Resonant threshold twophoton $e^e^+$ pair production onto the lowest Landau levels in a strong magnetic field
Abstract
The process of electronpositron pair production by two photons in a strong magnetic field has been studied. The process kinematics is considered, and the probability amplitude for arbitrary polarizations of particles is found. The resonance conditions are established, and the resonant crosssection is estimated in the case where the electron and the positron occupy the lowest levels ( 1, 0) that satisfy these resonance conditions.
pacs:
12.20.m, 13.88.+e539.1.01 \razd\seci
M.M. Dyachenko, O.P. Novak, R.I. Kholodov
I Introduction
The researches of quantum electrodynamic (QED) processes that take place at the collisions of heavy ions have a challenging character, which is associated with the progress achieved in the domain of heavyion accelerators. In such experiments, the main attention is usually concentrated on the researches dealing with properties of the strong interaction. However, the QED processes can also be studied even if nuclei do not approach each other at the distance characteristic of the strong interaction Baur02 (); Baur07 ().
In the course of collisions between heavy ions, the extremely intensive, rapidly varying electromagnetic fields are generated. The resulting strength of the field can exceed the critical QED value Gs, which, according to the theoretical reasoning, is the vacuum excitation threshold Greiner (). This fact opens vast opportunities for testing the QED predictions in the range of strong fields. A wide program of such experiments is planned to be fulfilled on the future FAIR (Facility for Antiproton and Ion Research) installation, which is under construction on the basis of the GSI (GSI Helmholtz Centre for Heavy Ion Research, Darmstadt, Germany) CDR ().
The production of electronpositron pairs at the collisions between ions is a challenging problem from the theoretical and experimental viewpoints. In particular, the production of a pair with the electron in a bound state changes the charge of one of the ions and is one of the principal origins of beam losses in modern colliders. On the other hand, the pair production by a strong total supercritical field of heavy nuclei is the evidence of a bound state diving in the negative energy continuum, as well as of the transition of the vacuum into a new state Greiner ().
A poorly studied issue in the problem of pair production at the collision of moving ions is the influence of the magnetic field created by the ions. Simple estimates testify that the field between the ions can reach the critical value or can even exceed it already at collision energies of the Coulomb barrier order. However, in the majority of researches, only the Coulomb field of ions is taken into account. The attempts to reveal the influence of a magnetic field were made for the first time in works Soff81 (); Rumrich87 (); Soff88 () in the framework of the model of quasimolecule (for lowenergy collisions). The corresponding numerical calculations showed the absence of the effect; however, the interaction of the created pair with the magnetic field was not taken into consideration.
In work Fomin98 (), the assumption that the created electronpositron pair captures the magnetic field similarly to the phenomenon, where the magnetic field lines “are frozen” into a plasma, was substantiated. The corresponding estimates testify that the lifetime of the selfconsistent system “pair + magnetic field” considerably exceeds the nuclear transit time. Therefore, the magnetic field can substantially affect the process. The presence of characteristic resonances in the corresponding channels can be the observable evidence of QED processes in the magnetic field created by colliding ions.
It has to be noted that, in the EPOS and ORANGE experiments carried out at the GSI, anomalous peaks were revealed in the channel of electronpositron pair production Backe78 (); Koenig87 (); Cowan86 (). The nature of peaks was not elucidated, and their very existence was not confirmed. In view of the similarity between the spectrum of anomalous peaks and the quasiequidistant spectrum of electron energy levels in the magnetic field, it is quite probable that further researches of the role of a magnetic field in ionic collisions will deepen our understanding of this phenomenon.
According to the results of work Fomin98 (), the lifetime of the magnetic field substantially exceeds the characteristic time of electromagnetic interaction. Therefore, the process can be considered as the electronpositron pair production in a constant uniform magnetic field. This approximation allows one to reveal the main features of the process and, at the same time, to obtain simple analytical expressions for the crosssection. Moreover, if the energy of ions is sufficiently high, the conditions for the application of the equivalentphoton method LandauIV () are satisfied. Hence, in the simplest case, our problem is approximately reduced to the study of the process of twophoton electronpositron pair production in a magnetic field.
Let us also mention possible applications of the results of this work to the problem of electron cooling of heavyion beams. The essence of the method consists in a decrease of the effective beam temperature owing to the collision of ions in the beam with electrons that move together with the beam and possess a small spread of velocities Budker78 (); Meshkov94 (); Parkhomchuk00 (). Although the method of electron cooling has been known for a long time and is widely used in accelerating facilities, the experimentally observed difference between the cooling efficiency for positive and negative particles remains unexplained Dikanskii88 (). In particular, the electron cooling of an antiproton beam is planned to be used in the HESR accumulator (FAIR), and this fact substantiates the problem urgency Galnander09 (); Bazhenov03 ().
The application of the method of quantum field theory to the problem of electron cooling Larkin59 (); Akhiezer61 () has considerable advantages in comparison with others (the method of pair collisions, the dielectric model, and so forth), because it contains no phenomenological parameters. The corresponding stopping power is expressed in terms of the polarization operator. The difference between the cooling of protons and antiprotons may probably be described in the second Born approximation. However, according to the optical theorem, the imaginary part of the polarization operator in the second order is equal to the total probability of the process of twophoton pair production.
For the first time, the process of twophoton electronpositron pair production in a magnetic field was considered in work Ng77 () in the simplest case of the headon photon collision along the magnetic field. In work Kozlenkov86 (), this process was analyzed for an arbitrary direction of photon propagation, but under the assumption that the energy of each photon is insufficient for the pair production in the onephoton process. This condition excludes the possibility of the resonance character of the reaction.
In this work, in contrast to the earlier researches, the process was considered in the case where the energy of one of the photons or each of them is sufficient for the pair production. The total amplitude of the process with arbitrary polarizations of particles and the conditions for the resonant character of the process are determined. The process crosssection is estimated for the lowest Landau levels that satisfy the resonance conditions.
Throughout the work, the relativistic system of units, , is used.
Ii Kinematics
It is known LandauIV () that the electron occupies discrete energy levels in a uniform magnetic field,
(1) 
where is the longitudinal momentum component with respect to the field, the level number, and the magnetic field measured in the units of . In the magnetic field, the conservation laws of the energy and the momentum component parallel to the field are obeyed and have the following form for the process of twophoton electronpositron pair production:
(2) 
Here, is the total energy, and is the total longitudinal momentum of photons.
Let us determine the threshold conditions of the pair production onto some Landau levels and . First, let us introduce the auxiliary function . The process threshold is determined by the condition , where is the point of a maximum of the function. After the differentiation, we find the value of electron momentum at the maximum,
(3) 
In view of the previous relations, the threshold values of the energy and the electron and positron momenta are expressed as follows:
(4) 
(5) 
From whence, the condition for the reaction threshold takes the form
(6) 
In the general case (above the threshold), system (2) gives the following expression for the momenta of particles:
(7) 
Here, the notations
(8) 
(9) 
(10) 
were introduced. The process is evidently impossible, if both photons move in parallel to , because in this case, and condition (6) is not satisfied. This situation is illustrated in Fig. 1.
Note that the Lorentz transformations along do not change the magnetic field itself. Therefore, without any loss of generality, the reference frame can be chosen to exclude the longitudinal momentum of photons: . In this reference frame, , and the threshold conditions have a simpler form,
(11) 
Iii Amplitude
The electron and positron wave functions look likeFomin00 ()
(12) 
where ,
(13) 
(14) 
Here, is the normalization area, the Hermite function, are the doubled spin projections of the electron and the positron, the normalization constants, and the constant bispinors:
(15) 
(16) 
(17) 
where the sign “” in corresponds to the electron. The wave functions (12)–(14) correspond to the gauge of the electromagnetic 4potential.
For the wave function of the initial photon, the standard expression is used LandauIV (),
(18) 
where is the normalization volume, is the 4vector of photon polarization, and
(19) 
Here, and are the azimuthal and polar angles, respectively; and and are polarization parameters.
where ’s are Dirac gamma matrices,
(22) 
(23) 
(24) 
The argument of Hermite functions in Eq. (21) looks like
and the primed function means its dependence on .
According to the QED rules, the twophoton electronpositron pair production amplitude is determined as
(25) 
where the primed quantities depend on . Figure 2 demonstrates the Feynman diagrams that correspond to amplitude (25). Substituting the wave functions and the propagator into Eq. (25) and carrying out the corresponding transformations, we obtain the amplitude in the form
(26) 
where the terms look like
Here, are the components of the photon polarization vectors, and the following notations are introduced:
(27) 
(28) 
(29) 
(30) 
where are determined by Eq. (17). The functions are typical of QED problems with the magnetic field Klepikov54 (); FIAN ():
(31) 
(32) 
(33) 
(34) 
(35) 
(36) 
where are the azimuthal angles of photons, and is the degenerate hypergeometric function. The term that corresponds to the exchange diagram is obtained by swapping the subscripts: .
Iv Resonance Conditions
The process acquires a resonant character if its kinematics permits an onshell virtual electron state, i.e. if the quantities and satisfy the standard relation between the electron energy and the momentum in a magnetic field,
(37) 
In this case, the denominator in propagator (20) vanishes. In order to avoid the resulting divergence, the radiation width of a virtual state, , is introduced according to the Breit–Wigner prescription Graziani95 (),
(38) 
Let us determine the resonance frequencies of photons in the ultraquantum approximation corresponding to the conditions
(39) 
Note that those conditions are characteristic of subcritical fields. We confine the consideration to the case where both photons propagate normally to the magnetic field, and their energy is close to the threshold one, i.e.
(40) 
Then, expression (7) for the momentum simplifies,
(41) 
Taking into account that the conservation laws are satisfied at the diagram vertices, we use condition (37) to find the resonance frequencies for the first diagram,
(42) 
From whence, it is evident that the pair is produced by the hard photon, whereas the soft one stimulates the transition of a virtual electron between the Landau levels. This result is not unexpected, because the process at the resonance can be regarded as the sequence of a onephoton pair production and a photon absorption.
V Resonant CrossSection
Let us estimate the resonant crosssection of the twophoton pair production in the ultraquantum approximation. Conditions (40)–(42) are supposed to be satisfied. In addition, let us select the energetically favorable particle polarizations Novak08 (); Novak09 () and the numbers of Landau levels that correspond to the lowest resonance:
(43) 
(44) 
In the sum over in amplitude (26), we keep only the resonant term with , in which the denominator tends to zero. In this case, the second diagram does not give a substantial contribution to the process, because the resonance conditions for it are not obeyed.
Taking the aforesaid, as well as expressions for resonance frequencies (42) and conditions (43) and (44), into account, let us expand amplitude (26) in a series in the small parameter . In the zeroorder approximation, we obtain
(45) 
According to the known QED rules, the process crosssection is determined as the squared probability amplitude multiplied by the interval of final states and divided by the flux , i.e.
(46) 
(47) 
where , is the time, and the angle between the photons.
The integration of Eq. (46) over can be executed with the help of functions. The process crosssection does not depend on . Therefore, the integration over is reduced to the multiplication of the expression by . Hence, there emerges a multiplier . According to work Klepikov54 (), we can get rid of it by identifying the normalization length with the coordinate of the Larmor orbit center, . Hence,
(48) 
The remaining integral over can be found using the relation
(49) 
In addition, let us express the quantities and in terms of the more convenient Stokes parameters,
(50) 
The ultimate expression for the resonant crosssection looks like
(51) 
where is the fine structure constant.
Vi Conclusions
Let us analyze the obtained expression (51) and demonstrate that the resonant crosssection can be factorized into the probabilities of the firstorder processes. In the ultraquantum approximation, the probabilities of the onephoton pair production and the magnetobremsstrahlung look like Novak09 ()
(52) 
(53) 
(here, conditions (37), (43), and (44) were used). Hence, the process crosssection (51) can be written in the form of Breit–Wigner formula,
(54) 
At last, let us evaluate crosssection (51) in the case of the headon collision of photons (). As an example, we choose the following values of parameters:
(55) 
(56) 
Then the radiation width and the crosssection approximately equal
(57) 
(58) 
М.М. Дяченко, О.П. Новак, Р.I. ХолодовПОРОГОВЕ РЕЗОНАНСНЕ
ДВОФОТОННЕ
НАРОДЖЕННЯ ПАРИ В СИЛЬНОМУ
МАГНIТНОМУ ПОЛI
НА НАЙНИЖЧI РIВНI ЛАНДАУ В роботi розглянуто процес народження
електронпозитронної пари двома фотонами в сильному
магнiтному полi. Дослiджена кiнематика та знайдена загальна
амплiтуда процесу з довiльною поляризацiєю частинок. Знайдено умови
резонансного перебiгу реакцiї та проведено оцiнку перерiзу для
випадку, коли електрон та позитрон займають найнижчi рiвнi ( 1, 0), що задовольняють умови резонансу.
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V.I. Ritus and A.I. Nikishov, Trudy Fiz. Inst. Akad. Nauk SSSR
111, 1 (1979).
Received 20.02.14.
Translated from Ukrainian by O.I. Voitenko