The Differential Form of Ampere's Law: Difference between revisions
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==Curl== | ==Curl== | ||
To have a model that is consistent with the theory of relativity, the property of a magnetic field called the "curl" must be utilized. The curl is the path integral of magnetic field per unit area, in the limit as the area goes to zero. This is useful because its value is proportional to the current density at the same location and time so there is an established relationship. | To have a model that is consistent with the theory of relativity, the property of a magnetic field called the "curl" must be utilized. The curl is the path integral of magnetic field per unit area, in the limit as the area goes to zero. This is useful because its value is proportional to the current density at the same location and time so there is an established relationship. This is known as a local relationship because both are evaluated at the same place and time, making it relativisticly correct because it isn't effected by relativistic retardation. | ||
===A Mathematical Model=== | |||
Definition of curl: | |||
[[File:Example.jpg]] | |||
===A Computational Model=== | ===A Computational Model=== | ||
Revision as of 21:26, 5 December 2015
Many physical laws taught in Physics I and II are only correct at non-relativistic speeds (where the speed is much less than the speed of light). This is caused by relativistic retardation, a term for how changes in magnetic and electric fields propagate at the speed of light so they cannot be measured instantly. Typically this is not an issue if the particles are moving much slower than the speed of light because although these physical laws are technically incorrect, the margin of error is so small that it is irrelevant. As particles approach speeds close to the speed of light these differences can become significant and methods for finding electric or magnetic fields (such as the Biot-Savart law) are no longer accurate. This is not true for Ampere's Law which makes it useful for problems involving particles moving at near light speeds.
Curl
To have a model that is consistent with the theory of relativity, the property of a magnetic field called the "curl" must be utilized. The curl is the path integral of magnetic field per unit area, in the limit as the area goes to zero. This is useful because its value is proportional to the current density at the same location and time so there is an established relationship. This is known as a local relationship because both are evaluated at the same place and time, making it relativisticly correct because it isn't effected by relativistic retardation.
A Mathematical Model
Definition of curl:
A Computational Model
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