It is impossible to make magnetic monopoles from abar magnet. If a bar magnet is cut in half, it isnot the case that one half has the north pole and the other half has the south pole. Instead, each piece has its own north and south poles. A magnetic monopole cannot be created from normal matter such asatoms andelectrons, but would instead be a newelementary particle.
Inparticle physics, amagnetic monopole is a hypotheticalelementary particle that is an isolatedmagnet with only one magnetic pole (a north pole without a south pole or vice versa).[1][2] A magnetic monopole would have a net north or south "magnetic charge". Modern interest in the concept stems fromparticle theories, notably thegrand unified andsuperstring theories, which predict their existence.[3][4]The known elementary particles that haveelectric charge are electric monopoles.
Magnetism inbar magnets andelectromagnets is not caused by magnetic monopoles, and indeed, there is no known experimental or observational evidence that magnetic monopoles exist.
Somecondensed matter systems contain effective (non-isolated) magnetic monopolequasi-particles,[5] or contain phenomena that are mathematically analogous to magnetic monopoles.[6]
Many early scientists attributed the magnetism oflodestones to two different "magnetic fluids" ("effluvia"), a north-pole fluid at one end and a south-pole fluid at the other, which attracted and repelled each other in analogy to positive and negativeelectric charge.[7][8] However, an improved understanding ofelectromagnetism in the nineteenth century showed that the magnetism of lodestones was properly explained not by magnetic monopole fluids, but rather by a combination ofelectric currents, theelectron magnetic moment, and themagnetic moments of other particles.Gauss's law for magnetism, one ofMaxwell's equations, is the mathematical statement that magnetic monopoles do not exist. Nevertheless,Pierre Curie pointed out in 1894[9] that magnetic monopolescould conceivably exist, despite not having been seen so far.
Thequantum theory of magnetic charge started with a paper by thephysicistPaul Dirac in 1931.[10] In this paper, Dirac showed that ifany magnetic monopoles exist in the universe, then all electric charge in the universe must bequantized (Dirac quantization condition).[11] The electric chargeis, in fact, quantized, which is consistent with (but does not prove) the existence of monopoles.[11]
Since Dirac's paper, several systematic monopole searches have been performed. Experiments in 1975[12] and 1982[13] produced candidate events that were initially interpreted as monopoles, but are now regarded as inconclusive.[14] Therefore, whether monopoles exist remains an open question. Further advances in theoreticalparticle physics, particularly developments ingrand unified theories andquantum gravity, have led to more compelling arguments (detailed below) that monopoles do exist.Joseph Polchinski, a string theorist, described the existence of monopoles as "one of the safest bets that one can make about physics not yet seen".[15] These theories are not necessarily inconsistent with the experimental evidence. In some theoreticalmodels, magnetic monopoles are unlikely to be observed, because they are too massive to create inparticle accelerators (see§ Searches for magnetic monopoles below), and also too rare in the Universe to enter aparticle detector with much probability.[15]
Somecondensed matter systems propose a structure superficially similar to a magnetic monopole, known as aflux tube. The ends of a flux tube form amagnetic dipole, but since they move independently, they can be treated for many purposes as independent magnetic monopolequasiparticles. Since 2009, numerous news reports from the popular media[16][17] have incorrectly described these systems as the long-awaited discovery of the magnetic monopoles, but the two phenomena are only superficially related to one another.[18][19] These condensed-matter systems remain an area of active research. (See§ "Monopoles" in condensed-matter systems below.)
All matter isolated to date, including every atom on theperiodic table and every particle in theStandard Model, has zero magnetic monopole charge. Therefore, the ordinary phenomena ofmagnetism andmagnets do not derive from magnetic monopoles.
Mathematically, the magnetic field of an object is often described in terms of amultipole expansion. This is an expression of the field as the sum of component fields with specific mathematical forms. The first term in the expansion is called themonopole term, the second is calleddipole, thenquadrupole, thenoctupole, and so on. Any of these terms can be present in the multipole expansion of anelectric field, for example. However, in the multipole expansion of amagnetic field, the "monopole" term is always exactly zero (for ordinary matter). A magnetic monopole, if it exists, would have the defining property of producing a magnetic field whosemonopole term is non-zero.
Amagnetic dipole is something whose magnetic field is predominantly or exactly described by the magnetic dipole term of the multipole expansion. The termdipole meanstwo poles, corresponding to the fact that a dipole magnet typically contains anorth pole on one side and asouth pole on the other side. This is analogous to anelectric dipole, which has positive charge on one side and negative charge on the other. However, an electric dipole and magnetic dipole are fundamentally quite different. In an electric dipole made of ordinary matter, the positive charge is made ofprotons and the negative charge is made ofelectrons, but a magnetic dipole doesnot have different types of matter creating the north pole and south pole. Instead, the two magnetic poles arise simultaneously from the aggregate effect of all the currents and intrinsic moments throughout the magnet. Because of this, the two poles of a magnetic dipole must always have equal and opposite strength, and the two poles cannot be separated from each other.
Maxwell's equations ofelectromagnetism relate the electric and magnetic fields to each other and to the distribution of electric charge and current. The standard equations provide for electric charge, but they posit zero magnetic charge and current. Except for this constraint, the equations aresymmetric under the interchange of the electric and magnetic fields. Maxwell's equations are symmetric when the charge andelectric current density are zero everywhere, as in vacuum.
Maxwell's equations can also be written in a fully symmetric form if one allows for "magnetic charge" analogous to electric charge.[20] With the inclusion of a variable for the density of magnetic charge, sayρm, there is also a "magnetic current density" variable in the equations,jm.
If magnetic charge does not exist – or if it exists but is absent in a region of space – then the new terms in Maxwell's equations are all zero, and the extended equations reduce to the conventional equations of electromagnetism such as∇ ⋅B = 0 (where∇⋅ is thedivergence operator andB is themagnetic flux density).
Left: Fields due to stationaryelectric and magnetic monopoles. Right: In motion (velocityv), anelectric charge induces aB field while amagnetic charge induces anE field.
Top:E field due to anelectric dipole momentd. Bottom left:B field due to amagnetic dipolem formed by two hypothetical magnetic monopoles. Bottom right:B field due to a naturalmagnetic dipole momentm found in ordinary matter (not from magnetic monopoles).(There should not be red and blue circles in the bottom right image.)
In theInternational System of Quantities used with theSI, there are two conventions for defining magnetic chargeqm, each with different units:weber (Wb) andampere-meter (A⋅m). The conversion between them isqm[Wb] =μ0qm[A⋅m], since the units are1 Wb = 1 H⋅A = (1 H⋅m−1)(1 A⋅m), where H is thehenry – the SI unit ofinductance.
Maxwell's equations then take the following forms (using the same notation above):[notes 1]
Maxwell's equations and Lorentz force equation with magnetic monopoles: SI units
The generalized Maxwell's equations possess a certain symmetry, called aduality transformation. One can choose any real angleξ, and simultaneously change the fields and charges everywhere in the universe as follows (in Gaussian units):[27]
Charges and currents
Fields
where the primed quantities are the charges and fields before the transformation, and the unprimed quantities are after the transformation. The fields and charges after this transformation still obey the same Maxwell's equations.
Because of the duality transformation, one cannot uniquely decide whether a particle has an electric charge, a magnetic charge, or both, just by observing its behavior and comparing that to Maxwell's equations. For example, it is merely a convention, not a requirement of Maxwell's equations, that electrons have electric charge but not magnetic charge; after aξ =π/2 transformation, it would be the other way around. The key empirical fact is that all particles ever observed have the same ratio of magnetic charge to electric charge.[27] Duality transformations can change the ratio to any arbitrary numerical value, but cannot change that all particles have the same ratio. Since this is the case, a duality transformation can be made that sets this ratio at zero, so that all particles have no magnetic charge. This choice underlies the "conventional" definitions of electricity and magnetism.[27]
One of the defining advances inquantum theory wasPaul Dirac's work on developing arelativistic quantum electromagnetism. Before his formulation, the presence of electric charge was simply inserted into the equations of quantum mechanics (QM), but in 1931 Dirac showed that a discrete charge is implied by QM.[28] That is to say, we can maintain the form ofMaxwell's equations and still have magnetic charges.
Consider a system consisting of a single stationary electric monopole (an electron, say) and a single stationary magnetic monopole, which would not exert any forces on each other. Classically, the electromagnetic field surrounding them has a momentum density given by thePoynting vector, and it also has a totalangular momentum, which is proportional to the productqeqm, and is independent of the distance between them.
Quantum mechanics dictates, however, that angular momentum is quantized as a multiple ofħ, so therefore the productqeqm must also be quantized. This means that if even a single magnetic monopole existed in the universe, and the form ofMaxwell's equations is valid, all electric charges would then bequantized.
Although it would be possible simply tointegrate over all space to find the total angular momentum in the above example, Dirac took a different approach. This led him to new ideas. He considered a point-like magnetic charge whose magnetic field behaves asqm/r 2 and is directed in the radial direction, located at the origin. Because the divergence ofB is equal to zero everywhere except for the locus of the magnetic monopole atr = 0, one can locally define thevector potential such that thecurl of the vector potentialA equals the magnetic fieldB.
However, the vector potential cannot be defined globally precisely because the divergence of the magnetic field is proportional to theDirac delta function at the origin. We must define one set of functions for the vector potential on the "northern hemisphere" (the half-spacez > 0 above the particle), and another set of functions for the "southern hemisphere". These two vector potentials are matched at the "equator" (the planez = 0 through the particle), and they differ by agauge transformation. Thewave function of an electrically charged particle (a "probe charge") that orbits the "equator" generally changes by a phase, much like in theAharonov–Bohm effect. This phase is proportional to the electric chargeqe of the probe, as well as to the magnetic chargeqm of the source. Dirac was originally considering anelectron whose wave function is described by theDirac equation.
Because the electron returns to the same point after the full trip around the equator, the phaseφ of its wave functioneiφ must be unchanged, which implies that the phaseφ added to the wave function must be a multiple of2π. This is known as theDirac quantization condition. In various units, this condition can be expressed as:
The hypothetical existence of a magnetic monopole would imply that the electric charge must be quantized in certain units; also, the existence of the electric charges implies that the magnetic charges of the hypothetical magnetic monopoles, if they exist, must be quantized in units inversely proportional to the elementary electric charge.
At the time it was not clear if such a thing existed, or even had to. After all, another theory could come along that would explain charge quantization without need for the monopole. The concept remained something of a curiosity. However, in the time since the publication of this seminal work, no other widely accepted explanation of charge quantization has appeared. (The concept of local gauge invariance—seeGauge theory—provides a natural explanation of charge quantization, without invoking the need for magnetic monopoles; but only if theU(1) gauge group is compact, in which case we have magnetic monopoles anyway.)
If we maximally extend the definition of the vector potential for the southern hemisphere, it is defined everywhere except for asemi-infinite line stretched from the origin in the direction towards the northern pole. This semi-infinite line is called theDirac string and its effect on the wave function is analogous to the effect of thesolenoid in theAharonov–Bohm effect. Thequantization condition comes from the requirement that the phases around the Dirac string are trivial, which means that the Dirac string must be unphysical. The Dirac string is merely an artifact of the coordinate chart used and should not be taken seriously.
The Dirac monopole is a singular solution of Maxwell's equation (because it requires removing the worldline from spacetime); in more sophisticated theories, it is superseded by a smooth solution such as the't Hooft–Polyakov monopole.
Agauge theory like electromagnetism is defined by a gauge field, which associates a group element to each path in space time. For infinitesimal paths, the group element is close to the identity, while for longer paths the group element is the successive product of the infinitesimal group elements along the way.
In electrodynamics, the group isU(1), unit complex numbers under multiplication. For infinitesimal paths, the group element is1 +iAμdxμ which implies that for finite paths parametrized bys, the group element is:
The map from paths to group elements is called theWilson loop or theholonomy, and for a U(1) gauge group it is the phase factor which the wavefunction of a charged particle acquires as it traverses the path. For a loop:
So that the phase a charged particle gets when going in a loop is themagnetic flux through the loop. When a smallsolenoid has a magnetic flux, there areinterference fringes for charged particles which go around the solenoid, or around different sides of the solenoid, which reveal its presence.
But if all particle charges are integer multiples ofe, solenoids with a flux of2π/e have no interference fringes, because the phase factor for any charged particle isexp(2πi) = 1. Such a solenoid, if thin enough, is quantum-mechanically invisible. If such a solenoid were to carry a flux of2π/e, when the flux leaked out from one of its ends it would be indistinguishable from a monopole.
Dirac's monopole solution in fact describes an infinitesimal line solenoid ending at a point, and the location of the solenoid is the singular part of the solution, the Dirac string. Dirac strings link monopoles and antimonopoles of opposite magnetic charge, although in Dirac's version, the string just goes off to infinity. The string is unobservable, so you can put it anywhere, and by using two coordinate patches, the field in each patch can be made nonsingular by sliding the string to where it cannot be seen.
In a U(1) gauge group with quantized charge, the group is a circle of radius2π/e. Such a U(1) gauge group is calledcompact. Any U(1) that comes from agrand unified theory (GUT) is compact – because only compact higher gauge groups make sense. The size of the gauge group is a measure of the inverse coupling constant, so that in the limit of a large-volume gauge group, the interaction of any fixed representation goes to zero.
The case of the U(1) gauge group is a special case because all itsirreducible representations are of the same size – the charge is bigger by an integer amount, but the field is still just a complex number – so that in U(1) gauge field theory it is possible to take the decompactified limit with no contradiction. The quantum of charge becomes small, but each charged particle has a huge number of charge quanta so its charge stays finite. In a non-compact U(1) gauge group theory, the charges of particles are generically not integer multiples of a single unit. Since charge quantization is an experimental certainty, it is clear that the U(1) gauge group of electromagnetism is compact.
GUTs lead to compact U(1) gauge groups, so they explain charge quantization in a way that seems logically independent from magnetic monopoles. However, the explanation is essentially the same, because in any GUT that breaks down into a U(1) gauge group at long distances, there are magnetic monopoles.
The argument is topological:
The holonomy of a gauge field maps loops to elements of the gauge group. Infinitesimal loops are mapped to group elements infinitesimally close to the identity.
If you imagine a big sphere in space, you can deform an infinitesimal loop that starts and ends at the north pole as follows: stretch out the loop over the western hemisphere until it becomes a great circle (which still starts and ends at the north pole) then let it shrink back to a little loop while going over the eastern hemisphere. This is calledlassoing the sphere.
Lassoing is a sequence of loops, so the holonomy maps it to a sequence of group elements, a continuous path in the gauge group. Since the loop at the beginning of the lassoing is the same as the loop at the end, the path in the group is closed.
If the group path associated to the lassoing procedure winds around the U(1), the sphere contains magnetic charge. During the lassoing, the holonomy changes by the amount of magnetic flux through the sphere.
Since the holonomy at the beginning and at the end is the identity, the total magnetic flux is quantized. The magnetic charge is proportional to the number of windingsN, the magnetic flux through the sphere is equal to2πN/e. This is the Dirac quantization condition, and it is a topological condition that demands that the long distance U(1) gauge field configurations be consistent.
When the U(1) gauge group comes from breaking acompact Lie group, the path that winds around the U(1) group enough times is topologically trivial in the big group. In a non-U(1) compact Lie group, thecovering space is aLie group with the sameLie algebra, but where all closed loops arecontractible. Lie groups are homogeneous, so that any cycle in the group can be moved around so that it starts at the identity, then its lift to the covering group ends atP, which is a lift of the identity. Going around the loop twice gets you toP2, three times toP3, all lifts of the identity. But there are only finitely many lifts of the identity, because the lifts can't accumulate. This number of times one has to traverse the loop to make it contractible is small, for example if the GUT group is SO(3), the covering group is SU(2), and going around any loop twice is enough.
This means that there is a continuous gauge-field configuration in the GUT group allows the U(1) monopole configuration to unwind itself at short distances, at the cost of not staying in the U(1). To do this with as little energy as possible, you should leave only the U(1) gauge group in the neighborhood of one point, which is called thecore of the monopole. Outside the core, the monopole has only magnetic field energy.
Hence, the Dirac monopole is atopological defect in a compact U(1) gauge theory. When there is no GUT, the defect is a singularity – the core shrinks to a point. But when there is some sort of short-distance regulator on spacetime, the monopoles have a finite mass. Monopoles occur inlattice U(1), and there the core size is the lattice size. In general, they are expected to occur whenever there is a short-distance regulator.
In the universe, quantum gravity provides the regulator. When gravity is included, the monopole singularity can be a black hole, and for large magnetic charge and mass, the black hole mass is equal to the black hole charge, so that the mass of the magnetic black hole is not infinite. If the black hole can decay completely byHawking radiation, the lightest charged particles cannot be too heavy.[30] The lightest monopole should have a mass less than or comparable to its charge innatural units.
So in a consistent holographic theory, of whichstring theory is the only known example, there are always finite-mass monopoles. For ordinary electromagnetism, the upper mass bound is not very useful because it is about same size as thePlanck mass.
In mathematics, a (classical) gauge field is defined as aconnection over aprincipal G-bundle over spacetime.G is the gauge group, and it acts on each fiber of the bundle separately.
Aconnection on aG-bundle tells you how to glue fibers together at nearby points ofM. It starts with a continuous symmetry groupG that acts on the fiberF, and then it associates a group element with each infinitesimal path. Group multiplication along any path tells you how to move from one point on the bundle to another, by having theG element associated to a path act on the fiberF.
In mathematics, the definition of bundle is designed to emphasize topology, so the notion of connection is added on as an afterthought. In physics, the connection is the fundamental physical object. One of the fundamental observations in the theory ofcharacteristic classes inalgebraic topology is that many homotopical structures of nontrivial principal bundles may be expressed as an integral of some polynomial overany connection over it. Note that a connection over a trivial bundle can never give us a nontrivial principal bundle.
A principalG-bundle overS2 is defined by coveringS2 by twocharts, eachhomeomorphic to the open 2-ball such that their intersection is homeomorphic to the stripS1×I. 2-balls are homotopically trivial and the strip is homotopically equivalent to the circleS1. So a topological classification of the possible connections is reduced to classifying the transition functions. The transition function maps the strip toG, and the different ways of mapping a strip intoG are given by the firsthomotopy group ofG.
So in theG-bundle formulation, a gauge theory admits Dirac monopoles providedG is notsimply connected, whenever there are paths that go around the group that cannot be deformed to a constant path (a path whose image consists of a single point). U(1), which has quantized charges, is not simply connected and can have Dirac monopoles while, itsuniversal covering group,is simply connected, doesn't have quantized charges and does not admit Dirac monopoles. The mathematical definition is equivalent to the physics definition provided that—following Dirac—gauge fields are allowed that are defined only patch-wise, and the gauge field on different patches are glued after a gauge transformation.
The total magnetic flux is none other than the firstChern number of the principal bundle, and depends only upon the choice of the principal bundle, and not the specific connection over it. In other words, it is a topological invariant.
This argument for monopoles is a restatement of the lasso argument for a pure U(1) theory. It generalizes tod + 1 dimensions withd ≥ 2 in several ways. One way is to extend everything into the extra dimensions, so that U(1) monopoles become sheets of dimensiond − 3. Another way is to examine the type of topological singularity at a point with the homotopy groupπd−2(G).
In more recent years, a new class of theories has also suggested the existence of magnetic monopoles.
During the early 1970s, the successes ofquantum field theory andgauge theory in the development ofelectroweak theory and the mathematics of thestrong nuclear force led many theorists to move on to attempt to combine them in a single theory known as aGrand Unified Theory (GUT). Several GUTs were proposed, most of which implied the presence of a real magnetic monopole particle. More accurately, GUTs predicted a range of particles known asdyons, of which the most basic state was a monopole. The charge on magnetic monopoles predicted by GUTs is either 1 or 2gD, depending on the theory.
The majority of particles appearing in any quantum field theory are unstable, and they decay into other particles in a variety of reactions that must satisfy variousconservation laws. Stable particles are stable because there are no lighter particles into which they can decay and still satisfy the conservation laws. For instance, the electron has alepton number of one and an electric charge of one, and there are no lighter particles that conserve these values. On the other hand, themuon, essentially a heavy electron, can decay into the electron plus two quanta of energy, and hence it is not stable.
The dyons in these GUTs are also stable, but for an entirely different reason. The dyons are expected to exist as a side effect of the "freezing out" of the conditions of the early universe, or asymmetry breaking. In this scenario, the dyons arise due to the configuration of thevacuum in a particular area of the universe, according to the original Dirac theory. They remain stable not because of a conservation condition, but because there is no simplertopological state into which they can decay.
The length scale over which this special vacuum configuration exists is called thecorrelation length of the system. A correlation length cannot be larger thancausality would allow, therefore the correlation length for making magnetic monopoles must be at least as big as the horizon size determined by themetric of the expandinguniverse. According to that logic, there should be at least one magnetic monopole per horizon volume as it was when the symmetry breaking took place.
Cosmological models of the events following theBig Bang make predictions about what the horizon volume was, which lead to predictions about present-day monopole density. Early models predicted an enormous density of monopoles, in clear contradiction to the experimental evidence.[31][32] This was called the "monopole problem". Its widely accepted resolution was not a change in the particle-physics prediction of monopoles, but rather in the cosmological models used to infer their present-day density. Specifically, more recent theories ofcosmic inflation drastically reduce the predicted number of magnetic monopoles, to a density small enough to make it unsurprising that humans have never seen one.[33] This resolution of the "monopole problem" was regarded as a success ofcosmic inflation theory. (However, of course, it is only a noteworthy success if the particle-physics monopole prediction is correct.[34]) For these reasons, monopoles became a major interest in the 1970s and 80s, along with the other "approachable" predictions of GUTs such asproton decay.
Many of the other particles predicted by these GUTs were beyond the abilities of current experiments to detect. For instance, a wide class of particles known as theX and Y bosons are predicted to mediate the coupling of the electroweak and strong forces, but these particles are extremely heavy and well beyond the capabilities of any reasonableparticle accelerator to create.
Experimental searches for magnetic monopoles can be placed in one of two categories: those that try to detect preexisting magnetic monopoles and those that try to create and detect new magnetic monopoles.
Passing a magnetic monopole through a coil of wire induces a net current in the coil. This is not the case for a magnetic dipole or higher order magnetic pole, for which the net induced current is zero, and hence the effect can be used as an unambiguous test for the presence of magnetic monopoles. In a wire with finite resistance, the induced current quickly dissipates its energy as heat, but in asuperconducting loop the induced current is long-lived. By using a highly sensitive "superconducting quantum interference device" (SQUID) one can, in principle, detect even a single magnetic monopole.
According to standard inflationary cosmology, magnetic monopoles produced before inflation would have been diluted to an extremely low density today. Magnetic monopoles may also have been produced thermally after inflation, during the period of reheating. However, the current bounds on the reheating temperature span 18 orders of magnitude and as a consequence the density of magnetic monopoles today is not well constrained by theory.
There have been many searches for preexisting magnetic monopoles. Although there has been one tantalizing event recorded, byBlas Cabrera Navarro on the night of February 14, 1982 (thus, sometimes referred to as the "Valentine's Day Monopole"[35]), there has never been reproducible evidence for the existence of magnetic monopoles.[13] The lack of such events places an upper limit on the number of monopoles of about one monopole per 1029nucleons.
Another experiment in 1975 resulted in the announcement of the detection of a moving magnetic monopole incosmic rays by the team led byP. Buford Price.[12] Price later retracted his claim, and a possible alternative explanation was offered byLuis Walter Alvarez.[36] In his paper it was demonstrated that the path of the cosmic ray event that was claimed due to a magnetic monopole could be reproduced by the path followed by aplatinum nucleusdecaying first toosmium, and then totantalum.
High-energy particle colliders have been used to try to create magnetic monopoles. Due to the conservation of magnetic charge, magnetic monopoles must be created in pairs, one north and one south. Due to conservation of energy, only magnetic monopoles with masses less than half of the center of mass energy of the colliding particles can be produced. Beyond this, very little is known theoretically about the creation of magnetic monopoles in high-energy particle collisions. This is due to their large magnetic charge, which invalidates all the usual calculational techniques. As a consequence, collider-based searches for magnetic monopoles cannot, as yet, provide lower bounds on the mass of magnetic monopoles. They can however provide upper bounds on the probability (or cross section) of pair production, as a function of energy.
TheATLAS experiment at theLarge Hadron Collider currently has the most stringent cross section limits for magnetic monopoles of 1 and 2 Dirac charges, produced throughDrell–Yan pair production. A team led byWendy Taylor searches for these particles based on theories that define them as long lived (they do not quickly decay), as well as being highly ionizing (their interaction with matter is predominantly ionizing). In 2019 the search for magnetic monopoles in the ATLAS detector reported its first results from data collected from the LHC Run 2 collisions at center of mass energy of 13 TeV, which at 34.4 fb−1 is the largest dataset analyzed to date.[37]
TheMoEDAL experiment, installed at the Large Hadron Collider, is currently searching for magnetic monopoles and large supersymmetric particles using nuclear track detectors and aluminum bars aroundLHCb'sVELO detector. The particles it is looking for damage the plastic sheets that comprise the nuclear track detectors along their path, with various identifying features. Further, the aluminum bars can trap sufficiently slowly moving magnetic monopoles. The bars can then be analyzed by passing them through a SQUID.
Since around 2003, variouscondensed-matter physics groups have used the term "magnetic monopole" to describe a different and largely unrelated phenomenon.[18][19]
The monopoles studied by condensed-matter groups have none of these properties. They are not a new elementary particle, but rather are anemergent phenomenon in systems of everyday particles (protons,neutrons,electrons,photons); in other words, they arequasi-particles. They are not sources for theB-field (i.e., they do not violate∇⋅B = 0); instead, they are sources for other fields, for example theH-field,[5] the "B*-field" (related tosuperfluid vorticity),[6][41] or various other quantum fields.[42] They are not directly relevant togrand unified theories or other aspects of particle physics, and do not help explaincharge quantization—except insofar as studies of analogous situations can help confirm that the mathematical analyses involved are sound.[43]
There are a number of examples incondensed-matter physics where collective behavior leads to emergent phenomena that resemble magnetic monopoles in certain respects,[17][44][45][46] including most prominently thespin ice materials.[5][47] While these should not be confused with hypothetical elementary monopoles existing in the vacuum, they nonetheless have similar properties and can be probed using similar techniques.
Some researchers use the termmagnetricity to describe the manipulation of magnetic monopole quasiparticles inspin ice,[48][49][47][50] in analogy to the word "electricity".
One example of the work on magnetic monopole quasiparticles is a paper published in the journalScience in September 2009, in which researchers described the observation ofquasiparticles resembling magnetic monopoles. A single crystal of thespin ice materialdysprosium titanate was cooled to a temperature between 0.6kelvin and 2.0 kelvin. Using observations ofneutron scattering, the magnetic moments were shown to align into interwoven tubelike bundles resemblingDirac strings. At thedefect formed by the end of each tube, the magnetic field looks like that of a monopole. Using an applied magnetic field to break the symmetry of the system, the researchers were able to control the density and orientation of these strings. A contribution to theheat capacity of the system from an effective gas of these quasiparticles was also described.[16][51]This research went on to win the 2012 Europhysics Prize for condensed matter physics.
In another example, a paper in the February 11, 2011 issue ofNature Physics describes creation and measurement of long-lived magnetic monopole quasiparticle currents in spin ice. By applying a magnetic-field pulse to crystal of dysprosium titanate at 0.36 K, the authors created a relaxing magnetic current that lasted for several minutes. They measured the current by means of the electromotive force it induced in a solenoid coupled to a sensitive amplifier, and quantitatively described it using a chemical kinetic model of point-like charges obeying the Onsager–Wien mechanism of carrier dissociation and recombination. They thus derived the microscopic parameters of monopole motion in spin ice and identified the distinct roles of free and bound magnetic charges.[50]
Insuperfluids, there is a fieldB*, related to superfluid vorticity, which is mathematically analogous to the magneticB-field. Because of the similarity, the fieldB* is called a "synthetic magnetic field". In January 2014, it was reported that monopole quasiparticles[52] for theB* field were created and studied in a spinor Bose–Einstein condensate.[6] This constitutes the first example of a quasi-magnetic monopole observed within a system governed by quantum field theory.[43]
Updates to the theoretical and experimental searches in matter can be found in the reports by G. Giacomelli (2000) and by S. Balestra (2011) in the Bibliography section.
^For the convention where magnetic charge has the weber as unit, seeJackson 1999. In particular, for Maxwell's equations, see section 6.11, equation (6.150), page 273, and for the Lorentz force law, see page 290, exercise 6.17(a). For the convention where magnetic charge has units of ampere-meters, seearXiv:physics/0508099v1, eqn (4), for example.
^Wen, Xiao-Gang; Witten, Edward, "Electric and magnetic charges in superstring models",Nuclear Physics B, Volume 261, pp. 651–677
^S. Coleman, "The Magnetic Monopole 50 years Later", reprinted inColeman, Sidney (February 26, 1988).Aspects of Symmetry: Selected Erice Lectures. Cambridge: Cambridge University Press.ISBN978-0521318273.
^abPrice, P. B.; Shirk, E. K.; Osborne, W. Z.; Pinsky, L. S. (August 25, 1975). "Evidence for Detection of a Moving Magnetic Monopole".Physical Review Letters.35 (8):487–490.Bibcode:1975PhRvL..35..487P.doi:10.1103/PhysRevLett.35.487.
^ab"Magnetic monopoles spotted in spin ices",Physics World, September 3, 2009. "Oleg Tchernyshyov at Johns Hopkins University [a researcher in this field] cautions that the theory and experiments are specific to spin ices, and are not likely to shed light on magnetic monopoles as predicted by Dirac."
^abGibney, Elizabeth (January 29, 2014). "Quantum cloud simulates magnetic monopole".Nature.doi:10.1038/nature.2014.14612.S2CID124109501.This is not the first time that physicists have created monopole analogues. In 2009, physicists observed magnetic monopoles in a crystalline material called spin ice, which, when cooled to near-absolute zero, seems to fill with atom-sized, classical monopoles. These are magnetic in a true sense, but cannot be studied individually. Similar analogues have also been seen in other materials, such as in superfluid helium. ... Steven Bramwell, a physicist at University College London who pioneered work on monopoles in spin ices, says that the [2014 experiment led by David Hall] is impressive, but that what it observed is not a Dirac monopole in the way many people might understand it. 'There's a mathematical analogy here, a neat and beautiful one. But they're not magnetic monopoles.'
^Griffiths, David J. (2013).Introduction to electrodynamics (Fourth ed.). Boston: Pearson. p. 339.ISBN978-0-321-85656-2.
^Alvarez, Luis W."Analysis of a Reported Magnetic Monopole". In Kirk, W. T. (ed.).Proceedings of the 1975 international symposium on lepton and photon interactions at high energies. International symposium on lepton and photon interactions at high energies, Aug 21, 1975. p. 967. Archived fromthe original on February 4, 2009. RetrievedMay 25, 2008.
^Magnetic Monopoles, report fromParticle data group, updated August 2015 by D. Milstead and E.J. Weinberg. "To date there have been no confirmed observations of exotic particles possessing magnetic charge."
^Arttu Rajantie (2016)."The search for magnetic monopoles".Physics Today.69 (10): 40.Bibcode:2016PhT....69j..40R.doi:10.1063/PT.3.3328.Magnetic monopoles have also inspired condensed-matter physicists to discover analogous states and excitations in systems such as spin ices and Bose–Einstein condensates. However, despite the importance of those developments in their own fields, they do not resolve the question of the existence of real magnetic monopoles. Therefore, the search continues.
^abGiblin, S. R.; Bramwell, S. T.; Holdsworth, P. C. W.; Prabhakaran, D.; Terry, I. (February 13, 2011). "Creation and measurement of long-lived magnetic monopole currents in spin ice".Nature Physics.7 (3):252–258.Bibcode:2011NatPh...7..252G.doi:10.1038/nphys1896.
^D.J.P. Morris; D.A. Tennant; S.A. Grigera; B. Klemke; C. Castelnovo; R. Moessner; C. Czter-nasty; M. Meissner; K.C. Rule; J.-U. Hoffmann; K. Kiefer; S. Gerischer; D. Slobinsky & R.S. Perry (September 3, 2009) [2009-07-09]. "Dirac Strings and Magnetic Monopoles in Spin Ice Dy2Ti2O7".Science.326 (5951):411–4.arXiv:1011.1174.Bibcode:2009Sci...326..411M.doi:10.1126/science.1178868.PMID19729617.S2CID206522398.