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The following diagram shows the graph of $y = g(x)$ - HSC - SSCE Mathematics Extension 2 - Question 3 - 2008 - Paper 1

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The following diagram shows the graph of $y = g(x)$. Draw separate one-third page sketches of the graphs of the following: (i) $y = |g(x)|$ (ii) $y = \frac{1}{g(x)... show full transcript

Worked Solution & Example Answer:The following diagram shows the graph of $y = g(x)$ - HSC - SSCE Mathematics Extension 2 - Question 3 - 2008 - Paper 1

Step 1

(i) Show that $\rho(z)$ has no real zeros.

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Answer

To show that ρ(z)=1+z2+z4\rho(z) = 1 + z^2 + z^4 has no real zeros, we can analyze the function. Notice that:

  1. The components of ρ(z)\rho(z) are always non-negative:

    • 11 is a positive constant.
    • z2z^2 and z4z^4 are non-negative for all zz.
  2. Thus, since the sum of non-negative terms is always positive, we can conclude that:

    • ρ(z)>0\rho(z) > 0 for all zRz \in \mathbb{R}.

This implies that ρ(z)\rho(z) has no real zeros.

Step 2

(ii) Show that $\alpha^6 = 1$.

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Answer

Given that α\alpha is a zero of ρ(z)\rho(z), we have:

ρ(α)=1+α2+α4=0.\rho(\alpha) = 1 + \alpha^2 + \alpha^4 = 0.

This can be rearranged to:

α4+α2+1=0.\alpha^4 + \alpha^2 + 1 = 0.

Letting x=α2x = \alpha^2, this gives:

x2+x+1=0.x^2 + x + 1 = 0.

Using the quadratic formula, we find:

x=1±142=1±32=1±i32.x = \frac{-1 \pm \sqrt{1 - 4}}{2} = \frac{-1 \pm \sqrt{-3}}{2} = \frac{-1 \pm i\sqrt{3}}{2}.

The roots of α\alpha, therefore, are complex. Use properties of complex numbers:

α6=α4α2=(α21)α2=α4α2=1.\alpha^6 = \alpha^4 \cdot \alpha^2 = (-\alpha^2 - 1) \cdot \alpha^2 = -\alpha^4 - \alpha^2 = 1.

Step 3

(iii) Show that $\alpha^2$ is also a zero of $\rho(z)$.

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Answer

To show that α2\alpha^2 is also a zero of ρ(z)\rho(z), we can substitute α2\alpha^2 back into ρ(z)\rho(z):

ρ(α2)=1+(α2)2+(α2)4=1+α4+α8.\rho(\alpha^2) = 1 + (\alpha^2)^2 + (\alpha^2)^4 = 1 + \alpha^4 + \alpha^8.

Using the earlier result from part (ii):

  • Since α4+α2+1=0\alpha^4 + \alpha^2 + 1 = 0, we know that α8=1\alpha^8 = 1 (because α6=1\alpha^6 = 1). Hence, we substitute it back:

ρ(α2)=1+α4+1=0.\rho(\alpha^2) = 1 + \alpha^4 + 1 = 0.

Thus, α2\alpha^2 is a zero of ρ(z)\rho(z).

Step 4

(i) Show that for $n \geq 1$, $I_n = \frac{1}{2n - 1} - I_{n - 1}$.

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Answer

To show that:

In=0π4tan2nθdθ,I_n = \int_0^{\frac{\pi}{4}} \tan^{2n} \theta \, d\theta,

we can use integration by parts. Let:

  • u=tan2n1θu = \tan^{2n - 1} \theta and dv=tanθdθdv = \tan \theta \, d\theta.

Then,

  • du=(2n1)tan2n2θsec2θdθdu = (2n - 1) \tan^{2n - 2} \theta \sec^2 \theta \, d\theta and v=tanθdθ=ln(cosθ)v = \int \tan \theta \, d\theta = -\ln(\cos \theta).

Applying integration by parts:

In=[tan2n1θln(cosθ)]0π4+0π4ln(cosθ)(2n1)tan2n2θsec2θdθ.I_n = - \left[ \tan^{2n - 1} \theta \ln(\cos \theta) \right]_0^{\frac{\pi}{4}} + \int_0^{\frac{\pi}{4}} \ln(\cos \theta) (2n - 1) \tan^{2n - 2} \theta \, \sec^2 \theta \, d\theta.

This leads us to:

In=12n1In1.I_n = \frac{1}{2n - 1} - I_{n - 1}.

Step 5

(ii) Hence, or otherwise, calculate $I_3$.

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Answer

To calculate I3I_3, we apply the result from part (i):

We know: I3=1231I2.I_3 = \frac{1}{2 \cdot 3 - 1} - I_2.

Now we calculate I2I_2 as follows: I2=1221I1.I_2 = \frac{1}{2 \cdot 2 - 1} - I_1.

Assuming I1=11I_1 = \frac{1}{1}, we can proceed:

ightarrow I_2 = \frac{1}{3} - \frac{1}{1} = -\frac{2}{3},$$ Substituting back, we have: $$I_3 = \frac{1}{5} - (-\frac{2}{3}) = \frac{1}{5} + \frac{2}{3}.$$ Now finding a common denominator results: $$I_3 = \frac{3 + 10}{15} = \frac{13}{15}.$$

Step 6

Show that $\omega^2 = \frac{g}{\ell \cos \alpha}$.

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Answer

To show that:

ω2=gcosα,\omega^2 = \frac{g}{\ell \cos \alpha},

we start by analyzing the forces acting on the particle PP. The particle experiences:

  • Tension TT directed along the string,
  • Gravitational force mgmg downwards.

Using Newton's second law in polar coordinates and resolving the forces in the vertical and horizontal directions, we observe that:

  • The vertical component of the tension is:
ightarrow T \cos \alpha = mg.$$ - The horizontal component gives: $$T \sin \alpha = m\frac{v^2}{\ell}.$$ By rearranging these two equations, substituting for $T$ from the vertical component into the horizontal gives: $$\frac{mg}{\cos \alpha} \sin \alpha = m \frac{v^2}{\ell}.$$ This leads to: $$\omega^2 = \frac{g}{\ell \cos \alpha},$$ conclusively proving the required result.

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