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Question: Consider the following setup: 2 charges of same sign and magnitudes $q, Q$ are placed on the walls ...

Consider the following setup:

2 charges of same sign and magnitudes q,Qq, Q are placed on the walls of a parabola y=ax2,a>0y = ax^2, a > 0. Both charges have masses mm and are placed at a height of h1h_1 from the horizontal. If both particles are dropped from the heights at t=0t = 0, then derive the following:

(a) The function of position with time x1(t)x_1(t) and x2(t)x_2(t) (b) The energy equations of the system (c) the equilibrium distance between the 2 charges.

Answer

(a) x1(t)=x(t)x_1(t)=-x(t) and x2(t)=x(t)x_2(t)=x(t) with

m[(1+4a2x2)x¨+4a2xx˙2]=2mgax+kQq2x2,x(0)=h1/a,  x˙(0)=0.m\Bigl[(1+4a^2x^2)\ddot x+4a^2x\,\dot x^2\Bigr] = -2mga\,x+\frac{kQq}{2x^2},\quad x(0)=\sqrt{h_1/a},\; \dot x(0)=0.

(b) Total energy

E=12m[(1+4a2x12)x˙12+(1+4a2x22)x˙22]+mga(x12+x22)+kQqx2x1.E = \frac{1}{2}m\Bigl[(1+4a^2x_1^2)\dot x_1^2+(1+4a^2x_2^2)\dot x_2^2\Bigr] + mga\,(x_1^2+x_2^2)+\frac{kQq}{|x_2-x_1|}.

For symmetry,

E=m[12(1+4a2x2)x˙2+gax2]+kQq2x.E= m\left[\frac{1}{2}(1+4a^2x^2)\dot x^2+ga\,x^2\right]+\frac{kQq}{2x}.

(c) Equilibrium when

8mgax03=kQqx0=(kQq8mga)1/3,deq=2x0.8mga\,x_0^3 = kQq\quad\Longrightarrow\quad x_0=\left(\frac{kQq}{8mga}\right)^{1/3},\quad d_{eq}=2x_0.
Explanation

Solution

Overview:

This problem involves analyzing the motion of two charged particles constrained to move along a parabolic path under the influence of gravity and electrostatic repulsion. The solution involves:

  1. Parameterizing the motion along y=ax2y=ax^2 so that kinetic energy becomes 12m(1+4a2x2)x˙2\frac{1}{2}m(1+4a^2x^2)\dot x^2.
  2. Writing the potential energies: gravitational mgax2mga\,x^2 for each and Coulomb kQq/(2x)kQq/(2x) (since d=2xd=2x).
  3. Using Lagrange’s equations (or energy conservation) one obtains the differential equation for x(t)x(t); hence the positions x1(t)=x(t)x_1(t)=-x(t) and x2(t)=x(t)x_2(t)=x(t).
  4. Minimizing the potential energy U(x)=2mgax2+kQq2xU(x)=2mga\,x^2+\frac{kQq}{2x} with respect to xx yields the equilibrium position x0=(kQq/(8mga))1/3x_0=(kQq/(8mga))^{1/3} and so the equilibrium distance is deq=2x0d_{eq}=2x_0.

Detailed Steps:

Equations of Motion:

Because each particle is constrained to lie on the parabola y=ax2y=ax^2 the arc‐length is

s(x)=0x1+(y)2dx=0x1+(2ax)2dx=0x1+4a2x2dx.s(x)=\int_0^x\sqrt{1+(y')^2}\,dx=\int_0^x\sqrt{1+(2ax)^2}\,dx=\int_0^x\sqrt{1+4a^2x^2}\,dx.

Thus the velocity is

v=dsdt=1+4a2x2x˙.v=\frac{ds}{dt}=\sqrt{1+4a^2x^2}\,\dot x.

Hence the kinetic energy for a particle is

K=12m(1+4a2x2)x˙2.K=\frac{1}{2}m\Bigl(1+4a^2x^2\Bigr)\dot x^2.

Now, for the two particles (we label the left one “(m,Q)(m,Q)” and the right one “(m,q)(m,q)” with Q>qQ>q) the energy contributions are:

  1. Gravitational potential energy (using y=ax2y=ax^2) for each is Ug=mgax2.U_g=mga x^2.
  2. Their mutual Coulomb potential energy is Ue=kQqd,U_e=\frac{k\,Qq}{d}, where the distance between them is, when symmetric, d=(x2x1)2+(a(x22x12))2.d= \sqrt{(x_2-x_1)^2 + \Bigl(a(x_2^2-x_1^2)\Bigr)^2}. But for x1=x,x2=xx_1=-x,x_2=x we have x2x1=2xx_2-x_1=2x and x22x12=x2x2=0,x_2^2-x_1^2=x^2-x^2=0, so that d=2x.d=2|x|.

Thus the Coulomb energy is

Ue=kQq2x.U_e=\frac{kQq}{2|x|}.

A Lagrange–Newton treatment along the xx–coordinate leads to the equation of motion

mddt[1+4a2x2x˙]=ddx[mgax2+kQq2x].m\frac{d}{dt}\Bigl[\sqrt{1+4a^2x^2}\,\dot x\Bigr] = -\frac{d}{dx}\Bigl[mga\,x^2+\frac{kQq}{2|x|}\Bigr].

In explicit form one may write

m[(1+4a2x2)x¨+4a2xx˙2]=2mgax+kQq2x2,m\Bigl[(1+4a^2x^2)\ddot x+4a^2x\,\dot x^2\Bigr] = -2mga\,x+\frac{kQq}{2x^2},

where (for x>0x>0) we have dropped the absolute value. Then the positions of the two charges are

x1(t)=x(t),x2(t)=x(t),x_1(t)=-x(t),\qquad x_2(t)=x(t),

with the above differential equation governing x(t)x(t). (One may “solve” for tt in terms of xx by writing

t=x(0)x(t)1+4a2x22m[mga(x(0)2x2)+kQq2(1x1x(0))]dx,t = \int_{x(0)}^{x(t)} \frac{\sqrt{1+4a^2x^2}}{\sqrt{\frac{2}{m}\Bigl[\,mga\,(x(0)^2-x^2)+\frac{kQq}{2}\Bigl(\frac{1}{x} -\frac{1}{x(0)}\Bigr)\Bigr]}}\,dx,

where x(0)=h1/ax(0)=\sqrt{h_1/a}, the initial position along xx, since the particles are dropped from a height h1h_1 above xx-axis.)

Energy equations

The total energy of the two–particle system is conserved. For each particle the energy is

  • Kinetic: Ki=12m(1+4a2xi2)x˙i2,K_i=\frac{1}{2}m\Bigl(1+4a^2x_i^2\Bigr)\dot x_i^2,
  • Gravitational potential: Ug,i=mgaxi2.U_{g,i}=mga\,x_i^2.

Thus, if we write the energies for the two and add the Coulomb interaction, the conserved energy reads

E=12m[(1+4a2x12)x˙12+(1+4a2x22)x˙22]+mga(x12+x22)+kQqx2x1.E = \frac{1}{2}m\Bigl[(1+4a^2x_1^2)\dot x_1^2+(1+4a^2x_2^2)\dot x_2^2\Bigr] + mga\,(x_1^2+x_2^2)+\frac{kQq}{|x_2-x_1|}.

For the symmetric case x1=xx_1=-x and x2=xx_2=x this becomes

E=m[12(1+4a2x2)x˙2+gax2]+kQq2x.E = m\left[\frac{1}{2}\Bigl(1+4a^2x^2\Bigr)\dot x^2 +ga\, x^2\right] +\frac{kQq}{2|x|}\,.

Equilibrium distance

In equilibrium the forces along the tangent vanish. Equivalently the energy is minimized with respect to xx. For the symmetric case, the potential energy (of the system) is

U(x)=2mgax2+kQq2x(x>0).U(x)=2mga\,x^2+\frac{kQq}{2x}\quad (x>0).

Setting dUdx=0\frac{dU}{dx}=0 we get

dUdx=4mgaxkQq2x2=0.\frac{dU}{dx} = 4mga\,x - \frac{kQq}{2x^2}=0.

Thus,

4mgax=kQq2x28mgax3=kQq.4mga\,x = \frac{kQq}{2x^2}\quad\Longrightarrow\quad 8mga\,x^3=kQq.

Therefore,

x0=(kQq8mga) ⁣1/3.x_0=\Bigl(\frac{kQq}{8mga}\Bigr)^{\!1/3}.

Since the charges are separated by a horizontal distance of 2x2x, the equilibrium distance is

deq=2x0=2(kQq8mga) ⁣1/3.d_{eq}=2x_0=2\Bigl(\frac{kQq}{8mga}\Bigr)^{\!1/3}\,.