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					 Journal of Electromagnetic Analysis and Applications, 2013, 5, 294-301  http://dx.doi.org/10.4236/jemaa.2013.57046 Published Online July 2013 (http://www.scirp.org/journal/jemaa)  Physical Interpretation of the Dirac Neutrino with  Electromagnetic Mass*  Héctor Torres-Silva    Escuela de Ingeniería Eléctrica Electrónica, Universidad de Tarapacá, Arica, Chile.  Email: htorres@uta.cl    Received April 6th, 2013; revised May 6th, 2013; accepted May 14th, 2013    Copyright © 2013 Héctor Torres-Silva. This is an open access article distributed under the Creative Commons Attribution License,  which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.  ABSTRACT  The usual choice of an orthogonal set of four plane-wave solutions of the free-particle Dirac equation does not lend it- self readily to direct and complete physical interpretation in the case of Dirac neutrino particle. A different choice of  solutions can be made which yields a direct physical interpretation at all energies. Besides the separation of positive and  negative energy states there is a further separation of states for which the spin is respectively parallel or antiparallel to  the direction of the momentum vector. This can be obtained from the Maxwell’s equation without charges and current  in the  H configuration. Scenery of our study is at high temperature T where coexist electron-positron pair and  neutrino-antineutrino pair, (i.e., ). Taking into consideration the possibility of negative mass, we can de- scribe the observed behavior of antimatter in response to electromagnetic fields by assuming that the anti Dirac neutrino  has a negative mass, so a new causal symmetry can be obtained.  1MeVT   Keywords: Chiral Neutrino; Dirac Equation; Maxwell System  1. Introduction  Neutrino electromagnetic properties, which are the main  subject of this paper, are of particular importance be- cause they provide a kind of bridge to “new physics”  beyond the standard model. In spite of reasonable efforts  in studies of neutrino electromagnetic properties, up to  now there is no experimental confirmation in favour of  non vanishing neutrino electromagnetic characteristics.  [1]. The group of elementary particles called neutrinos  (denoted by the greek letter “ ”) belongs to the lepton  family (together with electrons, muons and tauons). They  are electrically neutral and travel close to the speed of  light. There are three (known) flavours, or types, of neu-  trinos, electron neutrino   e , muon neutrino    and  tau neutrino   , all with their corresponding antiparti-  cles. All neutrino interactions are mediated by the weak  nuclear force (and of course gravitation) [2].    Electron neutrinos, muon neutrinos, and tau neutrinos  that can morph into one another. For example, when  cosmic rays strike the atmosphere, they create particles  called muons that decay much as neutrons do, to produce  muon neutrinos [3]. The muon neutrinos can then “oscil-  late” or “mix” into other flavors before reaching Earth, as  observed in 1998 by physicists using a detector Super-  Kamiokande in Japan. Electron neutrinos from the sun  also change flavor, as physicists at the Sudbury Neutrino  Observatory in Canada showed in 2001 [4].    This means that neutrinos interact weakly via the elec-  tromagnetic force at all, and this makes them very diffi-  cult to detect for us. The cross section of a typical neu-  trino is very small, and it is therefore able to pass though  ordinary matter very easily [5].  The mass of the neutrinos is not well known. Meas-  urements of the speed of neutrinos have failed to show  that they move slower than the speed of light, which in-  dicate no or an extremely small mass. However, evidence  for neutrino oscillation demands that neutrinos have  masses [6]. Neutrino oscillation enables neutrinos of one  flavour to change into another flavour. This happens with  a certain probability that is proportional to the difference  of the square of the masses. Since these flavour oscilla-  tions have been observed, neutrinos are believed to have  very small but non zero rest masses and that neutrinos  generally are relativistic (their energy is much larger than  their rest mass) [7].  *This work has been supported by the Proyecto Mayor 8731-13, 2013  of the Universidad de Tarapacá, Chile. In the course of the recent development of knowledge  Copyright © 2013 SciRes.                                                                               JEMAA  Physical Interpretation of the Dirac Neutrino with Electromagnetic Mass 295 on neutrino mixing and oscillations, supported by the  discovery of flavor conversions of neutrinos from differ-  ent sources, non-trivial neutrino electromagnetic proper-  ties seem to be very plausible [8].  In particular, right-handed neutrinos constitute a com-  mon new physics proposal, usually linked to the genera-  tion of neutrino masses. This is particularly interesting  nowadays, ever since we gathered compelling evidence  that neutrinos do have masses, that they lie well below  the other fermions’ ones, and that their mixing patterns  differ extraordinarily from those of the quark sector (for  a review on the matter of neutrino masses see, for exam-  ple, [1]). The most straightforward way to construct a  mass term for the neutrinos within the SM is just to rely  on the Higgs mechanism, and so to write the corre-  sponding Yukawa couplings; for that aim, one needs  some fermionic felds which carry no SM charge: right-  handed neutrinos. However, we do not know whether  neutrinos are Dirac or Majorana.  If they are Dirac, the smallness of the neutrino mass  scale remains unexplained, for it would be just a product  of the smallness of the corresponding Yukawa couplings.  In order to provide such an explanation, many models  and mechanisms have been proposed: in the so-called  see-saw models, the lightness of the neutrino mass scale  is a consequence of the heaviness of another scale. For  instance, this scale is the lepton-number-violating (LNV)  Majorana mass of the extra right-handed neutrinos in  type I see-saw [9]. Although some of these proposals do  not require right-handed neutrinos, for the sake of gener-  ality it is a good idea to consider their possible involve-  ment in the generation of neutrino masses.  The existence of a relic sea of neutrinos is a generic  feature of the standard hot big bang model, in number only  slightly below that of relic photons that constitute the  cosmic microwave background (CMB). This cosmic neu-  trino background (CNB) has not been detected yet, but it  presence is indirectly established by the accurate agree-  ment between the calculated and observed primordial  abundances of light elements, as well as from the analysis  of the power spectrum of CMB anisotropies and other  cosmological observables. In this introduction we will  summarize the evolution and main properties of the CNB.  Neutrinos are kept in equilibrium at high temperatures  by reaction involving radiation and weak nuclear force.  To keep the analysis as simple as possible, consider the  reaction where a strong electromagnetic wave (photon) in  its own reference frame, is split into two chiral photons  producing a electron-positron pair which collide to form  a tau neutrino-antitau neutrino pair  ee    .  At sufficiently high temperature the reverse reaction is  also possible. Hence the neutrinos are held in equilibrium.  While coupled to the rest of the primeval plasma (rela-  tivistic particles such as electrons, positrons, and photons),  neutrinos had a momentum spectrum with an equilibrium  Fermi-Dirac form with temperature T      1 ,exp 1 eq fpTpT      As the universe cools, the weak interaction rate  nc    falls below the expansion rate and one says  that neutrinos decouple from the rest of the plasma.  2 G     is the cross section of the electron-neutrino  processes with  G the Fermi constant and n  is the  neutrino number density. An estimate of the decoupling  temperature dec  can be found by equating the thermally T averaged value of the weak interaction rate   with the  expansion rate given by the Hubble parameter H (the  Hubble time   1 t  represents an upper limit to the  age of the Universe).  83 M      Here  is the total energy density, dominated by  4 T   relativistic particles, and 12 1 P G is the Planck mass.  If we approximate the numerical factors to unity, with  25 GT F   and   2 TM, we obtain the rough es- timate 1M dec TeV  (see Fi gure 1).  Although neutrino decoupling is not described by a  unique dec , it can be approximated as an instantaneous T process. The standard picture of instantaneous neutrino  decoupling is very simple (see e.g., [2]) and reasonably  accurate. In this approximation, the spectrum in   , eq pT  is preserved after decoupling, because both       Figure 1. Photon and neutrino temperatures during the  process of annihilations: evolution of their decrease with  the expansion a of the universe which is normalized to a (1  MeV).  Copyright © 2013 SciRes.                                                                               JEMAA  Physical Interpretation of the Dirac Neutrino with Electromagnetic Mass  296  neutrino momenta and temperature redshift identically  with the expansion of the universe. Shortly after neutrino  decoupling the temperature drops below the electron mass,  favouring  annihilations that heat the photons. If one e assumes that this entropy transfer did not affect the neu-  trinos because they were already completely decoupled, it  is easy to calculate the change in the photon temperature  before any  annihilation and after the electron-posi- e tron pairs disappear by assuming entropy conservation of  the electromagnetic plasma. Here, we quote the result  between T  and T  [2]  13 after before 11 1.40102 4 TT T T         which is also the ratio between the temperatures of relic  photons and neutrinos.  One can see in Figure 1 how in this epoch the photon  temperature decreases with the expansion less than the  inverse of the scale factor . Instead the temperature of  the decoupled neutrinos always falls as  a 1a. Our interest  is to study the electromagnetic process for the conversion    ee       at . This paper is  structured as follows. In Section 2 we start by reviewing  the Dirac equation under chiral representation. In Section  3 we obtain the Dirac equation deduced from Maxwell’s  equations with  1MeVT H applied to neutrino at   which can provide light neutrino masses under a chiral  electromagnetic mechanism. Section 4 discusses the chi-  ral electromagnetic neutrino.  1MeVT 2. Chiral Dirac Neutrino Equation  Plane-wave solutions of the Dirac equation are well  known, and it would appear to be necessary to justify a  reconsideration of this problem related with Dirac neu-  trino particles. The justification lies in the fact that the  solutions found in journals and elsewhere do not lend  themselves readily to a direct physical interpretation. In  the usual treatment of the problem, four mutually or-  thogonal solutions are obtained for a given value of the  momentum p, two of which correspond to positive en-  ergy and two to negative energy. However, the physical  distinction between a pair of solutions belonging to the  same energy does not appear until one considers the low  energy approximation in which the small components of  the state function are neglected and the two solutions  reduce to eigenfunctions of   belonging to eigenval-  ues .  1 The original Dirac equation is   2 ˆˆ cpmci t              (1a)  where ψ = ψ(r, t) is a complex four-component field ψ  that Dirac thought of as the wave function for the electron,  r and t are the space and time coordinates, m is the rest  mass of the electron,  is the momentum operator, c is  the speed of light speed, and  is the reduced Planck  constant Planck (h/2π). Furthermore,  ˆ p  ˆ  is a vector  operator whose components are 4 × 4 matrices:   123 ˆ,,  , and    is another 4 × 4 matrix.    In the usual notation, the Dirac Hamiltonian for a free  particle is [10]  2 ˆˆ cpmc   .          (1b)  This Hamiltonian commutes with the momentum vec-  tor , and the usual procedure is to seek simultaneous  eigenfunctions of H and p. These eigenfunctions are,  however, not uniquely determined, and for given eigen-  values of H and p, there remains a twofold degeneracy.  In order to resolve this degeneracy we seek a dynamical  variable which commutes with both H and . Such a  variable is  ˆ p ˆ p ˆˆ p , where ˆ  is the matrix Pauli. It is ob-  vious that this variable commutes with . To verify that  it also commutes with H, we write 11 ˆ p ˆˆˆ  , and  recalling that   commutes with operator ˆ , we have     11 ˆˆ ˆˆˆˆˆˆ0 cpp pcp    ,    (2)  since 1  commutes with ˆ .  We now proceed to find simultaneous eigenfunctions  of the commuting variables H, p and ˆˆ p . We have,  since the components of p commute,   22 ˆˆ pp  ,              (3)  where p is the magnitude of the momentum vector. Thus  for a simultaneous eigenstate of  and  ˆ pˆˆ p , the  value of ˆˆ p  will be +p or –p, corresponding to states  for which the spin is parallel or antiparallel, respectively,  to the momentum vector.  A simultaneous eigenfunction of H and p will have the  form of a plane wave [10]      ,exp, 1,2,3,4 jj rtip rWtj      ,  (4)  where    are the four components of the wave function  and   are four numbers to be determined. In the ar-  gument of the exponential function, p represents the ei-  genvalues of the components of the momentum for this  state and W the corresponding eigenvalue of H. The  possibility of positive mass and negative mass is for-  mally consistent with the positive and negative solutions  to the equations of the Special Theory of Relativity when  combined with quantum mechanics [11]. Then  can  have either of the two values.  W  1 2 242 2 Wmccp .            (5)  In Equation (5)  is the relativistic momentum and   is the invariant mass. There are two solutions to  Equation (5); a positive solution and a negative solution.  p m Copyright © 2013 SciRes.                                                                               JEMAA  Physical Interpretation of the Dirac Neutrino with Electromagnetic Mass 297 Dirac [11] described these as the “wanted” and “un-  wanted” solutions, respectively [12]. Pauli [13] consid-  ered that only the positive energy solutions had meaning.  By contrast, here in connection with Dirac neutrino we  interpret both the positive and negative energy solutions  to be real solutions that represent substances with posi-  tive mass and negative mass, respectively.  Antimatter was first detected by observing the tracks  left by positive electrons or positrons in cloud chambers  caused by the movement of particles with an apparent  charge-to-mass ratio   em   that was opposite in sign to  that of electrons [14-16]. Related to Dirac neutrino, as we  will show below, the anti Dirac neutrino could be de-  scribed as a negative mass and uncharged particle. To do  that, we now demand that   be also an eigenfunction  of ˆˆ p  belonging to one of the eigenvalues , say,  where . Employing the usual matrix representa-  tion for  p p ˆ p , we have  ˆˆ xy xy z ppip ppip p        .          (6)  In the above matrix,  p,  pand  p are operators,  but since this matrix is to operate on an eigenfunction of  p, the operators can be replaced by their eigenvalues. We  shall, without risk of confusion, use the same symbols for  the eigenvalues as for the corresponding operators.  The eigenvalue equation  ˆˆ pp ,              (7)  yields the following four equations:      12 12 34 34 zxy xy z zxy xy z ppip p pipp p ppip p pipp p 1 2 3 4           .         (8)  These equations are satisfied by    12 34 , , xy z xy z pippp pip pp , ,              (9)  where   is a number still to be determined (The con-  sistency of the equations is readily verified, recalling that  ).  pp We now make use of the requirement that   be an  eigenfunction of H belonging to the eigenvalue .     Then  W  0WH  ;             (10)  that is,   2 1ˆˆ 0Wc pmc      .        (11)  In terms of chiral matrices  ˆ , in Equation (11)  we replace ˆˆ p   by its eigenvalue to obtain   2 10Wcpmc  .          (12)  On expansion, we obtain      2 12 2 21 2 34 2 43 Wc p mc Wcpmc Wcp mcc Wcpmc   0 0 0 0           .        (13)  This system of equations is the chiral Dirac equation   0 ch imc               (13’)  The condition EW  ensures the consistency of  these equations. Comparing Equation (13) with Equation  (9), we find  2 2 Wcpmc Wcp mc     .           (14)  We can now write the components of   as follows:   exp jj iprWth  ,          (15)    where   is given by     1 2 3 4       2 2 , , , . xy z xy z pip pp Wcppipmc Wcppp mc              (16)  Since  can be given either of the two values  W W   and , the two values  p p , we have found for given p  four linearly independent plane wave solutions. It is eas-  ily verified that they are mutually orthogonal.  The physical interpretation of the solutions is now  clear. Each solution represents a homogeneous beam of  Dirac neutrino particles of definite momentum p, of defi-  nite energy, either W , and with the spin polarized ei-  ther parallel or antiparallel to the direction of propagation.  This condition can be obtained if we consider the Max-  well’s equations under a chiral approach [17-19]. Solu-  tions   of Equations (9) and (16) are still undeter-  mined because we need to link them with chiral Maxwell  equations. In the next section, solutions   will be re-  lated with the chiral electrodynamics when  H.  3. Dirac Neutrino Equation Deduced from  Maxwell’s Equations with  H  Here we show that it is possible to transform the Max-  well equation from six real components to four complex  components and in this form to obtain two spinor equa-  tions in the Weyl or chiral representation. First, we will  Copyright © 2013 SciRes.                                                                               JEMAA  Physical Interpretation of the Dirac Neutrino with Electromagnetic Mass  298  consider the Maxwell equations for a sourceless anisot-  ropic chiral homogeneous medium. Following [20,21],  with the time variation as:   1 tt c T   and c T is  as a chiral parameter, the Maxwell’s equations without  charges are expressed as:   11 tc rot T c    E,          (17)  0div E                 (18)   11 tc rot T c   H,         (19)  0div H                 (20)  Here, ,  rot   is the frequency and  is the  light velocity. Application of rot to (17) and (19) allows  us to write the wave equation for  c ,   or  .    22 22 2 2 2 2 1 0. c tt c t T rot rotrot cc Trotrot c             (21)  This chiral wave equation represents an equation of  fourth order. Here we consider the condition    22 22 1 c T ct       0 0            (22)  where Equation (21) is transformed from a fourth order  equation to a first order one.    2 c Trot              (23)  and the electric field is parallel to the magnetic field  i H. The linear Beltrami Equation (23), will be used  to construct the Dirac neutrino equation in chiral or Weyl  representation.  In [14], it was shown that the ordinary Dirac equation  is equivalent to the chiral quaternionic equation     0 cc DD        with 3  1 1 : cD ic mc  1      and the Maxwell Eq-  uations (17)-(22) are equivalent to the chiral Equation  (23) when the electric field   is parallel to the mag-  netic field     i H. Multiplying Equation (23) by  ˆ i  we have   ˆˆ 20 c iTirot     that is, with 0    ˆˆ ˆ 20 c iT    .  From this equation we can separate   ˆˆˆ 20 cc iT T   EE ,0 ,0    ˆˆ ˆ 20 cc iT T   HH  Let   ˆˆ , RL iE iH    ,     T 10 , and making ,1 tc iTc   and 2 c Tmc we  obtain   1 0ˆ L ic mc        (24)   1 0ˆ R ic mc  .       (25)  Equations (24) and (25) are equivalent to the quarter-  nionic chiral Dirac equation obtained in reference [14],  here  mm  is the Dirac neutrino mass. Solutions of  (24) and (25) may be called the Beltrami fields (see, e.g.,  [21]). R and L, subscripts are associated with circularly  polarized photons (right or left-handed spirals or chiral  photons), that is photons that have closed trajectories to  form standing waves that generate mass. The Dirac neu-  trino equation in chiral or Weyl representation is [15],   0 ch imc             (26)  In the chiral Dirac neutrino field   T , RL ,    and   are two different types of 2-component spinor,  they respectively correspond to the nonequivalent repre-  sentations (1/2, 0) and (0, 1/2) of the Lorentz group, and  the chiral Dirac neutrino equation presents a relation be-  tween the two spinors. If we consider parity, then it is no  longer sufficient to consider the 2-component spinors    and    separately, but the 4-component spinor     This 4-component spinor is an irreduci- ble representation of the Lorentz group extended by par- ity (i.e., the (1/2, 0) ⊕ (0, 1/2) representation).     T , RL  . Now we are in conditions of compare Equation (13’)  with Equation (26) and show that the dirac neutrino par-  ticle with mass generated by the  H configuration.    2 2 xy z xy z EE E cEE Wmc cEE Wmc                 E E E          (27)  where the electric field is given by 2 Wmc e  E and  W  T .  As c is positive or negative we can generalize the  product c as pT 2 c pT . For a massive Dirac neu-  trino, the electric and magnetic fields are 90˚ out of phase,  the energy density is constant and proportional to     222 2 0 44Gk   EH2 F  .   We find in SI units, that    . Here c is the critical  field for neutrino-antineutrino pair equivalent to the elec-  tron-positron pair production given by   2 2291 1 0 41.310 c kFEEm   E Copyright © 2013 SciRes.                                                                               JEMAA  Physical Interpretation of the Dirac Neutrino with Electromagnetic Mass 299 23 11181 1.3 10 Vm ce Emce    .       (28)  That is equivalent to . Observations indi-  cate that neutron stars have magnetic fields higher than   so neutrino-antineutrino pair is generated. In this  form we have a close connection between the Dirac neu-  trino equation and the Maxwell’s equation, with a direct  and complete physical interpretation in the  12 1.310G 12 10 G H T  con-  figuration. Here we are obtained a clear connection be-  tween the Planck constant , the quiral factor c, and  the electromagnetic mass which can be positive or nega-  tive according to .   c It is well known that matter and antimatter respond to  electromagnetic radiation in opposite ways. For example,  if an electron (Dirac neutrino) moves one way in an elec-  tromagnetic field, a positron (Dirac anti neutrino) will  move in the opposite way. We apply our theory of posi-  tive and negative mass to matter and antimatter and sug-  gest that it is productive to consider matter as having a  positive mass (+chirality) and antimatter as having a  negative mass (−chirality). The equations presented here,  which treat matter as having a positive mass and anti-  matter as having a negative mass, can account for the  experimental observations of matter and antimatter in  chiral electromagnetic fields. Our treatment allows the  symmetry between matter and antimatter to be treated in  a more causal manner.  T Taking into consideration the possibility of negative  mass, we can describe the observed behavior of antimat-  ter in response to electromagnetic fields by assuming that  the positron (anti Dirac neutrino) has a negative mass.  Given that particles and antiparticles respond oppositely  to an input of various forms of electromagnetic energy,  we considered the possibility that the mass can be con-  sidered in a causal symmetry. Taking into account the  concept of relative time, particularly the relativity of the  direction of time to describe antimatter, we now suggest  a more causal symmetry between matter and antimatter.  That is, instead of using CPT symmetry [22], where  matter is antisymmetrical with antimatter in terms of its  charge (C), parity (P) and direction in time (T), we sug-  gest that matter is antisymmetrical with antimatter in  terms of its mass, parity and time.  part conjantipart PT MPT .        (29)  So the combined MPT operations leaves invariant the  Dirac Equation (1)      2 2 : ˆˆ ˆˆ particle MPT cpmci t cpmc it              (30)  In the chiral representation also can be show that the  Dirac neutrino equation is invariant.  4. Chiral Electromagnetic Neutrino   Dirac introduced the concept of antiparticles, [23]. Now  we know that for every particle there is an antiparticle.    However some particles could be self-conjugate, in the  sense that particle and antiparticle could be the same. Of  course such particles have to be electrically neutral.  The possibility of a self-conjugate fermion was first  pointed out by Majorana [24], and hence they are called  Majorana fermions while the other fermions (with dis-  tinct particles and antiparticles) are called Dirac fermions,  Equations (24) and (25) [25]. Among the fermions of the  Standard Model, only neutrinos are electrically neutral  and hence qualify to be Majorana particles. But it is still  an open question whether neutrinos are Majorana parti-  cles or Dirac particles. In our theory we can discriminate  this situation if 1 2 c Tmc  with , RL mm or   3 2 c Tmc  with  mm  respectively.  If neutrinos are Majorana particles, lepton number L is  not conserved and this opens the door to generate an ex-  cess of leptons over antileptons in the early universe  which can subsequently generate an excess of baryons  over antibaryons, thus explaining how after annihilation  of most of the particles with antiparticles, a finite but  small residue of particles was left, to make up the present  Universe.   Equations (24) and (25) support the see-saw mecha-  nism to explain why the neutrino masses, although not  zero, are so tiny.The seesaw mechanism is a generic  model used to understand the relative sizes of observed  neutrino masses, of the order of eV. See‐saw mechanism  maybe the reason for the smallness of the masses.  *Provides an explanation for the smallness of the neu-  trino masses;  *0 L m   is natural, since a   mass term is forbid-  den by the SM symmetries;  * m, generated by the Higgs mechanism can be taken  the order of the charged lepton masses;  * m is not “protected” by the SM symmetries, and  can be taken large.  With our theory, using Equations (24) and (25) it is  possible to obtain a matrix mass  LD R mm mm        .             (31)  If  with  1eVm   D we obtain two Majo-  rana particles, an electron neutrino light  and a  sterile heavy one  mm  1eV   1TeV R. In addition to the non-  zero neutrino masses and mixing angles, the nonzero  magnetic moment  m  is another property of neutrinos  beyond the standard model of particle physics. The im-  Copyright © 2013 SciRes.                                                                               JEMAA  Physical Interpretation of the Dirac Neutrino with Electromagnetic Mass  300  portance of   was first mentioned by Pauli [18]. Sys-  tematic theoretical studies of neutrino electromagnetic  properties started after it was shown that in the extended  Standard Model with right-handed neutrinos the mag-  netic moment of a massive neutrino is, in general, non-  vanishing and that its value is determined by the neutrino  mass [26].  If neutrinos have a nonzero magnetic moment, it leads  to precession between left and right-handed neutrinos in  sufficiently strong magnetic fields [27]. In general,  nondiagonal elements of the magnetic moment matrix are  possible and neutrinos can be changed into different fla-  vours and chiralities, see Equations (24) and (25). Fur-  thermore, with the additional effect of coherent forward  scattering by matter, neutrinos can be resonantly con-  verted into those with different chiralities.  For a neutrino mass smaller than 1 eV, a Dirac neu-  trino has a non-zero magnetic moment proportional to  the neutrino mass, that yields a very small value for the  magnetic moment, 19 310   . As 2em  .  From our theory, the Bohr magneton is proportional to  c so in this case we have T8 10 c   Tecm  ). From  data obtained of astrophysics (considering the cooling of  red giant stars), we obtain    12 11 3 103 100.1 c Tm        corresponding to neutrino  . There is a gap of some  orders of magnitude between the present experimental  limits 11 12 10 10   15 10   [28], on neutrino magnetic  moments and the predictions of different extensions of  the Standard Model which hint at a range    14 10    [29]. The main problem in distin-  guishing Dirac from Majorana neutrino is the lack of  neutrino with positive helicity. One way is to reverse the  spin of the neutrino in an external magnetic field. The  problem is that we need large neutrino magnetic mo-  ments and large magnetic field to obtain visible effects.  However with our theory it is possible to reverse the spin  using laser technology to have sufficient energy density  to generate Dirac neutrino [30].    2 22291 41.310 ei HEE m     GE ei .  Here ei  is the critical field for electron positron  production  E18 1 1.3 10EVm  T . We think that by mea-  suring the chirality c of the processes, we may have an  improvement in the study of electromagnetic properties  of neutrinos.    An example is the modeling of neutrinos propagation  during core-collapse supernovae where very strong mag-  netic fields are believed to exist and in which the influ-  ence of neutrino electromagnetic properties has not yet  been taken into account. Equation (24) is well suited to  study the electromagnetic properties of neutrinos and  Majorana particles such as charge conjugation and time  reversal, allowing for an experimental study of our Equa-  tions (24)-(26).    5. Conclusions  The two-component Dirac neutrino equation, coming in  two related forms (24) and (25) that are connected by a  spin flip, represents the simplest possible covariant rela-  tivistic wave equation for a massive fermion. These two  forms represent the two irreducible representations of the  Lorentz group in terms of Pauli spinors and matrices.  Also the Dirac neutrino equation can directly be derived  by linearization of Equation (8), a procedure which leads  to (24) and (25) without explicit recourse to the Dirac  theory. An important characteristic of neutrino electro-  magnetic properties is that they are different from Dirac  and Majorana neutrinos. In particular, Majorana neutri-  nos cannot have diagonal magnetic or electric moments.  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