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| <span><img src="../../img/book.png"></span><span>Savchenko Solutions</span> | | <span><img src="../../img/book.png"></span><span>Savchenko Solutions</span> |
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| <p class="author"> | | <p class="author"> |
| Solutions of Savchenko Problems in Physics <br> | | Solutions of Savchenko Problems in Physics <br> |
| <i><b>knowledge must be free</b></i> | | <i><b>knowledge must be free</b></i> |
| </p> | | </p> |
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| <h3 id="back-link"><a href="../../#7.1">$\leftarrow$Back</a></h3> | | <h3 id="back-link"><a href="../../#7.1">$\leftarrow$Back</a></h3> |
| | | |
| <h3> Statement </h3> | | <h3> Statement </h3> |
| <p> | | <p> |
| $7.1.23^*.$ Find the period of small vibrations of a body of mass $m$, whose charge is $q$, inside a smooth sphere of radius $R$, if the charge $Q$ is fixed at the top point of the sphere. | | $7.1.23^*.$ Find the period of small vibrations of a body of mass $m$, whose charge is $q$, inside a smooth sphere of radius $R$, if the charge $Q$ is fixed at the top point of the sphere. |
| </p> | | </p> |
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| <img src="7.1.23.png" | | <img src="7.1.23.png" |
| loading="lazy" width="200" /> | | loading="lazy" width="200" /> |
| <figcaption> | | <figcaption> |
| For problem $7.1.23^*$ | | For problem $7.1.23^*$ |
| </figcaption> | | </figcaption> |
| </figure> | | </figure> |
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| <p> | | <p> |
| </p> | | </p> |
| | | |
| <h3>Solution</h3> | | <h3>Solution</h3> |
| <p> | | <p> |
| | | |
| </p> | | </p> |
| <center> | | <center> |
| <figure> | | <figure> |
| <img src="7.1.23_1.png" | | <img src="7.1.23_1.png" |
| loading="lazy" width="200" /> | | loading="lazy" width="200" /> |
| <figcaption> | | <figcaption> |
| Forces acting on the system of two charges | | Forces acting on the system of two charges |
| </figcaption> | | </figcaption> |
| </figure> | | </figure> |
| </center> | | </center> |
| <p> | | <p> |
| | | |
| Considering the fact that oscillations are small, $\varphi \ll 1$, we could use the approximations for small angle $\varphi$ | | Considering the fact that oscillations are small, $\varphi \ll 1$, we could use the approximations for small angle $\varphi$ |
| $$\sin\varphi \approx \varphi; \quad\cos\varphi \approx 1\quad(1)$$ | | $$\sin\varphi \approx \varphi; \quad\cos\varphi \approx 1\quad(1)$$ |
| From where, we could approximate that the distance between charges remains approximately the same | | From where, we could approximate that the distance between charges remains approximately the same |
| $$r\approx2R$$ | | $$r\approx2R$$ |
| Thus, the сoulomb's law for two charges | | Thus, the сoulomb's law for two charges |
| $$F_c = \frac{1}{4\pi\varepsilon_0}\frac{qQ}{4R^2}$$ | | $$F_c = \frac{1}{4\pi\varepsilon_0}\frac{qQ}{4R^2}$$ |
| Let's write Newton's second law on a tangential trajectory, in the direction of motion of a charge of mass $m$ | | Let's write Newton's second law on a tangential trajectory, in the direction of motion of a charge of mass $m$ |
| $$ma = mg \sin\varphi + F_c \sin\frac{\varphi}{2}$$ | | $$ma = mg \sin\varphi + F_c \sin\frac{\varphi}{2}$$ |
| Considering the approximation $(1)$ and the expression | | Considering the approximation $(1)$ and the expression |
| $$ma = -mg\frac{x}{R} - \frac{x}{2R} \frac{1}{4\pi\varepsilon_0}\frac{qQ}{4R^2}$$ | | $$ma = -mg\frac{x}{R} - \frac{x}{2R} \frac{1}{4\pi\varepsilon_0}\frac{qQ}{4R^2}$$ |
| $$a = -x\left(\frac{g}{R}+\frac{qQ}{32\pi\varepsilon_0mR^3}\right)$$ | | $$a = -x\left(\frac{g}{R}+\frac{qQ}{32\pi\varepsilon_0mR^3}\right)$$ |
| Solving the equation of harmonic oscillations $(\ddot{x}+\omega^2x(t)=0)$, we could obtain the value for angular velocity | | Solving the equation of harmonic oscillations $(\ddot{x}+\omega^2x(t)=0)$, we could obtain the value for angular velocity |
| $$\omega=\sqrt{\frac{g}{R}+\frac{qQ}{32\pi\varepsilon_0mR^3}}$$ | | $$\omega=\sqrt{\frac{g}{R}+\frac{qQ}{32\pi\varepsilon_0mR^3}}$$ |
| From here the period of oscillation | | From here the period of oscillation |
| $$\boxed{T=\frac{2\pi}{\omega} = \frac{2\pi}{\sqrt{\frac{g}{R}+\frac{qQ}{32\pi\varepsilon_0mR^3}}}}$$ | | $$\boxed{T=\frac{2\pi}{\omega} = \frac{2\pi}{\sqrt{\frac{g}{R}+\frac{qQ}{32\pi\varepsilon_0mR^3}}}}$$ |
| Since the expression under the square root cannot be less than zero, the ratio at which there will be no oscillations | | Since the expression under the square root cannot be less than zero, the ratio at which there will be no oscillations |
| $$\frac{g}{R}+\frac{qQ}{32\pi\varepsilon_0mR^3} > 0 \Leftrightarrow \boxed{\frac{qQ}{32\pi\varepsilon_0R^2}>-mg}$$ | | $$\frac{g}{R}+\frac{qQ}{32\pi\varepsilon_0mR^3} > 0 \Leftrightarrow \boxed{\frac{qQ}{32\pi\varepsilon_0R^2}>-mg}$$ |
| </p> | | </p> |
| | | |
| <h4>Answer</h4> | | <h4>Answer</h4> |
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