This problem concerns the motion of an object on a rotating surface. The objective is to find the coefficient \( x \) in the expression for the radial velocity of a steel ball as it exits the rotating surface.
The forces acting on the ball are considered. As the surface rotates at an angular velocity \( \omega \), a centrifugal force is exerted radially outward on the ball. This force is defined by the equation \( F = m \omega^2 r \), where \( r \) denotes the radial distance from the rotational center.
The ball originates at a radial distance \( r_0 = 1 \, \text{m} \) from the center. During its outward progression, it experiences no tangential force due to a smooth channel and accumulates radial kinetic energy solely from the centrifugal force. Upon reaching the edge of the rotating surface at \( r = 3 \, \text{m} \), its radial kinetic energy is quantified as:
\[ \frac{1}{2} m v_r^2 = \int_{r_0}^{3} m \omega^2 r \, dr \]
The integral calculation yields:
\[ \int_{1}^{3} \omega^2 r \, dr = \left. \frac{\omega^2 r^2}{2} \right|_{1}^{3} = \frac{\omega^2 (3^2 - 1^2)}{2} = \frac{\omega^2 (9 - 1)}{2} = 4\omega^2 \]
The kinetic energy is then equated:
\[ \frac{1}{2} m v_r^2 = m \cdot 4\omega^2 \]
Simplification leads to:
\[ v_r^2 = 8\omega^2 \]
\[ v_r = \sqrt{8}\omega = 2\sqrt{2}\omega \]
Consequently, the ball's final radial velocity is \( 2\sqrt{2}\omega \, \text{m/s} \). By comparing this with the expression \( x\sqrt{2}\omega \, \text{m/s} \), we deduce that \( x = 2 \).
This resultant value falls within the specified bounds of \( 2,2 \).