Elastic Collisions, Protons, and Electric Potential of Rings and Disks

Elastic Collision and Closest Approach of Two Protons

  • Problem Description:

    • Two protons travel directly towards each other and collide head-on in a perfectly elastic manner.

    • Initial State (t0t_0): The protons are infinitely far apart, heading directly at one another.

    • Final State (tyt_y): After the interaction, they move away and end up infinitely far apart again.

    • Goal: Determine the final velocities of the two protons when far apart and calculate their minimum separation distance (rminr_{min}).

  • System Parameters and Physical Constants:

    • Mass of Proton (mpm_p): 1.67×10−27 kg1.67 \times 10^{-27}\,\text{kg}.

    • Charge of Proton (qpq_p): 1.609×10−19 C1.609 \times 10^{-19}\,\text{C} (also noted as 1.602×10−19 C1.602 \times 10^{-19}\,\text{C} in calculation steps).

    • Initial Velocity of Proton A (vA1v_{A1}): 1.98×104 m/si^1.98 \times 10^4\,\text{m/s} \hat{i}.

    • Initial Velocity of Proton B (vB1v_{B1}): −8.62×104 m/si^-8.62 \times 10^4\,\text{m/s} \hat{i}.

    • Coulomb Constant (kk): 8.99×109 N m2 C−28.99 \times 10^9\,\text{N}\,\text{m}^2\,\text{C}^{-2}.

  • Conservation Principles:

    • Linear Momentum: The system consists of two protons with no external forces. Gravity is explicitly identified as being too weak to have a measurable effect.

    • Equation: mpvA1+mpvB1=mpvA4+mpvB4m_p v_{A1} + m_p v_{B1} = m_p v_{A4} + m_p v_{B4}.

    • Simplified (since masses cancel): vA1+vB1=vA4+vB4v_{A1} + v_{B1} = v_{A4} + v_{B4}.

    • Total Energy: Since it is an elastic collision, kinetic energy (KK) and potential energy (UU) are conserved.

    • Initial energy is purely kinetic (U≈0U \approx 0 at infinity).

  • Part (a): Final Velocities (vA4,vB4v_{A4}, v_{B4}):

    • Step 1: Momentum Conservation:

    • 1.98×104+(−8.62×104)=vA4+vB41.98 \times 10^4 + (-8.62 \times 10^4) = v_{A4} + v_{B4}

    • −6.64×104 m/s=vA4+vB4-6.64 \times 10^4\,\text{m/s} = v_{A4} + v_{B4}

    • Expression for vA4v_{A4}: vA4=−6.64×104−vB4v_{A4} = -6.64 \times 10^4 - v_{B4}.

    • Step 2: Kinetic Energy Conservation:

    • 12mp(vA1)2+12mp(vB1)2=12mp(vA4)2+12mp(vB4)2\frac{1}{2} m_p (v_{A1})^2 + \frac{1}{2} m_p (v_{B1})^2 = \frac{1}{2} m_p (v_{A4})^2 + \frac{1}{2} m_p (v_{B4})^2

    • (1.98×104)2+(−8.62×104)2=(vA4)2+(vB4)2(1.98 \times 10^4)^2 + (-8.62 \times 10^4)^2 = (v_{A4})^2 + (v_{B4})^2

    • 3.92×108+74.30×108=7.82×109 m2 s−2=(vA4)2+(vB4)23.92 \times 10^8 + 74.30 \times 10^8 = 7.82 \times 10^9\,\text{m}^2\,\text{s}^{-2} = (v_{A4})^2 + (v_{B4})^2.

    • Step 3: Solving the Quadratic System:

    • Substitute vA4v_{A4} into the energy equation:

    • 7.82×109=(−6.64×104−vB4)2+(vB4)27.82 \times 10^9 = (-6.64 \times 10^4 - v_{B4})^2 + (v_{B4})^2

    • 7.82×109=4.41×109+1.328×105vB4+vB42+vB427.82 \times 10^9 = 4.41 \times 10^9 + 1.328 \times 10^5 v_{B4} + v_{B4}^2 + v_{B4}^2

    • 2vB42+1.328×105vB4−3.41×109=02 v_{B4}^2 + 1.328 \times 10^5 v_{B4} - 3.41 \times 10^9 = 0.

    • Step 4: Results:

    • Solving the quadratic provides two solutions: the initial velocities and the final swapped velocities.

    • Final Velocity Proton A (vA4v_{A4}): −8.62×104 m/s-8.62 \times 10^4\,\text{m/s}.

    • Final Velocity Proton B (vB4v_{B4}): 1.98×104 m/s1.98 \times 10^4\,\text{m/s}.

  • Part (b): Minimum Separation (rminr_{min}):

    • Condition for Closest Approach: This occurs when the relative velocity is zero. At time t2t_2, both protons travel at the same velocity (vAz=vBz=vzv_{Az} = v_{Bz} = v_z).

    • Calculating vzv_z:

    • Using momentum: mp(vA1+vB1)=(mp+mp)vzm_p (v_{A1} + v_{B1}) = (m_p + m_p) v_z

    • vz=−6.64×1042=−3.32×104 m/sv_z = \frac{-6.64 \times 10^4}{2} = -3.32 \times 10^4\,\text{m/s}.

    • Energy Balance at Closest Approach:

    • Kinitial=Kt2+Ut2K_{initial} = K_{t2} + U_{t2}

    • Kinitial=6.53×10−18 JK_{initial} = 6.53 \times 10^{-18}\,\text{J} (Calculated as 3.27×10−19+6.204×10−183.27 \times 10^{-19} + 6.204 \times 10^{-18}).

    • Kinetic Energy at t2t_2 (Kt2K_{t2}): 12(2mp)(vz)2=(1.67×10−27)(−3.32×104)2=1.84×10−18 J\frac{1}{2}(2 m_p)(v_z)^2 = (1.67 \times 10^{-27})(-3.32 \times 10^4)^2 = 1.84 \times 10^{-18}\,\text{J}.

    • Potential Energy at t2t_2 (Ut2U_{t2}): kqp2rmin=(8.99×109)(1.602×10−19)2rmin\frac{k q_p^2}{r_{min}} = \frac{(8.99 \times 10^9)(1.602 \times 10^{-19})^2}{r_{min}}.

    • Solving for rminr_{min}:

    • 6.53×10−18=1.84×10−18+2.31×10−28rmin6.53 \times 10^{-18} = 1.84 \times 10^{-18} + \frac{2.31 \times 10^{-28}}{r_{min}}

    • 4.69×10−18=2.31×10−28rmin4.69 \times 10^{-18} = \frac{2.31 \times 10^{-28}}{r_{min}}

    • rmin=4.92×10−11 mr_{min} = 4.92 \times 10^{-11}\,\text{m}.

Electric Potential of a Uniformly Charged Ring

  • Problem Setup:

    • A ring of radius RR carries a total charge QQ.

    • The ring is centered at the origin in the x−yx-y plane.

    • Field Point (PP): Located at (0,0,z0)(0, 0, z_0) on the zz-axis.

  • Symmetry Analysis:

    • The electric potential (VV) is NOT expected to be zero.

    • For V=0V=0 due to symmetry, the field point must be halfway between identical shapes with equal magnitude of charge but opposite signs.

  • Derivation Process:

    • Identify Charge Element (dqdq): The charge is 1D, so break it into points along the ring.

    • dq=λds=Qds2πRdq = \lambda ds = Q \frac{ds}{2\pi R}.

    • In polar coordinates: ds=Rdθds = R d\theta, so dq=Q2πdθdq = \frac{Q}{2\pi} d\theta.

    • Distance (rr): The distance from any point (x,y,0)(x, y, 0) on the ring to point P(0,0,z0)P(0, 0, z_0).

    • vector r=(0−x)i+(0−y)j+(z0−0)k\mathbf{r} = (0-x)\mathbf{i} + (0-y)\mathbf{j} + (z_0-0)\mathbf{k}.

    • magnitude ∣r∣=x2+y2+z02|r| = \sqrt{x^2 + y^2 + z_0^2}.

    • Since x2+y2=R2x^2 + y^2 = R^2 on the ring, r=R2+z02r = \sqrt{R^2 + z_0^2}.

    • Integration:

    • dV=kdqr=k(Q/2π)dθR2+z02dV = \frac{k dq}{r} = \frac{k (Q / 2\pi) d\theta}{\sqrt{R^2 + z_0^2}}

    • V=∫02πkQ2πR2+z02dθV = \int_0^{2\pi} \frac{k Q}{2\pi \sqrt{R^2 + z_0^2}} d\theta

    • V=kQ2πR2+z02[θ]02π=kQR2+z2V = \frac{k Q}{2\pi \sqrt{R^2 + z_0^2}} [\theta]_0^{2\pi} = \frac{k Q}{\sqrt{R^2 + z^2}}.

  • Verification and Limits:

    • Point Charge Limit: If z≫Rz \gg R, the denominator R2+z2≈z\sqrt{R^2 + z^2} \approx z.

    • Result: V≈kQzV \approx \frac{k Q}{z}, which is the potential of a point charge at distance zz.

    • Electric Field Check: The field EzE_z can be derived from the negative derivative of the potential.

    • Ez=−dVdz=−kQddz(R2+z2)−1/2E_z = -\frac{dV}{dz} = -kQ \frac{d}{dz} (R^2 + z^2)^{-1/2}

    • Ez=−kQ[−12(R2+z2)−3/2(2z)]=kQz(R2+z2)3/2E_z = -kQ [-\frac{1}{2}(R^2 + z^2)^{-3/2}(2z)] = \frac{k Q z}{(R^2 + z^2)^{3/2}}.

    • This matches the expected electric field formula derived in previous classes.

Electric Potential of a Uniformly Charged Disk

  • Problem Setup:

    • A flat disk of radius RR carries a total charge QQ uniformly distributed over its area.

    • The disk is centered at the origin in the x−yx-y plane.

    • Goal: Find the potential at point P(0,0,z0)P(0, 0, z_0).

  • Method: Summation of Rings:

    • A disk is treated as a collection of thin rings with radius rr and thickness drdr.

    • Area Element (dAdA): dA=2πrdrdA = 2\pi r dr.

    • Charge Element (dqdq): Based on the fraction of the total area.

    • dq=Q(dAAtotal)=Q2πrdrπR2=2QrdrR2dq = Q \left( \frac{dA}{A_{total}} \right) = Q \frac{2\pi r dr}{\pi R^2} = \frac{2Q r dr}{R^2}.

  • Integration:

    • Using the potential formula for a single ring from the previous section: dV=kdqr2+z2dV = \frac{k dq}{\sqrt{r^2 + z^2}}.

    • dV=k(2Qrdr/R2)r2+z2dV = \frac{k (2Q r dr / R^2)}{\sqrt{r^2 + z^2}}.

    • Integrate from r=0r=0 to r=Rr=R:

    • V=2kQR2∫0Rrdrr2+z2V = \frac{2kQ}{R^2} \int_0^R \frac{r dr}{\sqrt{r^2 + z^2}}.

    • Substitution: Let u=r2+z2u = r^2 + z^2, then du=2rdrdu = 2r dr.

    • V=2kQR2[r2+z2]0RV = \frac{2kQ}{R^2} [\sqrt{r^2 + z^2}]_0^R

    • Final Formula: V=2kQR2(R2+z2−z)V = \frac{2kQ}{R^2} (\sqrt{R^{2} + z^{2}} - z).

  • Verification against Electric Field:

    • The electric field EzE_z is the negative derivative of the potential with respect to zz:

    • E=−dVdz=−2kQR2ddz[(R2+z2)1/2−z]E = -\frac{dV}{dz} = -\frac{2kQ}{R^2} \frac{d}{dz} [ (R^2 + z^2)^{1/2} - z ]

    • E=−2kQR2[12(R2+z2)−1/2(2z)−1]E = -\frac{2kQ}{R^2} [ \frac{1}{2}(R^2 + z^2)^{-1/2}(2z) - 1 ]

    • E=2kQR2[1−zR2+z2]E = \frac{2kQ}{R^2} [ 1 - \frac{z}{\sqrt{R^2 + z^2}} ].

    • This reproduces the established formula for the electric field of a charged disk.

Questions & Discussion

  • Q: Why do we use tyt_y and tzt_z?

    • A: These time steps represent specific phases of the interaction. t0t_0 is the start (infinite distance), t1t_1 is just before interaction, t2t_2 is the point of closest approach (velocities equalized), and tyt_y is the reprise of the infinite distance state after the collision.

  • Q: Is gravity included?

    • A: No, the transcript explicitly states gravity is too weak to have any effect in the context of these proton-proton interactions.

  • Q: How do we handle symmetry in potential vs. field?

    • A: Potential is a scalar, so we do not need to calculate vector components. However, symmetry is still useful to determine if the potential might be zero. For the ring and disk, the potential remains non-zero on the zz-axis because all charge elements are at the same distance and have the same sign.