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.

Short Answer

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In summary, we have proven that in relativistic mechanics, the time rate of change of the angular momentum of a particle about an origin is equal to the couple of the applied force about the origin, and the space-space part of the equation \((\mathrm{d} / \mathrm{d} \tau) L^{\mu \nu}=G^{\mu \nu}\) corresponds to this three-vector result. We first found the time derivative of the angular momentum and related it to the velocity and force. Then we differentiated the four-angular momentum with respect to proper time and correlated it with the fourcouple. Finally, we confirmed that the space-space components of this equation reflected the three-vector result we previously derived.

Step by step solution

01

Define the variables

Begin by defining the given variables in the problem statement: - \(h = \mathbf{r} \times p\) is the angular momentum, where \(\mathbf{r}\) is the position vector of the particle and \(p\) is its linear momentum in both relativistic and Newtonian mechanics. - \(\mathbf{f}\) is the applied force on the particle. - \(L^{\mu \nu}\) is the particle's four-angular momentum. - \(G^{\mu \nu} = x^{\mu} F^{v} - x^{v} F^{\mu}\) is the fourcouple, where \(x^{\mu}\) and \(F^{\mu}\) are the four-vectors corresponding to \(\mathbf{r}\) and \(\mathbf{f}\), respectively.
02

Relate angular momentum to applied force

Let's first establish that, in relativistic mechanics, the time rate of change of angular momentum is equal to the couple of the applied force: \(h = \mathbf{r} \times p\) Take the time derivative of the angular momentum: \(\frac{dh}{dt} = \frac{d}{dt} (\mathbf{r} \times p)\) Now, using the product rule for vector derivatives: \(\frac{dh}{dt} = \frac{d\mathbf{r}}{dt} \times p + \mathbf{r} \times \frac{dp}{dt}\) The time derivative of the position vector (\(\frac{d\mathbf{r}}{dt}\)) is the velocity vector (\(\mathbf{v}\)), and the time derivative of the momentum (\(\frac{dp}{dt}\)) is the force (\(\mathbf{f}\)): \(\frac{dh}{dt} = \mathbf{v} \times p + \mathbf{r} \times \mathbf{f}\) Since velocity and momentum are parallel in both relativistic and Newtonian mechanics, their cross product is zero: \(\frac{dh}{dt} = \mathbf{r} \times \mathbf{f}\) This proves that the time rate of change of angular momentum is equal to the couple of the applied force in both relativistic and Newtonian mechanics.
03

Show that \((\mathrm{d} / \mathrm{d} \tau) L^{\mu \nu}=G^{\mu \nu}\)

First, let's write the four-angular momentum: \(L^{\mu \nu} = x^{\mu} p^{\nu} - x^{\nu} p^{\mu}\) Now, differentiate with respect to the proper time \(\tau\): \(\frac{d}{d\tau} L^{\mu \nu} = \frac{d}{d\tau} (x^{\mu} p^{\nu} - x^{\nu} p^{\mu})\) Using the product rule: \(\frac{d}{d\tau} L^{\mu \nu} = (\frac{dx^{\mu}}{d\tau} p^{\nu} + x^{\mu} \frac{dp^{\nu}}{d\tau}) - (\frac{dx^{\nu}}{d\tau} p^{\mu} + x^{\nu} \frac{dp^{\mu}}{d\tau})\) Now, we know that \(\frac{dx^{\mu}}{d\tau} = V^{\mu}\) (four-velocity) and \(\frac{dp^{\mu}}{d\tau} = F^{\mu}\) (four-force). Replacing these in the equation, we get: \(\frac{d}{d\tau} L^{\mu \nu} = (V^{\mu} p^{\nu} + x^{\mu} F^{\nu}) - (V^{\nu} p^{\mu} + x^{\nu} F^{\mu})\) Comparing this with the definition of fourcouple: \(G^{\mu \nu} = x^{\mu} F^{\nu} - x^{\nu} F^{\mu}\) We see that \((\mathrm{d} / \mathrm{d} \tau) L^{\mu \nu}=G^{\mu \nu}\).
04

Find the space-space part of the equation

To show that the space-space part of the equation \((\mathrm{d} / \mathrm{d} \tau) L^{\mu \nu}=G^{\mu \nu}\) corresponds to the three-vector result, i.e., \(\frac{dh}{dt} = \mathbf{r} \times \mathbf{f}\), we only need to consider the space components (\(\mu,\nu=1,2,3\)) of the equation: \((\mathrm{d} / \mathrm{d} \tau) L^{ij} = G^{ij}\) Since \(L^{ij} = x^i p^j - x^j p^i\) and \(G^{ij} = x^i F^j - x^j F^i\), this equation represents the same three-vector relation we have already found: \(\frac{dh}{dt} = \mathbf{r} \times \mathbf{f}\) In conclusion, we have proved that in relativistic mechanics, the time rate of change of the angular momentum of a particle about an origin is equal to the couple of the applied force about the origin, and the space-space part of the equation \((\mathrm{d} / \mathrm{d} \tau) L^{\mu \nu}=G^{\mu \nu}\) corresponds to this three-vector result.

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Most popular questions from this chapter

. 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.

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15\. A rocket propels itself rectilinearly by emitting radiation in the direction opposite to its motion. If \(V\) is its final velocity relative to its initial rest frame, prove \(a b\) initio that the ratio of the initial to the final rest mass of the rocket is given by $$ \frac{M_{\mathrm{i}}}{M_{\mathrm{f}}}=\left(\frac{c+V}{c-V}\right)^{1 / 2} $$ and compare this with the result of Exercise 5 above. [Hint: equate energies and momenta at the beginning and at the end of the acceleration, writing \(\Sigma h v\) and \(\Sigma h v / c\) for the total energy and momentum, respectively, of the emitted photons.]

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