In physics, magnetic pressure is an energy density associated with a magnetic field. In SI units, the energy density
PB
B
PB=
| B2 | |
| 2\mu0 |
\mu0
Any magnetic field has an associated magnetic pressure contained by the boundary conditions on the field. It is identical to any other physical pressure except that it is carried by the magnetic field rather than (in the case of a gas) by the kinetic energy of gas molecules. A gradient in field strength causes a force due to the magnetic pressure gradient called the magnetic pressure force.
In SI units, the magnetic pressure
PB
B
PB=
| B2 | |
| 2\mu0 |
\mu0
PB
v
J
\rho
B
p
| \rho\left( | \partial |
| \partialt |
+v ⋅ \nabla\right)v=J x B-\nablap,
\mu0J=\nabla x B
\tfrac12\nabla(B ⋅ B)=(B ⋅ \nabla)B+B x (\nabla x B)
J x B={(B ⋅ \nabla)B\over\mu0}-\nabla\left(
| B2 | |
| 2\mu0 |
\right),
Magnetic tension and pressure are both implicitly included in the Maxwell stress tensor. Terms representing these two forces are present along the main diagonal where they act on differential area elements normal to the corresponding axis.
The magnetic pressure force is readily observed in an unsupported loop of wire. If an electric current passes through the loop, the wire serves as an electromagnet, such that the magnetic field strength inside the loop is much greater than the field strength just outside the loop. This gradient in field strength gives rise to a magnetic pressure force that tends to stretch the wire uniformly outward. If enough current travels through the wire, the loop of wire will form a circle. At even higher currents, the magnetic pressure can create tensile stress that exceeds the tensile strength of the wire, causing it to fracture, or even explosively fragment. Thus, management of magnetic pressure is a significant challenge in the design of ultrastrong electromagnets.
The force (in cgs) exerted on a coil by its own current is[3]
F=\dfrac{I2}{c2R}\left[ln\left(\dfrac{8R}{a}\right)-1+Y\right]
where Y is the internal inductance of the coil, defined by the distribution of current. Y is 0 for high frequency currents carried mostly by the outer surface of the conductor, and 0.25 for DC currents distributed evenly throughout the conductor. See inductance for more information.
Interplay between magnetic pressure and ordinary gas pressure is important to magnetohydrodynamics and plasma physics. Magnetic pressure can also be used to propel projectiles; this is the operating principle of a railgun.
See main article: Force-free magnetic field. When all electric currents present in a conducting fluid are parallel to the magnetic field, the magnetic pressure gradient and magnetic tension force are balanced, and the Lorentz force vanishes. If non-magnetic forces are also neglected, the field configuration is referred to as force-free. Furthermore, if the current density is zero, the magnetic field is the gradient of a magnetic scalar potential, and the field is subsequently referred to as potential.