Exact relativistic plasma dispersion functions

On the ground of the theory of singular integrals with Cauchy kernel the exact plasma dispersion functions (PDFs) are introduced and studied. Those PDFs make more exact the weakly relativistic PDFs and generalize them on the case of arbitrary plasma temperature. На основі теорії сингулярних інтеграл...

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Опубліковано в: :Вопросы атомной науки и техники
Дата:2005
Автори: Pavlov, S.S., Castejon, F.
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Мова:Англійська
Опубліковано: Національний науковий центр «Харківський фізико-технічний інститут» НАН України 2005
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Цитувати:Exact relativistic plasma dispersion functions / S.S. Pavlov, F. Castejon // Вопросы атомной науки и техники. — 2005. — № 2. — С. 55-57. — Бібліогр.: 13 назв. — англ.

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Digital Library of Periodicals of National Academy of Sciences of Ukraine
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author Pavlov, S.S.
Castejon, F.
author_facet Pavlov, S.S.
Castejon, F.
citation_txt Exact relativistic plasma dispersion functions / S.S. Pavlov, F. Castejon // Вопросы атомной науки и техники. — 2005. — № 2. — С. 55-57. — Бібліогр.: 13 назв. — англ.
collection DSpace DC
container_title Вопросы атомной науки и техники
description On the ground of the theory of singular integrals with Cauchy kernel the exact plasma dispersion functions (PDFs) are introduced and studied. Those PDFs make more exact the weakly relativistic PDFs and generalize them on the case of arbitrary plasma temperature. На основі теорії сингулярних інтегралів з ядром Коші вводяться і досліджуються точні плазмові дисперсійні функції (ПДФ), уточнюючі слабо релятивістські ПДФ і узагальнюючі їх на випадок довільної температури. На основе теории сингулярных интегралов с ядром Коши вводятся и исследуются плазменные дисперсионные функции (ПДФ), уточняющие слабо релятивистские ПДФ и обобщающие их на случай произвольной температуры.
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fulltext EXACT RELATIVISTIC PLASMA DISPERSION FUNCTIONS S.S. Pavlov1 and F. Castejon2 1 Institute of Plasma Physics, NSC KhIPT, Akademicheskaya 1, 61108, Kharkov, Ukraine; 2 Asociación EURATOM-CIEMAT PARA Fusión, 28040, Madrid, Spain On the ground of the theory of singular integrals with Cauchy kernel the exact plasma dispersion functions (PDFs) are introduced and studied. Those PDFs make more exact the weakly relativistic PDFs and generalize them on the case of arbitrary plasma temperature. PACS: 52.27.Ny 1. INTRODUCTION Plasma waves have a wide range of applications. Essential to each of the applications is knowledge of the dielectric properties of the plasma. Analytical treatment of those properties leads to expressions for the dielectric tensor in terms of plasma dispersion functions (PDFs). As the non-relativistic PDF, +−= 1)[exp()( 2zzW ∫ z dtti 0 2 ])exp()/2( π , introduced into the theory of plasma and tabulated in complex region in the works [1,2], respectively, (or PDF, )()( zWizZ π= , introduced in the work [3]), so and the weakly relativistic PDFs, introduced in the work [4], are approximate ones, since have been derived through some approximations in the parameter μ/1 ( ,2 0 )/( TVc=μ 00 / mTVT = , is the rest mass of electron). 0m Problems of Atomic Science and Technology. Series: Plasma Physics (11). 2005. № 2. P. 55-57 55 The primary purpose of the present work is introducing the exact relativistic PDFs, which makes more exact the non-relativistic PDF and the weakly relativistic PDFs and generalize them on the case of arbitrary plasma temperature. It is achieved on the ground of a deep connection between the theory of plasma waves and the theory of Cauchy type integrals. 2. INTRODUCING OF THE EXACT RELATIVISTIC PDFs Starting from the 1st integral form of Trubnikov’s plasma dielectric tensor, that neglects ion dynamics, one can write it in Cartesian coordinates with z -axis directed along static magnetic field in the next equivalent form [5] ( ) ×⎟ ⎠ ⎞ ⎜ ⎝ ⎛ ⎟ ⎠ ⎞ ⎜ ⎝ ⎛ ⎟⎟ ⎠ ⎞ ⎜⎜ ⎝ ⎛ −= ∑∑ ∞ = ∞ −∞= k k kn n n p jiji k C nK 2!2! 1 2 0 , 2 2 λλ μ μ ω ω δε ( ) ( )( ) , (1) μωτπ ,,, // , c rkn nij nNkn ij Ω+ where ω and pω are an angular wave and plasma frequencies, ( )μ2K is Macdonald function of second order, ωckN //// = is longitudinal refractive index, =Ωc )( 0 cmeB is the electron cyclotron frequency, ( ) ( )[ ] ( ) ( )!!2 !2!1 , knkn knn C k kn ++ +− = , λ π 2n xx = , ( ) λ ππ knn iyxxy + =−= , λ ππ n zxxz == , ( )( ) ( )λλ π 122 1222 −+ −++ += kn knknkn yy , ( ) λ ππ knn izyyz + −=−= , 1=zzπ , ( )( ) ( ) ×⎟ ⎠ ⎞ ⎜ ⎝ ⎛ + =Ω + + knr c rkn n kn nN ij ij 2! ,, 2 // , μμμωτ ( ) ∫ ∫ ∞ ∞− ∞ + + −+− + ⎟ ⎠ ⎞ ⎜ ⎝ ⎛ ++ 0 2 //1 //// 122 // n kn kn xpr x pxx dxeeppd ij β μμ . (2) In the expression (2) )( 0cmpp = is normalized momentum, ( ) ( )2 // 22 // 11 pppx +−++= ⊥ , ( ) −+= 2 //1 pnβ ωcnpN Ω−//// and 0==== yyyxxyxx rrrr , == zxxz rr , 1== zyyz rr 2=zzr . Bortnatici and Ruffina shown that for the case anti-Hermitian parts of the functions, 0≥n ( ) ( ) ( ), can be exactly expressed in terms of modified spherical Bessel functions [6]. Obviously, the same result takes place and for functions, μωτπμμω μ ,,2,, // 0, // 0 23 c q ncq nNenNF Ω=Ω+ ( ) ( )( ) /,,, // 0, // 0 23 ωτμω c q ncq nNnNZ Ω=Ω+ ))(2( 2 μK , that appear in the expression (1) since they differ from functions, ( μω,,// 0 23 cq nNF Ω+ ) , by the factor not depending of two first arguments. In first, let us generalize these results on the case of arbitrary harmonic number, , using some facts from the theory of Cauchy type integrals [7,8]. Then on the same way we’ll give the exact analytical expressions for the Hermitian parts of the functions, n ( )μω,,// 0 23 cq nNZ Ω+ and define these whole functions as the exact relativistic PDFs. Using in the inside integral of the expression (2) the first of the Sokhotskii-Plemelj formulas, ( ) ( ) ( ) ∫ +∞ ∞− + − += t dP i ttF τ ττϕ π ϕ 2 1 2 , ( ) ( ) ( ) ∫ +∞ ∞− − − +−= t dP i ttF τ ττϕ π ϕ 2 1 2 , (3) corresponding to the Landau rule of passing the pole, and passing to the arguments used by Robinson [9-11]: 2// μpx = , ( )ωμ cnz Ω−= 1 , 22 //Na μ= one can, at once, receive ( ) ( ) × − = +− + !)(2 21,,Im 2 21 23 qK ezaZ ij ij rqzr q μμ πμ μ ( )∫ + − ⎥⎦ ⎤ ⎢⎣ ⎡ −−+−− x x q xa dxxazxxaze )2(22 2212212 21 μ , (4) where limits of integration, , can be obtained from the condition of appearing the pole in the inside integral of the expression (2): ±x 0≤nβ . Then for the limits of integration equal 10 // <≤ N ( ) ±−=± μβ zax 1[ 21 ])2(2 μzza +− and for ones equal , 1// >N +∞=+x ( ) ])2(1[ 221 μμβ zzazax +−−−=− ; here for shortness was used denoting ( )a2−= μμβ . The direct integration in the expression (4) gives anti-Hermitian parts of functions ( μ,,23 zaZ ijr q+ 56 ) . So, for the case 0=jir and 10 // <≤ N ( ) × ⎟⎟ ⎟ ⎠ ⎞ ⎜⎜ ⎜ ⎝ ⎛ +− −= + + 21 2 2 2123 0 23 )2( )(2 ,,Im q q a zza K zaZ μ μμ βπμ ( )[ ] ⎟ ⎠ ⎞ ⎜ ⎝ ⎛ +−−− + )2(22exp 221 21 μβμβ zzaaIaz q , ( ),(5) ∗< az ( ) 0,,Im 0 23 ≡+ μzaZq , ( ), (6) ∗≥ az here )(21 xIq+ is modified Bessel function of half-integer order and ( )βμ 11−=∗a . By the similar way for 0=jir and 1// >N ( ) × ⎟⎟ ⎟ ⎠ ⎞ ⎜⎜ ⎜ ⎝ ⎛ +−− −= + + 21 2 2 21 0 23 )2( )(2 )(,,Im q q a zza K zaZ μ μμ πβμ ( )[ ] ⎟ ⎠ ⎞ ⎜ ⎝ ⎛ +−−−− + )2(22exp 221 21 μβμβ zzaaKaz q , (7) for arbitrary z ; here )(21 xK q+ is Mac Donald function of half-integer order. It is known [7, 8] that for the density of Cauchy integral, ( )tϕ , satisfied to the Holder condition and integrated along the real axis in the Cauchy sense real and imagine parts of the boundary function, , are mutually single significantly connected by the Hilbert transforms )()()( tivtutF +=+ ( ) ( ) ∫ +∞ ∞− − = t duP i tiv τ ττ π 1 , ( ) ( ) ∫ +∞ ∞− − = t divP i tu τ ττ π 1 . (8) Here and everywhere letter P before integrals shows that integrals are understood in the sense of principle value. Consequently, implying ( μ,,Im)( 0 23 zaZtv q+= ) one can use the second transform to express real parts of the boundary functions, ( μ,,0 23 zaZ q+ ) , through their imagine parts. Then for the case one can receive 10 // <≤ N ( ) ( ) P aK ezaZ q aa q 21 2 )2(2121 0 23 )(2 ,,Re + −−− + ∗ = μμ βπμ μβ ∫ ∞+ ∗ − + + +− ⎟ ⎠ ⎞ ⎜ ⎝ ⎛ ++++ 0 221 21 212 )2(2))2(( zau dueaaIa u q q βμττβμττ . (9) In correspondence with the Sokhotskii-Plemely formula, giving the right sign (as in the weakly relativistic case) of anti-Hermitian parts of the functions, ( ) , and corresponding to passing of the contour of integration above the pole, one can receive the exact integral form for the whole those functions μ,,0 23 zaZq+ ( ) ( ) ×= + − + 21 2 0 23 )(2 ,, qq aK e zaZ μμ πβ μ βμ ∫ ∞+ − + + +−− ⎟ ⎠ ⎞ ⎜ ⎝ ⎛ ++ 0 21 21 21 )1( /1)2/((2)/1)2/((( zu dueuuaIuu u q q βμ βμββμ β . (10) For the case using the expression (7) for anti- Hermitian parts of the functions, 1// >N ( ) , by the similar way one can obtain ( ) [ ] ( ) × −− −−= ++ 21 2 0 23 )(2 2exp,, qq aK azaZ μπμ μβ βμ ( ) ∫ ∞ ∞− + + − ⎟ ⎠ ⎞ ⎜ ⎝ ⎛ +−−+− z daaKa q q τ ττβμττβμττ exp)2(2))2(( 221 21 212 , (11) where the contour of integration is passing below the pole. Integral forms (10), (11) define analytically the exact relativistic PDFs for the cases and , respectively. 10 // <≤ N 1// >N 3. ANALYTICAL PROPERTIES OF THE EXACT PDFs In first, let us study the integral form (10) defining the exact relativistic PDFs for the case 10 // <≤ N that is interesting from the point of view of the EC waves description in magnetized plasma; for shortness of writing from now on we are missing arguments of these functions. Using the recurrent formula for modified Bessel functions, )()/2()()( 11 zIzzIzI ννν ν−= −+ , one can receive =+−−++ +++ 0 21 20 23 0 25 )]2([)21( qqq ZzzaZqaZ μββ ( ) × − − 21 2 )(22 q aK e μμ πβ μ β βμ (12) ∫ ∞ . − − −∗ ⎟ ⎠ ⎞ ⎜ ⎝ ⎛ ++− 0 21 21 21 /1)2/((2)/1)2/(()(( dueuuaIuuua u q q ββμββμ Both integrals in the expression (12), using the known integral [12] × ⎟⎟ ⎟ ⎠ ⎞ ⎜⎜ ⎜ ⎝ ⎛ − =++ + − ∞+ ∫ 21 22 2 0 2 2 )()( ν ν ν ν ν π cp zcdxexzxcIxzx px ⎟ ⎠ ⎞ ⎜ ⎝ ⎛ −+ 22 21 2/ 2 cpzKe pz ν , ( cp ReRe > ; 1Re −>ν , π<zarg ), can be integrated ( ) ( ) )( )( 2)( )(2 20 21 21 21 21 2 μ μ β μμ πβ β βμ K K duesaIs aK e qu q q q =∫ ∞ − − − − − , (13) ( ) ( ) =−∫ ∞ − − −∗ − − 0 21 21 21 21 2 2))(( )(2 duesaIsua aK e u q q q β βμ β μμ πβ )( )()( 2 1 μ μμ μ K KK qq − − + , (14) here, for shortness, noting βμ /1)2/(( += uus was used. Thus, from (12) we receive a recurrent relation for the exact PDFs =+−−++ +++ 0 21 20 23 0 25 )]2([)21( qqq ZzzaZqaZ μββ )(/)]()()1[( 2 21 μμμμβ KKKz qq ++− . (15) For the case , that is interesting for the description of ICR waves in relativistic plasma, by the similar way one can receive the same recursive relation (15). Only in this case it is necessary to use the recurrent formula for Mac Donald functions, 1// >N += −+ )()( 11 zKzK νν )()/2( zKz νν , and the integral μ,,0 23 zaZ q+ One can verify the formulas for the 1st and 2nd derivatives of the exact PDFs in the parameter z × ⎟ ⎟ ⎟ ⎠ ⎞ ⎜ ⎜ ⎜ ⎝ ⎛ − =⎟ ⎠ ⎞ ⎜ ⎝ ⎛ +⎟ ⎠ ⎞ ⎜ ⎝ ⎛ + + ∞ ∞− ∫ 21 22 2222 2 ν ν ν ν π bp z pdxezxpKzx bx ⎟ ⎠ ⎞ ⎜ ⎝ ⎛ −+ 22 21 bpzKν , ( 1Re −>ν ) ])1([)( 0 1 00 −−+=′ qqq ZzZZ μβ , { }0 2 20 1 020 )1()](1)1(2[)( −− −++−+=′′ qqqq ZzZzZZ μβμμβ . (20) Excepting PDFs, and from the expressions (15), (20) one can obtain the usual linear deferential equation in the parameter 0 1−qZ 0 1−qZ z for the exact PDFs that follows by integrating in the parameter from the known integral [13] p ∫ ∞ +− ⎟ ⎠ ⎞ ⎜ ⎝ ⎛ − − = 0 22 1 22 22 bpzK bp pzchbxdxe zxp , ( bp ReRe > ; ). 0Re >z −′′+−− )))(2/()(( 02 qZzzaz μμ +′+−−+−+++−− )))](2/()(32()2())2/()((2[ 022 qZzzqqazzaz μμμμβ ++−−+−+++−− 022 ))]2/()(32()2())2/()([( qZzzqqazzz μμμμβ 0)2/(])([)( 2 3 2523 32 =−−− −− KKzKz qq μμμμβ , (21) Then instead integrals (13), (14) one can obtain the integrals [ ] ( ) ( ) ( )∫ ∞ ∞− − − − =− −− − ττββ μπμ μβ β dsaKs aK a q q q exp2)( )(2 2exp 21 21 21 21 2 )( )( 2 μ μ K Kq , (16) that also may be useful for their study. At last, from the formulas (4) by differentiation in the parameter a it follows the identity )(/ 0 1 0 ′′= +qq ZdadZ , [ ] ( ) ( ) ( )∫ ∞ ∞− − − − =− −− − ττββ μπμ μβ β dsaKs aK a q q q exp2)( )(2 2exp 21 21 21 21 2 )( )()( 2 1 μ μμ μ K KK qq − − + . (17) connecting derivatives of these PDFs in the parameter and a z that coincides with the respective identity for the weakly relativistic PDFs. REFERENCES Here, for shortness, noting )2(2 μττ +−= as was used. 1. G.V. Gordeev// JETPh (24). 1953, p.445 (in Russian). The integrals (13), (14) and (16), (17) are moments on the density in the respective Cauchy integrals defining the exact PDFs, 0 21+qZ , and have the next physical sense: the integrals (13), (16) are the densities of resonance electrons in the respective Dopler spectral line of absorption, the integrals (14), (17) define z -coordinate of this spectral line. 2. V.N. Faddeeva and N.M. Terentjev. Tabulation of the function ])exp(21)[exp()( 0 22 dttizzW z ∫+−= π of complex argument. Moscow. 1954 (in Russian). 3. B.D. Fried and S.D. Conte. The plasma dispersion function. New York: Academic Press. 1961. 4. I.P. Shkarofsky// Phys. Fluids (9), 1966, p.561. 5. M. Brambilla. Kinetic theory of plasma waves, homogeneous plasmas. Oxford: Oxford University Press. 1998. So, from all those integrals it follows the next theorem: z-coordinates of Dopler absorption spectral lines and densities of resonance electrons in these lines don’t depend from the direction of waves propagation and are defined by the moments (13), (14), (16), (17) of anti- Hermitian parts of the exact PDFs. 6. M. Bortnatici, U. Ruffina// IL Nuovo Cimento, vol. 6D, 1985, N.3, p.231. 7. N.I. Muskhelishvili. Singular integral equations. /3 ed., Moscow, 1968 (in Russian). Those integrals have also and the mathematical sense: (13), (16) are first and (14), (17) second coefficients in asymptotic expansion of the PDF, 0 21+qZ , 8. F.D. Gakhov. Boundary problems. / 2 ed., Moscow, 1963 (in Russian). 9. P.A. Robinson// J. Math. Phys. 1986, 27(5), p.1206. =+ − −= + + ... )( )()( )( )( 2 2 1 2 0 21 zK KK zK K Z qqq q μ μμ μ μ μ ⎟ ⎟ ⎠ ⎞ ⎜ ⎜ ⎝ ⎛ +++ ...1 2 211 0 z A z A A z qq q . 10. P.A. Robinson// J. Math. Phys. 1987, 28(5), p.1203. 11. P.A. Robinson// J. Math. Phys. 1989, 30(11), p.2484. 12. A.P. Prudnikov, Yu.A. Brychkov, O.I. Marichev. Integrals and series (Special functions). Moscow: “Science”. 1983 (in Russian). (18) Substituting the expression (18) into the recursive relation (15) one can receive recurrent formulas for calculating an arbitrary coefficient in this expansion through first two coefficients 13. A.P. Prudnikov, Yu.A. Brychkov, O.I. Marichev. Integrals and series (Elementary functions). Moscow: “Science”. 1981 (in Russian). q n q n q n q n q n AaAAqaAA 12 1 2 2 2 )21( −− + − + − +−++= βββ . (19) ТОЧНЫЕ РЕЛЯТИВИСТСКИЕ ПЛАЗМЕННЫЕ ДИСПЕРСИОННЫЕ ФУНКЦИИ С.С. Павлов и Ф. Кастехон На основе теории сингулярных интегралов с ядром Коши вводятся и исследуются плазменные дисперсионные функции (ПДФ), уточняющие слабо релятивистские ПДФ и обобщающие их на случай произвольной температуры. ТОЧНІ РЕЛЯТИВІСТСЬКІ ПЛАЗМОВІ ДИСПЕРСІЙНІ ФУНКЦІЇ С.С. Павлов і Ф. Кастехон На основі теорії сингулярних інтегралів з ядром Коші вводяться і досліджуються точні плазмові дисперсійні функції (ПДФ), уточнюючі слабо релятивістські ПДФ і узагальнюючі їх на випадок довільної температури. 57 EXACT RELATIVISTIC PLASMA DISPERSION FUNCTIONS
id nasplib_isofts_kiev_ua-123456789-79343
institution Digital Library of Periodicals of National Academy of Sciences of Ukraine
issn 1562-6016
language English
last_indexed 2025-11-30T16:51:54Z
publishDate 2005
publisher Національний науковий центр «Харківський фізико-технічний інститут» НАН України
record_format dspace
spelling Pavlov, S.S.
Castejon, F.
2015-03-31T13:49:55Z
2015-03-31T13:49:55Z
2005
Exact relativistic plasma dispersion functions / S.S. Pavlov, F. Castejon // Вопросы атомной науки и техники. — 2005. — № 2. — С. 55-57. — Бібліогр.: 13 назв. — англ.
1562-6016
PACS: 52.27.Ny
https://nasplib.isofts.kiev.ua/handle/123456789/79343
On the ground of the theory of singular integrals with Cauchy kernel the exact plasma dispersion functions (PDFs) are introduced and studied. Those PDFs make more exact the weakly relativistic PDFs and generalize them on the case of arbitrary plasma temperature.
На основі теорії сингулярних інтегралів з ядром Коші вводяться і досліджуються точні плазмові дисперсійні функції (ПДФ), уточнюючі слабо релятивістські ПДФ і узагальнюючі їх на випадок довільної температури.
На основе теории сингулярных интегралов с ядром Коши вводятся и исследуются плазменные дисперсионные функции (ПДФ), уточняющие слабо релятивистские ПДФ и обобщающие их на случай произвольной температуры.
en
Національний науковий центр «Харківський фізико-технічний інститут» НАН України
Вопросы атомной науки и техники
Basic plasma physics
Exact relativistic plasma dispersion functions
Точні релятивістські плазмові дисперсійні функції
Точные релятивистские плазменные дисперсионные функции
Article
published earlier
spellingShingle Exact relativistic plasma dispersion functions
Pavlov, S.S.
Castejon, F.
Basic plasma physics
title Exact relativistic plasma dispersion functions
title_alt Точні релятивістські плазмові дисперсійні функції
Точные релятивистские плазменные дисперсионные функции
title_full Exact relativistic plasma dispersion functions
title_fullStr Exact relativistic plasma dispersion functions
title_full_unstemmed Exact relativistic plasma dispersion functions
title_short Exact relativistic plasma dispersion functions
title_sort exact relativistic plasma dispersion functions
topic Basic plasma physics
topic_facet Basic plasma physics
url https://nasplib.isofts.kiev.ua/handle/123456789/79343
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