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Problem Irodov 3.377

A relativistic proton enters, at t=0t = 0, a region of uniform electric field E\vect E, its velocity v0\vect v_0 at entry being perpendicular to E\vect E. As functions of time, find:

  1. the angle θ\theta between the proton’s velocity v\vect v and its initial direction of motion;

  2. the component vxv_x of v\vect v along that initial direction.

The proton p arriving with velocity v_0 at the region of uniform field E, which is perpendicular to v_0; the field is seen side on.

The proton pp arriving with velocity v0\vect v_0 at the region of uniform field E\vect E, which is perpendicular to v0\vect v_0; the field is seen side on.

Given
  • v0⊥E\vect v_0 \perp \vect E
  • EE uniform
  • entry at t=0t = 0
Find
(a) θ(t)\theta(t) · (b) vx(t)v_x(t)

Solution

Step 1The two components of the momentum

Take xx along v0\vect v_0 and yy along E\vect E, with β0=v0/c\beta_0 = v_0/c and mm the proton’s rest mass. There is no force along xx, so pxp_x keeps its entry value p0p_0; along yy the constant force eEeE builds the momentum up from zero:

px=p0=mv01−β02,py=eEt(1) p_x = p_0 = \frac{m v_0}{\sqrt{1 - \beta_0^2}}, \qquad p_y = eEt \tag{1}
The proton's momentum p at time t: the constant component p_0 along the initial direction x and the growing component eEt along the field. The velocity has the direction of p, at the angle θ to x.

The proton’s momentum p\vect p at time tt: the constant component p0p_0 along the initial direction xx and the growing component eEteEt along the field. The velocity has the direction of p\vect p, at the angle θ\theta to xx.

Step 2(a) The angle of the velocity

The velocity v=pc2/W\vect v = \vect p c^2/W, with WW the total energy, is parallel to the momentum, so θ\theta is the angle of p\vect p. Its tangent is the ratio of the components (1):

tan⁡θ=pypx=eEtmv0/1−β02\tan\theta = \frac{p_y}{p_x} = \frac{eEt}{m v_0/\sqrt{1 - \beta_0^2}}
tan⁡θ=eEtmv01−β02\tan\theta = \frac{eEt}{m v_0}\sqrt{1 - \beta_0^2}
(2)
Step 3The total energy as it grows

The total energy follows from the momentum through W2=(pc)2+(mc2)2W^2 = (pc)^2 + (mc^2)^2. At entry it is W0=mc2/1−β02W_0 = mc^2/\sqrt{1 - \beta_0^2}, and the growing pyp_y adds to it:

W2=(p0c)2+(mc2)2+(eEct)2=W02+(eEct)2(3) W^2 = (p_0c)^2 + (mc^2)^2 + (eEct)^2 = W_0^2 + (eEct)^2 \tag{3}
Step 4(b) The forward component of the velocity

The forward component is vx=pxc2/Wv_x = p_xc^2/W. At entry p0c2=v0W0p_0c^2 = v_0W_0; with (3) for WW, then dividing through by W0W_0:

vx=p0c2W=v0W0W02+(eEct)2=v01+(eEct/W0)2,eEctW0=eEtmc1−β02\begin{aligned} v_x &= \frac{p_0c^2}{W} = \frac{v_0W_0}{\sqrt{W_0^2 + (eEct)^2}} = \frac{v_0}{\sqrt{1 + (eEct/W_0)^2}}, \\ \frac{eEct}{W_0} &= \frac{eEt}{mc}\sqrt{1 - \beta_0^2} \end{aligned}
vx=v01+(1−β02) (eEt/mc)2v_x = \frac{v_0}{\sqrt{1 + (1 - \beta_0^2)\,(eEt/mc)^2}}
(4)
Check

Units: eEteEt is an impulse, so eEt/(mc)eEt/(mc) and eEt/(mv0)eEt/(mv_0) are pure numbers. Newtonian limit c→∞c \to \infty: β0→0\beta_0 \to 0 and eEt/(mc)→0eEt/(mc) \to 0, so tan⁡θ→eEt/(mv0)\tan\theta \to eEt/(mv_0) and vx→v0v_x \to v_0, the parabola of a slow particle. At t=0t = 0, θ=0\theta = 0 and vx=v0v_x = v_0. At late times vxv_x falls off as 1/t1/t while vy=pyc2/W→cv_y = p_yc^2/W \to c, so θ→90∘\theta \to 90^\circ and the speed stays below cc.

Remark

No force acts along xx, yet vxv_x falls. The momentum px=Wvx/c2p_x = W v_x/c^2 is what stays constant; the field keeps pumping energy WW into the proton, so the forward velocity must drop to keep the product fixed. In Newtonian mechanics the two motions are independent; in relativity the transverse push drags on the forward motion through the shared energy.