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    Current Subject
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    Applied Physics
    GE-169
    Progress0 / 45 topics
    Topics
    1. Electric Force and Its Applications2. Conservation of Charge3. Charge Quantization4. Electric Fields Due to Point Charge and Lines of Force5. Electric Fields: Ring of Charge and Disk of Charge6. A Point Charge in an Electric Field7. Dipole in an Electric Field8. Flux of a Vector Field9. Flux of an Electric Field10. Gauss’ Law and Its Applications11. Spherically Symmetric Charge Distribution12. Charge Isolated Conductor13. Electric Potential Energy14. Electric Potentials and Related Problems15. Calculating Potential from the Field16. Potential Due to Point and Continuous Charge Distribution17. Potential Due to a Dipole18. Equipotential Surfaces19. Calculating the Field from the Potential20. Electric Current and Current Density21. Resistance, Resistivity, and Conductivity22. Ohm's Law and Its Applications23. The Hall Effect24. Magnetic Force on a Current25. The Biot-Savart Law26. Line of Magnetic Field (B)27. Two Parallel Conductors28. Ampere's Law29. Solenoids and Toroids30. Faraday's Experiments and Law of Induction31. Lenz's Law32. Motional EMF33. Induced Electric Fields34. The Basic Equations of Electromagnetism35. Induced Magnetic Fields36. The Displacement Current37. Reflection and Refraction of Light Waves38. Total Internal Reflection39. Two Source Interference40. Double-Slit Interference and Related Problems41. Interference from Thin Films42. Diffraction and Wave Theory43. Single-Slit Diffraction and Related Problems44. Polarization of Electromagnetic Waves45. Polarizing Sheets and Related Problems
    GE-169›Electric Potentials and Related Problems
    Applied PhysicsTopic 14 of 45

    Electric Potentials and Related Problems

    13 minread
    2,173words
    Intermediatelevel

    Electric Potentials and Related Problems

    1. Definition of Electric Potential

    Electric potential (also known as electric potential energy per unit charge) is a scalar quantity that represents the electric potential energy a unit charge would have at a specific point in space due to the presence of other charges or electric fields. It is often denoted by VVV and is defined as:

    V=UqV = \frac{U}{q}V=qU​

    Where:

    • UUU is the electric potential energy,
    • qqq is the charge.

    The electric potential at a point is the amount of work done by an external force in bringing a unit positive charge from infinity (where potential is defined as zero) to that point, without causing any acceleration.


    2. Electric Potential Due to Point Charge

    The electric potential VVV due to a point charge QQQ at a distance rrr from the charge is given by:

    V=keQrV = \frac{k_e Q}{r}V=rke​Q​

    Where:

    • ke=8.99×109 N\cdotpm2/C2k_e = 8.99 \times 10^9 \, \text{N·m}^2/\text{C}^2ke​=8.99×109N\cdotpm2/C2 is Coulomb's constant,

    • QQQ is the source charge,

    • rrr is the distance from the charge to the point where the potential is being calculated.

    • The electric potential due to a positive charge is positive and decreases as rrr increases.

    • The electric potential due to a negative charge is negative and increases as rrr increases.

    This formula assumes that the electric potential at infinity is zero.


    3. Electric Potential Due to Multiple Point Charges

    For a system of point charges, the total electric potential at a point is the algebraic sum of the potentials due to each individual charge. Since electric potential is a scalar quantity, it simply adds up:

    Vtotal=∑i=1nkeqiriV_{\text{total}} = \sum_{i=1}^n \frac{k_e q_i}{r_i}Vtotal​=i=1∑n​ri​ke​qi​​

    Where:

    • qiq_iqi​ is the iii-th charge,
    • rir_iri​ is the distance from the iii-th charge to the point where the potential is being calculated.

    This formula is valid because electric potential is a scalar, unlike electric fields which are vector quantities.


    4. Relation Between Electric Field and Electric Potential

    The electric field E\mathbf{E}E and the electric potential VVV are closely related. The electric field is the negative gradient of the electric potential, meaning that the electric field points in the direction of greatest decrease of electric potential, and its magnitude is the rate of change of potential with distance. Mathematically:

    E=−∇V\mathbf{E} = -\nabla VE=−∇V

    In one-dimensional problems (along a straight line), this relationship simplifies to:

    E=−dVdxE = -\frac{dV}{dx}E=−dxdV​

    Where:

    • EEE is the electric field in a given direction,
    • dVdx\frac{dV}{dx}dxdV​ is the rate of change of potential with respect to distance.

    This equation shows that the electric field is the spatial rate of change of the electric potential. If the potential decreases in the direction of the field, the electric field points in that direction.


    5. Equipotential Surfaces

    An equipotential surface is a surface on which the electric potential is constant. No work is required to move a charge along an equipotential surface because there is no change in potential energy.

    Key points about equipotential surfaces:

    • The electric field is always perpendicular to an equipotential surface.
    • No component of the electric field acts along the surface, so moving a charge along an equipotential does not do work.
    • Equipotential surfaces are often drawn as spheres around a point charge, and the spacing between these surfaces increases with distance from the charge.

    For example, around a point charge, the equipotential surfaces are concentric spheres centered at the charge.


    6. Electric Potential Energy and Potential Difference

    The potential difference VABV_{\text{AB}}VAB​ between two points AAA and BBB in an electric field is the work done by the electric field in moving a unit positive charge from AAA to BBB. It is given by:

    VAB=VB−VA=−∫ABE⋅drV_{\text{AB}} = V_B - V_A = - \int_A^B \mathbf{E} \cdot d\mathbf{r}VAB​=VB​−VA​=−∫AB​E⋅dr

    Where:

    • VBV_BVB​ and VAV_AVA​ are the electric potentials at points BBB and AAA,
    • E\mathbf{E}E is the electric field vector,
    • drd\mathbf{r}dr is the differential displacement vector along the path from AAA to BBB.

    The potential difference is independent of the path taken (it depends only on the initial and final points), making it a conservative quantity. This is a result of the fact that electric forces are conservative.


    7. Potential Energy in an Electric Field

    The potential energy UUU of a charge qqq at a point in an electric field with potential VVV is:

    U=qVU = qVU=qV

    For example, for a point charge QQQ in the electric field due to another charge, the potential energy of a test charge qqq placed at a distance rrr from QQQ is:

    U=q⋅keQrU = q \cdot \frac{k_e Q}{r}U=q⋅rke​Q​

    This formula represents the energy stored in the electric field due to the interaction between the two charges.


    8. Electric Potential Energy of a Dipole in an Electric Field

    A dipole consists of two charges of equal magnitude but opposite sign, separated by a fixed distance. The electric potential energy of a dipole p\mathbf{p}p in an external electric field E\mathbf{E}E is given by:

    U=−p⋅EU = -\mathbf{p} \cdot \mathbf{E}U=−p⋅E

    Where:

    • p=qd\mathbf{p} = q \mathbf{d}p=qd is the dipole moment, with qqq being the magnitude of each charge and d\mathbf{d}d the separation vector between the charges,
    • E\mathbf{E}E is the external electric field.

    The potential energy is minimized when the dipole is aligned with the electric field, i.e., when p∥E\mathbf{p} \parallel \mathbf{E}p∥E.


    9. Problems Involving Electric Potentials

    Problem 1: Electric Potential Due to a Point Charge

    Problem: What is the electric potential at a point 2 meters away from a charge of +5 μC+5 \, \mu C+5μC?

    Solution:

    The formula for the electric potential due to a point charge is:

    V=keQrV = \frac{k_e Q}{r}V=rke​Q​

    Where:

    • ke=8.99×109 N\cdotpm2/C2k_e = 8.99 \times 10^9 \, \text{N·m}^2/\text{C}^2ke​=8.99×109N\cdotpm2/C2,
    • Q=5×10−6 CQ = 5 \times 10^{-6} \, \text{C}Q=5×10−6C,
    • r=2 mr = 2 \, \text{m}r=2m.

    Substituting the values:

    V=(8.99×109)(5×10−6)2V = \frac{(8.99 \times 10^9)(5 \times 10^{-6})}{2}V=2(8.99×109)(5×10−6)​ V=22,475 VV = 22,475 \, \text{V}V=22,475V

    So, the electric potential at the point is 22,475 V.


    Problem 2: Electric Potential Due to Multiple Charges

    Problem: Two point charges Q1=+3 μCQ_1 = +3 \, \mu CQ1​=+3μC and Q2=−2 μCQ_2 = -2 \, \mu CQ2​=−2μC are placed 1 meter apart. What is the electric potential at a point halfway between them?

    Solution:

    The electric potential at a point due to multiple charges is the sum of the potentials due to each charge. At the midpoint, the distance from each charge is r=0.5 mr = 0.5 \, \text{m}r=0.5m.

    The total potential at the midpoint is:

    Vtotal=keQ1r+keQ2rV_{\text{total}} = \frac{k_e Q_1}{r} + \frac{k_e Q_2}{r}Vtotal​=rke​Q1​​+rke​Q2​​

    Substitute the values:

    Vtotal=(8.99×109)(3×10−6)0.5+(8.99×109)(−2×10−6)0.5V_{\text{total}} = \frac{(8.99 \times 10^9)(3 \times 10^{-6})}{0.5} + \frac{(8.99 \times 10^9)(-2 \times 10^{-6})}{0.5}Vtotal​=0.5(8.99×109)(3×10−6)​+0.5(8.99×109)(−2×10−6)​ Vtotal=53,940 V−35,960 VV_{\text{total}} = 53,940 \, \text{V} - 35,960 \, \text{V}Vtotal​=53,940V−35,960V Vtotal=17,980 VV_{\text{total}} = 17,980 \, \text{V}Vtotal​=17,980V

    So, the electric potential at the midpoint is 17,980 V.


    Problem 3: Potential Energy of a System of Charges

    Problem: What is the total electric potential energy of a system of two charges, q1=2 μCq_1 = 2 \, \mu Cq1​=2μC and q2=−3 μCq_2 = -3 \, \mu Cq2​=−3μC, separated by a distance of 0.1 m?

    Solution:

    The potential energy UUU of a system of two point charges is given by:

    U=keq1q2rU = \frac{k_e q_1 q_2}{r}U=rke​q1​q2​​

    Substitute the given values:

    U=(8.99×109)(2×10−6)(−3×10−6)0.1U = \frac{(8.99 \times 10^9)(2 \times 10^{-6})(-3 \times 10^{-6})}{0.1}U=0.1(8.99×109)(2×10−6)(−3×10−6)​ U=−539.4 JU = -539.4 \, \text{J}U=−539.4J

    So, the total electric potential energy of the system is -539.4 J.


    Summary of Key Concepts

    1. Electric Potential (VVV) is the energy per unit charge at a point in space.
    2. The electric potential due to a point charge is V=keQrV = \frac{k_e Q}{r}V=rke​Q​.
    3. The electric potential at a point due to multiple charges is the algebraic sum of the potentials due to each individual charge.
    4. The electric field is related to the potential by E=−∇V\mathbf{E} = -\nabla VE=−∇V, or E=−dVdxE = -\frac{dV}{dx}E=−dxdV​.
    5. Equipotential surfaces are surfaces of constant electric potential, and no work is done in moving a charge along such a surface.
    6. Potential energy is the work done in assembling a system of charges, and the potential energy of a charge in a field is U=qVU = qVU=qV.
    7. Potential energy of a dipole in an external electric field is given by U=−p⋅EU = -\mathbf{p} \cdot \mathbf{E}U=−p⋅E.

    Electric potential plays a crucial role in understanding electrostatics and energy storage in electric fields. The related problems test understanding of concepts such as potential due to point charges, potential difference, and potential energy in various configurations.

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    Calculating Potential from the Field

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