[solution]
**Step 1: Fixed points and multiplier.**
Setting $f(x) = x$ gives $x = (a-x)^3$. The substitution $u = a - x$ (so $x = a - u$) transforms this to
\begin{align*}
a - u = u^3 \implies a = u^3 + u.
\end{align*}
Since $\phi(u) = u^3 + u$ is strictly increasing ($\phi'(u) = 3u^2 + 1 > 0$), there is a unique $u^*$ — and hence a unique fixed point $x^* = a - u^*$ — for each $a > 0$.
The multiplier is
\begin{align*}
\lambda = f'(x^*) = -3(a - x^*)^2 = -3(u^*)^2.
\end{align*}
Since $\lambda \le 0$ for all $u^* \ge 0$, the multiplier never reaches $+1$ (no saddle-node bifurcation in this range).
**Step 2: Period-doubling bifurcation.**
The fixed point is stable when $|\lambda| < 1$, i.e.,
\begin{align*}
3(u^*)^2 < 1 \implies u^* < \frac{1}{\sqrt{3}}.
\end{align*}
At $u^* = 1/\sqrt{3}$, the multiplier is $\lambda = -1$, and the corresponding bifurcation parameter is
\begin{align*}
a_c = \left(\frac{1}{\sqrt{3}}\right)^3 + \frac{1}{\sqrt{3}} = \frac{1}{3\sqrt{3}} + \frac{1}{\sqrt{3}} = \frac{4}{3\sqrt{3}} = \frac{4\sqrt{3}}{9} \approx 0.770.
\end{align*}
For $a < a_c$ the fixed point is stable ($u^*$ is small, $|\lambda| < 1$). For $a > a_c$ it is unstable ($|\lambda| > 1$). The transition is a **period-doubling bifurcation**.
**Step 3: Period-2 orbit condition.**
A period-2 orbit $\{x_1, x_2\}$ with $x_1 \neq x_2$ satisfies $f(x_1) = x_2$ and $f(x_2) = x_1$. With $u = a - x_1$ and $v = a - x_2$:
\begin{align*}
a - u = v^3, \quad a - v = u^3.
\end{align*}
Subtracting the second from the first: $v - u = v^3 - u^3 = (v - u)(v^2 + uv + u^2)$. Since $u \neq v$, dividing by $v - u$ gives
\begin{align*}
u^2 + uv + v^2 = 1.
\end{align*}
This is an ellipse in the $(u, v)$ plane, which admits real solutions for a range of $a$.
**Step 4: Multiplier of the period-2 orbit.**
Using $f'(x_i) = -3(a - x_i)^2$, the orbit multiplier is
\begin{align*}
\Lambda = f'(x_1) f'(x_2) = (-3u^2)(-3v^2) = 9u^2 v^2 = 9P^2,
\end{align*}
where $P := uv$. We determine the range of $P$. From $u^2 + uv + v^2 = 1$:
\begin{align*}
(u + v)^2 = u^2 + 2uv + v^2 = 1 + P,
\end{align*}
which requires $P \ge -1$ for real solutions. The constraint $u^2 + v^2 = 1 - P \ge 0$ gives $P \le 1$, and the inequality $u^2 + v^2 \ge 2|uv|$ gives $1 - P \ge 2|P|$. For $P > 0$: $P \le 1/3$, with equality when $u = v = 1/\sqrt{3}$ (the fixed point, not a distinct orbit). So the admissible range for the period-2 orbit is $P \in [-1, 1/3)$.
**Step 5: Stability range.**
The orbit is stable when $|\Lambda| < 1$:
\begin{align*}
9P^2 < 1 \iff |P| < \frac{1}{3}.
\end{align*}
At the period-doubling bifurcation ($u = v = 1/\sqrt{3}$, $P = 1/3$), the orbit is born with $\Lambda = 9 \cdot (1/3)^2 = 1$. As $a$ increases past $a_c$, the orbit opens up and $P$ decreases from $1/3$. The orbit is stable for $P \in (-1/3, 1/3)$ and becomes unstable when $P$ passes through $-1/3$, at which point $\Lambda = 1$ again. This secondary bifurcation ($\Lambda = 1$ for the period-2 orbit, i.e., a period-doubling of the second iterate $f^2$) initiates a period-4 orbit — the next step in the period-doubling cascade.
[/solution]