Dynamics of a magnetic monopole in matter, Maxwell equations in dyonic matter and detection of electric dipole moments

For a monopole, the analogue of the Lorentz equation in matter is shown to be f = g(H-v×D). Dual-symmetric Maxwell equations, for matter containing hidden magnetic charges in addition to electric ones, are given. They apply as well to ordinary matter if the particles possess T-violating electric dip...

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Datum:2001
Hauptverfasser: Artru, X., Fayolle, D.
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Veröffentlicht: Національний науковий центр «Харківський фізико-технічний інститут» НАН України 2001
Schriftenreihe:Вопросы атомной науки и техники
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spelling irk-123456789-794362015-04-02T03:01:58Z Dynamics of a magnetic monopole in matter, Maxwell equations in dyonic matter and detection of electric dipole moments Artru, X. Fayolle, D. Electrodynamics of high energies in matter and strong fields For a monopole, the analogue of the Lorentz equation in matter is shown to be f = g(H-v×D). Dual-symmetric Maxwell equations, for matter containing hidden magnetic charges in addition to electric ones, are given. They apply as well to ordinary matter if the particles possess T-violating electric dipole moments. Two schemes of experiments for the detection of such moments in macroscopic pieces of matter are proposed. 2001 Article Dynamics of a magnetic monopole in matter, Maxwell equations in dyonic matter and detection of electric dipole moments / X. Artru, D. Fayolle // Вопросы атомной науки и техники. — 2001. — № 6. — С. 110-114. — Бібліогр.: 3 назв. — англ. 1562-6016 PACS: 14.80.Hv 03.50.De 11.30.Er http://dspace.nbuv.gov.ua/handle/123456789/79436 en Вопросы атомной науки и техники Національний науковий центр «Харківський фізико-технічний інститут» НАН України
institution Digital Library of Periodicals of National Academy of Sciences of Ukraine
collection DSpace DC
language English
topic Electrodynamics of high energies in matter and strong fields
Electrodynamics of high energies in matter and strong fields
spellingShingle Electrodynamics of high energies in matter and strong fields
Electrodynamics of high energies in matter and strong fields
Artru, X.
Fayolle, D.
Dynamics of a magnetic monopole in matter, Maxwell equations in dyonic matter and detection of electric dipole moments
Вопросы атомной науки и техники
description For a monopole, the analogue of the Lorentz equation in matter is shown to be f = g(H-v×D). Dual-symmetric Maxwell equations, for matter containing hidden magnetic charges in addition to electric ones, are given. They apply as well to ordinary matter if the particles possess T-violating electric dipole moments. Two schemes of experiments for the detection of such moments in macroscopic pieces of matter are proposed.
format Article
author Artru, X.
Fayolle, D.
author_facet Artru, X.
Fayolle, D.
author_sort Artru, X.
title Dynamics of a magnetic monopole in matter, Maxwell equations in dyonic matter and detection of electric dipole moments
title_short Dynamics of a magnetic monopole in matter, Maxwell equations in dyonic matter and detection of electric dipole moments
title_full Dynamics of a magnetic monopole in matter, Maxwell equations in dyonic matter and detection of electric dipole moments
title_fullStr Dynamics of a magnetic monopole in matter, Maxwell equations in dyonic matter and detection of electric dipole moments
title_full_unstemmed Dynamics of a magnetic monopole in matter, Maxwell equations in dyonic matter and detection of electric dipole moments
title_sort dynamics of a magnetic monopole in matter, maxwell equations in dyonic matter and detection of electric dipole moments
publisher Національний науковий центр «Харківський фізико-технічний інститут» НАН України
publishDate 2001
topic_facet Electrodynamics of high energies in matter and strong fields
url http://dspace.nbuv.gov.ua/handle/123456789/79436
citation_txt Dynamics of a magnetic monopole in matter, Maxwell equations in dyonic matter and detection of electric dipole moments / X. Artru, D. Fayolle // Вопросы атомной науки и техники. — 2001. — № 6. — С. 110-114. — Бібліогр.: 3 назв. — англ.
series Вопросы атомной науки и техники
work_keys_str_mv AT artrux dynamicsofamagneticmonopoleinmattermaxwellequationsindyonicmatteranddetectionofelectricdipolemoments
AT fayolled dynamicsofamagneticmonopoleinmattermaxwellequationsindyonicmatteranddetectionofelectricdipolemoments
first_indexed 2025-07-06T03:29:08Z
last_indexed 2025-07-06T03:29:08Z
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fulltext DYNAMICS OF A MAGNETIC MONOPOLE IN MATTER, MAXWELL EQUATIONS IN DYONIC MATTER AND DETECTION OF ELECTRIC DIPOLE MOMENTS X. Artrua, D. Fayolleb aInstitut de Physique Nucléaire de Lyon IN2P3-CNRS & Université Claude Bernard, France e-mail: x.artru@ipnl.in2p3.fr bLaboratoire de Physique Corpusculaire de Clermont IN2P3-CNRS & Université Blaise Pascal, France For a monopole, the analogue of the Lorentz equation in matter is shown to be f = g(H-v×D). Dual-symmetric Maxwell equations, for matter containing hidden magnetic charges in addition to electric ones, are given. They apply as well to ordinary matter if the particles possess T-violating electric dipole moments. Two schemes of experiments for the detection of such moments in macroscopic pieces of matter are proposed. PACS: 14.80.Hv 03.50.De 11.30.Er 1. INTRODUCTION The question of which classical macroscopic fields exert a force on a magnetic monopole of charge g in matter is still controversial [1]. For the static force, the formula f = gH (1) instead of f = gB, is generally accepted. However, for the velocity dependent force, there is no consensus between f = -gv×E and f = -gv×D (we use rationalized equations with c=ε0=µ0=1). A more general problem is to generalize the macroscopic Maxwell equations to the dual-symmetric matter. The atoms or molecules of such a matter would be made not only of electrically, but also of magnetically charged particles. Thus they can possess • electric dipole moments coming from decentered electric charges as well as spinning magnetic charges • magnetic moments comming from spinning electric charges as well as decentered magnetic charges. After a rederivation and a discussion of Eq.(1), we will present below a consistent solution for the velocity- dependent force and the dual-symmetric Maxwell equations in matter, using simple physical arguments. We will consider only isotropic matter and assume that its electric and magnetic polarizations P and M are linear in D and B (or E and H). It will appear that our equations can also take into account the electric dipole moments (e.d.m.) of the ordinary fermions generated by T-violating interactions, and we will propose two kinds of possible measurements of the e.d.m. in macroscopic matter. 2. STATIC FORCE ON A MONOPOLE IN MATTER If the force acting on a monopole in matter were f = gB, a monopole following a closed magnetic line of a permanent magnet could gain energy at each turn, providing a perpetual motion of the first species. This is an argument for chosing f = gH, whose curl is zero for a static system. One might object that the monopole can gain energy at each turn at the expense of the magnetic energy stored by the magnet and will eventually erase the magnetization of the metal. This is indeed what happens when a monopole is circulating through a super- conducting loop : the varying flux of the monopole field through the loop produces a counter-electromotive force which damps the supercurrent. However, in the case of a ferroelectric annulus, the magnetized state has the lowest energy and the annulus cannot yield any energy to the monopole. Another argument for (1) comes from the (gedan- ken) following experiment: Let us measure the force on a magnetic charge immersed in a ferrofluid. The latter is a practical realization of a liquid magnetizable matter. No static frictional force can perturb the measurement. We protect the monopole from the fluid by a waterproof box. This should not change the result~; anyway the physical monopole is probably dressed by a swarm of ordinary particles. In the absence of the monopole, we denote by B ≡ µH the field outside the box and by Bbox = Hbox the field inside the box. The fields coming 110 PROBLEMS OF ATOMIC SCIENCE AND TECHNOLOGY. 2001, № 6, 110-114 from the monopole will be denoted by a prime. Let us consider two shapes of box (Fig.1): a) the box is elongated parallel to B. Then Bbox = H and the measured force is f = gH; b) the box is flattened perpendicular to B. Then Bbox = B. The force acting on the pole is f1 = gB, which is different from case a). On the other hand, in front of the box the total field Btot = B + B´ is larger than behind. The magnetic grains of the ferrofluid are therefore attracted toward this region and build a hydrostatic pressure which pushes the box backwards. Quantita-tively, the force acting on one grain of magnetic moment m in the nonuniform field Btot is tot jij tot ijji BmBmf ∂=∂= (2) since ∇×Btot = 0 for a static system. Repeated indices are summed over. The resulting macroscopic force by unit volume is Fig. 1. Force acting on a monopole in a ferrofluid. (a) elongated box parallel to the field (b) flattened box perpendicular to the field )BB( 2r3 tottot i tot ji tot j i BM d dF ⋅∂χ=∂= where Mtot = M+M´ = χ(B+B´)is the magnetization density and χ=(µ-1)/µ. This field of force builds the pressure p=(χ/2)Btot.Btot=(χ/2)(B2+B´2)+M.B´ The first two terms are symmetrical about the box and exert no net force on it. The last term gives f2=-∫(M.B´)dS=-∫(B´.dS)M=-gM Here dS is the vector representation of a surface element of the box and is directed outward. Permuting dS and M was allowed because they are parallel in the region where B’ is important. The last equality comes from Gauss theorem for magnetic charges. Adding f1 and f2 one recovers the result (1): f=f1+f2=g(B-M)=gH. (3) Most probably, (1) can be generalized to any shape of box. Thus, the relevant field which drives a monopole in matter is H. It is the field found in a parallel elongated cavity, as for the force f = eE driving an electric charge inside a dielectric. Mnemonic: this kind of cavity allows the test charge to follow the force without touching the matter. Eq. (1) allows trapping a (not too heavy) monopole in the pole of a permanent magnet, where the lines of gH converge from all directions. This would not be true for gB. MICROSCOPIC INTERPRETATION Atomic magnetic dipoles are often pictured as microscopic loops of electrical current. Then B appears as the average of the microscopic field b over semi- macroscopic volumes sufficiently large compared to the atomic scale. The work of b along a straight line L is therefore g∫Lb dl = g∫LB dl In contrast, the work along a line L’ which avoids passing through the loops is g∫L b dl = g∫L H dl . Eq. (1) implies that the monopole avoids passing through the microscopic current loops or more likely that the loops move to "dodge" the monopole. This was of course the case with the ferrofluid, but in solid matter the atoms cannot escape from the monopole trajectory. Does it means that (1) is false if the monopole goes through an atom? Not necessarily. At the approach of the pole, the electron wave functions are deformed and, if the monopole is sufficiently slow, they return adiabatically to the ground states. Thus no energy is exchanged between the monopole and the atom, as if the loop "dodges" the monopole. 3. VELOCITY-DEPENDENT FORCE In vacuum, the analog of the Lorentz force for a moving monopole is f = – gv×E. Accordingly, a piece dl of wire carrying a current I* of magnetic charges is subjected to the dual Laplace force df = – I*dl×E. Following the ferrofluid example, we consider a wire protected by a waterproof tube in a liquid dielectric (Fig. 2): a) the tube is flattened perpendicular to D = εE. Then Etube=D and the measured force is df = – I*dl×D. b) the tube is flattened parallel to D = εE. Then Etube=E. The force acting on the wire is df1 = – I*dl×E. On the other hand, on the right of the tube, the total field D + D’ is larger than on the left. The polar molecules are therefore attracted toward this region, building an excess of pressure which pushes the tube toward the left. Calculations like those between Eqs. (2) and (3) give the thrust df2 = – I*dl×P, where P is the macroscopic electric polarization. In total, df=df1+df2=– I*dl×(E+P) (4) 111 is equivalent to (4). Thus the field acting on a wire of magnetic current is D. It is the field found in a perpendicular flattened cavity, as for the Laplace force df = Idl×B on an ordinary current in a magnetized matter. Mnemonic: this cavity allows the wire to follow the force without touching the matter. For a moving monopole, (4) becomes f = – gv×D. (4') Fig. 2. Force acting on a wire carrying the dual current I*, in a dielectric liquid. The tube is flattened (a) perpendicular (b) parallel to the field MICROSCOPIC INTERPRETATION In a dielectric, E is the average of the microscopic field e over volumes sufficiently large compared to the molecular scale. The work of e when the wire sweeps a flat surface S is I*∫∫Se dS = I*∫∫SE dS In contrast, the work of e along a surface S’ which avoids cutting the dipole molecules is I*∫∫S e dS = I*∫∫S D dS Eq.(4) implies that a moving dual wire avoids cutting the dipole molecules, or that the molecules "dodge" the wire. This has a well-defined topological meaning. Let us recall however that this wire was introduced to make the problem time-independent. For a moving monopole, there is no swept surface and the topological interpretation is lost. Gathering (1) and (4'), the total force on a magnetic charge is f = g (H – v×D). (5) This result does not take into account dissipation and holds only for sufficiently slow monopoles, such that atoms and molecules evolve adiabatically under the influence of the monopole field. 4. MAXWELL EQUATIONS IN DYONIC MATTER We consider matter containing magnetic charges ±g bound in magnetically neutral molecules, in addition to ordinary particles. These molecules pass magnetic dipoles of the form gr, building a macroscopic magnetic polarization p* (r is the north-south charge separation). If they have spin, they also possess electric dipoles of the form γ*S building a macroscopic electric polarization m* (γ* is the "giro-electric" ratio). p* and m* are dual respectively to the polarization p and the magnetization m built by the ordinary particles. The dual-symmetric Maxwell equations for the space average of the microscopic fields are jje-b t δ+=∂×∇ δ ρρ +=⋅∇ e *j*jb-e t δ+=∂×− ∇ **e δ ρρ +=⋅∇ Here (ρ, j) is the external ordinary charge-current density and (δρ, δj) the induced one, given by δρ = –∇.p δj = ∇×m + ∂tp Similarly, for the magnetic charge analogues, δρ*= –∇.p* δj* = ∇×m*+∂tp* From these equations, we can write the dual-symmetric Maxwell equations in matter: ∇×H–∂tD = j ∇.D = ρ –∇×E-∂tB = j* ∇.B = ρ* (6) where H = b – m, D = ē + p as usual, but E = ē – m* and B = b + p*. We see that E and B can no more be interpreted as the spatial averages of the microscopic fields. In that sense they are no more "fundamental" than D and H. In fact the dual of E is not B but H, whereas the dual of B is D. The usual relations D = E + P, B = H + M (7) are recovered, defining P ≡ p + m*, M ≡ m + p* (8) It means that the microscopic nature of the dipole is forgotten at the level of the macroscopic Maxwell equations. Only their long range fields in 1/r3 are relevant. As in ordinary matter, E and H are the fields found in elongated cavities parallel to the respective fields, whereas D and B are found in perpendicular flat cavities. 5. THE DYONIC PERMITTIVITY- PERMEABILITY MATRIX We assume that the polarizations P and M respond linearly to the macroscopic fields D and B. [ ] [ ]     =    =    H E B D M P 'χχ (9) 112 with [1+χ´]≡[1–χ]–1. In ordinary matter χ11=χe=χe´/ε , χe´≡ε-1; χ22=χm=χm´/µ, χm´≡µ-1, and χ12=χ21=0. In a matter containing only one species of dyon (e,g)and antidyon (– e, – g) bound in polar molecules, P = p and M = p* are linked by ge *pp = , j i j i B p gD p c ∂ ∂= ∂ ∂ 11 (10) wherefrom [ ]     = 2 2 geg egeC teχ . (11) An analogous matrix, with e ↔ g, is obtained with dipoles coming from spinning dyons (m/e = m*/g). We note that [χ] and [χ´] are symmetrical matrices. This remains true for a mixture of different species of molecules. Thus, the usual relations D = εE, B = µH are replaced by [ ]     −=    B D H E χ1 (12) The speed of light is c = (det[1-χ])1/2 (cvac.≡ 1) (13) Whatever they come from, the nondiagonal elements of [χ] violate P- and T- symmetries, since they connect vector to pseudovectors. However PT is conserved. 6. ENERGY-MOMENTUM TENSOR The various components of the energy-momentum tensor Θµν can be derived from energy and momentum conservation in simple physical systems. Let us suppose that the whole space is filled with dual-symmetric matter. To get Θi0 (energy flow) and Θij (momentum flow) one considers a sandwich made of three slab-like regions of the z coordinate, R1 = [– a, 0], R2 = [0, b] and R3 = [b, b + a]. R1 carries uniform electric and magnetic charge-current densities, {ρ, j; ρ*, j*} and R3 carries the opposite densities, such that the fields vanish outside the sandwich. Solving (6) and (12) with appropriate ρ , j; ρ*, j*, any kind of uniform field configuration {E, D; H, B} can be obtained in R2. These fields are linearly attenuated in R1 and R3. In R3 a power r3dtd dW = E.j + H.j* (14) is dissipated and a force r f 3d d = ρE + j × B + ρ*H – j* × D (15) is exerted per unit of volume. The same quantities per unit of area (integrated over z in R3) give Θz0 and Θzi in R2. To get Θ00 (energy density) and Θ0i (momentum density) one has to "rotate" the sandwich in the 4- dimensional space-time, replacing z by t and slabs by time-slices or "epoch" T1, T2, T3.During T1 the (3- dimensional) space is filled with uniform current densities j and j*, which progressively build uniform fields according (6) and (12). The second epoch is current-free and the uniform fields remain constant. The last epoch destroys the fields with opposite currents. Integrating (14) and (15) over t in T3 give Θ00 and Θ0i in T2. This method is detailled in [2]. One obtains     −−Θ× ×⋅+⋅ =Θ jijiij HBEDδ µ ν 00 )(2/1 HE BDBHDE (16) as in ordinary matter. The Dirac condition in matter. One way to derive the Dirac condition between an electron and a monopole is to quantize the joint angular momentum of their fields which are 34 r erD π = , 34 r erB π = where r (resp. r´) is the distance from the charge (resp. the pole) to the observation point. According to (15) the momentum density is Θ0i = (D×B)i, from which one gets the angular momentum J = ∫∫∫d3r r×(D×B)=(eg/4π) n̂ (17) where n̂ is the unit vector from the charge toward the pole. The usual Dirac condition eg = 2nπħ is obtained from the quantization rule J. n̂ = n ħ/2. Note that if the momentum density were E×H, as sometimes advocated (see the discussion in [3]), the Dirac condition in medium would not be consistent with that in vacuum. 7. APPLICATION TO THE SEARCH FOR AN ELECTRIC DIPOLE MOMENT The dual-symmetric formalism applies as well to the case were the electron (or the nucleus) possesses an electric dipole moment (e.d.m.) d  = γ*S in addition to the usual magnetic moment m = γ*S .Then we have m/ γ= m*/γ* and a nondiagonal [χ] matrix element is generated, like with dyonic molecules (Eqs.10-11): [ ]         += mm mme r rr χχ χχχχ 2 (18) where r ≡ γ*/γ. χm = (η-1)/η comes from the spinning electrons and χe = (ε-1)/ε from polar molecules. A nonzero χ may be generated in another way~: the e.d.m. tends to align the spin of an electron along the internal electric field of a polar molecule. It couples m to p. Here we consider only the first mechanism. Eq.(18) suggests two possible measurements of r: a) In Fig.3a, a cylinder of magnetizable, but insulating, material is immersed in a large magnetic field B0. The inside field B induces a small electric polarization P = χm r B and an electric field E.If the cylinder is much broader than high, we have B = B0, D ≅ 0 and E ≅ – P. More generally one has 〈E〉 = – xχm r B0 (19) where the coefficient x < 1 depends on the container geometry. Let us take a cubic container of size L. Between the top and the bottom, we can measure a potential difference U = EL. The ratio between the stored electrostatic energy W = (1/2)ε E2L3 and the magnetic one W0 = (1/(2µ)) 2 0B L3 is W/W0 = εµ (xχmr)2. (20) in terms of common units and r16 = 1016r, we have tesla B metre Lrx volt U m 0 16 8103 χ−⋅= , 113 2 0 3 2 16 228105.2          ⋅= − tesla B metre Lrx eV W mε χ . [useful relations are:1tesla = 3.108 volt/metre, 1(tesla)2 (metre)3 = 0.8.106joule, 1eV = 1.6.10-19 joule ≅ 104 kelvin = 5.106 ħ/metre and γe = eħ/me =4⋅10−11 e⋅cm]. Let us assume r = 1016, which corresponds to an electron e.d.m. of 2.10-27 e × cm, ε ~1, χm ~ 0.5 and x ~ 0.5. For a field of 1 tesla, and a cube of 1 meter, a potential difference of about 0.5.10-8 volt is obtained, W ~ 10-9 eV ~ 10-5 kelvin. The voltmetre has to be cooled at least to this temperature to prevent thermal noise. Fig. 3. Scheme of e.d.m. search in macroscopic matter. (a) container in a magnetic field; a small potential difference is measured with the voltmetre V. (b) container in an electric field; a small magnetic flux is measured with a SQUID b) In Fig. 3b the same container is put in a large electric field E0. Using the second matrix of (9) [ ]     − ≅ mm m r r '' '1 ' χε χ ε χε χ , (18′) with χm´≡ µ – 1,we predict a small magnetization M = ε χ´m rE. If the cylinder is much higher than broad, we have E ≅ E0, H ≅ 0 and B ≅ M. For a cubic container we assume B ≅ – x ε χ´m r E0 (21) with x ~ 0.5. This field can be measured by a SQUID encircling the container. The phase shift of the wave function in one loop is ϕ =eL2B/ħ =0.5.10-4x ε χm´r16 metrevolt E metre L /105 0 2      . This phase can be multiplied by a large number of turns around the cylinder. The ratio between the output (magnetostatic) energy W and the input (electric) one W0 is still given by (20), but W and W0 are typically 105 times smaller and the temperature must be much lower than in case a). 8. CONCLUSION We have given arguments that the macroscopic fields acting on magnetic charges and currents are H and D. Comparing with electric charges and currents, one has a unified mnemonic principle: in each case, the acting field is the one found in a parallel-elongated (resp. flat-perpendicular) cavity in which a charge (resp. current wire) can follow the force without touching the medium. In a classical microscopic picture, a monopole avoids passing through the microscopic current loops and a dual current wire avoids cutting the dipole molecules. Quantum mechanically, it means that the perturbation of the atoms and molecules lying on the trajectory of the monopole is adiabatic. This should be the case at low enough velocity in a liquid. The monopole will be presumably accompanied by a swarm of atoms magnetically (or electrically, for a dyon) bound to it. In a solid, such a swarm could forbid the monopole to move without producing cracks. The dual-symmetric Maxwell equations in matter are formally unchanged, but E and B can no more be interpreted as the spatial averages of the microscopic fields. The duality correspondance is E → H and D → B. When dyons are present, or when ordinary particles possess electric dipole moments, ε and µ are replaced by a permittivity-permeability matrix [1-χ] whose nondiagonal elements violate the P- and T- symmetries (but not PT). The energy momentum tensor is also unchanged. The usual Dirac condition eg = 2nπħ is obtained provided the momentum density is D × B. These results have been obtained under the hypothesis that P and M are linear in the fields. As an application of the dual-symmetric formalism, two possible measurements of the electron e.d.m. have been suggested. They are at the limit of the present technological possibilities. However, mechanisms like the m – p coupling in a polar molecule mentioned in Sect. 7 might enhance the signal. REFERENCES 1. Y. Hara. Electromagnetic force on a magnetic monopole // Phys. Rev. 1985, v. A32, p. 1002-1006. 2. D. Fayolle. Dynamique d'un monopôle magnétique dans la matière, LYCEN/9961, July 1999 (unpublished). 3. F.N.H. Robinson. Electromagnetic stress and momentum in matter // Phys. Rep. 1975, v. C16, p. 313-354. 114