Derive coulomb's law from gauss's law

Collegedunia Team logo

Collegedunia Team

Content Curator

According to gauss's law, the total electric flux (ϕ) through any close surface in free space is equal to 1/∈0 times the total electric charge (q) enclosed by the surface.

Derive coulombs law from gausss law que phy

Mathematically,

\(\phi = \oint _S \overrightarrow{E} . \overrightarrow{ds} = \frac{q}{ \in _0}\)

According to coulomb’s law, the magnitude of the force of attraction and repulsion between any two point charges at rest is directly proportional to the product of the magnitude of charges and inversely proportional to the square of the distance between them.

Mathematically, it is given by:

\(F=k \frac{q_1q_2}{r_2}\)

Derivation of coulomb’s law from gauss’s law

Consider two point charges q1 and q2 are separated by distance r in a vacuum.

Derivation of coulomb’s law from gauss’s law

Let E be the magnitude of the electric field at distance r from charge q1. Therefore, the force(F) experienced by charge q2 due to electric field(E) is given by:

F = q2E …(i)

Draw a gaussian surface of radius r taking the center as the location of charge q1.

The intensity of the electric field is constant at every point of this surface.

The intensity of the electric field is constant at every point of this surface.

According to gauss’s law, the net electric flux through this surface is given by

\(\oint _S \overrightarrow{E} . \overrightarrow{ds} = \frac{q_1}{ \in _0}\)

\(\oint _S\) Eds cosθ = \(\frac{q_1}{ \in _0}\)

Direction of the electric field is always perpendicular to the surface. So, the angle between E and ds is 0.

\(\oint _S\)Eds cos0 = \(\frac{q_1}{ \in _0}\)

\(\oint _S\) Eds = \(\frac{q_1}{ \in _0}\)

Since the electric field is constant at every point of the gaussian surface, therefore we can write

\(\oint _S\) ds = \(\frac{q_1}{ \in _0}\)

But, \(\oint _S\) ds = 4πr2 is the surface area of sphere

⇒ E x 4πr= \(\frac{q_1}{ \in _0}\)

Using equation (i), we get

\(\frac{F}{q_2}\) x 4πr2  = \(\frac{q_1}{ \in _0}\)

⇒ F = \(\frac{1}{4 \pi \in _o} \frac{q_1q_2}{r_2}\)


Also Read:

CBSE CLASS XII Related Questions

  • 1.
    Two heaters rated as \((P_1,V)\) and \((P_2,V)\) are connected in series across a dc source of \(V/2\) volt. The power consumed by the combination will be –

      • \((P_1+P_2)\)
      • \(\dfrac{P_1+P_2}{2}\)
      • \(\dfrac{P_1P_2}{2(P_1+P_2)}\)
      • \(\dfrac{P_1P_2}{4(P_1+P_2)}\)

    • 2.
      Two small identical metallic balls having charges \( q \) and \( -2q \) are kept far at a separation \( r \). They are brought in contact and then separated at distance \( \frac{r}{2} \). Compared to the initial force \( F \), they will now:

        • attract with a force \( \frac{F}{2} \)
        • repel with a force \( \frac{F}{2} \)
        • repel with a force \( F \)
        • attract with a force \( F \)

      • 3.
        If Bohr’s quantization postulate (angular momentum \( = \frac{nh}{2\pi} \)) is a basic law of nature, it should be equally valid for the case of planetary motion also. Why, then, do we never speak of quantization of orbits of planets around the Sun? Explain.


          • 4.
            A light copper ring is freely suspended by a light string. A bar magnet is held horizontally with its length along the axis of the ring. The magnet is moved towards the ring with its N pole facing the loop. What will happen to the ring and its position? Explain.


              • 5.
                If both the number of protons and the neutrons are conserved in each nuclear reaction, in what way is mass converted into energy (or vice versa) in a nuclear reaction? Explain.


                  • 6.
                    Photoemission of electrons occurs from a metal (\( \phi_0 = 1.96 \, \text{eV} \)) when light of frequency \( 6.4 \times 10^{14} \, \text{Hz} \) is incident on it. Calculate: Energy of a photon in the incident light, The maximum kinetic energy of the emitted electrons, and The stopping potential.

                      CBSE CLASS XII Previous Year Papers

                      Comments


                      No Comments To Show