1 Electric Charge and Fields
Progresses from electric charge and Coulomb’s law to electric fields, flux, and Gauss’s law, showing how these ideas describe and calculate electric interactions.
Charge and its basic properties
is a property of matter with two forms: positive and negative. Like charges repel, while unlike charges attract. A proton has charge , and an electron has charge , where the elementary charge has magnitude approximately . Charge is quantized, so an object’s net charge is an integer multiple of . In ordinary charging, electrons transfer between objects; the total charge of an isolated system remains constant.
These properties set up two central questions: what force do charges exert on one another, and how can their influence be described at locations in space?
Force between charges
For two stationary point charges separated by a distance , gives the force magnitude:
The force grows with the magnitude of either charge and decreases with the square of the separation. It acts along the line joining the charges: like signs repel, and opposite signs attract.
For example, charges of and , separated by , exert a force with magnitude
Because the charges have opposite signs, the force is attractive. With several source charges, calculate each force as a vector and add the vectors; adding magnitudes alone would lose directional information.
and superposition
An describes the force a source charge would exert per unit positive test charge. The field and the force on a test charge are related by
The field is measured in newtons per coulomb. Its direction is defined by the force on a positive test charge: field lines point away from positive charges and toward negative charges.
For a point source charge , the field at distance is
where points from the source to the field point. A positive source produces an outward field; a negative source produces an inward field.
The says that fields from multiple charges add vectorially. For a continuous charge distribution, the contributions can be summed by integration. For example, a point charge produces a field of magnitude approximately at a distance of , directed outward.
Takeaway: calculates forces between charges; the describes the influence of source charges at each point in space.
through surfaces
measures how much field passes through a surface. For a flat surface in a uniform field,
where is the surface area and is the angle between the field and the area vector. The area vector is perpendicular to the surface. Flux is greatest when the field points along this vector, so it crosses the surface perpendicularly; flux is zero when the field is parallel to the surface.
For a curved surface or a field that varies across the surface, add the contributions over the surface:
For a closed surface, the area vectors point outward and the integral uses a closed-surface symbol. Flux is measured in .
For example, a uniform field of crossing a flat surface of area at an angle of to its area vector gives
and symmetry
connects the net flux through any closed surface to the net charge enclosed:
Only the net enclosed charge determines the total flux. Charges outside the surface may affect the field at points on it, but they do not change the net flux through it.
A is an imaginary closed surface chosen to help analyze a charge distribution. is always valid, but it is especially useful for finding the field when the distribution has enough symmetry—typically spherical, cylindrical, or planar symmetry—to simplify the field over the chosen surface.
For a point charge , choose a spherical of radius . Symmetry makes the field radial and equal in magnitude everywhere on the sphere, so
This recovers the point-charge field. In general, match the to the symmetry, determine the enclosed charge, and use the flux integral to solve for the field.
Takeaway: always relates closed-surface flux to enclosed charge; symmetry often makes it a practical tool for calculating fields.