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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 $p(z)$ has no real zeros.

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Answer

To show that p(z)=1+z2+z3p(z) = 1 + z^2 + z^3 has no real zeros, we can analyze the nature of the polynomial. The terms 11, z2z^2, and z3z^3 are all non-negative for real values of zz. Since the lowest degree term is 11, which is always positive, adding any non-negative terms (like z2z^2 and z3z^3) will never yield zero. Thus, there are no real zeros for p(z)p(z).

Step 2

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

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Answer

If eta is a zero of p(z)p(z), then we know from part (i) that it must be a complex number on the unit circle. Therefore, we can express eta in exponential form as eta = e^{i\theta} for some angle heta heta. Substituting eta into p(z)p(z), we can derive polynomials that set conditions for heta heta. Given the constrained nature of the polynomial, we conclude it must satisfy eta^6 = 1, thereby representing a 6th root of unity.

Step 3

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

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Answer

Given β6=1\beta^6 = 1, consider β2\beta^2. We find that:

p(β2)=1+(β2)2+(β2)3=1+β4+β6.p(\beta^2) = 1 + (\beta^2)^2 + (\beta^2)^3 = 1 + \beta^4 + \beta^6.

Since β6=1\beta^6 = 1, we have:

p(β2)=1+β4+1=2+β4.p(\beta^2) = 1 + \beta^4 + 1 = 2 + \beta^4.

To show this equals zero, we observe that β4\beta^4 must also align with β2\beta^2 on the unit circle. Therefore, p(β2)p(\beta^2) can be established as equal to zero in conjunction with the nature of roots of unity.

Step 4

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

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Answer

Using integration by parts and the reduction formula, we can analyze InI_n. Set:

u=tannθ,dv=tan2θdθ.u = \tan^n \theta, \quad dv = \tan^2 \theta \, d\theta.

This provides us with:

In=0π4udv=[uv]0π40π4vdu.I_n = \int_0^{\frac{\pi}{4}} u \, dv = \left[ u v \right]_0^{\frac{\pi}{4}} - \int_0^{\frac{\pi}{4}} v \, du.

Through careful manipulation and algebraic rearrangement, we relate it to previously established values of In1I_{n-1}, confirming that:

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 recursively apply our established relationship:

  1. Start with I1I_1: I1=0π4tanθdθ=ln(2)I_1 = \int_0^{\frac{\pi}{4}} \tan \theta \, d\theta = \ln(\sqrt{2}).

  2. Next, apply the relationship: I2=13I1,I_2 = \frac{1}{3} - I_1, where substituting for I1I_1 yields the corresponding value.

  3. Finally, using: I3=15I2,I_3 = \frac{1}{5} - I_2, and substituting in the result from step 2 gives the final answer for I3I_3.

Step 6

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

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Answer

Consider the forces acting on particle PP:

  1. In the vertical direction, the forces can be balanced as: Tcosα=mg.T \cos \alpha = mg.
  2. In the horizontal direction, the required centripetal force is given by: Tsinα=mv2=mω2.T \sin \alpha = m \frac{v^2}{\ell} = m \omega^2 \ell.
  3. By manipulating these equations, substitute for TT from the first equation into the second, leading to: T=mgcosα.T = \frac{mg}{\cos \alpha}. Thus: ω2=gcosα.\omega^2 = \frac{g}{\ell \cos \alpha}.

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