (5.115), it is straightforward that

(5.159) y+−y​u0=y2​(1−1+4​Q+2​γn−y)=2​Q+γn1+1+4​Q+2​γn−y∈[Cn−1,Cn],\displaystyle y+\sqrt{-y}u_{0}=\frac{y}{2}\Big(1-\sqrt{1+\frac{4Q+2\gamma_{n}}{-y}}\Big)=\frac{2Q+\gamma_{n}}{1+\sqrt{1+\frac{4Q+2\gamma_{n}}{-y}}}\in[C_{n}^{-1},C_{n}],

for some dimensional constant Cn>0C_{n}>0. Therefore,

(5.160) ey+G⁡(u0)≤Cn​(−y)Q+14+12​n,\displaystyle e^{y+G(u_{0})}\leq C_{n}(-y)^{Q+\frac{1}{4}+\frac{1}{2n}},

and hence

(5.161) Φ♯⁡(β,α,y)≤Cn​(−y)Q+1n=Cn​(−y)−β.\displaystyle\Ku(\fb,\fa,y)\leq C_{n}(-y)^{Q+\frac{1}{n}}=C_{n}(-y)^{-\beta}.

This completes the proof. ∎

Converting into the variables zz we obtain

Corollary 5.12.1.

There exists Cn>0C_{n}>0 such that for all z≥1z\geq 1, we have

(5.162) Cn−1⋅e−jk⋅zn2⋅(jk​zn)β−α\displaystyle C_{n}^{-1}\cdot e^{-\frac{j_{k}\cdot z^{n}}{2}}\cdot(j_{k}z^{n})^{\beta-\alpha} ≤𝒟k​(z)≤Cn⋅e−jk⋅zn2⋅(jk​zn)β−α,\displaystyle\leq\mathcal{D}_{k}(z)\leq C_{n}\cdot e^{-\frac{j_{k}\cdot z^{n}}{2}}\cdot(j_{k}z^{n})^{\beta-\alpha},
(5.163) Cn−1⋅ejk⋅zn2⋅(jk​zn)−β\displaystyle C_{n}^{-1}\cdot e^{\frac{j_{k}\cdot z^{n}}{2}}\cdot(j_{k}z^{n})^{-\beta} ≤𝒢k​(z)≤Cn⋅ejk⋅zn2⋅(jk​zn)−β.\displaystyle\leq\mathcal{G}_{k}(z)\leq C_{n}\cdot e^{\frac{j_{k}\cdot z^{n}}{2}}\cdot(j_{k}z^{n})^{-\beta}.

We end this subsection by making some remarks regarding the above estimates on Φ♯\Ku and Ψ♭\Tri. Notice that in the case Q≡α−β−1≤1Q\equiv\fa-\fb-1\leq 1 we applied Laplace’s method to turn the problem into estimates on exponential integrals. One may wonder how far the uniform estimates in Lemma 5.9 is from optimal comparing to the non-uniform estimate with the optimal order in Lemma 5.12. We can consider two extreme cases depending on the size of QQ compared with −y-y.

First we assume Q2−y≪1\frac{Q^{2}}{-y}\ll 1, which obviously includes the case when we fix QQ and let y→−∞y\rightarrow-\infty. Then by definition we see that

(5.164) t0=Q−y+O⁡((Q−y)2),t_{0}=\frac{Q}{-y}+O\Big((\frac{Q}{-y})^{2}\Big),

and we get

(5.165) F⁡(t0)=y​t0+Q​log⁡t0t0+1=−Q+Q​log⁡Q−Q​log⁡(−y)+O⁡(Q−y).F(t_{0})=yt_{0}+Q\log\frac{t_{0}}{t_{0}+1}=-Q+Q\log Q-Q\log(-y)+O(\frac{Q}{-y}).

So by Lemma 5.9 we get

(5.166) Cn−1​Q−14−12​n​ey​(−y)−Q−1​QQ​e−Q≤Ψ♭≤Cn​1Γ⁡(α−β)​ey​(−y)−Q​QQ​e−Q​Q14.C_{n}^{-1}Q^{-\frac{1}{4}-\frac{1}{2n}}e^{y}(-y)^{-Q-1}Q^{Q}e^{-Q}\leq\Tri\leq C_{n}\frac{1}{\Gamma(\alpha-\beta)}e^{y}(-y)^{-Q}Q^{Q}e^{-Q}Q^{\frac{1}{4}}.

Notice by Stirling’s formula for QQ large Γ⁡(α−β)=Q​Γ​(Q)\Gamma(\alpha-\beta)=Q\Gamma(Q) is comparable to Cn​Q32​QQ​e−QC_{n}Q^{\frac{3}{2}}Q^{Q}e^{-Q}. So up to polynomial errors in QQ this estimate is optimal comparing with (A.27). Similarly, we have

(5.167) u0=(−y)12​(1+Q+12​γn−y+O⁡((Q−y)2)),u_{0}=(-y)^{\frac{1}{2}}\Big(1+\frac{Q+\frac{1}{2}\gamma_{n}}{-y}+O((\frac{Q}{-y})^{2})\Big),

and

(5.168) G⁡(u0)=−u02+2​(−y)12​u0+(2​Q+γn)​log⁡u0≤Cn​e−y​(−y)Q+γn2.G(u_{0})=-u_{0}^{2}+2(-y)^{\frac{1}{2}}u_{0}+(2Q+\gamma_{n})\log u_{0}\leq C_{n}e^{-y}(-y)^{Q+\frac{\gamma_{n}}{2}}.

So

(5.169) Φ♯≤Cn​Γ⁡(α)Γ⁡(α−β)​(−y)1−2​α4​(−y)Q+γn2=Cn​Γ⁡(α)Γ⁡(α−β)​(−y)−β,\Ku\leq C_{n}\frac{\Gamma(\alpha)}{\Gamma(\alpha-\beta)}(-y)^{\frac{1-2\alpha}{4}}(-y)^{Q+\frac{\gamma_{n}}{2}}=C_{n}\frac{\Gamma(\alpha)}{\Gamma(\alpha-\beta)}(-y)^{-\beta},

which is again optimal comparing with (A.34).

Secondly we assume the other extreme Q(−y)3≫1\frac{Q}{(-y)^{3}}\gg 1. In this case we have

(5.170) t0=Q−y−12+O⁡(−yQ).t_{0}=\sqrt{\frac{Q}{-y}}-\frac{1}{2}+O(\sqrt{\frac{-y}{Q}}).

Then we get

(5.171) F⁡(t0)=−2​−Q​y−12​y+O⁡(1),F(t_{0})=-2\sqrt{-Qy}-\frac{1}{2}y+O(1),

and

(5.172) Cn−1​Q−14−12​n​e12​y−−Q​y​(−y)−Q−1≤Ψ♭⁡(y)≤Cn​1Γ⁡(α−β)​Q14​(−y)−Q​e12​y−2​−Qy.C_{n}^{-1}Q^{-\frac{1}{4}-\frac{1}{2n}}e^{\frac{1}{2}y-\sqrt{-Qy}}(-y)^{-Q-1}\leq\Tri(y)\leq C_{n}\frac{1}{\Gamma(\alpha-\beta)}Q^{\frac{1}{4}}(-y)^{-Q}e^{\frac{1}{2}y-2\sqrt{-Qy}}.

Similarly, we get

(5.173) G⁡(u0)=2​−Q​y−y2+(Q+12​γn)​log⁡Q−Q.G(u_{0})=2\sqrt{-Qy}-\frac{y}{2}+(Q+\frac{1}{2}\gamma_{n})\log Q-Q.

So

(5.174) Φ♯⁡(y)≤Cn⋅Γ⁡(α)Γ⁡(α−β)​(−y)1−2​α4​e12​y+2​−Qy​e−Q​QQ+12​γn.\Ku(y)\leq C_{n}\cdot\frac{\Gamma(\alpha)}{\Gamma(\alpha-\beta)}(-y)^{\frac{1-2\alpha}{4}}e^{\frac{1}{2}y+2\sqrt{-Qy}}e^{-Q}Q^{Q+\frac{1}{2}\gamma_{n}}.

In this case even though in the produce Ψ♭⋅Φ♯\Tri\cdot\Ku there is a good cancellation each of them does behave quite differently from the previous case. This also gives a reason why we do get an optimal estimate (up to polynomial errors in yy and QQ) for the product Ψ♭⋅Φ♯\Tri\cdot\Ku, comparing with (A.27) and (A.34).

Original mathematics by the credited authors. Source-backed reader collection; mathematical self-containment is not assessed.