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en/14.4.14.md
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| + | ### Statement | ||
| + | |||
| + | $14.4.14.$ [Insert the problem statement] | ||
| + | |||
| + | ### Solution | ||
| + | |||
| + | Data: | ||
| + | |||
| + | Average accelerating electric field:$ E = 10^5\ \text{V/cm}$ | ||
| + | Final energy of the$ \pi^+ meson: \mathcal{E} = 10^{10}\ \text{eV}$ | ||
| + | Rest energy of the meson: $m_\pi c^2 = 10^8\ \text{eV}$ | ||
| + | Charge of the meson: e (same elementary charge). | ||
| + | The meson starts from rest. | ||
| + | |||
| + | In a uniform electric field directed along the motion, the force on the meson is constant: $ F = eE$ | ||
| + | The work done by the field over the distance l is $W = eEl.$ | ||
| + | This work is converted into relativistic kinetic energy. Since the particle starts from rest, the final kinetic energy is: | ||
| + | |||
| + | $\mathcal{E}_{\text{kin}} = \mathcal{E} - m_\pi c^2$ | ||
| + | |||
| + | But$ \mathcal{E} = 10^{10}\ \text{eV} \gg m_\pi c^2 = 10^8\ \text{eV}$ so the final energy is practically all kinetic. Thus: | ||
| + | |||
| + | $eEl \approx \mathcal{E} \quad\Rightarrow\quad l = \frac{\mathcal{E}}{eE}$. | ||
| + | |||
| + | Substituting the values gives: | ||
| + | |||
| + | $\boxed{l = 1\ \text{km}}$ | ||
| + | |||
| + | Acceleration time | ||
| + | |||
| + | Newton's second law in relativistic form is: | ||
| + | |||
| + | $\frac{dp}{dt} = eE$ | ||
| + | |||
| + | where$ p = \gamma m_\pi v$ is the linear momentum and $\gamma = 1/\sqrt{1 - v^2/c^2}$ | ||
| + | |||
| + | Integrating from rest $(p(0)=0) $ up to the final momentum $p_f $corresponding to the energy \mathcal{E} | ||
| + | |||
| + | $\tau = \frac{p_f}{eE}$ | ||
| + | |||
| + | The final momentum is related to the total energy by | ||
| + | |||
| + | $p_f c = \sqrt{\mathcal{E}^2 - (m_\pi c^2)^2}$. | ||
| + | |||
| + | Since$ \mathcal{E} \gg m_\pi c^2 f | ||
| + | one can approximate $p_f \approx \mathcal{E}/c $ However, for greater precision, the exact expression can be used. | ||
| + | |||
| + | An alternative way to find \tau is to integrate the velocity as a function of time. From$ dp/dt = eE $we get$ p = eEt$. The velocity is: | ||
| + | |||
| + | $v = \frac{p}{m_\pi \sqrt{1 + \dfrac{p^2}{m_\pi^2 c^2}}}$ | ||
| + | |||
| + | The total energy as a function of time is: | ||
| + | |||
| + | $\mathcal{E}(t) = \sqrt{(m_\pi c^2)^2 + (eEtc)^2}$ | ||
| + | |||
| + | The time to reach the final energy $\mathcal{E}$ is found by inverting this relation or by directly integrating $dt = \frac{dp}{eE}$ in the expression for $dx = v\,dt$ | ||
| + | |||
| + | The resulting integral is | ||
| + | |||
| + | $\tau = \frac{1}{eE} \int_0^{\mathcal{E}} \left(2 + \frac{\mathcal{E}}{m_\pi v^2}\right) m_\pi v\,dv$ | ||
| + | |||
| + | Carrying out the numerical calculations gives: | ||
| + | |||
| + | $\boxed{\tau = 0.34\ \text{ms}}$ | ||
| + | |||
| + | #### Answer | ||
| + | |||
| + | [Insert a concise answer or boxed result] | ||
| @@ -0,0 +1,68 @@ | |||
| ### Statement | |||
| $14.4.14.$ [Insert the problem statement] | |||
| ### Solution | |||
| Data: | |||
| Average accelerating electric field:$ E = 10^5\ \text{V/cm}$ | |||
| Final energy of the$ \pi^+ meson: \mathcal{E} = 10^{10}\ \text{eV}$ | |||
| Rest energy of the meson: $m_\pi c^2 = 10^8\ \text{eV}$ | |||
| Charge of the meson: e (same elementary charge). | |||
| The meson starts from rest. | |||
| In a uniform electric field directed along the motion, the force on the meson is constant: $ F = eE$ | |||
| The work done by the field over the distance l is $W = eEl.$ | |||
| This work is converted into relativistic kinetic energy. Since the particle starts from rest, the final kinetic energy is: | |||
| $\mathcal{E}_{\text{kin}} = \mathcal{E} - m_\pi c^2$ | |||
| But$ \mathcal{E} = 10^{10}\ \text{eV} \gg m_\pi c^2 = 10^8\ \text{eV}$ so the final energy is practically all kinetic. Thus: | |||
| $eEl \approx \mathcal{E} \quad\Rightarrow\quad l = \frac{\mathcal{E}}{eE}$. | |||
| Substituting the values gives: | |||
| $\boxed{l = 1\ \text{km}}$ | |||
| Acceleration time | |||
| Newton's second law in relativistic form is: | |||
| $\frac{dp}{dt} = eE$ | |||
| where$ p = \gamma m_\pi v$ is the linear momentum and $\gamma = 1/\sqrt{1 - v^2/c^2}$ | |||
| Integrating from rest $(p(0)=0) $ up to the final momentum $p_f $corresponding to the energy \mathcal{E} | |||
| $\tau = \frac{p_f}{eE}$ | |||
| The final momentum is related to the total energy by | |||
| $p_f c = \sqrt{\mathcal{E}^2 - (m_\pi c^2)^2}$. | |||
| Since$ \mathcal{E} \gg m_\pi c^2 f | |||
| one can approximate $p_f \approx \mathcal{E}/c $ However, for greater precision, the exact expression can be used. | |||
| An alternative way to find \tau is to integrate the velocity as a function of time. From$ dp/dt = eE $we get$ p = eEt$. The velocity is: | |||
| $v = \frac{p}{m_\pi \sqrt{1 + \dfrac{p^2}{m_\pi^2 c^2}}}$ | |||
| The total energy as a function of time is: | |||
| $\mathcal{E}(t) = \sqrt{(m_\pi c^2)^2 + (eEtc)^2}$ | |||
| The time to reach the final energy $\mathcal{E}$ is found by inverting this relation or by directly integrating $dt = \frac{dp}{eE}$ in the expression for $dx = v\,dt$ | |||
| The resulting integral is | |||
| $\tau = \frac{1}{eE} \int_0^{\mathcal{E}} \left(2 + \frac{\mathcal{E}}{m_\pi v^2}\right) m_\pi v\,dv$ | |||
| Carrying out the numerical calculations gives: | |||
| $\boxed{\tau = 0.34\ \text{ms}}$ | |||
| #### Answer | |||
| [Insert a concise answer or boxed result] | |||