Exam : STEP2 | Year : 2003 | Questions : Q1—Q7 | Total marks per question : 20
All questions are pure mathematics. Solutions and examiner commentary are included below.
Q Topic Difficulty Key Techniques 1 线性方程组(Systems of Linear Equations) Standard 参数讨论,线性方程组求解,约束优化 2 三角函数与反三角函数(Trigonometric and Inverse Trigonometric Functions) Standard 辅助角公式,反三角函数恒等式 3 无理数与证明(Irrationality and Proof) Challenging 反证法,数学归纳法,极限构造 4 解析几何(Analytic Geometry) Standard 弓形面积公式,反余弦函数,坐标变换 5 向量(Vectors) Standard 向量参数方程,中点公式,共面条件 6 函数迭代与积分(Function Iteration and Integration) Challenging 函数迭代,绝对值函数图像,三角函数积分 7 积分与级数(Integration and Series) Challenging 分部积分,反常积分,级数放缩
Topic : 线性方程组(Systems of Linear Equations) | Difficulty : Standard | Marks : 20
1 Consider the equations
a x − y − z = 3 , ax - y - z = 3 , a x − y − z = 3 ,
2 a x − y − 3 z = 7 , 2ax - y - 3z = 7 , 2 a x − y − 3 z = 7 ,
3 a x − y − 5 z = b , 3ax - y - 5z = b , 3 a x − y − 5 z = b ,
where a a a and b b b are given constants.
(i) In the case a = 0 a = 0 a = 0 , show that the equations have a solution if and only if b = 11 b = 11 b = 11 .
(ii) In the case a ≠ 0 a \neq 0 a = 0 and b = 11 b = 11 b = 11 show that the equations have a solution with z = λ z = \lambda z = λ for any given number λ \lambda λ .
(iii) In the case a = 2 a = 2 a = 2 and b = 11 b = 11 b = 11 find the solution for which x 2 + y 2 + z 2 x^2 + y^2 + z^2 x 2 + y 2 + z 2 is least.
(iv) Find a value for a a a for which there is a solution such that x > 10 6 x > 10^6 x > 1 0 6 and y 2 + z 2 < 1 y^2 + z^2 < 1 y 2 + z 2 < 1 .
Model Solution
Part (i)
When a = 0 a = 0 a = 0 , the equations become:
− y − z = 3 , − y − 3 z = 7 , − y − 5 z = b . -y - z = 3, \qquad -y - 3z = 7, \qquad -y - 5z = b. − y − z = 3 , − y − 3 z = 7 , − y − 5 z = b .
Subtracting the first from the second:
( − y − 3 z ) − ( − y − z ) = 7 − 3 ⟹ − 2 z = 4 ⟹ z = − 2. (-y - 3z) - (-y - z) = 7 - 3 \implies -2z = 4 \implies z = -2. ( − y − 3 z ) − ( − y − z ) = 7 − 3 ⟹ − 2 z = 4 ⟹ z = − 2.
Substituting into the first equation: − y − ( − 2 ) = 3 ⟹ − y + 2 = 3 ⟹ y = − 1 -y - (-2) = 3 \implies -y + 2 = 3 \implies y = -1 − y − ( − 2 ) = 3 ⟹ − y + 2 = 3 ⟹ y = − 1 .
Substituting y = − 1 y = -1 y = − 1 and z = − 2 z = -2 z = − 2 into the third equation:
− ( − 1 ) − 5 ( − 2 ) = b ⟹ 1 + 10 = b ⟹ b = 11. -(-1) - 5(-2) = b \implies 1 + 10 = b \implies b = 11. − ( − 1 ) − 5 ( − 2 ) = b ⟹ 1 + 10 = b ⟹ b = 11.
So the equations have a solution if and only if b = 11 b = 11 b = 11 . ■ \quad \blacksquare ■
Part (ii)
When b = 11 b = 11 b = 11 , the system is:
a x − y − z = 3 , 2 a x − y − 3 z = 7 , 3 a x − y − 5 z = 11. ax - y - z = 3, \qquad 2ax - y - 3z = 7, \qquad 3ax - y - 5z = 11. a x − y − z = 3 , 2 a x − y − 3 z = 7 , 3 a x − y − 5 z = 11.
Subtracting the first equation from the second:
a x − 2 z = 4 (...) ax - 2z = 4 \qquad \text{(...)} a x − 2 z = 4 (...)
Subtracting the second from the third:
a x − 2 z = 4 (...) ax - 2z = 4 \qquad \text{(...)} a x − 2 z = 4 (...)
So the third equation is redundant (it gives the same condition as the first two combined). From ( ∗ ) (*) ( ∗ ) : a x = 4 + 2 z ax = 4 + 2z a x = 4 + 2 z . Since a ≠ 0 a \neq 0 a = 0 :
x = 4 + 2 z a . x = \frac{4 + 2z}{a}. x = a 4 + 2 z .
From the first equation: y = a x − z − 3 = ( 4 + 2 z ) − z − 3 = 1 + z y = ax - z - 3 = (4 + 2z) - z - 3 = 1 + z y = a x − z − 3 = ( 4 + 2 z ) − z − 3 = 1 + z .
Setting z = λ z = \lambda z = λ :
x = 4 + 2 λ a , y = 1 + λ , z = λ . x = \frac{4 + 2\lambda}{a}, \qquad y = 1 + \lambda, \qquad z = \lambda. x = a 4 + 2 λ , y = 1 + λ , z = λ .
This is a valid solution for any λ \lambda λ . ■ \quad \blacksquare ■
Part (iii)
With a = 2 a = 2 a = 2 and b = 11 b = 11 b = 11 , the solution from part (ii) gives:
x = 4 + 2 λ 2 = 2 + λ , y = 1 + λ , z = λ . x = \frac{4 + 2\lambda}{2} = 2 + \lambda, \qquad y = 1 + \lambda, \qquad z = \lambda. x = 2 4 + 2 λ = 2 + λ , y = 1 + λ , z = λ .
We minimise x 2 + y 2 + z 2 x^2 + y^2 + z^2 x 2 + y 2 + z 2 :
x 2 + y 2 + z 2 = ( 2 + λ ) 2 + ( 1 + λ ) 2 + λ 2 x^2 + y^2 + z^2 = (2 + \lambda)^2 + (1 + \lambda)^2 + \lambda^2 x 2 + y 2 + z 2 = ( 2 + λ ) 2 + ( 1 + λ ) 2 + λ 2
= 4 + 4 λ + λ 2 + 1 + 2 λ + λ 2 + λ 2 = 3 λ 2 + 6 λ + 5. = 4 + 4\lambda + \lambda^2 + 1 + 2\lambda + \lambda^2 + \lambda^2 = 3\lambda^2 + 6\lambda + 5. = 4 + 4 λ + λ 2 + 1 + 2 λ + λ 2 + λ 2 = 3 λ 2 + 6 λ + 5.
Completing the square:
3 λ 2 + 6 λ + 5 = 3 ( λ 2 + 2 λ ) + 5 = 3 ( λ + 1 ) 2 − 3 + 5 = 3 ( λ + 1 ) 2 + 2. 3\lambda^2 + 6\lambda + 5 = 3(\lambda^2 + 2\lambda) + 5 = 3(\lambda + 1)^2 - 3 + 5 = 3(\lambda + 1)^2 + 2. 3 λ 2 + 6 λ + 5 = 3 ( λ 2 + 2 λ ) + 5 = 3 ( λ + 1 ) 2 − 3 + 5 = 3 ( λ + 1 ) 2 + 2.
This is minimised when λ = − 1 \lambda = -1 λ = − 1 , giving x = 1 x = 1 x = 1 , y = 0 y = 0 y = 0 , z = − 1 z = -1 z = − 1 .
The minimum value of x 2 + y 2 + z 2 x^2 + y^2 + z^2 x 2 + y 2 + z 2 is 2 2 2 , and the solution is ( x , y , z ) = ( 1 , 0 , − 1 ) (x, y, z) = (1, 0, -1) ( x , y , z ) = ( 1 , 0 , − 1 ) .
Part (iv)
From part (ii), with z = λ z = \lambda z = λ , a ≠ 0 a \neq 0 a = 0 and b = 11 b = 11 b = 11 :
x = 4 + 2 λ a , y = 1 + λ , z = λ . x = \frac{4 + 2\lambda}{a}, \qquad y = 1 + \lambda, \qquad z = \lambda. x = a 4 + 2 λ , y = 1 + λ , z = λ .
We need x > 10 6 x > 10^6 x > 1 0 6 and y 2 + z 2 < 1 y^2 + z^2 < 1 y 2 + z 2 < 1 . From y 2 + z 2 < 1 y^2 + z^2 < 1 y 2 + z 2 < 1 :
( 1 + λ ) 2 + λ 2 < 1 ⟹ 2 λ 2 + 2 λ + 1 < 1 ⟹ 2 λ ( λ + 1 ) < 0. (1 + \lambda)^2 + \lambda^2 < 1 \implies 2\lambda^2 + 2\lambda + 1 < 1 \implies 2\lambda(\lambda + 1) < 0. ( 1 + λ ) 2 + λ 2 < 1 ⟹ 2 λ 2 + 2 λ + 1 < 1 ⟹ 2 λ ( λ + 1 ) < 0.
So − 1 < λ < 0 -1 < \lambda < 0 − 1 < λ < 0 . In particular, 4 + 2 λ > 2 4 + 2\lambda > 2 4 + 2 λ > 2 (since λ > − 1 \lambda > -1 λ > − 1 ).
To make x = 4 + 2 λ a > 10 6 x = \frac{4 + 2\lambda}{a} > 10^6 x = a 4 + 2 λ > 1 0 6 , we need a a a to be small and positive (since 4 + 2 λ > 0 4 + 2\lambda > 0 4 + 2 λ > 0 ).
For example, choose λ = − 1 2 \lambda = -\frac{1}{2} λ = − 2 1 (which satisfies − 1 < λ < 0 -1 < \lambda < 0 − 1 < λ < 0 ). Then y = 1 2 y = \frac{1}{2} y = 2 1 , z = − 1 2 z = -\frac{1}{2} z = − 2 1 , so y 2 + z 2 = 1 2 < 1 y^2 + z^2 = \frac{1}{2} < 1 y 2 + z 2 = 2 1 < 1 . And x = 3 a x = \frac{3}{a} x = a 3 , which exceeds 10 6 10^6 1 0 6 when a < 3 10 6 = 3 × 10 − 6 a < \frac{3}{10^6} = 3 \times 10^{-6} a < 1 0 6 3 = 3 × 1 0 − 6 .
So any a a a with 0 < a < 3 × 10 − 6 0 < a < 3 \times 10^{-6} 0 < a < 3 × 1 0 − 6 works. For instance, a = 10 − 6 a = 10^{-6} a = 1 0 − 6 is a valid choice.
Topic : 三角函数与反三角函数(Trigonometric and Inverse Trigonometric Functions) | Difficulty : Standard | Marks : 20
2 Write down a value of θ \theta θ in the interval π / 4 < θ < π / 2 \pi/4 < \theta < \pi/2 π /4 < θ < π /2 that satisfies the equation
4 cos θ + 2 3 sin θ = 5. 4 \cos \theta + 2\sqrt{3} \sin \theta = 5 . 4 cos θ + 2 3 sin θ = 5.
Hence, or otherwise, show that
π = 3 arccos ( 5 / 28 ) + 3 arctan ( 3 / 2 ) . \pi = 3 \arccos(5/\sqrt{28}) + 3 \arctan(\sqrt{3}/2) . π = 3 arccos ( 5/ 28 ) + 3 arctan ( 3 /2 ) .
Show that
π = 4 arcsin ( 7 2 / 10 ) − 4 arctan ( 3 / 4 ) . \pi = 4 \arcsin(7\sqrt{2}/10) - 4 \arctan(3/4) . π = 4 arcsin ( 7 2 /10 ) − 4 arctan ( 3/4 ) .
Model Solution
Finding θ
We use the auxiliary angle form. Write
4 cos θ + 2 3 sin θ = R cos ( θ − α ) 4\cos\theta + 2\sqrt{3}\sin\theta = R\cos(\theta - \alpha) 4 cos θ + 2 3 sin θ = R cos ( θ − α )
where R cos α = 4 R\cos\alpha = 4 R cos α = 4 and R sin α = 2 3 R\sin\alpha = 2\sqrt{3} R sin α = 2 3 . Then
R = 16 + 12 = 28 = 2 7 , tan α = 2 3 4 = 3 2 . R = \sqrt{16 + 12} = \sqrt{28} = 2\sqrt{7}, \qquad \tan\alpha = \frac{2\sqrt{3}}{4} = \frac{\sqrt{3}}{2}. R = 16 + 12 = 28 = 2 7 , tan α = 4 2 3 = 2 3 .
So α = arctan ( 3 / 2 ) \alpha = \arctan(\sqrt{3}/2) α = arctan ( 3 /2 ) . The equation becomes
28 cos ( θ − α ) = 5 ⟹ cos ( θ − α ) = 5 28 . \sqrt{28}\cos(\theta - \alpha) = 5 \implies \cos(\theta - \alpha) = \frac{5}{\sqrt{28}}. 28 cos ( θ − α ) = 5 ⟹ cos ( θ − α ) = 28 5 .
Hence θ − α = ± arccos ( 5 / 28 ) \theta - \alpha = \pm\arccos(5/\sqrt{28}) θ − α = ± arccos ( 5/ 28 ) , giving θ = α ± arccos ( 5 / 28 ) \theta = \alpha \pm \arccos(5/\sqrt{28}) θ = α ± arccos ( 5/ 28 ) .
Taking the positive sign: θ = arctan ( 3 / 2 ) + arccos ( 5 / 28 ) \theta = \arctan(\sqrt{3}/2) + \arccos(5/\sqrt{28}) θ = arctan ( 3 /2 ) + arccos ( 5/ 28 ) .
Numerically: α ≈ 40.9 ° \alpha \approx 40.9° α ≈ 40.9° and arccos ( 5 / 28 ) ≈ 19.1 ° \arccos(5/\sqrt{28}) \approx 19.1° arccos ( 5/ 28 ) ≈ 19.1° , so θ ≈ 60 ° = π / 3 \theta \approx 60° = \pi/3 θ ≈ 60° = π /3 .
We verify that θ = π / 3 \theta = \pi/3 θ = π /3 lies in ( π / 4 , π / 2 ) (\pi/4, \pi/2) ( π /4 , π /2 ) and satisfies the equation:
4 cos π 3 + 2 3 sin π 3 = 4 ⋅ 1 2 + 2 3 ⋅ 3 2 = 2 + 3 = 5. ✓ 4\cos\frac{\pi}{3} + 2\sqrt{3}\sin\frac{\pi}{3} = 4\cdot\frac{1}{2} + 2\sqrt{3}\cdot\frac{\sqrt{3}}{2} = 2 + 3 = 5. \quad \checkmark 4 cos 3 π + 2 3 sin 3 π = 4 ⋅ 2 1 + 2 3 ⋅ 2 3 = 2 + 3 = 5. ✓
So θ = π / 3 \theta = \pi/3 θ = π /3 .
Show that π = 3 arccos ( 5 / 28 ) + 3 arctan ( 3 / 2 ) \pi = 3\arccos(5/\sqrt{28}) + 3\arctan(\sqrt{3}/2) π = 3 arccos ( 5/ 28 ) + 3 arctan ( 3 /2 )
From the auxiliary angle form with θ = π / 3 \theta = \pi/3 θ = π /3 :
28 cos ( π 3 − α ) = 5 ⟹ cos ( π 3 − α ) = 5 28 . \sqrt{28}\cos\!\left(\frac{\pi}{3} - \alpha\right) = 5 \implies \cos\!\left(\frac{\pi}{3} - \alpha\right) = \frac{5}{\sqrt{28}}. 28 cos ( 3 π − α ) = 5 ⟹ cos ( 3 π − α ) = 28 5 .
Since π / 3 − α ≈ 19.1 ° ∈ ( 0 , π / 2 ) \pi/3 - \alpha \approx 19.1° \in (0, \pi/2) π /3 − α ≈ 19.1° ∈ ( 0 , π /2 ) , we have
π 3 − α = arccos ( 5 28 ) . \frac{\pi}{3} - \alpha = \arccos\!\left(\frac{5}{\sqrt{28}}\right). 3 π − α = arccos ( 28 5 ) .
Rearranging:
π 3 = arccos ( 5 28 ) + α = arccos ( 5 28 ) + arctan ( 3 2 ) . \frac{\pi}{3} = \arccos\!\left(\frac{5}{\sqrt{28}}\right) + \alpha = \arccos\!\left(\frac{5}{\sqrt{28}}\right) + \arctan\!\left(\frac{\sqrt{3}}{2}\right). 3 π = arccos ( 28 5 ) + α = arccos ( 28 5 ) + arctan ( 2 3 ) .
Multiplying both sides by 3:
π = 3 arccos ( 5 28 ) + 3 arctan ( 3 2 ) . ■ \pi = 3\arccos\!\left(\frac{5}{\sqrt{28}}\right) + 3\arctan\!\left(\frac{\sqrt{3}}{2}\right). \qquad \blacksquare π = 3 arccos ( 28 5 ) + 3 arctan ( 2 3 ) . ■
Show that π = 4 arcsin ( 7 2 / 10 ) − 4 arctan ( 3 / 4 ) \pi = 4\arcsin(7\sqrt{2}/10) - 4\arctan(3/4) π = 4 arcsin ( 7 2 /10 ) − 4 arctan ( 3/4 )
Let ϕ = arcsin ( 7 2 / 10 ) \phi = \arcsin(7\sqrt{2}/10) ϕ = arcsin ( 7 2 /10 ) and β = arctan ( 3 / 4 ) \beta = \arctan(3/4) β = arctan ( 3/4 ) . We show that ϕ − β = π / 4 \phi - \beta = \pi/4 ϕ − β = π /4 .
From sin ϕ = 7 2 / 10 \sin\phi = 7\sqrt{2}/10 sin ϕ = 7 2 /10 , since ϕ \phi ϕ is acute:
cos ϕ = 1 − 98 100 = 1 50 = 2 10 . \cos\phi = \sqrt{1 - \frac{98}{100}} = \sqrt{\frac{1}{50}} = \frac{\sqrt{2}}{10}. cos ϕ = 1 − 100 98 = 50 1 = 10 2 .
From tan β = 3 / 4 \tan\beta = 3/4 tan β = 3/4 (a 3-4-5 right triangle):
sin β = 3 5 , cos β = 4 5 . \sin\beta = \frac{3}{5}, \qquad \cos\beta = \frac{4}{5}. sin β = 5 3 , cos β = 5 4 .
Computing sin ( ϕ − β ) \sin(\phi - \beta) sin ( ϕ − β ) :
sin ( ϕ − β ) = sin ϕ cos β − cos ϕ sin β = 7 2 10 ⋅ 4 5 − 2 10 ⋅ 3 5 = 28 2 − 3 2 50 = 25 2 50 = 2 2 . \sin(\phi - \beta) = \sin\phi\cos\beta - \cos\phi\sin\beta = \frac{7\sqrt{2}}{10}\cdot\frac{4}{5} - \frac{\sqrt{2}}{10}\cdot\frac{3}{5} = \frac{28\sqrt{2} - 3\sqrt{2}}{50} = \frac{25\sqrt{2}}{50} = \frac{\sqrt{2}}{2}. sin ( ϕ − β ) = sin ϕ cos β − cos ϕ sin β = 10 7 2 ⋅ 5 4 − 10 2 ⋅ 5 3 = 50 28 2 − 3 2 = 50 25 2 = 2 2 .
Since 0 < β < ϕ < π / 2 0 < \beta < \phi < \pi/2 0 < β < ϕ < π /2 , we have 0 < ϕ − β < π / 2 0 < \phi - \beta < \pi/2 0 < ϕ − β < π /2 . The unique angle in ( 0 , π / 2 ) (0, \pi/2) ( 0 , π /2 ) with sine 2 / 2 \sqrt{2}/2 2 /2 is π / 4 \pi/4 π /4 . Therefore
ϕ − β = π 4 . \phi - \beta = \frac{\pi}{4}. ϕ − β = 4 π .
Multiplying by 4:
4 ϕ − 4 β = π ⟹ π = 4 arcsin ( 7 2 10 ) − 4 arctan ( 3 4 ) . ■ 4\phi - 4\beta = \pi \implies \pi = 4\arcsin\!\left(\frac{7\sqrt{2}}{10}\right) - 4\arctan\!\left(\frac{3}{4}\right). \qquad \blacksquare 4 ϕ − 4 β = π ⟹ π = 4 arcsin ( 10 7 2 ) − 4 arctan ( 4 3 ) . ■
Topic : 无理数与证明(Irrationality and Proof) | Difficulty : Challenging | Marks : 20
3 Prove that the cube root of any irrational number is an irrational number.
Let u n = 5 1 / ( 3 n ) u_n = 5^{1/(3^n)} u n = 5 1/ ( 3 n ) . Given that 5 3 \sqrt[3]{5} 3 5 is an irrational number, prove by induction that u n u_n u n is an irrational number for every positive integer n n n .
Hence, or otherwise, give an example of an infinite sequence of irrational numbers which converges to a given integer m m m .
[An irrational number is a number that cannot be expressed as the ratio of two integers.]
Model Solution
Part 1: Cube root of irrational is irrational
We prove the contrapositive: if x 3 \sqrt[3]{x} 3 x is rational, then x x x is rational.
Suppose x 3 \sqrt[3]{x} 3 x is rational. Then there exist integers p , q p, q p , q with q ≠ 0 q \neq 0 q = 0 such that
x 3 = p q . \sqrt[3]{x} = \frac{p}{q} . 3 x = q p .
Cubing both sides:
x = p 3 q 3 . x = \frac{p^3}{q^3} . x = q 3 p 3 .
Since p p p and q q q are integers, p 3 p^3 p 3 and q 3 q^3 q 3 are integers, and q 3 ≠ 0 q^3 \neq 0 q 3 = 0 . Therefore x x x is rational.
By contrapositive, if x x x is irrational, then x 3 \sqrt[3]{x} 3 x is irrational. ■ \blacksquare ■
Part 2: Induction that u n = 5 1 / 3 n u_n = 5^{1/3^n} u n = 5 1/ 3 n is irrational
Base case (n = 1 n = 1 n = 1 ): u 1 = 5 1 / 3 = 5 3 u_1 = 5^{1/3} = \sqrt[3]{5} u 1 = 5 1/3 = 3 5 , which is given to be irrational.
Inductive step : Suppose u k = 5 1 / 3 k u_k = 5^{1/3^k} u k = 5 1/ 3 k is irrational for some positive integer k k k . We show u k + 1 u_{k+1} u k + 1 is irrational.
Observe that
u k + 1 3 = ( 5 1 / 3 k + 1 ) 3 = 5 3 / 3 k + 1 = 5 1 / 3 k = u k . u_{k+1}^3 = \left(5^{1/3^{k+1}}\right)^3 = 5^{3/3^{k+1}} = 5^{1/3^k} = u_k . u k + 1 3 = ( 5 1/ 3 k + 1 ) 3 = 5 3/ 3 k + 1 = 5 1/ 3 k = u k .
So u k + 1 = u k 3 u_{k+1} = \sqrt[3]{u_k} u k + 1 = 3 u k . By the induction hypothesis, u k u_k u k is irrational. By Part 1, the cube root of an irrational number is irrational. Therefore u k + 1 u_{k+1} u k + 1 is irrational.
By induction, u n u_n u n is irrational for every positive integer n n n . ■ \blacksquare ■
Part 3: An infinite sequence of irrationals converging to integer m m m
Consider the sequence
a n = ( m − 1 ) + 5 1 / 3 n for n = 1 , 2 , 3 , … a_n = (m - 1) + 5^{1/3^n} \quad \text{for } n = 1, 2, 3, \ldots a n = ( m − 1 ) + 5 1/ 3 n for n = 1 , 2 , 3 , …
Each a n a_n a n is irrational: if a n a_n a n were rational, then 5 1 / 3 n = a n − ( m − 1 ) 5^{1/3^n} = a_n - (m-1) 5 1/ 3 n = a n − ( m − 1 ) would be rational (since the difference of two rationals is rational), contradicting Part 2.
As n → ∞ n \to \infty n → ∞ , 3 n → ∞ 3^n \to \infty 3 n → ∞ , so 1 3 n → 0 \frac{1}{3^n} \to 0 3 n 1 → 0 and 5 1 / 3 n → 5 0 = 1 5^{1/3^n} \to 5^0 = 1 5 1/ 3 n → 5 0 = 1 . Therefore
a n → ( m − 1 ) + 1 = m . a_n \to (m - 1) + 1 = m . a n → ( m − 1 ) + 1 = m .
Thus { a n } \{a_n\} { a n } is an infinite sequence of irrational numbers converging to m m m . ■ \blacksquare ■
Topic : 解析几何(Analytic Geometry) | Difficulty : Standard | Marks : 20
4 The line y = d y = d y = d , where d > 0 d > 0 d > 0 , intersects the circle x 2 + y 2 = R 2 x^2 + y^2 = R^2 x 2 + y 2 = R 2 at G G G and H H H . Show that the area of the minor segment G H GH G H is equal to
R 2 arccos ( d R ) − d R 2 − d 2 . (*) R^2 \arccos \left( \frac{d}{R} \right) - d \sqrt{R^2 - d^2} . \qquad \text{(*)} R 2 arccos ( R d ) − d R 2 − d 2 . (*)
In the following cases, the given line intersects the given circle. Determine how, in each case, the expression (∗ * ∗ ) should be modified to give the area of the minor segment.
(i) Line: y = c y = c y = c ; circle: ( x − a ) 2 + ( y − b ) 2 = R 2 (x - a)^2 + (y - b)^2 = R^2 ( x − a ) 2 + ( y − b ) 2 = R 2 .
(ii) Line: y = m x + c y = mx + c y = m x + c ; circle: x 2 + y 2 = R 2 x^2 + y^2 = R^2 x 2 + y 2 = R 2 .
(iii) Line: y = m x + c y = mx + c y = m x + c ; circle: ( x − a ) 2 + ( y − b ) 2 = R 2 (x - a)^2 + (y - b)^2 = R^2 ( x − a ) 2 + ( y − b ) 2 = R 2 .
Model Solution
Main derivation
The line y = d y = d y = d meets x 2 + y 2 = R 2 x^2 + y^2 = R^2 x 2 + y 2 = R 2 at points G G G and H H H where x 2 = R 2 − d 2 x^2 = R^2 - d^2 x 2 = R 2 − d 2 , so G = ( − R 2 − d 2 , d ) G = (-\sqrt{R^2 - d^2},\; d) G = ( − R 2 − d 2 , d ) and H = ( R 2 − d 2 , d ) H = (\sqrt{R^2 - d^2},\; d) H = ( R 2 − d 2 , d ) .
The minor segment is the cap above y = d y = d y = d . Its area equals the area of the circular sector subtended by arc G H GH G H minus the area of triangle O G H OGH O G H (where O O O is the origin).
Sector angle : The angle θ \theta θ that O H OH O H makes with the positive y y y -axis satisfies
cos θ = d R , so θ = arccos ( d R ) . \cos \theta = \frac{d}{R}, \qquad \text{so} \qquad \theta = \arccos\left(\frac{d}{R}\right). cos θ = R d , so θ = arccos ( R d ) .
The full angle subtended by arc G H GH G H at the centre is 2 θ = 2 arccos ( d / R ) 2\theta = 2\arccos(d/R) 2 θ = 2 arccos ( d / R ) .
Sector area :
A sector = 1 2 R 2 ⋅ 2 θ = R 2 arccos ( d R ) . A_{\text{sector}} = \frac{1}{2} R^2 \cdot 2\theta = R^2 \arccos\left(\frac{d}{R}\right). A sector = 2 1 R 2 ⋅ 2 θ = R 2 arccos ( R d ) .
Triangle area : Triangle O G H OGH O G H has base G H = 2 R 2 − d 2 GH = 2\sqrt{R^2 - d^2} G H = 2 R 2 − d 2 and height d d d (the perpendicular distance from O O O to line G H GH G H ):
A △ = 1 2 ⋅ 2 R 2 − d 2 ⋅ d = d R 2 − d 2 . A_{\triangle} = \frac{1}{2} \cdot 2\sqrt{R^2 - d^2} \cdot d = d\sqrt{R^2 - d^2} . A △ = 2 1 ⋅ 2 R 2 − d 2 ⋅ d = d R 2 − d 2 .
Segment area :
A segment = A sector − A △ = R 2 arccos ( d R ) − d R 2 − d 2 as required. ■ A_{\text{segment}} = A_{\text{sector}} - A_{\triangle} = R^2 \arccos\left(\frac{d}{R}\right) - d\sqrt{R^2 - d^2} \qquad \text{as required.} \quad \blacksquare A segment = A sector − A △ = R 2 arccos ( R d ) − d R 2 − d 2 as required. ■
Key observation for parts (i)—(iii)
Formula (*) depends only on two geometric quantities:
R R R : the radius of the circle;
d d d : the perpendicular distance from the centre of the circle to the chord (line).
In each case below, we compute the perpendicular distance δ \delta δ from the circle’s centre to the given line and substitute d → δ d \to \delta d → δ in (*).
Part (i)
Line: y = c y = c y = c ; circle: ( x − a ) 2 + ( y − b ) 2 = R 2 (x - a)^2 + (y - b)^2 = R^2 ( x − a ) 2 + ( y − b ) 2 = R 2 .
The circle has centre ( a , b ) (a, b) ( a , b ) and radius R R R . The line y = c y = c y = c is horizontal, so the perpendicular distance from the centre to the line is
δ = ∣ b − c ∣ . \delta = |b - c| . δ = ∣ b − c ∣.
Substituting d → ∣ b − c ∣ d \to |b - c| d → ∣ b − c ∣ in (*):
R 2 arccos ( ∣ b − c ∣ R ) − ∣ b − c ∣ R 2 − ( b − c ) 2 . \boxed{R^2 \arccos\left(\frac{|b - c|}{R}\right) - |b - c|\sqrt{R^2 - (b - c)^2}} . R 2 arccos ( R ∣ b − c ∣ ) − ∣ b − c ∣ R 2 − ( b − c ) 2 .
Part (ii)
Line: y = m x + c y = mx + c y = m x + c , i.e.\ m x − y + c = 0 mx - y + c = 0 m x − y + c = 0 ; circle: x 2 + y 2 = R 2 x^2 + y^2 = R^2 x 2 + y 2 = R 2 (centre at origin).
The perpendicular distance from the origin to the line m x − y + c = 0 mx - y + c = 0 m x − y + c = 0 is
δ = ∣ m ⋅ 0 − 0 + c ∣ m 2 + 1 = ∣ c ∣ m 2 + 1 . \delta = \frac{|m \cdot 0 - 0 + c|}{\sqrt{m^2 + 1}} = \frac{|c|}{\sqrt{m^2 + 1}} . δ = m 2 + 1 ∣ m ⋅ 0 − 0 + c ∣ = m 2 + 1 ∣ c ∣ .
Substituting d → ∣ c ∣ m 2 + 1 d \to \dfrac{|c|}{\sqrt{m^2 + 1}} d → m 2 + 1 ∣ c ∣ in (*):
R 2 arccos ( ∣ c ∣ R m 2 + 1 ) − ∣ c ∣ m 2 + 1 R 2 − c 2 m 2 + 1 . R^2 \arccos\left(\frac{|c|}{R\sqrt{m^2 + 1}}\right) - \frac{|c|}{\sqrt{m^2 + 1}} \sqrt{R^2 - \frac{c^2}{m^2 + 1}} . R 2 arccos ( R m 2 + 1 ∣ c ∣ ) − m 2 + 1 ∣ c ∣ R 2 − m 2 + 1 c 2 .
Simplify the square root:
R 2 − c 2 m 2 + 1 = R 2 ( m 2 + 1 ) − c 2 m 2 + 1 = R 2 ( m 2 + 1 ) − c 2 m 2 + 1 . \sqrt{R^2 - \frac{c^2}{m^2 + 1}} = \sqrt{\frac{R^2(m^2 + 1) - c^2}{m^2 + 1}} = \frac{\sqrt{R^2(m^2 + 1) - c^2}}{\sqrt{m^2 + 1}} . R 2 − m 2 + 1 c 2 = m 2 + 1 R 2 ( m 2 + 1 ) − c 2 = m 2 + 1 R 2 ( m 2 + 1 ) − c 2 .
So the second term becomes
∣ c ∣ m 2 + 1 ⋅ R 2 ( m 2 + 1 ) − c 2 m 2 + 1 = ∣ c ∣ R 2 ( m 2 + 1 ) − c 2 m 2 + 1 . \frac{|c|}{\sqrt{m^2 + 1}} \cdot \frac{\sqrt{R^2(m^2 + 1) - c^2}}{\sqrt{m^2 + 1}} = \frac{|c|\sqrt{R^2(m^2 + 1) - c^2}}{m^2 + 1} . m 2 + 1 ∣ c ∣ ⋅ m 2 + 1 R 2 ( m 2 + 1 ) − c 2 = m 2 + 1 ∣ c ∣ R 2 ( m 2 + 1 ) − c 2 .
The modified formula is:
R 2 arccos ( ∣ c ∣ R m 2 + 1 ) − ∣ c ∣ R 2 ( m 2 + 1 ) − c 2 m 2 + 1 . \boxed{R^2 \arccos\left(\frac{|c|}{R\sqrt{m^2 + 1}}\right) - \frac{|c|\sqrt{R^2(m^2 + 1) - c^2}}{m^2 + 1}} . R 2 arccos ( R m 2 + 1 ∣ c ∣ ) − m 2 + 1 ∣ c ∣ R 2 ( m 2 + 1 ) − c 2 .
Part (iii)
Line: y = m x + c y = mx + c y = m x + c , i.e.\ m x − y + c = 0 mx - y + c = 0 m x − y + c = 0 ; circle: ( x − a ) 2 + ( y − b ) 2 = R 2 (x - a)^2 + (y - b)^2 = R^2 ( x − a ) 2 + ( y − b ) 2 = R 2 (centre ( a , b ) (a, b) ( a , b ) ).
The perpendicular distance from ( a , b ) (a, b) ( a , b ) to the line m x − y + c = 0 mx - y + c = 0 m x − y + c = 0 is
δ = ∣ m a − b + c ∣ m 2 + 1 . \delta = \frac{|ma - b + c|}{\sqrt{m^2 + 1}} . δ = m 2 + 1 ∣ ma − b + c ∣ .
Substituting d → ∣ m a − b + c ∣ m 2 + 1 d \to \dfrac{|ma - b + c|}{\sqrt{m^2 + 1}} d → m 2 + 1 ∣ ma − b + c ∣ in (*):
R 2 arccos ( ∣ m a − b + c ∣ R m 2 + 1 ) − ∣ m a − b + c ∣ m 2 + 1 R 2 − ( m a − b + c ) 2 m 2 + 1 . R^2 \arccos\left(\frac{|ma - b + c|}{R\sqrt{m^2 + 1}}\right) - \frac{|ma - b + c|}{\sqrt{m^2 + 1}} \sqrt{R^2 - \frac{(ma - b + c)^2}{m^2 + 1}} . R 2 arccos ( R m 2 + 1 ∣ ma − b + c ∣ ) − m 2 + 1 ∣ ma − b + c ∣ R 2 − m 2 + 1 ( ma − b + c ) 2 .
Simplify the square root as before:
R 2 − ( m a − b + c ) 2 m 2 + 1 = R 2 ( m 2 + 1 ) − ( m a − b + c ) 2 m 2 + 1 . \sqrt{R^2 - \frac{(ma - b + c)^2}{m^2 + 1}} = \frac{\sqrt{R^2(m^2 + 1) - (ma - b + c)^2}}{\sqrt{m^2 + 1}} . R 2 − m 2 + 1 ( ma − b + c ) 2 = m 2 + 1 R 2 ( m 2 + 1 ) − ( ma − b + c ) 2 .
The modified formula is:
R 2 arccos ( ∣ m a − b + c ∣ R m 2 + 1 ) − ∣ m a − b + c ∣ R 2 ( m 2 + 1 ) − ( m a − b + c ) 2 m 2 + 1 . \boxed{R^2 \arccos\left(\frac{|ma - b + c|}{R\sqrt{m^2 + 1}}\right) - \frac{|ma - b + c|\sqrt{R^2(m^2 + 1) - (ma - b + c)^2}}{m^2 + 1}} . R 2 arccos ( R m 2 + 1 ∣ ma − b + c ∣ ) − m 2 + 1 ∣ ma − b + c ∣ R 2 ( m 2 + 1 ) − ( ma − b + c ) 2 .
Summary : In every case, the modification is to replace d d d in formula (*) with the perpendicular distance δ \delta δ from the centre of the circle to the line:
Case δ \delta δ Original d d d (i) ∣ b − c ∣ \lvert b - c \rvert ∣ b − c ∣ (ii) ∣ c ∣ m 2 + 1 \dfrac{\lvert c \rvert}{\sqrt{m^2 + 1}} m 2 + 1 ∣ c ∣ (iii) ∣ m a − b + c ∣ m 2 + 1 \dfrac{\lvert ma - b + c \rvert}{\sqrt{m^2 + 1}} m 2 + 1 ∣ ma − b + c ∣
Topic : 向量(Vectors) | Difficulty : Standard | Marks : 20
5 The position vectors of the points A A A , B B B and P P P with respect to an origin O O O are a i a\mathbf{i} a i , b j b\mathbf{j} b j and l i + m j + n k l\mathbf{i} + m\mathbf{j} + n\mathbf{k} l i + m j + n k , respectively, where a a a , b b b , and n n n are all non-zero. The points E E E , F F F , G G G and H H H are the midpoints of O A OA O A , B P BP B P , O B OB O B and A P AP A P , respectively. Show that the lines E F EF E F and G H GH G H intersect.
Let D D D be the point with position vector d k d\mathbf{k} d k , where d d d is non-zero, and let S S S be the point of intersection of E F EF E F and G H GH G H . The point T T T is such that the mid-point of D T DT D T is S S S . Find the position vector of T T T and hence find d d d in terms of n n n if T T T lies in the plane O A B OAB O A B .
Model Solution
Position vectors of the midpoints
E = a 2 i , F = l 2 i + b + m 2 j + n 2 k , G = b 2 j , H = a + l 2 i + m 2 j + n 2 k . E = \frac{a}{2}\,\mathbf{i}, \quad F = \frac{l}{2}\,\mathbf{i} + \frac{b + m}{2}\,\mathbf{j} + \frac{n}{2}\,\mathbf{k}, \quad G = \frac{b}{2}\,\mathbf{j}, \quad H = \frac{a + l}{2}\,\mathbf{i} + \frac{m}{2}\,\mathbf{j} + \frac{n}{2}\,\mathbf{k}. E = 2 a i , F = 2 l i + 2 b + m j + 2 n k , G = 2 b j , H = 2 a + l i + 2 m j + 2 n k .
Showing that E F EF E F and G H GH G H intersect
We first observe that
E + F = a + l 2 i + b + m 2 j + n 2 k = G + H . E + F = \frac{a + l}{2}\,\mathbf{i} + \frac{b + m}{2}\,\mathbf{j} + \frac{n}{2}\,\mathbf{k} = G + H. E + F = 2 a + l i + 2 b + m j + 2 n k = G + H .
Therefore the midpoint of segment E F EF E F equals the midpoint of segment G H GH G H :
M = E + F 2 = G + H 2 = a + l 4 i + b + m 4 j + n 4 k . M = \frac{E + F}{2} = \frac{G + H}{2} = \frac{a + l}{4}\,\mathbf{i} + \frac{b + m}{4}\,\mathbf{j} + \frac{n}{4}\,\mathbf{k}. M = 2 E + F = 2 G + H = 4 a + l i + 4 b + m j + 4 n k .
Since M M M is the midpoint of segment E F EF E F , it lies on line E F EF E F (at parameter t = 1 / 2 t = 1/2 t = 1/2 in r = E + t ( F − E ) \mathbf{r} = E + t(F - E) r = E + t ( F − E ) ). Similarly, M M M lies on line G H GH G H (at parameter s = 1 / 2 s = 1/2 s = 1/2 in r = G + s ( H − G ) \mathbf{r} = G + s(H - G) r = G + s ( H − G ) ). Hence both lines pass through M M M .
To confirm the lines are distinct (not the same line), we check that the direction vectors E F → \overrightarrow{EF} E F and G H → \overrightarrow{GH} G H are not parallel:
E F → = l 2 i + b + m − a 2 j + n 2 k , G H → = a + l 2 i + m − b 2 j + n 2 k . \overrightarrow{EF} = \frac{l}{2}\,\mathbf{i} + \frac{b + m - a}{2}\,\mathbf{j} + \frac{n}{2}\,\mathbf{k}, \qquad \overrightarrow{GH} = \frac{a + l}{2}\,\mathbf{i} + \frac{m - b}{2}\,\mathbf{j} + \frac{n}{2}\,\mathbf{k}. E F = 2 l i + 2 b + m − a j + 2 n k , G H = 2 a + l i + 2 m − b j + 2 n k .
If E F → = λ G H → \overrightarrow{EF} = \lambda\,\overrightarrow{GH} E F = λ G H , comparing k \mathbf{k} k -components gives λ = 1 \lambda = 1 λ = 1 (since n ≠ 0 n \neq 0 n = 0 ). Then i \mathbf{i} i -components give l = a + l l = a + l l = a + l , i.e.\ a = 0 a = 0 a = 0 , contradicting a ≠ 0 a \neq 0 a = 0 . So the lines are distinct.
Therefore E F EF E F and G H GH G H intersect at the unique point
S = a + l 4 i + b + m 4 j + n 4 k . ■ S = \frac{a + l}{4}\,\mathbf{i} + \frac{b + m}{4}\,\mathbf{j} + \frac{n}{4}\,\mathbf{k}. \qquad \blacksquare S = 4 a + l i + 4 b + m j + 4 n k . ■
Finding T T T and d d d
Since S S S is the midpoint of D T DT D T with D = d k D = d\mathbf{k} D = d k :
S = D + T 2 ⟹ T = 2 S − D = a + l 2 i + b + m 2 j + n 2 k − d k , S = \frac{D + T}{2} \implies T = 2S - D = \frac{a + l}{2}\,\mathbf{i} + \frac{b + m}{2}\,\mathbf{j} + \frac{n}{2}\,\mathbf{k} - d\,\mathbf{k}, S = 2 D + T ⟹ T = 2 S − D = 2 a + l i + 2 b + m j + 2 n k − d k ,
T = a + l 2 i + b + m 2 j + ( n 2 − d ) k . T = \frac{a + l}{2}\,\mathbf{i} + \frac{b + m}{2}\,\mathbf{j} + \left(\frac{n}{2} - d\right)\mathbf{k}. T = 2 a + l i + 2 b + m j + ( 2 n − d ) k .
The plane O A B OAB O A B is the x y xy x y -plane (since O O O , A A A , B B B all have zero k \mathbf{k} k -component). For T T T to lie in this plane, its k \mathbf{k} k -component must be zero:
n 2 − d = 0 ⟹ d = n 2 . \frac{n}{2} - d = 0 \implies d = \frac{n}{2}. 2 n − d = 0 ⟹ d = 2 n .
Topic : 函数迭代与积分(Function Iteration and Integration) | Difficulty : Challenging | Marks : 20
6 The function f f f is defined by
f ( x ) = ∣ x − 1 ∣ , f(x) = |x - 1| , f ( x ) = ∣ x − 1∣ ,
where the domain is R \mathbf{R} R , the set of all real numbers. The function g n = f n g_n = f^n g n = f n , with domain R \mathbf{R} R , so for example g 3 ( x ) = f ( f ( f ( x ) ) ) g_3(x) = f(f(f(x))) g 3 ( x ) = f ( f ( f ( x ))) . In separate diagrams, sketch graphs of g 1 g_1 g 1 , g 2 g_2 g 2 , g 3 g_3 g 3 and g 4 g_4 g 4 .
The function h h h is defined by
h ( x ) = ∣ sin π x 2 ∣ , h(x) = \left| \sin \frac{\pi x}{2} \right| , h ( x ) = sin 2 π x ,
where the domain is R \mathbf{R} R . Show that if n n n is even,
∫ 0 n ( h ( x ) − g n ( x ) ) d x = 2 n π − n 2 . \int_0^n (h(x) - g_n(x)) \ dx = \frac{2n}{\pi} - \frac{n}{2} . ∫ 0 n ( h ( x ) − g n ( x )) d x = π 2 n − 2 n .
Model Solution
Sketches of g 1 , g 2 , g 3 , g 4 g_1, g_2, g_3, g_4 g 1 , g 2 , g 3 , g 4
Each g n g_n g n is piecewise linear with slopes ± 1 \pm 1 ± 1 on every unit interval. The key pattern is:
g n ( k ) = { 0 if n + k is even , 1 if n + k is odd , for every integer k ≥ 0. g_n(k) = \begin{cases} 0 & \text{if } n + k \text{ is even}, \\ 1 & \text{if } n + k \text{ is odd}, \end{cases} \qquad \text{for every integer } k \geq 0. g n ( k ) = { 0 1 if n + k is even , if n + k is odd , for every integer k ≥ 0.
This means each g n g_n g n is a zigzag of unit triangles on [ 0 , n ] [0, n] [ 0 , n ] .
Graph of g 1 ( x ) = ∣ x − 1 ∣ g_1(x) = |x - 1| g 1 ( x ) = ∣ x − 1∣ : V-shape with vertex at ( 1 , 0 ) (1, 0) ( 1 , 0 ) . Passes through ( 0 , 1 ) (0, 1) ( 0 , 1 ) ; slope − 1 -1 − 1 for x < 1 x < 1 x < 1 , slope + 1 +1 + 1 for x > 1 x > 1 x > 1 .
Graph of g 2 ( x ) g_2(x) g 2 ( x ) : Zigzag on [ 0 , 2 ] [0, 2] [ 0 , 2 ] . Passes through ( 0 , 0 ) (0, 0) ( 0 , 0 ) , ( 1 , 1 ) (1, 1) ( 1 , 1 ) , ( 2 , 0 ) (2, 0) ( 2 , 0 ) . A tent (inverted V) shape: rises from ( 0 , 0 ) (0, 0) ( 0 , 0 ) to ( 1 , 1 ) (1, 1) ( 1 , 1 ) , then falls to ( 2 , 0 ) (2, 0) ( 2 , 0 ) . For x > 2 x > 2 x > 2 , continues with slope + 1 +1 + 1 .
Graph of g 3 ( x ) g_3(x) g 3 ( x ) : Zigzag on [ 0 , 3 ] [0, 3] [ 0 , 3 ] . Passes through ( 0 , 1 ) (0, 1) ( 0 , 1 ) , ( 1 , 0 ) (1, 0) ( 1 , 0 ) , ( 2 , 1 ) (2, 1) ( 2 , 1 ) , ( 3 , 0 ) (3, 0) ( 3 , 0 ) . Alternating V-shapes: falls from ( 0 , 1 ) (0, 1) ( 0 , 1 ) to ( 1 , 0 ) (1, 0) ( 1 , 0 ) , rises to ( 2 , 1 ) (2, 1) ( 2 , 1 ) , falls to ( 3 , 0 ) (3, 0) ( 3 , 0 ) . For x > 3 x > 3 x > 3 , continues with slope + 1 +1 + 1 .
Graph of g 4 ( x ) g_4(x) g 4 ( x ) : Zigzag on [ 0 , 4 ] [0, 4] [ 0 , 4 ] . Passes through ( 0 , 0 ) (0, 0) ( 0 , 0 ) , ( 1 , 1 ) (1, 1) ( 1 , 1 ) , ( 2 , 0 ) (2, 0) ( 2 , 0 ) , ( 3 , 1 ) (3, 1) ( 3 , 1 ) , ( 4 , 0 ) (4, 0) ( 4 , 0 ) . Repeating tents: rises from ( 0 , 0 ) (0, 0) ( 0 , 0 ) to ( 1 , 1 ) (1, 1) ( 1 , 1 ) , falls to ( 2 , 0 ) (2, 0) ( 2 , 0 ) , rises to ( 3 , 1 ) (3, 1) ( 3 , 1 ) , falls to ( 4 , 0 ) (4, 0) ( 4 , 0 ) . For x > 4 x > 4 x > 4 , continues with slope + 1 +1 + 1 .
Proof of the integral identity
We establish two results and then combine them.
Step 1: ∫ 0 n g n ( x ) d x = n 2 \int_0^n g_n(x) \, dx = \frac{n}{2} ∫ 0 n g n ( x ) d x = 2 n for even n n n .
We prove by induction on n n n that g n g_n g n satisfies:
(a) g n g_n g n is piecewise linear with slope ± 1 \pm 1 ± 1 on every interval [ k , k + 1 ] [k, k+1] [ k , k + 1 ] , k ∈ { 0 , 1 , … , n − 1 } k \in \{0, 1, \ldots, n-1\} k ∈ { 0 , 1 , … , n − 1 } ;
(b) g n ( k ) = 0 g_n(k) = 0 g n ( k ) = 0 if n + k n + k n + k is even, and g n ( k ) = 1 g_n(k) = 1 g n ( k ) = 1 if n + k n + k n + k is odd, for each integer k ∈ { 0 , 1 , … , n } k \in \{0, 1, \ldots, n\} k ∈ { 0 , 1 , … , n } .
Base case n = 1 n = 1 n = 1 : g 1 ( x ) = ∣ x − 1 ∣ g_1(x) = |x - 1| g 1 ( x ) = ∣ x − 1∣ . At integers: g 1 ( 0 ) = 1 g_1(0) = 1 g 1 ( 0 ) = 1 (since 1 + 0 = 1 1 + 0 = 1 1 + 0 = 1 is odd), g 1 ( 1 ) = 0 g_1(1) = 0 g 1 ( 1 ) = 0 (since 1 + 1 = 2 1 + 1 = 2 1 + 1 = 2 is even). Slope is − 1 -1 − 1 on [ 0 , 1 ] [0, 1] [ 0 , 1 ] , + 1 +1 + 1 on [ 1 , ∞ ) [1, \infty) [ 1 , ∞ ) . Both (a) and (b) hold.
Inductive step : Assume (a) and (b) hold for g n g_n g n . We show they hold for g n + 1 = f ∘ g n g_{n+1} = f \circ g_n g n + 1 = f ∘ g n .
For (a): On each interval [ k , k + 1 ] [k, k+1] [ k , k + 1 ] , g n g_n g n is linear with slope ± 1 \pm 1 ± 1 , so g n g_n g n takes values in [ 0 , 1 ] ⊆ [ 0 , ∞ ) [0, 1] \subseteq [0, \infty) [ 0 , 1 ] ⊆ [ 0 , ∞ ) . On this range, f ( y ) = ∣ y − 1 ∣ = 1 − y f(y) = |y - 1| = 1 - y f ( y ) = ∣ y − 1∣ = 1 − y , which is linear in y y y . The composition of two linear functions is linear. Since g n g_n g n has slope ± 1 \pm 1 ± 1 and f f f has slope − 1 -1 − 1 on [ 0 , 1 ] [0, 1] [ 0 , 1 ] , the composition g n + 1 g_{n+1} g n + 1 has slope ± 1 \pm 1 ± 1 .
For (b): At k = 0 k = 0 k = 0 : g n ( 0 ) g_n(0) g n ( 0 ) has parity n m o d 2 n \bmod 2 n mod 2 by (b). So g n ( 0 ) = 0 g_n(0) = 0 g n ( 0 ) = 0 if n n n is even, g n ( 0 ) = 1 g_n(0) = 1 g n ( 0 ) = 1 if n n n is odd. Then g n + 1 ( 0 ) = ∣ g n ( 0 ) − 1 ∣ g_{n+1}(0) = |g_n(0) - 1| g n + 1 ( 0 ) = ∣ g n ( 0 ) − 1∣ , giving g n + 1 ( 0 ) = 1 g_{n+1}(0) = 1 g n + 1 ( 0 ) = 1 if n n n is even, g n + 1 ( 0 ) = 0 g_{n+1}(0) = 0 g n + 1 ( 0 ) = 0 if n n n is odd. In both cases, g n + 1 ( 0 ) g_{n+1}(0) g n + 1 ( 0 ) has parity ( n + 1 ) m o d 2 (n+1) \bmod 2 ( n + 1 ) mod 2 .
At k = 1 k = 1 k = 1 : By (b), g n ( 1 ) = 0 g_n(1) = 0 g n ( 1 ) = 0 when n + 1 n+1 n + 1 is even (i.e.\ n n n odd), and g n ( 1 ) = 1 g_n(1) = 1 g n ( 1 ) = 1 when n + 1 n+1 n + 1 is odd (i.e.\ n n n even). In fact, from the base case: g 1 ( 1 ) = 0 g_1(1) = 0 g 1 ( 1 ) = 0 , and each subsequent application of f f f flips between 0 and 1. So g n ( 1 ) = 0 g_n(1) = 0 g n ( 1 ) = 0 when n n n is odd, g n ( 1 ) = 1 g_n(1) = 1 g n ( 1 ) = 1 when n n n is even. Then g n + 1 ( 1 ) = ∣ g n ( 1 ) − 1 ∣ g_{n+1}(1) = |g_n(1) - 1| g n + 1 ( 1 ) = ∣ g n ( 1 ) − 1∣ : if n n n is odd, g n + 1 ( 1 ) = 1 g_{n+1}(1) = 1 g n + 1 ( 1 ) = 1 ; if n n n is even, g n + 1 ( 1 ) = 0 g_{n+1}(1) = 0 g n + 1 ( 1 ) = 0 . In both cases, g n + 1 ( 1 ) g_{n+1}(1) g n + 1 ( 1 ) has parity ( n + 2 ) m o d 2 = n m o d 2 (n + 2) \bmod 2 = n \bmod 2 ( n + 2 ) mod 2 = n mod 2 , which matches ( n + 1 ) + 1 m o d 2 (n+1)+1 \bmod 2 ( n + 1 ) + 1 mod 2 . ✓
At k ≥ 2 k \geq 2 k ≥ 2 : By (b), g n ( k ) ∈ { 0 , 1 } g_n(k) \in \{0, 1\} g n ( k ) ∈ { 0 , 1 } with parity ( n + k ) m o d 2 (n+k) \bmod 2 ( n + k ) mod 2 . Then g n + 1 ( k ) = ∣ g n ( k ) − 1 ∣ ∈ { 0 , 1 } g_{n+1}(k) = |g_n(k) - 1| \in \{0, 1\} g n + 1 ( k ) = ∣ g n ( k ) − 1∣ ∈ { 0 , 1 } , which flips the value. If g n ( k ) = 0 g_n(k) = 0 g n ( k ) = 0 then g n + 1 ( k ) = 1 g_{n+1}(k) = 1 g n + 1 ( k ) = 1 ; if g n ( k ) = 1 g_n(k) = 1 g n ( k ) = 1 then g n + 1 ( k ) = 0 g_{n+1}(k) = 0 g n + 1 ( k ) = 0 . So g n + 1 ( k ) g_{n+1}(k) g n + 1 ( k ) has parity 1 − ( ( n + k ) m o d 2 ) = ( n + k + 1 ) m o d 2 = ( ( n + 1 ) + k ) m o d 2 1 - ((n+k) \bmod 2) = (n+k+1) \bmod 2 = ((n+1)+k) \bmod 2 1 − (( n + k ) mod 2 ) = ( n + k + 1 ) mod 2 = (( n + 1 ) + k ) mod 2 . ✓
This completes the induction.
Computing the integral : On each interval [ k , k + 1 ] [k, k+1] [ k , k + 1 ] with 0 ≤ k ≤ n − 1 0 \leq k \leq n - 1 0 ≤ k ≤ n − 1 , g n g_n g n is linear connecting the points ( k , g n ( k ) ) (k, g_n(k)) ( k , g n ( k )) and ( k + 1 , g n ( k + 1 ) ) (k+1, g_n(k+1)) ( k + 1 , g n ( k + 1 )) . By property (b), these endpoints are { 0 , 1 } \{0, 1\} { 0 , 1 } in some order, so g n ( k ) + g n ( k + 1 ) = 1 g_n(k) + g_n(k+1) = 1 g n ( k ) + g n ( k + 1 ) = 1 . The area under a linear function on a unit interval is the average of the endpoint values:
∫ k k + 1 g n ( x ) d x = g n ( k ) + g n ( k + 1 ) 2 ⋅ 1 = 1 2 . \int_k^{k+1} g_n(x) \, dx = \frac{g_n(k) + g_n(k+1)}{2} \cdot 1 = \frac{1}{2}. ∫ k k + 1 g n ( x ) d x = 2 g n ( k ) + g n ( k + 1 ) ⋅ 1 = 2 1 .
Summing over all n n n intervals:
∫ 0 n g n ( x ) d x = ∑ k = 0 n − 1 1 2 = n 2 . ( ⋆ ) \int_0^n g_n(x) \, dx = \sum_{k=0}^{n-1} \frac{1}{2} = \frac{n}{2}. \qquad (\star) ∫ 0 n g n ( x ) d x = ∑ k = 0 n − 1 2 1 = 2 n . ( ⋆ )
Step 2: ∫ 0 n h ( x ) d x = 2 n π \int_0^n h(x) \, dx = \frac{2n}{\pi} ∫ 0 n h ( x ) d x = π 2 n for even n n n .
Since h ( x ) = ∣ sin π x 2 ∣ h(x) = \left|\sin \frac{\pi x}{2}\right| h ( x ) = sin 2 π x has period 2, and n n n is even:
∫ 0 n h ( x ) d x = n 2 ∫ 0 2 h ( x ) d x . \int_0^n h(x) \, dx = \frac{n}{2} \int_0^2 h(x) \, dx. ∫ 0 n h ( x ) d x = 2 n ∫ 0 2 h ( x ) d x .
On [ 0 , 2 ] [0, 2] [ 0 , 2 ] : sin π x 2 ≥ 0 \sin \frac{\pi x}{2} \geq 0 sin 2 π x ≥ 0 for x ∈ [ 0 , 1 ] x \in [0, 1] x ∈ [ 0 , 1 ] and sin π x 2 ≤ 0 \sin \frac{\pi x}{2} \leq 0 sin 2 π x ≤ 0 for x ∈ [ 1 , 2 ] x \in [1, 2] x ∈ [ 1 , 2 ] . So
∫ 0 2 h ( x ) d x = ∫ 0 1 sin π x 2 d x + ∫ 1 2 ( − sin π x 2 ) d x . \int_0^2 h(x) \, dx = \int_0^1 \sin \frac{\pi x}{2} \, dx + \int_1^2 \left(-\sin \frac{\pi x}{2}\right) dx. ∫ 0 2 h ( x ) d x = ∫ 0 1 sin 2 π x d x + ∫ 1 2 ( − sin 2 π x ) d x .
For the first integral:
∫ 0 1 sin π x 2 d x = [ − 2 π cos π x 2 ] 0 1 = − 2 π cos π 2 + 2 π cos 0 = 0 + 2 π = 2 π . \int_0^1 \sin \frac{\pi x}{2} \, dx = \left[-\frac{2}{\pi} \cos \frac{\pi x}{2}\right]_0^1 = -\frac{2}{\pi}\cos\frac{\pi}{2} + \frac{2}{\pi}\cos 0 = 0 + \frac{2}{\pi} = \frac{2}{\pi}. ∫ 0 1 sin 2 π x d x = [ − π 2 cos 2 π x ] 0 1 = − π 2 cos 2 π + π 2 cos 0 = 0 + π 2 = π 2 .
For the second integral:
∫ 1 2 ( − sin π x 2 ) d x = [ 2 π cos π x 2 ] 1 2 = 2 π cos π − 2 π cos π 2 = − 2 π − 0 = 2 π . \int_1^2 \left(-\sin \frac{\pi x}{2}\right) dx = \left[\frac{2}{\pi} \cos \frac{\pi x}{2}\right]_1^2 = \frac{2}{\pi}\cos\pi - \frac{2}{\pi}\cos\frac{\pi}{2} = -\frac{2}{\pi} - 0 = \frac{2}{\pi}. ∫ 1 2 ( − sin 2 π x ) d x = [ π 2 cos 2 π x ] 1 2 = π 2 cos π − π 2 cos 2 π = − π 2 − 0 = π 2 .
Wait: 2 π cos π = 2 π ( − 1 ) = − 2 π \frac{2}{\pi}\cos\pi = \frac{2}{\pi}(-1) = -\frac{2}{\pi} π 2 cos π = π 2 ( − 1 ) = − π 2 . So the second integral is − 2 π − 0 = − 2 π -\frac{2}{\pi} - 0 = -\frac{2}{\pi} − π 2 − 0 = − π 2 ? Let me recompute.
∫ 1 2 ( − sin π x 2 ) d x = [ 2 π cos π x 2 ] 1 2 = 2 π cos π − 2 π cos π 2 = − 2 π − 0 = − 2 π . \int_1^2 \left(-\sin \frac{\pi x}{2}\right) dx = \left[\frac{2}{\pi} \cos \frac{\pi x}{2}\right]_1^2 = \frac{2}{\pi}\cos\pi - \frac{2}{\pi}\cos\frac{\pi}{2} = -\frac{2}{\pi} - 0 = -\frac{2}{\pi}. ∫ 1 2 ( − sin 2 π x ) d x = [ π 2 cos 2 π x ] 1 2 = π 2 cos π − π 2 cos 2 π = − π 2 − 0 = − π 2 .
But this should be positive since the integrand is non-negative on [ 1 , 2 ] [1, 2] [ 1 , 2 ] . Let me recheck the antiderivative.
d d x [ 2 π cos π x 2 ] = 2 π ⋅ ( − sin π x 2 ) ⋅ π 2 = − sin π x 2 . \frac{d}{dx}\left[\frac{2}{\pi}\cos\frac{\pi x}{2}\right] = \frac{2}{\pi} \cdot \left(-\sin\frac{\pi x}{2}\right) \cdot \frac{\pi}{2} = -\sin\frac{\pi x}{2}. d x d [ π 2 cos 2 π x ] = π 2 ⋅ ( − sin 2 π x ) ⋅ 2 π = − sin 2 π x .
So ∫ ( − sin π x 2 ) d x = 2 π cos π x 2 + C \int(-\sin\frac{\pi x}{2})\,dx = \frac{2}{\pi}\cos\frac{\pi x}{2} + C ∫ ( − sin 2 π x ) d x = π 2 cos 2 π x + C . ✓
Evaluating:
[ 2 π cos π x 2 ] 1 2 = 2 π cos π − 2 π cos π 2 = 2 π ( − 1 ) − 2 π ( 0 ) = − 2 π . \left[\frac{2}{\pi}\cos\frac{\pi x}{2}\right]_1^2 = \frac{2}{\pi}\cos\pi - \frac{2}{\pi}\cos\frac{\pi}{2} = \frac{2}{\pi}(-1) - \frac{2}{\pi}(0) = -\frac{2}{\pi}. [ π 2 cos 2 π x ] 1 2 = π 2 cos π − π 2 cos 2 π = π 2 ( − 1 ) − π 2 ( 0 ) = − π 2 .
This is negative, which contradicts the integrand being non-negative. Let me recheck whether − sin π x 2 ≥ 0 -\sin\frac{\pi x}{2} \geq 0 − sin 2 π x ≥ 0 on [ 1 , 2 ] [1, 2] [ 1 , 2 ] .
At x = 1.5 x = 1.5 x = 1.5 : sin 3 π 4 = 2 2 > 0 \sin\frac{3\pi}{4} = \frac{\sqrt{2}}{2} > 0 sin 4 3 π = 2 2 > 0 , so − sin 3 π 4 < 0 -\sin\frac{3\pi}{4} < 0 − sin 4 3 π < 0 .
The issue is: sin π x 2 \sin\frac{\pi x}{2} sin 2 π x on [ 1 , 2 ] [1, 2] [ 1 , 2 ] : at x = 1 x = 1 x = 1 , sin π 2 = 1 > 0 \sin\frac{\pi}{2} = 1 > 0 sin 2 π = 1 > 0 ; at x = 2 x = 2 x = 2 , sin π = 0 \sin\pi = 0 sin π = 0 . So sin π x 2 ≥ 0 \sin\frac{\pi x}{2} \geq 0 sin 2 π x ≥ 0 on [ 1 , 2 ] [1, 2] [ 1 , 2 ] as well! Therefore h ( x ) = sin π x 2 h(x) = \sin\frac{\pi x}{2} h ( x ) = sin 2 π x on all of [ 0 , 2 ] [0, 2] [ 0 , 2 ] .
So:
∫ 0 2 h ( x ) d x = ∫ 0 2 sin π x 2 d x = [ − 2 π cos π x 2 ] 0 2 = − 2 π cos π + 2 π cos 0 = 2 π + 2 π = 4 π . \int_0^2 h(x) \, dx = \int_0^2 \sin \frac{\pi x}{2} \, dx = \left[-\frac{2}{\pi}\cos\frac{\pi x}{2}\right]_0^2 = -\frac{2}{\pi}\cos\pi + \frac{2}{\pi}\cos 0 = \frac{2}{\pi} + \frac{2}{\pi} = \frac{4}{\pi}. ∫ 0 2 h ( x ) d x = ∫ 0 2 sin 2 π x d x = [ − π 2 cos 2 π x ] 0 2 = − π 2 cos π + π 2 cos 0 = π 2 + π 2 = π 4 .
Therefore:
∫ 0 n h ( x ) d x = n 2 ⋅ 4 π = 2 n π . ( ⋆ ⋆ ) \int_0^n h(x) \, dx = \frac{n}{2} \cdot \frac{4}{\pi} = \frac{2n}{\pi}. \qquad (\star\star) ∫ 0 n h ( x ) d x = 2 n ⋅ π 4 = π 2 n . ( ⋆ ⋆ )
Combining the results
From ( ⋆ ) (\star) ( ⋆ ) and ( ⋆ ⋆ ) (\star\star) ( ⋆ ⋆ ) :
∫ 0 n ( h ( x ) − g n ( x ) ) d x = 2 n π − n 2 . ■ \int_0^n \bigl(h(x) - g_n(x)\bigr) \, dx = \frac{2n}{\pi} - \frac{n}{2}. \qquad \blacksquare ∫ 0 n ( h ( x ) − g n ( x ) ) d x = π 2 n − 2 n . ■
Topic : 积分与级数(Integration and Series) | Difficulty : Challenging | Marks : 20
7 Show that, if n > 0 n > 0 n > 0 , then
∫ e 1 / n ∞ ln x x n + 1 d x = 2 n 2 e . \int_{e^{1/n}}^{\infty} \frac{\ln x}{x^{n+1}} dx = \frac{2}{n^2 e} . ∫ e 1/ n ∞ x n + 1 l n x d x = n 2 e 2 .
You may assume that ln x x → 0 \frac{\ln x}{x} \to 0 x l n x → 0 as x → ∞ x \to \infty x → ∞ .
Explain why, if 1 < a < b 1 < a < b 1 < a < b , then
∫ b ∞ ln x x n + 1 d x < ∫ a ∞ ln x x n + 1 d x . \int_{b}^{\infty} \frac{\ln x}{x^{n+1}} dx < \int_{a}^{\infty} \frac{\ln x}{x^{n+1}} dx . ∫ b ∞ x n + 1 l n x d x < ∫ a ∞ x n + 1 l n x d x .
Deduce that
∑ n = 1 N 1 n 2 < e 2 ∫ e 1 / N ∞ 1 − x − N x 2 − x ln x d x , \sum_{n=1}^{N} \frac{1}{n^2} < \frac{e}{2} \int_{e^{1/N}}^{\infty} \frac{1 - x^{-N}}{x^2 - x} \ln x dx , ∑ n = 1 N n 2 1 < 2 e ∫ e 1/ N ∞ x 2 − x 1 − x − N ln x d x ,
Model Solution
Part (i): Show that ∫ e 1 / n ∞ ln x x n + 1 d x = 2 n 2 e \int_{e^{1/n}}^{\infty} \frac{\ln x}{x^{n+1}} \, dx = \frac{2}{n^2 e} ∫ e 1/ n ∞ x n + 1 l n x d x = n 2 e 2
We use integration by parts with
u = ln x , d v = x − ( n + 1 ) d x , u = \ln x, \qquad dv = x^{-(n+1)} \, dx , u = ln x , d v = x − ( n + 1 ) d x ,
so that
d u = 1 x d x , v = − 1 n x n . du = \frac{1}{x} \, dx, \qquad v = -\frac{1}{n x^n} . d u = x 1 d x , v = − n x n 1 .
Applying integration by parts:
∫ e 1 / n ∞ ln x x n + 1 d x = [ − ln x n x n ] e 1 / n ∞ + 1 n ∫ e 1 / n ∞ 1 x n + 1 d x (*) \int_{e^{1/n}}^{\infty} \frac{\ln x}{x^{n+1}} \, dx = \left[ -\frac{\ln x}{n x^n} \right]_{e^{1/n}}^{\infty} + \frac{1}{n} \int_{e^{1/n}}^{\infty} \frac{1}{x^{n+1}} \, dx \qquad \text{(*)} ∫ e 1/ n ∞ x n + 1 l n x d x = [ − n x n l n x ] e 1/ n ∞ + n 1 ∫ e 1/ n ∞ x n + 1 1 d x (*)
Evaluating the boundary term. As x → ∞ x \to \infty x → ∞ :
ln x x n = ln x x ⋅ 1 x n − 1 . \frac{\ln x}{x^n} = \frac{\ln x}{x} \cdot \frac{1}{x^{n-1}} . x n l n x = x l n x ⋅ x n − 1 1 .
Since n > 0 n > 0 n > 0 , for n ≥ 1 n \geq 1 n ≥ 1 the factor 1 x n − 1 \frac{1}{x^{n-1}} x n − 1 1 is bounded (by 1 1 1 when n = 1 n = 1 n = 1 , or tends to 0 0 0 when n > 1 n > 1 n > 1 ), and we are given that ln x x → 0 \frac{\ln x}{x} \to 0 x l n x → 0 . So ln x x n → 0 \frac{\ln x}{x^n} \to 0 x n l n x → 0 as x → ∞ x \to \infty x → ∞ .
At the lower limit x = e 1 / n x = e^{1/n} x = e 1/ n :
− ln ( e 1 / n ) n ( e 1 / n ) n = − 1 / n n ⋅ e = − 1 n 2 e . -\frac{\ln(e^{1/n})}{n(e^{1/n})^n} = -\frac{1/n}{n \cdot e} = -\frac{1}{n^2 e} . − n ( e 1/ n ) n l n ( e 1/ n ) = − n ⋅ e 1/ n = − n 2 e 1 .
Therefore:
[ − ln x n x n ] e 1 / n ∞ = 0 − ( − 1 n 2 e ) = 1 n 2 e . \left[ -\frac{\ln x}{n x^n} \right]_{e^{1/n}}^{\infty} = 0 - \left( -\frac{1}{n^2 e} \right) = \frac{1}{n^2 e} . [ − n x n l n x ] e 1/ n ∞ = 0 − ( − n 2 e 1 ) = n 2 e 1 .
Evaluating the remaining integral.
1 n ∫ e 1 / n ∞ x − ( n + 1 ) d x = 1 n [ x − n − n ] e 1 / n ∞ = 1 n ( 0 − ( e 1 / n ) − n − n ) = 1 n ⋅ e − 1 n = 1 n 2 e . \frac{1}{n} \int_{e^{1/n}}^{\infty} x^{-(n+1)} \, dx = \frac{1}{n} \left[ \frac{x^{-n}}{-n} \right]_{e^{1/n}}^{\infty} = \frac{1}{n} \left( 0 - \frac{(e^{1/n})^{-n}}{-n} \right) = \frac{1}{n} \cdot \frac{e^{-1}}{n} = \frac{1}{n^2 e} . n 1 ∫ e 1/ n ∞ x − ( n + 1 ) d x = n 1 [ − n x − n ] e 1/ n ∞ = n 1 ( 0 − − n ( e 1/ n ) − n ) = n 1 ⋅ n e − 1 = n 2 e 1 .
Substituting both results into ( ∗ ) (*) ( ∗ ) :
∫ e 1 / n ∞ ln x x n + 1 d x = 1 n 2 e + 1 n 2 e = 2 n 2 e ■ \int_{e^{1/n}}^{\infty} \frac{\ln x}{x^{n+1}} \, dx = \frac{1}{n^2 e} + \frac{1}{n^2 e} = \frac{2}{n^2 e} \qquad \blacksquare ∫ e 1/ n ∞ x n + 1 l n x d x = n 2 e 1 + n 2 e 1 = n 2 e 2 ■
Part (ii): Explain why ∫ b ∞ ln x x n + 1 d x < ∫ a ∞ ln x x n + 1 d x \int_{b}^{\infty} \frac{\ln x}{x^{n+1}} dx < \int_{a}^{\infty} \frac{\ln x}{x^{n+1}} dx ∫ b ∞ x n + 1 l n x d x < ∫ a ∞ x n + 1 l n x d x when 1 < a < b 1 < a < b 1 < a < b
For x > 1 x > 1 x > 1 , we have ln x > 0 \ln x > 0 ln x > 0 and x n + 1 > 0 x^{n+1} > 0 x n + 1 > 0 , so the integrand ln x x n + 1 > 0 \frac{\ln x}{x^{n+1}} > 0 x n + 1 l n x > 0 .
Since a < b a < b a < b , we can split the integral from a a a :
∫ a ∞ ln x x n + 1 d x = ∫ a b ln x x n + 1 d x + ∫ b ∞ ln x x n + 1 d x . \int_{a}^{\infty} \frac{\ln x}{x^{n+1}} \, dx = \int_{a}^{b} \frac{\ln x}{x^{n+1}} \, dx + \int_{b}^{\infty} \frac{\ln x}{x^{n+1}} \, dx . ∫ a ∞ x n + 1 l n x d x = ∫ a b x n + 1 l n x d x + ∫ b ∞ x n + 1 l n x d x .
The first integral on the right is strictly positive (integral of a strictly positive function over [ a , b ] [a, b] [ a , b ] with a < b a < b a < b ). Therefore:
∫ b ∞ ln x x n + 1 d x < ∫ a ∞ ln x x n + 1 d x ■ \int_{b}^{\infty} \frac{\ln x}{x^{n+1}} \, dx < \int_{a}^{\infty} \frac{\ln x}{x^{n+1}} \, dx \qquad \blacksquare ∫ b ∞ x n + 1 l n x d x < ∫ a ∞ x n + 1 l n x d x ■
Part (iii): Deduce the series inequality
From part (i), each term satisfies
1 n 2 = e 2 ∫ e 1 / n ∞ ln x x n + 1 d x . \frac{1}{n^2} = \frac{e}{2} \int_{e^{1/n}}^{\infty} \frac{\ln x}{x^{n+1}} \, dx . n 2 1 = 2 e ∫ e 1/ n ∞ x n + 1 l n x d x .
For each n n n with 1 ≤ n ≤ N 1 \leq n \leq N 1 ≤ n ≤ N , since n ≤ N n \leq N n ≤ N we have 1 N ≤ 1 n \frac{1}{N} \leq \frac{1}{n} N 1 ≤ n 1 , hence e 1 / N ≤ e 1 / n e^{1/N} \leq e^{1/n} e 1/ N ≤ e 1/ n . Applying part (ii) with a = e 1 / n a = e^{1/n} a = e 1/ n and b = e 1 / N b = e^{1/N} b = e 1/ N :
∫ e 1 / N ∞ ln x x n + 1 d x ≤ ∫ e 1 / n ∞ ln x x n + 1 d x = 2 n 2 e (**) \int_{e^{1/N}}^{\infty} \frac{\ln x}{x^{n+1}} \, dx \leq \int_{e^{1/n}}^{\infty} \frac{\ln x}{x^{n+1}} \, dx = \frac{2}{n^2 e} \qquad \text{(**)} ∫ e 1/ N ∞ x n + 1 l n x d x ≤ ∫ e 1/ n ∞ x n + 1 l n x d x = n 2 e 2 (**)
Note: the inequality is strict whenever n < N n < N n < N (i.e. e 1 / N < e 1 / n e^{1/N} < e^{1/n} e 1/ N < e 1/ n ), and becomes an equality only when n = N n = N n = N .
Multiplying ( ∗ ∗ ) (**) ( ∗ ∗ ) by e 2 \frac{e}{2} 2 e :
e 2 ∫ e 1 / N ∞ ln x x n + 1 d x ≤ 1 n 2 . \frac{e}{2} \int_{e^{1/N}}^{\infty} \frac{\ln x}{x^{n+1}} \, dx \leq \frac{1}{n^2} . 2 e ∫ e 1/ N ∞ x n + 1 l n x d x ≤ n 2 1 .
Summing over n = 1 , 2 , … , N n = 1, 2, \ldots, N n = 1 , 2 , … , N :
e 2 ∑ n = 1 N ∫ e 1 / N ∞ ln x x n + 1 d x ≤ ∑ n = 1 N 1 n 2 . \frac{e}{2} \sum_{n=1}^{N} \int_{e^{1/N}}^{\infty} \frac{\ln x}{x^{n+1}} \, dx \leq \sum_{n=1}^{N} \frac{1}{n^2} . 2 e ∑ n = 1 N ∫ e 1/ N ∞ x n + 1 l n x d x ≤ ∑ n = 1 N n 2 1 .
Since all integrals share the same limits, we combine them:
e 2 ∫ e 1 / N ∞ ( ∑ n = 1 N 1 x n + 1 ) ln x d x ≤ ∑ n = 1 N 1 n 2 . \frac{e}{2} \int_{e^{1/N}}^{\infty} \left( \sum_{n=1}^{N} \frac{1}{x^{n+1}} \right) \ln x \, dx \leq \sum_{n=1}^{N} \frac{1}{n^2} . 2 e ∫ e 1/ N ∞ ( ∑ n = 1 N x n + 1 1 ) ln x d x ≤ ∑ n = 1 N n 2 1 .
The inner sum is a geometric series with first term 1 x 2 \frac{1}{x^2} x 2 1 and common ratio 1 x \frac{1}{x} x 1 :
∑ n = 1 N 1 x n + 1 = 1 x 2 + 1 x 3 + ⋯ + 1 x N + 1 = 1 x 2 ⋅ 1 − ( 1 / x ) N 1 − 1 / x = 1 − x − N x 2 ( 1 − x − 1 ) = 1 − x − N x 2 − x . \sum_{n=1}^{N} \frac{1}{x^{n+1}} = \frac{1}{x^2} + \frac{1}{x^3} + \cdots + \frac{1}{x^{N+1}} = \frac{1}{x^2} \cdot \frac{1 - (1/x)^N}{1 - 1/x} = \frac{1 - x^{-N}}{x^2(1 - x^{-1})} = \frac{1 - x^{-N}}{x^2 - x} . ∑ n = 1 N x n + 1 1 = x 2 1 + x 3 1 + ⋯ + x N + 1 1 = x 2 1 ⋅ 1 − 1/ x 1 − ( 1/ x ) N = x 2 ( 1 − x − 1 ) 1 − x − N = x 2 − x 1 − x − N .
Substituting:
e 2 ∫ e 1 / N ∞ ( 1 − x − N ) ln x x 2 − x d x ≤ ∑ n = 1 N 1 n 2 . \frac{e}{2} \int_{e^{1/N}}^{\infty} \frac{(1 - x^{-N}) \ln x}{x^2 - x} \, dx \leq \sum_{n=1}^{N} \frac{1}{n^2} . 2 e ∫ e 1/ N ∞ x 2 − x ( 1 − x − N ) l n x d x ≤ ∑ n = 1 N n 2 1 .
Strict inequality for N ≥ 2 N \geq 2 N ≥ 2 . The bound ( ∗ ∗ ) (**) ( ∗ ∗ ) is an equality only when n = N n = N n = N . For every n n n with 1 ≤ n < N 1 \leq n < N 1 ≤ n < N , the bound is strict. Since N ≥ 2 N \geq 2 N ≥ 2 ensures that n = 1 n = 1 n = 1 satisfies n < N n < N n < N , at least one strict inequality appears in the sum. Therefore:
∑ n = 1 N 1 n 2 < e 2 ∫ e 1 / N ∞ 1 − x − N x 2 − x ln x d x ( N ≥ 2 ) ■ \sum_{n=1}^{N} \frac{1}{n^2} < \frac{e}{2} \int_{e^{1/N}}^{\infty} \frac{1 - x^{-N}}{x^2 - x} \ln x \, dx \qquad (N \geq 2) \qquad \blacksquare ∑ n = 1 N n 2 1 < 2 e ∫ e 1/ N ∞ x 2 − x 1 − x − N ln x d x ( N ≥ 2 ) ■