Controlled Thermonuclear Fusion — Question 5

Section 43-7 · Physics pages 7280–7281

Question 5 A magnetic field bends ion motion without supplying kinetic energy A singly charged deuteron has mass 3.34 × 10−27 kg and perpendicular speed 106 m/s in uniform B=5.00 T. Use charge 1.60 × 10−19 C and neglect collisions. rL B⊙ v⊥ Schematic; labels, not drawing lengths, specify the data. (a) Find gyro-radius and gyro-period. (b) Show that the magnetic field does no work, and explain why a small orbit radius alone does not prove long-term plasma confinement.
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Question 5 - Solution A magnetic field bends ion motion without supplying kinetic energy rL B⊙ v⊥ (a) Method and calculation |q|v⊥B = mv2 ⊥/rL ⇒rL = mv⊥ |q|B = 4.175 × 10−3 m . Tg = 2πm |q|B = 2.62323 × 10−8 s . (b) Interpretation and further calculation dK dt = q(v × B) · v = 0 . F · ˆB = 0 ⇒v∥is not stopped by a uniform magnetic field. Physical check Particles can stream along open field lines. Collisions, drifts and collective instabilities also affect confinement beyond the single-particle orbit.

Question 5

A magnetic field bends ion motion without supplying kinetic energy

A singly charged deuteron has mass 3.34×10−273.34\times10^{-27} kg and perpendicular speed 10610^6 m/s in uniform B=5.00 T. Use charge 1.60×10−191.60\times10^{-19} C and neglect collisions.

Diagram shown in the original SVG worksheet.

  1. Find gyro-radius and gyro-period.

  2. Show that the magnetic field does no work, and explain why a small orbit radius alone does not prove long-term plasma confinement.

Question 5 - Solution

A magnetic field bends ion motion without supplying kinetic energy

Diagram shown in the original SVG worksheet.

(a) Method and calculation

|q|v⟂B=mv⟂2/rL⇒rL=mv⟂|q|B=4.175×10−3m.|q|v_\perp B=mv_\perp^2/r_L\Rightarrow\boxed{r_L=\frac{mv_\perp}{|q|B}=4.175\times10^{-3}\,\mathrm m}.Tg=2πm|q|B=2.62323×10−8s.\boxed{T_g=\frac{2\pi m}{|q|B}=2.62323\times10^{-8}\,\mathrm s}.

(b) Interpretation and further calculation

dKdt=q(𝒗×𝑩)⋅𝒗=0.\boxed{\frac{dK}{dt}=q(\mathbf v\times\mathbf B)\cdot\mathbf v=0}.𝑭⋅𝑩̂=0⇒v∥ is not stopped by a uniform magnetic field.\mathbf F\cdot\hat{\mathbf B}=0\Rightarrow v_\parallel\text{ is not stopped by a uniform magnetic field}.

Physical check

Particles can stream along open field lines. Collisions, drifts and collective instabilities also affect confinement beyond the single-particle orbit.