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Valter edited
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+### Statement
+
+$2.1.63.$ [Insert the problem statement]
+
+### Solution
+
+### Statement
+
+$2.1.63.$ A horizontal disk begins to spin around its axis with an angular velocity that increases linearly with time $\omega = \varepsilon t$. At what angular velocity will a body located at a distance $r$ from the disk's axis begin to slide off it, if the coefficient of friction between them is $\mu$?
+
+### Solution
+
+Because the angular velocity is constantly changing, the body experiences two components of acceleration on the plane of the disk:
+1. Centripetal (normal) acceleration, directed towards the center: $a_n = \omega^2 r$
+2. Tangential acceleration, directed perpendicular to the radius: $a_\tau = \varepsilon r$
+
+Since these two vectors are strictly perpendicular, we find the total magnitude of acceleration $a$ using the Pythagorean theorem:
+$$a = \sqrt{a_n^2 + a_\tau^2} = \sqrt{(\omega^2 r)^2 + (\varepsilon r)^2} = r \sqrt{\omega^4 + \varepsilon^2}$$
+
+The body starts to slide at the exact moment when the required force to maintain this total acceleration exceeds the maximum possible static friction force $F_{\text{fr}} = \mu N = \mu mg$.
+Writing Newton's second law for the threshold of slipping:
+$$ma = \mu mg \implies a = \mu g$$
+
+Substitute the expression for total acceleration:
+$$r \sqrt{\omega^4 + \varepsilon^2} = \mu g$$
+
+Square both sides to solve for $\omega$:
+$$r^2 (\omega^4 + \varepsilon^2) = \mu^2 g^2$$
+$$\omega^4 + \varepsilon^2 = \frac{\mu^2 g^2}{r^2}$$
+$$\omega^4 = \frac{\mu^2 g^2}{r^2} - \varepsilon^2$$
+
+Taking the fourth root, we find the angular velocity $\omega$:
+$$\omega = \left( \frac{\mu^2 g^2}{r^2} - \varepsilon^2 \right)^{1/4}$$
+
+<i>Note: This solution is physically meaningful only if the expression under the root is positive, i.e., $\varepsilon < \mu g / r$. If the angular acceleration $\varepsilon$ is extremely large ($\varepsilon \ge \mu g / r$), the tangential acceleration alone immediately overcomes friction, and the body slips at $t=0$ when $\omega = 0$.</i>
+
+#### Answer
+$\omega = 0$ for $\varepsilon \ge \mu g/r$;
+$\omega = (\mu^2 g^2/r^2 - \varepsilon^2)^{1/4}$ for $\varepsilon < \mu g/r$
+
+#### Answer
+
+[Insert a concise answer or boxed result]