Threshold electron-positron pair production by a polarized electron in a strong magnetic field

Resonant e⁺e⁻–-pair production by an electron in a magnetic field near the process threshold is analytically studied. Using the Nikishov's theorem we estimate the number of events in the magnetic field equivalent to laser wave in the SLAC experiment. The obtained estimate is in reasonable agree...

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Автори: Novak, O.P., Kholodov, R.I.
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Опубліковано: Institute of Applied Physics NAS of Ukraine 2012
Назва видання:Вопросы атомной науки и техники
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Цитувати:Threshold electron-positron pair production by a polarized electron in a strong magnetic field / O.P. Novak, R.I. Kholodov // Вопросы атомной науки и техники. — 2012. — № 1. — С. 102-104. — Бібліогр.: 14 назв. — англ.

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spelling irk-123456789-1070052016-10-11T03:02:30Z Threshold electron-positron pair production by a polarized electron in a strong magnetic field Novak, O.P. Kholodov, R.I. Section B. QED Processes at High Energies Resonant e⁺e⁻–-pair production by an electron in a magnetic field near the process threshold is analytically studied. Using the Nikishov's theorem we estimate the number of events in the magnetic field equivalent to laser wave in the SLAC experiment. The obtained estimate is in reasonable agreement with the experimental data. Аналитически исследовано образование e⁺e⁻–-пары электроном в магнитном поле вблизи порога процесса. Произведена оценка числа событий в эксперименте SLAC с использованием теоремы Никишова. Полученное число событий согласуется с экспериментальными данными. Аналітично досліджено утворення e⁺e⁻–-пари електроном в магнітному полі поблизу порогу процесу. Одержана оцінка числа подій в експерименті SLAC з використанням теореми Нікішова. Знайдене число подій узгоджується з експериментальними даними. 2012 Article Threshold electron-positron pair production by a polarized electron in a strong magnetic field / O.P. Novak, R.I. Kholodov // Вопросы атомной науки и техники. — 2012. — № 1. — С. 102-104. — Бібліогр.: 14 назв. — англ. 1562-6016 PACS: 12.20.-m, 13.88.+e http://dspace.nbuv.gov.ua/handle/123456789/107005 en Вопросы атомной науки и техники Institute of Applied Physics NAS of Ukraine
institution Digital Library of Periodicals of National Academy of Sciences of Ukraine
collection DSpace DC
language English
topic Section B. QED Processes at High Energies
Section B. QED Processes at High Energies
spellingShingle Section B. QED Processes at High Energies
Section B. QED Processes at High Energies
Novak, O.P.
Kholodov, R.I.
Threshold electron-positron pair production by a polarized electron in a strong magnetic field
Вопросы атомной науки и техники
description Resonant e⁺e⁻–-pair production by an electron in a magnetic field near the process threshold is analytically studied. Using the Nikishov's theorem we estimate the number of events in the magnetic field equivalent to laser wave in the SLAC experiment. The obtained estimate is in reasonable agreement with the experimental data.
format Article
author Novak, O.P.
Kholodov, R.I.
author_facet Novak, O.P.
Kholodov, R.I.
author_sort Novak, O.P.
title Threshold electron-positron pair production by a polarized electron in a strong magnetic field
title_short Threshold electron-positron pair production by a polarized electron in a strong magnetic field
title_full Threshold electron-positron pair production by a polarized electron in a strong magnetic field
title_fullStr Threshold electron-positron pair production by a polarized electron in a strong magnetic field
title_full_unstemmed Threshold electron-positron pair production by a polarized electron in a strong magnetic field
title_sort threshold electron-positron pair production by a polarized electron in a strong magnetic field
publisher Institute of Applied Physics NAS of Ukraine
publishDate 2012
topic_facet Section B. QED Processes at High Energies
url http://dspace.nbuv.gov.ua/handle/123456789/107005
citation_txt Threshold electron-positron pair production by a polarized electron in a strong magnetic field / O.P. Novak, R.I. Kholodov // Вопросы атомной науки и техники. — 2012. — № 1. — С. 102-104. — Бібліогр.: 14 назв. — англ.
series Вопросы атомной науки и техники
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AT kholodovri thresholdelectronpositronpairproductionbyapolarizedelectroninastrongmagneticfield
first_indexed 2025-07-07T19:21:37Z
last_indexed 2025-07-07T19:21:37Z
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fulltext THRESHOLD ELECTRON-POSITRON PAIR PRODUCTION BY A POLARIZED ELECTRON IN A STRONG MAGNETIC FIELD O.P. Novak ∗and R.I. Kholodov Institute of Applied Physics NAS of Ukraine, Sumy, Ukraine (Received October 31, 2011) Resonant e+e−-pair production by an electron in a magnetic field near the process threshold is analytically studied. Using the Nikishov’s theorem we estimate the number of events in the magnetic field equivalent to laser wave in the SLAC experiment. The obtained estimate is in reasonable agreement with the experimental data. PACS: 12.20.-m, 13.88.+e 1. INTRODUCTION Quantum electrodynamic processes in strong mag- netic field keep their urgency for both theoretical and experimental study. Strong magnetic field modifies physical processes and allows new ones to occur, like e+e− pair production by a moving electron. The field strength is measured with respect to the so called critical Schwinger field Bc = m2c3/e� ≈ 4.4 · 1013 G. When magnetic field strength B is com- parable with the critical one, the quantum electrody- namical treatment of QED processes is necessary. Critical and subcritical magnetic fields are not feasible in laboratory conditions at present time. The strongest field was created using explosive genera- tors [1] and had the strength of about 30 MG, which is still much less than Bc. Nevertheless, neutron stars are believed to have surface magnetic fields within the range from 1012 G for radiopulsars to 1015 G for mag- netars. Thus, QED processes in magnetic field are of great importance in astrophysics. It is necessary to mention the possibility to study QED processes in subcritical magnetic field in exper- iments on heavy ion collisions [2]. If the impact para- meter has order of magnitude ∼ 10−10 cm, then mag- netic field of moving ions can approach magnitude of ∼ 1012 G in the region between the ions. These ex- periments could be carried out at the facilities like LHC or FAIR, which is under construction at the present time in GSI (Darmstadt, Germany). It is necessary to notice that reaction of e+e− pair production by an electron in intense laser field was experimentally studied at SLAC [3]. Up to 106 ± 14 events were reported to be observed in collisions of ∼ 50 GeV electron beam with terawatt laser pulses. In Ref. [4] this process was studied numerically. In the present work the second-order process of e+e− pair production by an electron in strong mag- netic field (see Figure) is analytically studied near the process threshold. Analytical expressions for the total process rate were obtained for subcritical mag- netic field strength B � Bc. It is shown, that the main contribution to the rate is determined by the resonant case in agreement with Refs. [3, 4]. 2p 1p p k 1p 2p +p p k +p Feynman diagrams of e+e−-pair production by an electron in the magnetic field. Double lines represent solutions of Dirac equation for the electron in the magnetic field 2. PROCESS RATE The process of e+e− pair production of electron in magnetic field can be described by two exchange Feynman graphs as on the Figure, where double lines represent solutions of Dirac equation in magnetic field. The calculations have been made in frame of Furry picture, thus the following condition should be satisfied: b = B Bc � 1. (1) The process is considered near the threshold, when the final particles occupy ground Landau levels and the initial electron energy is (hereinafter rela- tivistic units with � = c = 1 are used): E = 3m. (2) ∗Corresponding author E-mail address: novak-o-p@ukr.net 102 PROBLEMS OF ATOMIC SCIENCE AND TECHNOLOGY, 2012, N 1. Series: Nuclear Physics Investigations (57), p. 102-104. Thus, final spin states are determined. Lorentz transformation to the reference frame moving along magnetic field does not change the field, therefore without loss of generality one can set longi- tudinal momentum of the initial electron to zero pz = 0. The process probability amplitude reads: Sfi = iα ∫∫ d4xd4x′× × [ (Ψ̄2γ μΨ)Dμν(Ψ̄′ 1γ νΨ′ +)− −(Ψ̄1γ μΨ)Dμν(Ψ̄′ 2γ νΨ′ +) ] , (3) where Dμν is the photon propagator, Dμν = gμν (2π)4 ∫ d4k e−ik(x−x′) 4π kiki . (4) When process kinematics allows to be k2 = 0, then a resonant divergence arises. In this case the in- termediate photon becomes real and the interaction range goes to infinity [5]. The divergence was elimi- nated introducing small imaginary part into the prop- agator denominator using Breit-Wigner prescription: ω → ω − i Δ 2 , (5) where Δ is the corresponding state width. Nonres- onant contribution to the process is negligible com- pared to the resonant part. The general expressions for the process rate near the threshold with account of spin projections is ob- tained in Ref. [6]. Taking into account, that interfer- ence of the diagrams can be neglected, the rate takes on the following form: W+ ≈ α2m 3π2 √ 3l! Y, (6) W− ∼ bW+, (7) where superscript denotes the initial electron spin projection, α is fine structure constant, l is Landau level number of the initial electron, b = B/Bc, B is the magnetic field, Bc is the critical field, and Y = ∫∫ ds du ∣∣∣e−s2 D ∣∣∣2 , (8) D = ∫ (s + iq)l r2 − q2 e−q2−2iuqdq. (9) Here, the following notations are used: s = mΩ(x0 − x01), u = mΩ(x0 − x02), q = kx/m √ 2b, r2 = Ω2 − s2, Ω2 = 2/b, (10) x0, x01 and x02 are x-coordinates of classical orbit centers of initial and final electrons respectively, kx is x-component of intermediate photon momentum. The analysis shows, that the main contribution in the integral (9) is made by the summand with sl when r2 > 0 and the integrand has a singularity. Taking into account, that the quantity Δ is small, integration in Eqs. (9)-(8) can be carried out analyti- cally. After performing corresponding calculations it could be found that Y = bπ2 √ π Ω2le−2Ω2 Δ/m Γ(l + 1/2) l! , (11) where Γ(l + 1/2) is gamma-function. Averaging the rate over the initial electron spin projection, finally we obtain (in CGS units): W = α2 ( mc2 � ) b √ π 6 √ 3 Ω2le−2Ω2 Δ/m Γ(l + 1/2) (l!)2 . (12) In the resonant case, the total probability can be expressed via the product of the rates of the first- order processes of photon radiation and pair produc- tion by a single photon. Near the process threshold, when the condition E ≈ 3m is true and consequently bl = 4 and l � 1 are also valid, the process rate can be found in the following form: W = √ b 3 √ 6 We→γeWγ→ee+ Δ . (13) Here, We→γe and Wγ→ee+ are the rates of the corre- sponding first-order processes [7, 8]: We→γe = αm √ π Ω2le−Ω2 Γ(l + 1/2)l , (14) Wγ→ee+ = αm be−Ω2 √ 2 δE/m , (15) where δE = E − 3m ∼ mb is the kinematic factor. The intermediate photon width is determined mainly by the total radiation rate of the initial elec- tron. The radiation process was studied in a number of works, e. g. [8–13]. As an example, let us calculate the rate (12) when field strength is b = 0.1 (B ≈ 4.4 · 1012 G): Δ ≈ 7 · 1017s−1, (16) W = 7 · 103 s−1. (17) 3. DISCUSSION It should be noted, that according to Lorentz trans- formation arbitrary electromagnetic field goes to al- most equal crossed electric and magnetic fields in the rest frame of a relativistic particle. This means physical equivalence of any field configuration and electromagnetic wave, if the field changes slowly in comparison with characteristic electromagnetic time (∼ 10−21 s). The latter statement known as Nik- ishov theorem [14] allows to compare the result (12) with SLAC experiment on observation of e+e− pair production by electron in intense laser wave. 103 For this purpose one should calculate the rate (12) in the equivalent magnetic field Beq and carry out av- eraging over the wave oscillations [14]: Wemw = 2 π π/2∫ 0 W (Beq sinφ)dφ, (18) where Beq = 2Femw and Femw is the strength of an electromagnetic wave. However, Eq. (12) is true near the process thresh- old only, when the condition E ≈ 3m is fulfilled. Therefore before the comparison with the SLAC ex- periment it is necessary to pass from the laboratory frame to the “threshold” one where the electron beam energy is E ≈ 3m. The amplitude value of equal mag- netic field in the threshold frame is Beq ≈ 6.1·1012 G, and b ≈ 0.14 respectively. When calculating the rate Eq. (12) it is necessary to take into account limited interaction time as well as the radiative width (16). Therefore the intermedi- ate state width is a sum of the radiative width and the quantity 1/ΔtT , where ΔtT is laser-electron in- teraction time in the threshold frame. The number of produced pairs is Ne+e− = k · Nint(1 − e−WeqΔtT ), (19) where k = 21 962 is number of collisions of the electron and laser beams [3], Nint is the number of electrons in the interaction region. The values of Nint and ΔtT can be estimated using the data from Ref. [3]: ΔtL ≈ 0.002 fs, Nint ∼ 1.7 ·108. Finally, the number of events according to Eq. (19) is Ne+e− ≈ 80, (20) which is in reasonable agreement with the experimen- tal result of 106± 14 indicated in Ref. [3]. We thank V.Yu. Storizhko and S.P. Roshchupkin for useful discussions. References 1. A.D. Saharov // Usp. Fiz. Nauk. 1991, v. 161 (5), p. 29-34 (in Russian). 2. P.I. Fomin, R.I. Kholodov // Reports of Na- tional academy of sciences of Ukraine. 1998, v. 12, p. 91. 3. D.L. Burke et al. // Phys. Rev. Lett. 1997, v. 79, p. 1626-1629. 4. H. Hu, C. Müller, and C. H. Keitel // Phys. Rev. Lett. 2010, v. 105, p. 080401-080405. 5. C. Graziani, A.K. Harding, R. Sina // Phys. Rev. D. 1995, v. 51, p. 7097-7110. 6. O.P. Novak, R.I. Kholodov, and P.I. Fomin // JETP. 2010, v. 110, p. 978-982. 7. A.P. Novak and R.I. Kholodov // Ukr. Phys. J. 2008, v. 53 (2), p. 185-193. 8. O.P. Novak, R.I. Kholodov // Phys. Rev. 2009, v. D80, p. 025025-025035. 9. N.P. Klepikov // Zh. Eksp. Teor. Fiz. 1954, v. 26, p. 19. 10. A.A. Sokolov and I.M. Ternov // Synchrotron Radiation from Relativistic Electrons. New York: “American Institute of Physics”, 1986. 11. H. Herold, H. Ruder, and G. Wunner // As- tronomy & Astrophysics. 1982, v. 115, p. 90-96. 12. A.K. Harding and R. Preece // The Astrophys- ical Journal. 1987, v. 319, p. 939. 13. G.G. Pavlov, V.G. Bezchastnov, P. Meszaros, and S.G. Alexander // The Astrophysical Jour- nal. 1991, v. 380, p. 541. 14. A.I. Nikishov // Tr. Fiz. Inst. im. P.N. Lebede- va, Akad. 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