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Worked Examples · Example 1.7

Q.An electron falls through a distance of 1.5 cm1.5\,\text{cm} in a uniform electric field of magnitude 2.0×104 N C−12.0 \times 10^{4}\,\text{N C}^{-1} [Fig. 1.10(a)]. The direction of the field is reversed keeping its magnitude unchanged and a proton falls through the same distance [Fig. 1.10(b)]. Compute the time of fall in each case. Contrast the situation with that of 'free fall under gravity'.

Figure 1.10
Figure 1.10
Rajasthan RbseTextbookSubjective· 3mImportance★★★★★
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Both particles undergo constant acceleration a=qE/ma=qE/m, so t=2s/at=\sqrt{2s/a}: the electron takes 2.92×10−9 s2.92\times10^{-9}\,\text{s} and the proton 1.25×10−7 s1.25\times10^{-7}\,\text{s}. Unlike free fall (where a=ga=g is mass‑independent), here the time depends on q/mq/m, and both are far shorter than a gravitational fall.

A uniform field exerts a constant force F=qEF=qE, hence a constant acceleration by Newton's second law. Starting from rest, kinematics gives s=12at2s=\tfrac12 a t^2, so t=2s/at=\sqrt{2s/a}.

Given: s=1.5 cm=0.015 ms=1.5\,\text{cm}=0.015\,\text{m}, E=2.0×104 N/CE=2.0\times10^{4}\,\text{N/C}, e=1.6×10−19 Ce=1.6\times10^{-19}\,\text{C}, me=9.11×10−31 kgm_e=9.11\times10^{-31}\,\text{kg}, mp=1.67×10−27 kgm_p=1.67\times10^{-27}\,\text{kg}. In (a) the field points up and the electron (negative) is pushed down; in (b) the field is reversed and the proton (positive) is also pushed down — so each falls through the same ss.

Electron.

ae=eEme=(1.6×10−19)(2.0×104)9.11×10−31=3.51×1015 m/s2,a_e=\frac{eE}{m_e}=\frac{(1.6\times10^{-19})(2.0\times10^{4})}{9.11\times10^{-31}}=3.51\times10^{15}\,\text{m/s}^2,

te=2sae=2(0.015)3.51×1015=8.55×10−18=2.92×10−9 s.t_e=\sqrt{\frac{2s}{a_e}}=\sqrt{\frac{2(0.015)}{3.51\times10^{15}}}=\sqrt{8.55\times10^{-18}}=2.92\times10^{-9}\,\text{s}.

Proton. The force magnitude eE=3.2×10−15 NeE=3.2\times10^{-15}\,\text{N} is the same, but the proton is about 18361836 times heavier:

ap=eEmp=(1.6×10−19)(2.0×104)1.67×10−27=1.92×1012 m/s2,a_p=\frac{eE}{m_p}=\frac{(1.6\times10^{-19})(2.0\times10^{4})}{1.67\times10^{-27}}=1.92\times10^{12}\,\text{m/s}^2,

tp=2sap=2(0.015)1.92×1012=1.57×10−14=1.25×10−7 s.t_p=\sqrt{\frac{2s}{a_p}}=\sqrt{\frac{2(0.015)}{1.92\times10^{12}}}=\sqrt{1.57\times10^{-14}}=1.25\times10^{-7}\,\text{s}.

Contrast with free fall under gravity. In free fall the acceleration is g≈9.8 m/s2g\approx9.8\,\text{m/s}^2, identical for every body regardless of mass. Here the acceleration a=qE/ma=qE/m is enormous (∼1012\sim10^{12}–1015 m/s210^{15}\,\text{m/s}^2) and depends on the charge‑to‑mass ratio, so electron and proton fall in very different times. A purely gravitational fall through the same 0.015 m0.015\,\text{m} would take tg=2s/g≈0.055 st_g=\sqrt{2s/g}\approx0.055\,\text{s} — millions of times longer, which is why gravity is negligible for charged particles in such fields.

✓Final answer

te=2.92×10−9 st_e=2.92\times10^{-9}\,\text{s} (electron) and tp=1.25×10−7 st_p=1.25\times10^{-7}\,\text{s} (proton).

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