. Show that a photon cannot spontaneously disintegrate into an electron- positron pair. [Hint: four-momentum conservation.] But in the presence of a stationary nucleus (acting as a kind of catalyst) it can. If the rest mass of the nucleus is \(N\), and that of the electron (and positron) is \(m\), what is the threshold frequency of the photon? Verify that for large \(N\) the efficiency is \(\sim 100\) per cent (cf. the preceding problem), so that the nucleus then comes close to being a pure catalyst.

Short Answer

Expert verified
A: The threshold frequency of the photon (ν) can be found using the equation: $$ \nu = \frac{2mc^2 + (M_N^{'}-M_N)c^2}{h} $$ Q: Verify the efficiency of the process for a large nucleus mass N. A: For large N, the efficiency of the process can be defined as: $$ \eta = \frac{2mc^2}{2mc^2 + (M_N^{'}-M_N)c^2} \approx 1 $$ This means that for large N, the efficiency is close to 100% and the nucleus comes close to being a pure catalyst.

Step by step solution

01

Spontaneous disintegration without a nucleus

We need to check if energy and momentum conservation laws are upheld for spontaneous disintegration of a photon into an electron-positron pair. The energy conservation equation is: $$ E_{\gamma} = E_{e^-} + E_{e^+} $$ The momentum conservation equation is: $$ \vec{p}_{\gamma} = \vec{p}_{e^-} + \vec{p}_{e^+} $$ where \(E_{\gamma}\) and \(\vec{p}_{\gamma}\) are the energy and momentum of the photon, and \(E_{e^-}\), \(E_{e^+}\), \(\vec{p}_{e^-}\) and \(\vec{p}_{e^+}\) are those of the electron and positron. For the photon, we have \(E_{\gamma}=p_{\gamma}c\) and for each of electron and positron \(E_{\text{particle}}^2 = (m_{\text{particle}}c^2)^2+(\vec{p}_{\text{particle}}c)^2\) Since the photon has no mass, its four-momentum conservation equation is not upheld in this case, and the photon cannot spontaneously disintegrate into an electron-positron pair.
02

Disintegration with a stationary nucleus

In the presence of a stationary nucleus, we have a photon, a nucleus, an electron, and a positron. We can write the energy and momentum conservation equations as: $$ E_{\gamma} + M_Nc^2 = E_{e^-} + E_{e^+} + M_N^{'}c^2 $$ and $$ \vec{p}_{\gamma} = \vec{p}_{e^-} + \vec{p}_{e^+} + \vec{p}_N^{'} $$ Where \(M_N\) and \(M_N^{'}\) are the rest mass of the nucleus before and after the interaction, respectively. To satisfy momentum conservation, the final sum of the nucleus and electron-positron pair momenta should be equal to the initial photon momentum. As a result, this process can occur.
03

Threshold frequency of the photon

To find the threshold frequency of the photon, we will analyze the energy conservation equation, where the nucleus's kinetic energy (and thus momentum change) is minimized: $$ E_{\gamma} = E_{e^-} + E_{e^+} + (M_N^{'}-M_N)c^2 $$ In the threshold condition, we have \(E_{\text{particle}}=m_{\text{particle}}c^2\) for electron and positron $$ E_{\gamma} = 2mc^2 + (M_N^{'}-M_N)c^2 $$ The photon's energy is \(E_{\gamma} = h\nu\), with \(\nu\) being the frequency and \(h\) being the Planck constant. The threshold frequency is: $$ \nu = \frac{2mc^2 + (M_N^{'}-M_N)c^2}{h} $$
04

Efficiency verification

The efficiency of the process can be defined as: $$ \eta = \frac{2mc^2}{E_{\gamma}} $$ In the limit of large N, we have \(M_N^{'} \approx M_N\) $$ \eta = \frac{2mc^2}{2mc^2 + (M_N^{'}-M_N)c^2} \approx 1 $$ Therefore, for large N, the efficiency is close to 100%, and the nucleus comes close to being a pure catalyst.

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Most popular questions from this chapter

taking \(h=6.63 \times 10^{-27} \mathrm{crgs}\) and \(c=300000 \mathrm{~km} \mathrm{~s}^{-1}\), calculate how many photons of wavelength \(5 \times 10^{-5} \mathrm{~cm}\) (in the yellowgreen of the visible spectrum) must fall per second on a blackened plate to produce a force of one dyne. [Answer: \(7.3 \times 10^{21}\). Hint: force equals momentum absorbed per unit time.]

If a photon with four-momentum \(P\) is observed by two observers having four- velocities \(\mathrm{U}_{0}\) and \(\mathrm{U}_{1}\), prove that the observed frequencies are in the ratio \(\mathbf{U}_{0} \cdot \mathbf{P} / \mathbf{U}_{1} \cdot \mathbf{P}\). Hence rederive equation (17.3).

Prove that, in relativistic as in Newtonian mechanics, the time rate of change of the angular momentum \(h=\mathbf{r} \times p\) of a particle about an origin \(\mathrm{O}\) is equal to the couple \(\mathrm{r} \times \mathrm{f}\) of the applied force about \(\mathrm{O}\). If 1 \(^{\mu v}\) is the particle's four- angular momentum, and if we define the fourcouple \(G^{\mu v}=x^{\mu} F^{v}-x^{v} F^{\mu}\), where \(x^{\mu}\) and \(F^{\mu}\) are the four-vectors corresponding to \(\mathbf{r}\) and \(\mathbf{f}\), prove that \((\mathrm{d} / \mathrm{d} \tau) L^{\mu \nu}=G^{\mu \nu}\) and that the spacc-space part of this equation corresponds to the above threevector result.

Uniform parallel radiation is observed in two arbitrary inertial frames \(\mathbf{S}\) and \(\mathbf{S}^{\prime}\) in which it has frequencies \(v\) and \(v^{\prime}\) respectively. If \(p, g, \sigma\) denote, respectively, the radiation pressure, momentum density, and energy density of the radiation in \(S\), and primed symbols denote corresponding quantities in \(S^{\prime}\), prove \(p^{\prime} / p=g^{\prime} / g=\sigma^{\prime} / \sigma\) \(=v^{\prime 2} / v^{2} .[\) Hint: Exercise III \((17) .]\)

A particle moves rectilinearly under a rest mass preserving force in some inertial frame. Show that the product of its rest mass and its instantaneous proper acceleration equals the magnitude of the relativistic three-force acting on the particle in that frame. [Hint: (14.1) and (35.14).] Show also that this is not necessarily true when the motion is not rectilinear.

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