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Magnetic field

In electromagnetism, magnetic field is a physical property of space that quantifies the magnetic strength at a given location. Magnetic fields deflect moving electric charges, apply torques on magnets to twist them in the direction of the magnetic field, and attract or repel magnets and magnetic material such as iron. In addition, a time varying magnetic field induces electrical currents.

Interactions with electric currents and moving electric charges
Currents of electric charges both generate a magnetic field and feel a force due to magnetic B-fields. Force on moving charges and current Magnetic force on a charged particle . A charged particle moving in a -field experiences a sideways force that is proportional to the strength of the magnetic field, the component of the velocity that is perpendicular to the magnetic field and the charge of the particle. This force is known as the Lorentz force, and is given by: {{Equation box 1 where is the force, is the electric charge of the particle, is the instantaneous velocity of the particle, and is the magnetic field (in teslas). The direction of force on the charge can be determined by the right-hand rule (see the figure). The Lorentz force is always perpendicular to both the velocity of the particle and the magnetic field that created it. When a charged particle moves in a static magnetic field, it traces a helical path in which the helix axis is parallel to the magnetic field, and in which the speed of the particle remains constant. Force on current-carrying wire When a wire carrying a steady electric current is placed in an external magnetic field, each of the moving charges in the wire experience the Lorentz force. Together, these forces produce a net macroscopic force on the wire. This force (on a macroscopic current) is often referred to as the Laplace force. For a straight, stationary wire in a uniform magnetic field, this force is given by: {{Equation box 1 where is the current and is a vector whose magnitude is the length of the wire, and whose direction is along the wire, aligned with the direction of the current. If the wire is not straight or the magnetic field is non-uniform, the total force can be computed by applying the formula to each infinitesimal segment of wire \mathrm d \boldsymbol \ell , then adding up all these forces by integration. In this case, the net force on a stationary wire carrying a steady current is {{Equation box 1 This force creates an attractive/repulsive force between 2 parallel wires as the current through each produces a magnetic field that pushes/pulls on the other. Too, a loop of current in a magnetic field will experience a torque due to the different direction of the force on different sides of the loop as describe in the next section. Net force and torque on current loops A magnetic field acting on a current carrying loop produces both a torque and a net force (if the magnetic field is non-uniform). This effect is important for driving certain types of motors and in modeling forces and torques on atoms. Calculating the torque on a rectangular loop is straightforward. The diagram to the right shows a rectangular loop of current in a uniform magnetic field (with a direction indicated by the green arrows). For simplicity the loop is aligned so that it is along the direction of the magnetic field. The magnetic force on opposite sides of the loop are equal and opposite producing no net force on the loop. The forces on the short sides (here shown as violet arrows), though, produce a net torque equal to the product of the force and the perpendicular distance between them. Denoting the short side length as , the magnitude of that force is = using the equation for the magnetic force on a straight wire given in the previous section. The magnitude of the net torque (along dashed axis) is therefore = . Using the fact that the area = and generalizing for all angles gives {{Equation box 1 Here the direction of the area is the normal to the area as determined by the right hand grip rule of the current loop. While derived for a rectangular loop this equation is valid for a flat loop of any shape and orientation. As described above, there is no net force on a loop in a uniform magnetic field. However, non-uniform magnetic fields do produce a net force. This net force tends to pull the object in direction of the stronger magnetic field. Net force and torque on a magnetic dipole Since the net force on a loop is proportional to the current of the loop times it area it is natural to define a quantity called the magnetic dipole moment such that {{Equation box 1 In cases where this is valid, the details of the current loop such as it shape, area, orientation, and current around the loop are all hidden in and otherwise do not matter. All current loops with the same dipole moment are affected the same way. Such loops that are sufficiently small that the details (other than ) do not matter are called magnetic dipoles. Applying the Lorentz force to a loop of arbitrary shape and imagine shrinking it down small enough with produce a torque on the magnetic dipole of: {{Equation box 1 and a force on the magnetic dipole of {{Equation box 1 where \nabla represents the gradient. This force tends to push the magnetic dipole into the direction of increasing . Magnetic field due to electrical currents : a current flowing in the direction of the white arrow produces a magnetic field shown by the red arrows. All moving charged particles produce magnetic fields. Moving point charges, such as electrons, produce complicated but well known magnetic fields that depend on the charge, velocity, and acceleration of the particles. These equations become much simpler when the moving charges form a steady state electrical current, the study of which is called magnetostatics. In general, magnetic field lines form concentric circles around a current-carrying wire. The direction of such a magnetic field can be determined by using the "right-hand grip rule" (see figure at right). The strength of the magnetic field decreases with distance from the wire. (For an infinite length wire the strength is inversely proportional to the distance.) Magnetic field of a long straight wire The magnetic field of a steady current through a sufficiently long straight wire is: {{Equation box 1 \mathbf{H} = \frac{I}{2\pi r}\, \hat{\phi}, \end{align} where is the perpendicular distance to the wire. The direction \hat{\phi} of the magnetic field is tangent to a circle perpendicular to the wire according to the right hand rule. Magnetic field of an arbitrarily shaped thin wire More specifically, the magnetic field generated by a steady current (a constant flow of electric charges, in which charge neither accumulates nor is depleted at any point) is described by the Biot–Savart law: {{Equation box 1 \mathbf{H} = \frac{I}{4\pi}\int_{\mathrm{wire}}\frac{\mathrm{d}\boldsymbol{\ell} \times \mathbf{\hat r}}{r^2},\end{align} where the integral sums over the wire length where vector is the vector line element with direction in the same sense as the current , is the magnetic constant, is the distance between the location of and the location where the magnetic field is calculated, and is a unit vector in the direction of . Magnetic field of a solenoid with electric current running through it behaves like a magnet. Bending a current-carrying wire into a loop concentrates the magnetic field inside the loop while weakening it outside. Bending a wire into multiple closely spaced loops to form a coil or 'solenoid' enhances this effect. A device so formed around an iron core may act as an electromagnet, generating a strong, well-controlled magnetic field. An infinitely long solenoid has a uniform magnetic field inside, and no magnetic field outside. The magnetic field only exists inside of the solenoid and is {{Equation box 1 where is the number of turns per unit length of the solenoid and the direction of is along the length of the solenoid. A finite length solenoid produces a more complicated magnetic field that can be evaluated mathematically. For other examples of using the Biot-Savart law to calculate the magnetic fields for other common current configurations see #Common formulæ below. Ampere's law A slightly more general way of relating the current I to the -field is through Ampère's law: {{Equation box 1 \oint \mathbf{H} \cdot \mathrm{d}\boldsymbol{\ell} = I_{\mathrm{enc}}, \end{align} where the line integral is over any arbitrary loop and I_\text{enc} is the current enclosed by that loop. The I_\text{enc} is slightly different for the 2 equations in that includes the difficult to calculate bound current in magnetic material while does not. Ampère's law is always valid for steady currents and can be used to easily calculate the magnetic fields of certain highly symmetric situations such as an infinite wire or an infinite solenoid. In a modified form that accounts for time varying electric fields, Ampère's law is one of four Maxwell's equations that describe electricity and magnetism. ==Magnetic field of permanent magnets==
Magnetic field of permanent magnets
Permanent magnets are objects that produce their own persistent magnetic fields. They are made of ferromagnetic materials, such as iron and nickel, that have been magnetized. They have both a north and a south pole. The magnetic field of permanent magnets, like all magnetized material, is created at the atomic level. The proper description of this effect involves quantum mechanics and even relativity. Fortunately, the net effect of adding up these magnetic interactions can often be calculated using much simpler models for the magnetic field created by the constituent atoms in the magnetic material. This occurs because at large enough distance (or equivalently for small enough magnets) the magnetic field of any magnetic object can be described by a single (vector) quantity, the magnetic dipole moment, . Objects that can be modeled this way, for example atoms, are called magnetic dipoles. The magnetic field produced by the magnet then is the net magnetic field of these dipoles. Too, the net force on the magnet is a result of adding up the forces on the individual dipoles. There are two simplified models for the nature of these dipoles: the Amperian loop model and the magnetic pole model. These two models produce two different magnetic fields, and , respectively. A realistic model of magnetism is more complicated than either of these models, but the Amperian loop model is generally better. The magnetic pole model, on the other hand, is incorrect about the nature of magnetism (magnetic charges do not exist) and makes incorrect prediction in certain cases. It, however, has the advantage of simplicity and (with care) can be used make correct predictions. Amperian loop model {{Multiple image|header=The Amperian loop model In this model developed by Ampere, the elementary magnetic dipole that makes up all magnets is a sufficiently small Amperian loop with current and loop area . Such a current loop has a magnetic dipole moment of {{Equation box 1 where the direction of is perpendicular to the area of the loop, , and depends on the direction of the current using the right-hand rule. These magnetic dipoles produce a magnetic -field. With this model, the Biot-Savart law can be used to calculate the correct while the Lorentz force law can be used to predict the correct torque, and force. Magnetic pole model Unlike the amperian loop model, the magnetic pole model has no basis in physical reality. However its mathematical simplicity combined with the fact that it can lead to correct results, makes it useful if used correctly. In this model, a magnetic -field is produced by fictitious magnetic charges that are spread over the surface of a magnetic pole with each magnet having both a north and a south pole having opposite 'charges'. A north pole feels a force in the direction of the -field while the force on the south pole is opposite to the -field. Near the north pole, therefore, all -field lines point away from the north pole (whether inside the magnet or out) while near the south pole all -field lines point toward the south pole (whether inside the magnet or out). The -field, therefore, is analogous to the electric field and, provided the equivalent 'magnetic charge' of the poles can be estimated, then all of the tools used for calculating can be used to calculate . In the magnetic pole model, the elementary magnetic dipole is formed by two opposite magnetic poles of pole strength separated by a small distance vector , such that . The magnetic pole model predicts correctly the field both inside and outside magnetic materials, in particular the fact that is opposite to the magnetization field inside a permanent magnet. Since it is based on the fictitious idea of a magnetic charge density, the pole model has limitations. Magnetic poles cannot exist apart from each other as electric charges can, but always come in north–south pairs. If a magnetized object is divided in half, a new pole appears on the surface of each piece, so each has a pair of complementary poles. The magnetic pole model does not account for magnetism that is produced by electric currents, nor the inherent connection between angular momentum and magnetism. The pole model usually treats magnetic charge as a mathematical abstraction, rather than a physical property of particles. However, a magnetic monopole is a hypothetical particle (or class of particles) that physically has only one magnetic pole (either a north pole or a south pole). In other words, it would possess a "magnetic charge" analogous to an electric charge. Magnetic field lines would start or end on magnetic monopoles, so if they exist, they would give exceptions to the rule that magnetic field lines neither start nor end. Some theories (such as Grand Unified Theories) have predicted the existence of magnetic monopoles, but so far, none have been observed. ==Interactions with magnets==
Interactions with magnets
Force between magnets Specifying the force between two small magnets is quite complicated because it depends on the strength and orientation of both magnets and their distance and direction relative to each other. The force is particularly sensitive to rotations of the magnets due to magnetic torque. The force on each magnet depends on its magnetic moment and the magnetic field of the other. To understand the force between magnets, it is useful to examine the magnetic pole model given above. In this model, the -field of one magnet pushes and pulls on both poles of a second magnet. If this -field is the same at both poles of the second magnet then there is no net force on that magnet since the force is opposite for opposite poles. If, however, the magnetic field of the first magnet is nonuniform (such as the near one of its poles), each pole of the second magnet sees a different field and is subject to a different force. This difference in the two forces moves the magnet in the direction of increasing magnetic field and may also cause a net torque. This is a specific example of a general rule that magnets are attracted (or repulsed depending on the orientation of the magnet) into regions of higher magnetic field. Any non-uniform magnetic field, whether caused by permanent magnets or electric currents, exerts a force on a small magnet in this way. The details of the Amperian loop model are different and more complicated but yield the same result: that magnetic dipoles are attracted/repelled into regions of higher magnetic field. Mathematically, the force on a small magnet having a magnetic moment due to a magnetic field is: {{Equation box 1 where the gradient is the change of the quantity per unit distance and the direction is that of maximum increase of . The dot product , where and represent the magnitude of the and vectors and is the angle between them. If is in the same direction as then the dot product is positive and the gradient points "uphill" pulling the magnet into regions of higher -field (more strictly larger ). This equation is strictly only valid for magnets of zero size, but is often a good approximation for not too large magnets. The magnetic force on larger magnets is determined by dividing them into smaller regions each having their own then summing up the forces on each of these very small regions. Magnetic torque on permanent magnets If two like poles of two separate magnets are brought near each other, and one of the magnets is allowed to turn, it promptly rotates to align itself with the first. In this example, the magnetic field of the stationary magnet creates a magnetic torque on the magnet that is free to rotate. This magnetic torque tends to align a magnet's poles with the magnetic field lines. A compass, therefore, turns to align itself with Earth's magnetic field. {{Multiple image|header=Torque on a dipole Mathematically, the torque on a small magnet is proportional both to the applied magnetic field and to the magnetic moment of the magnet: {{Equation box 1 where × represents the vector cross product. This equation includes all of the qualitative information included above. There is no torque on a magnet if is in the same direction as the magnetic field, since the cross product is zero for two vectors that are in the same direction. Further, all other orientations feel a torque that twists them toward the direction of magnetic field. ==Relation between H and B==
Relation between H and B
The formulas derived for the magnetic field above are correct when dealing with the entire current. A magnetic material placed inside a magnetic field, though, generates its own bound current, which can be a challenge to calculate. (This bound current is due to the sum of atomic sized current loops and the spin of the subatomic particles such as electrons that make up the material.) The -field as defined above helps factor out this bound current; but to see how, it helps to introduce the concept of magnetization first. Magnetization The magnetization vector field represents how strongly a region of material is magnetized. It is defined as the net magnetic dipole moment per unit volume of that region. The magnetization of a uniform magnet is therefore a material constant, equal to the magnetic moment of the magnet divided by its volume. Since the SI unit of magnetic moment is A⋅m2, the SI unit of magnetization is ampere per meter, identical to that of the -field. The magnetization field of a region points in the direction of the average magnetic dipole moment in that region. Magnetization field lines, therefore, begin near the magnetic south pole and ends near the magnetic north pole. (Magnetization does not exist outside the magnet.) In the Amperian loop model, the magnetization is due to combining many tiny Amperian loops to form a resultant current called bound current. This bound current, then, is the source of the magnetic field due to the magnet. Given the definition of the magnetic dipole, the magnetization field follows a similar law to that of Ampere's law: \oint \mathbf{M} \cdot \mathrm{d}\boldsymbol{\ell} = I_\mathrm{b}, where the integral is a line integral over any closed loop and is the bound current enclosed by that closed loop. In the magnetic pole model, magnetization begins at and ends at magnetic poles. If a given region, therefore, has a net positive "magnetic pole strength" (corresponding to a north pole) then it has more magnetization field lines entering it than leaving it. Mathematically this is equivalent to: \oint_S \mu_0 \mathbf{M} \cdot \mathrm{d}\mathbf{A} = - q_\mathrm{M}, where the integral is a closed surface integral over the closed surface and is the "magnetic charge" (in units of magnetic flux) enclosed by . (A closed surface completely surrounds a region with no holes to let any field lines escape.) The negative sign occurs because the magnetization field moves from south to north. H-field and magnetic materials In SI units, the H-field is related to the B-field by \mathbf{H}\ \equiv \ \frac{\mathbf{B}}{\mu_0} - \mathbf{M}. In terms of the H-field, Ampere's law is \oint \mathbf{H} \cdot \mathrm{d}\boldsymbol{\ell} = \oint \left(\frac{\mathbf{B}}{\mu_0} - \mathbf{M}\right) \cdot \mathrm{d}\boldsymbol{\ell} = I_\mathrm{tot} - I_\mathrm{b} = I_\mathrm{f}, where represents the 'free current' enclosed by the loop so that the line integral of does not depend at all on the bound currents. For the differential equivalent of this equation see Maxwell's equations. Ampere's law leads to the boundary condition \left(\mathbf{H_1^\parallel} - \mathbf{H_2^\parallel}\right) = \mathbf{K}_\mathrm{f} \times \hat{\mathbf{n}}, where is the surface free current density and the unit normal \hat{\mathbf{n}} points in the direction from medium 2 to medium 1. Similarly, a surface integral of over any closed surface is independent of the free currents and picks out the "magnetic charges" within that closed surface: \oint_S \mu_0 \mathbf{H} \cdot \mathrm{d}\mathbf{A} = \oint_S (\mathbf{B} - \mu_0 \mathbf{M}) \cdot \mathrm{d}\mathbf{A} = 0 - (-q_\mathrm{M}) = q_\mathrm{M}, which does not depend on the free currents. The -field, therefore, can be separated into two independent parts: \mathbf{H} = \mathbf{H}_0 + \mathbf{H}_\mathrm{d}, where is the applied magnetic field due only to the free currents and is the demagnetizing field due only to the bound currents. The magnetic -field, therefore, re-factors the bound current in terms of "magnetic charges". The field lines loop only around "free current" and, unlike the magnetic field, begins and ends near magnetic poles as well. Magnetism Most materials respond to an applied -field by producing their own magnetization and therefore their own -fields. Typically, the response is weak and exists only when the magnetic field is applied. The term magnetism describes how materials respond on the microscopic level to an applied magnetic field and is used to categorize the magnetic phase of a material. Materials are divided into groups based upon their magnetic behavior: • Diamagnetic materials produce a magnetization that opposes the magnetic field. • Paramagnetic materials can have a magnetization independent of an applied B-field with a complex relationship between the two fields. • Superconductors (and ferromagnetic superconductors) are materials that are characterized by perfect conductivity below a critical temperature and magnetic field. They also are highly magnetic and can be perfect diamagnets below a lower critical magnetic field. Superconductors often have a broad range of temperatures and magnetic fields (the so-named mixed state) under which they exhibit a complex hysteretic dependence of on . In the case of paramagnetism and diamagnetism, the magnetization is often proportional to the applied magnetic field such that: \mathbf{B} = \mu \mathbf{H}, where is a material dependent parameter called the permeability. In some cases the permeability may be a second rank tensor so that may not point in the same direction as . These relations between and are examples of constitutive equations. However, superconductors and ferromagnets have a more complex -to- relation; see magnetic hysteresis. == Electrodynamics ==
Electrodynamics
For time varying magnetic fields (and more generally changing electrical currents or accelerating electrical charges), the magnetic and electric fields become linked such that a change in one induces the other. Together, the electric and magnetic fields form an electromagnetic field. The study of how the electric and magnetic fields interact in this way is called electrodynamics and includes many phenomenon that are important in physics and electrical engineering. It underlies transformers, and the generation and transmission of electrical power through wires and through space in the form of electromagnetic radiation of which light is one form. Too, it allow magnetic fields to store and transmit energy. Magnetic flux rule A time varying magnetic field through a loop of wire induces a current (more properly an EMF) through that loop. This is known as electromagnetic induction and is important for many electronic devices such as inductors, transformers, and electrical generators. The equation governing this is known as the flux rule or Faraday's law of induction: \mathcal{E} = - \frac{\mathrm{d}\Phi}{\mathrm{d}t} where \mathcal{E} is the electromotive force (or EMF, the voltage generated around a closed loop) and is the magnetic flux—the product of the area times the magnetic field normal to that area. (This definition of magnetic flux is why is often referred to as magnetic flux density.) The negative sign represents the fact that any current generated by a changing magnetic field in a coil produces a magnetic field that opposes the change in the magnetic field that induced it. This phenomenon is known as Lenz's law. Stored energy Energy is needed to generate a magnetic field both to work against the electric field that a changing magnetic field creates and to change the magnetization of any material within the magnetic field. The energy density of just creating the field at a given region is: u_{mag} = \frac{\mathbf{B} \cdot \mathbf{B}}{2\mu_0}. For non-dispersive materials, the energy used to magnetize the material is released when the magnetic field is destroyed so that the energy can be modeled as being stored in the magnetic field. If the non-dispersive material is also linear (such that where is frequency-independent), then the total energy density stored in the magnetic field and in magnetizing the material at a location is: u_{mag} = \frac{\mathbf{B} \cdot \mathbf{H}}{2}= \frac{\mathbf{B} \cdot \mathbf{B}}{2\mu} = \frac{\mu\mathbf{H} \cdot \mathbf{H}}{2}. The above equation cannot be used for nonlinear materials, though. In general, the incremental amount of work per unit volume needed to cause a small change of magnetic field is: \delta W = \mathbf{H}\cdot\delta\mathbf{B}. Once the relationship between and is known this equation is used to determine the work needed to reach a given magnetic state. For hysteretic materials such as ferromagnets and superconductors, the work needed also depends on how the magnetic field is created. For linear non-dispersive materials, though, the general equation leads directly to the simpler energy density equation given above. Poynting vector according to the Poynting vector S, calculated using the electric field E (due to the voltage V) and the magnetic field H (due to current I).Magnetic field, together with the electric field, transmit electrical power. The amount of electrical power (per unit area) transmitted this way is called the poynting vector, , which depends on the magnetic field as the cross product: The first type of source (an outflow source) causes the vector field to flow out (or in for a sink) to a given point. The second (or circulation) source causes the vector field to rotate around a given point (forming vortices). Both of these sources have well defined definitions and can be calculated from the vector field they create using a well-understood vector operator. The divergence of a vector field , is defined such that applying the divergence operator to a given vector field will yield the outflow sources. The curl is defined such that yields the circulation source. An example of the power of these vector operators is: since it is an experimental fact that magnetic charges do not exist (and therefore there are no source nor sinks of ) the divergence of must be zero, = 0, which is one of Maxwell's equations. Maxwell's equation has 2 major versions: a microscopic version which necessitates knowing all of the charges and currents (including the complex ones at the atomic level) and the macroscopic version which depends only on the know 'free' charge and 'free' currents. Here the term 'free' means any charge or current that is directly controlled by the experiment and does not include the atomic level 'bound' charges and currents in a material which happen as a response to the electric and magnetic fields present in that material. Maxwell's macroscopic equations are written as: \begin{align} \nabla \cdot \mathbf{D} \,\,\, &= \rho_f \\ \nabla \cdot \mathbf{B} \,\,\, &= 0 \\ \nabla \times \mathbf{E} &= -\frac{\partial \mathbf{B}}{\partial t} \\ \nabla \times \mathbf{H} &= \mathbf{J}_f + \frac{\partial \mathbf{D}}{\partial t}. \end{align}In these equations, \mathbf{D} is the electric displacement field, \mathbf{E} the electric field, \rho_f the free electric charge density, and \mathbf{J}_f the free current density. The first of Maxwell's equations is known as Gauss' Law but does not involve magnetic field so does not warrant further discussion here. The second equation is Gauss' law for magnetism which reflects the non-existence of magnetic charge and allows to be determined as the curl of a vector potential . The third equation is Faraday's law of induction. And, the fourth equation is Ampère's law with Maxwell's correction. ==Uses and examples==
Uses and examples
Uses in advanced physics As different aspects of the same phenomenon According to the special theory of relativity, the partition of the electromagnetic force into separate electric and magnetic components is not fundamental, but varies with the observational frame of reference: An electric force perceived by one observer may be perceived by another (in a different frame of reference) as a magnetic force, or a mixture of electric and magnetic forces. The magnetic field existing as electric field in other frames can be shown by consistency of equations obtained from Lorentz transformation of four force from Coulomb's Law in particle's rest frame with Maxwell's laws considering definition of fields from Lorentz force and for non accelerating condition. The form of magnetic field hence obtained by Lorentz transformation of four-force from the form of Coulomb's law in source's initial frame is given by: \mathbf{B} = \frac q {4 \pi \varepsilon_0 r^3} \frac {1- \beta^2} {(1- \beta^2 \sin^2 \theta)^{3/2}} \frac{\mathbf{v} \times \mathbf{r}}{c^2} = \frac{\mathbf{v} \times \mathbf{E}}{c^2} where q is the charge of the point source, \varepsilon_0 is the vacuum permittivity, \mathbf{r} is the position vector from the point source to the point in space, \mathbf{v} is the velocity vector of the charged particle, \beta is the ratio of speed of the charged particle divided by the speed of light and \theta is the angle between \mathbf{r} and \mathbf{v}. This form of magnetic field can be shown to satisfy Maxwell's laws within the constraint of particle being non accelerating. The above reduces to Biot-Savart law for non relativistic stream of current (\beta\ll 1). Formally, special relativity combines the electric and magnetic fields into a rank-2 tensor, called the electromagnetic tensor. Changing reference frames mixes these components. This is analogous to the way that special relativity mixes space and time into spacetime, and mass, momentum, and energy into four-momentum. Similarly, the energy stored in a magnetic field is mixed with the energy stored in an electric field in the electromagnetic stress–energy tensor. Magnetic vector potential In advanced topics such as quantum mechanics and relativity it is often easier to work with a potential formulation of electrodynamics rather than in terms of the electric and magnetic fields. In this representation, the magnetic vector potential , and the electric scalar potential , are defined using gauge fixing such that: \begin{align} \mathbf{B} &= \nabla \times \mathbf{A}, \\ \mathbf{E} &= -\nabla \varphi - \frac{ \partial \mathbf{A} }{ \partial t }. \end{align} The vector potential, '' given by this form may be interpreted as a generalized potential momentum per unit charge just as is interpreted as a generalized potential energy per unit charge''. There are multiple choices one can make for the potential fields that satisfy the above condition. However, the choice of potentials is represented by its respective gauge condition. Maxwell's equations when expressed in terms of the potentials in Lorenz gauge can be cast into a form that agrees with special relativity. In relativity, together with forms a four-potential regardless of the gauge condition, analogous to the four-momentum that combines the momentum and energy of a particle. Using the four potential instead of the electromagnetic tensor has the advantage of being much simpler—and it can be easily modified to work with quantum mechanics. Propagation of Electric and Magnetic fields Special theory of relativity imposes the condition for events related by cause and effect to be time-like separated, that is that causal efficacy propagates no faster than light. Maxwell's equations for electromagnetism are found to be in favor of this as electric and magnetic disturbances are found to travel at the speed of light in space. Electric and magnetic fields from classical electrodynamics obey the principle of locality in physics and are expressed in terms of retarded time or the time at which the cause of a measured field originated given that the influence of field travelled at speed of light. The retarded time for a point particle is given as solution of: t_r = \mathbf{t} - \frac{\left|\mathbf{r} - \mathbf{r}_s(t_r)\right|}{c} where t_r is retarded time or the time at which the source's contribution of the field originated, r_s(t) is the position vector of the particle as function of time, \mathbf{r} is the point in space, \mathbf{t} is the time at which fields are measured and c is the speed of light. The equation subtracts the time taken for light to travel from particle to the point in space from the time of measurement to find time of origin of the fields. The uniqueness of solution for t_r for given \mathbf{t}, \mathbf{r} and r_s(t) is valid for charged particles moving slower than speed of light. which is incorporated into a more complete theory known as the Standard Model of particle physics. In QED, the magnitude of the electromagnetic interactions between charged particles (and their antiparticles) is computed using perturbation theory. These rather complex formulas produce a remarkable pictorial representation as Feynman diagrams in which virtual photons are exchanged. Predictions of QED agree with experiments to an extremely high degree of accuracy: currently about 10−12 (and limited by experimental errors); for details see precision tests of QED. This makes QED one of the most accurate physical theories constructed thus far. All equations in this article are in the classical approximation, which is less accurate than the quantum description mentioned here. However, under most everyday circumstances, the difference between the two theories is negligible. Uses in geology Earth's magnetic field The Earth's magnetic field is produced by convection of a liquid iron alloy in the outer core. In a dynamo process, the movements drive a feedback process in which electric currents create electric and magnetic fields that in turn act on the currents. The field at the surface of the Earth is approximately the same as if a giant bar magnet were positioned at the center of the Earth and tilted at an angle of about 11° off the rotational axis of the Earth (see the figure). The north pole of a magnetic compass needle points roughly north, toward the North Magnetic Pole. However, because a magnetic pole is attracted to its opposite, the North Magnetic Pole is actually the south pole of the geomagnetic field. This confusion in terminology arises because the pole of a magnet is defined by the geographical direction it points. Earth's magnetic field is not constant—the strength of the field and the location of its poles vary. Moreover, the poles periodically reverse their orientation in a process called geomagnetic reversal. The most recent reversal occurred 780,000 years ago. Uses in Engineering Rotating magnetic fields The rotating magnetic field is a common design principle in the operation of alternating-current motors. A permanent magnet in such a field rotates so as to maintain its alignment with the external field. Magnetic torque is used to drive electric motors. In one simple motor design, a magnet is fixed to a freely rotating shaft and is subjected to a magnetic field from an array of electromagnets. By continuously switching the electric current through each of the electromagnets, thereby flipping the polarity of their magnetic fields, like poles are kept next to the rotor; the resultant torque is transferred to the shaft. A rotating magnetic field can be constructed using two coils at right angles with a phase difference of 90 degrees between their AC currents. In practice, three-phase systems are used where the three currents are equal in magnitude and have a phase difference of 120 degrees. Three similar coils at mutual geometrical angles of 120 degrees create the rotating magnetic field. The ability of the three-phase system to create a rotating field, utilized in electric motors, is one of the main reasons why three-phase systems dominate the world's electrical power supply systems. Synchronous motors use DC-voltage-fed rotor windings, which lets the excitation of the machine be controlled—and induction motors use short-circuited rotors (instead of a magnet) following the rotating magnetic field of a multicoiled stator. The short-circuited turns of the rotor develop eddy currents induced by the rotating field of the stator, and these currents in turn produce a torque on the rotor through the Lorentz force. The Italian physicist Galileo Ferraris and the Serbian-American electrical engineer Nikola Tesla independently researched the use of rotating magnetic fields in electric motors. In 1888, Ferraris published his research in a paper to the Royal Academy of Sciences in Turin and Tesla gained for his work. Magnetic circuits An important use of is in magnetic circuits where inside a linear material. Here, is the magnetic permeability of the material. This result is similar in form to Ohm's law , where is the current density, is the conductance and is the electric field. Extending this analogy, the counterpart to the macroscopic Ohm's law () is: \Phi = \frac F R_\mathrm{m}, where \Phi = \int \mathbf{B}\cdot \mathrm{d}\mathbf{A} is the magnetic flux in the circuit, F = \int \mathbf{H}\cdot \mathrm{d}\boldsymbol{\ell} is the magnetomotive force applied to the circuit, and is the reluctance of the circuit. Here the reluctance is a quantity similar in nature to resistance for the flux. Using this analogy it is straightforward to calculate the magnetic flux of complicated magnetic field geometries, by using all the available techniques of circuit theory. Uses in material science Hall effect The charge carriers of a current-carrying conductor placed in a transverse magnetic field experience a sideways Lorentz force; this results in a charge separation in a direction perpendicular to the current and to the magnetic field. The resultant voltage in that direction is proportional to the applied magnetic field. This is known as the Hall effect. The Hall effect is often used to measure the magnitude of a magnetic field. It is used as well to find the sign of the dominant charge carriers in materials such as semiconductors (negative electrons or positive holes). Largest magnitude magnetic fields The largest magnitude magnetic field produced over a macroscopic volume outside a lab setting is 2.8 kT (VNIIEF in Sarov, Russia, 1998). The largest magnitude magnetic field produced in a laboratory over a macroscopic volume was 1.2 kT by researchers at the University of Tokyo in 2018. The largest magnitude microscopic magnetic fields produced in a laboratory occur in particle accelerators, such as RHIC, inside the collisions of heavy ions, where microscopic fields reach 1014 T. Magnetars have the strongest known macroscopic magnetic fields of any naturally occurring object, ranging from 0.1 to 100 GT (108 to 1011 T). == Common formulæ==
Common formulæ
^3}, on the axial plane (given that x \gg R), where x can also be negative to indicate position at the opposite direction on the axis, and \mathbf m is the magnetic dipole moment. Additional magnetic field values can be found through the magnetic field of a finite beam, for example, that the magnetic field of an arc of angle \theta and radius R at the center is B={\mu_0\theta I\over 4\pi R}, or that the magnetic field at the center of a N-sided regular polygon of side a is B= {\mu_0NI\over\pi a} \sin{\pi\over N}\tan{\pi\over N}, both outside of the plane with proper directions as inferred by right hand thumb rule. ==History==
History
, 1644, showing the Earth attracting lodestones. It illustrated his theory that magnetism was caused by the circulation of tiny helical particles, "threaded parts", through threaded pores in magnets. Early developments While magnets and some properties of magnetism were known to ancient societies, the research of magnetic fields began in 1269 when French scholar Petrus Peregrinus de Maricourt mapped out the magnetic field on the surface of a spherical magnet using iron needles. Noting the resulting field lines crossed at two points he named those points "poles" in analogy to Earth's poles. He also articulated the principle that magnets always have both a north and south pole, no matter how finely one slices them. Almost three centuries later, William Gilbert of Colchester replicated Petrus Peregrinus' work and was the first to state explicitly that Earth is a magnet. Published in 1600, Gilbert's work, De Magnete, helped to establish magnetism as a science. Mathematical development , Der Geist in der Natur, 1854 In 1750, John Michell stated that magnetic poles attract and repel in accordance with an inverse square law Then André-Marie Ampère showed that parallel wires with currents attract one another if the currents are in the same direction and repel if they are in opposite directions. Finally, Jean-Baptiste Biot and Félix Savart announced empirical results about the forces that a current-carrying long, straight wire exerted on a small magnet, determining the forces were inversely proportional to the perpendicular distance from the wire to the magnet. which became known as the Biot–Savart law, as Laplace did not publish his findings. Extending these experiments, Ampère published his own successful model of magnetism in 1825. In it, he showed the equivalence of electrical currents to magnets Between 1861 and 1865, James Clerk Maxwell developed and published Maxwell's equations, which explained and united all of classical electricity and magnetism. The first set of these equations was published in a paper entitled On Physical Lines of Force in 1861. These equations were valid but incomplete. Maxwell completed his set of equations in his later 1865 paper A Dynamical Theory of the Electromagnetic Field and demonstrated the fact that light is an electromagnetic wave. Heinrich Hertz published papers in 1887 and 1888 experimentally confirming this fact. Modern developments In 1887, Tesla developed an induction motor that ran on alternating current. The motor used polyphase current, which generated a rotating magnetic field to turn the motor (a principle that Tesla claimed to have conceived in 1882). Tesla received a patent for his electric motor in May 1888. In 1885, Galileo Ferraris independently researched rotating magnetic fields and subsequently published his research in a paper to the Royal Academy of Sciences in Turin, just two months before Tesla was awarded his patent, in March 1888. The twentieth century showed that classical electrodynamics is already consistent with special relativity, and extended classical electrodynamics to work with quantum mechanics. Albert Einstein, in his paper of 1905 that established relativity, showed that both the electric and magnetic fields are part of the same phenomena viewed from different reference frames. Finally, the emergent field of quantum mechanics was merged with electrodynamics to form quantum electrodynamics, which first formalized the notion that electromagnetic field energy is quantized in the form of photons. ==See also==
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