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  • VOLUME 87, NUMBER 27 P H Y S I C A L R E V I E W L E T T E R S 31 DECEMBER 2001

    ensional Child-Langmuir Law

    Leubantcli

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    an2Dhig

    Itionequonsodecurintulatithis

    0, 0, of this emission strip since, as J is increased tolyn

    ne

    3)

    o-nt

    278understanding of the 2D limiting current density. Thisproblem is clearly also relevant to the edge emission inh power diodes.n this paper, we shall not seek a complete 2D solu-

    to the force law, continuity equation, and the Poissonation. Instead, we simply derive the condition for theet of turbulent behavior when a finite patch of the cath-surface is allowed to emit, with a uniform emission

    rent density across the patch. The theory is simple anditive, and is in excellent agreement with earlier simu-

    on results [6]. As we shall see toward the end ofpaper, the physical insight even leads to the predic-

    the 2D limiting value, the space charge field there exactcancels the vacuum electric field, VD, causing reflectioof the emitted electrons.

    Let rx, z be the charge density within the gap. Aincremental line charge, located at x, z with a line chargdensity rx, zDxDz, yields an electric field at x, z0, 0 with a magnitude

    DE rx, zDxDz

    2p0px2 1 z2

    . (

    On the center line, we need only to consider the z compnent of the electric field by symmetry, and this componeSimple Theory for the Two-Dim

    Y. Y.Department of Nuclear Engineering and Radiological Scienc

    (Received 11 April 2001; pThis paper presents, for the first time, a simple

    Langmuir law. For electron emission over a finite paderived approximately from first principles. The scaresults. They predict the onset of virtual cathodeelectrons emitted from a cathode over only a restricthe classical (1D) Child-Langmuir value.DOI: 10.1103/PhysRevLett.87.278301

    The Child-Langmuir Law [13] gives the maximumcurrent density that can be transported across a planargap of gap separation D and gap voltage V . In the one-dimensional model, this maximum current density is givenby

    J1 409D2

    2em

    12V 32, (1)

    where e and m are, respectively, the charge and mass ofthe emitted particle, and 0 is the free space permittiv-ity. Implicit in Eq. (1) is the neglect of relativistic ef-fects and the assumption of zero electron emission velocity.While Eq. (1) was published ninety years ago, no analo-gous derivation for two dimensions (2D) has appeared inthe intervening years. This paper partially fills this void.

    The complete solution of the 2D limiting current densityin a diode is extremely difficult to obtain analytically. Itrequires the simultaneous solution of the force law, thecontinuity equation, and the Poisson equation in two di-mensions. Such 2D theories are very complicated [4]; theresults are neither transparent nor readily usable [5]. How-ever, this 2D problem is of fundamental interest becauseelectron emission is often restricted to a finite patch on thecathode surface. For example, modern cathodes, such asferroelectric cathodes, laser-triggered cathodes, field emit-ter arrays, etc., have at times displayed an emission cur-rent density higher than that expected from the classical1D Child-Langmuir value [Eq. (1)]. The proper interpre-tation of such results would have required, at a minimum,301-1 0031-90070187(27)278301(3)$15.00au*s, University of Michigan, Ann Arbor, Michigan 48109-2104lished 10 December 2001)alytic theory for the two-dimensional (2D) Child-h on a planar cathode, the limiting current density isng laws are in excellent agreement with simulationrmation in a 2D geometry; they also indicate thatd area may have a current density much exceeding

    PACS numbers: 85.45.w, 52.59.Mv

    tion of the limiting current density for a three-dimensionalgeometry.

    A few years ago, the lack of a 2D Child-Langmuir solu-tion prompted Luginsland et al. [6] to use two very differ-ent particle-in-cell codes to simulate the maximum currentdensity, J2. The emission current density is uniform andis restricted to a strip of width W on the cathode surface.The strip is infinitely long. From the simulation data, thefollowing 2D Child-Langmuir Law was synthesized [6]:

    J2J1

    1 1 0.3145D

    W, (2)

    where D is the anode-cathode separation. Luginslandfound that Eq. (2) fits the numerical data to within a fewpercent for all WD . 0.1. This statement is valid re-gardless of the external magnetic field (ranging from zeroto 100 T) that is imposed along the electron flow direction.When the emission current density exceeds the value givenin Eq. (2), the emitted electrons from the center line of theemission strip are the first ones to be reflected, initiatinga virtual cathode [6]. It is clear from Eq. (2) that the 1DChild-Langmuir law is recovered in the limit W D.

    We shall first provide a derivation of Eq. (2), under theassumption W D. In the model, the cathode is locatedat z 0, and the anode is located at z D. Electrons areemitted with a uniform current density, J, over the infinitestrip, 2W2 , x , W2, on the cathode. We impose aninfinite magnetic field in the z direction. We shall focusmainly on the space charge field on the center line, x, z 2001 The American Physical Society 278301-1

  • VOLUME 87, NUMBER 27 P H Y S I C A L R E V I E W L E T T E R S 31 DECEMBER 2001

    is obtained by multiplying Eq. (3) by the directional co-2 2 12

    we obtain yz Jrz Cz23 for some constant C.

    sine, zx 1 z . Thus, the space charge field on thecenter line of the emitting strip is given by, upon summingover the space charge within the gap,

    E Z D

    0dz

    Z W22W2

    dxrx, zz

    2p0x2 1 z2. (4)

    We now assume that W D, so that the charge densityr is roughly independent of x. With rx, z rz, thex integration in Eq. (4) can be performed to yield

    E 1p0

    Z D0dz rz tan21

    W2z

    1

    20

    Z D0dz rz

    1 2

    4zpW

    , (5)

    where, in writing the last expression of Eq. (5), wehave used the approximation, tan21p p2 2 1pfor p 1. Since the injection current density, J rzyz constant, where yz is the electron velocity,we may write the total electric field, due only to the spacecharge, as

    E G

    J20

    Z D0

    dzyz

    1 2

    4zpW

    , (6)

    where we have included a multiplication factor, G, to ac-count for the contributions due to the image charges. SinceE is the space charge electric field at a single location, itmust be proportional to J, and we take G to be the pro-portionality constant defined by Eq. (6). The 2D limit-ing current density, J2, is reached when this total self-electric field equals the vacuum field, VD. This gives

    G

    J220

    Z D0

    dz

    yz

    1 2

    4zpW

    V

    D. (7)

    The 1D Child-Langmuir law is obtained by settingW equalto infinity. Thus, by definition, we have, from Eq. (7),

    G

    J120

    Z D0

    dzyz

    VD

    . (8)

    Note that the value of G in Eq. (8) may easily be obtainedby using Eq. (1) and the familiar 1D Child-Langmuir ve-locity solution yz in Eq. (8). Note further that this valueof G takes into account, exactly, the effects of all imagecharges in this 1D limit. We assume that this G is alsoapplicable for the large but finite value of W [cf. Eq. (7)],and this latter assumption is on the same footing as ap-proximating rx, z by rz in Eqs. (4) and (5).

    We take the ratio of Eqs. (7) and (8) to obtain, to firstorder in 1W ,

    J2J1

    1 1

    RD0

    dzyz

    4zpW RD

    0dzyz

    . (9)

    Since the last term in Eq. (9) is already a correction due to2D effects, we may use the 1D Child-Langmuir velocityprofile yz in that term. From the well-known densityprofile, rz z223, in the 1D Child-Langmuir solution,

    278301-2Using this 1D velocity profile in Eq. (9), we obtainJ2J1

    1 1DpW

    , (10)

    which is in remarkable agreement with the empirical for-mula [Eq. (2)].

    While Eq. (10) is derived under the assumptionWD 1, the simulation data [6] show that it happensto be applicable even if WD is as small as 0.1.

    It is therefore tempting to apply the same derivation toother geometries of emission. Before we do this, let usrecapitulate the main assumptions used to derive Eq. (10):(a) WD 1; (b) rx, z rz; (c) the image chargefactor, G, in Eqs. (7) and (8), is the same whether W isfinite or infinite; and (d) the 1D Child-Langmuir solutionis used to approximate the correction due to 2D effects.

    For the case where electron emission is restricted to acircular patch of radius R on the cathode, we may useexactly the same procedure to arrive at the following 2DChild-Langmuir law in the limit RD 1:

    J2J1

    1 1D

    4R. (11)

    Note the similarity between Eqs. (10) and (11). Fromthe excellent agreement between Eq. (10) and Eq. (2), itwould not be surprising if Eq. (11) happens to give an ex-cellent approximation for RD , 1. Indeed, Luginsland[7] recently confirmed that Eq. (11) agrees with simulationdata to within a few percent whenever RD . 0.5.

    The simple scaling laws, Eqs. (10) and (11), allow usto postulate the maximum current density, J3, when theemitting area on the planar cathode is an ellipse with semi-axes R and W2, with the restriction R . W2. This el-lipse reduces to a circle of radius R in the R W2 limit,and to an infinite strip of width W in the R W limit.Thus, we postulate

    J3J1

    1 1DpW

    1

    142

    12p

    DR

    1 1 0.32DW

    1 0.091DR

    , R $W2

    ,

    (12)so that Eq. (12) reduces to Eq. (10) in the R W limit,and to Eq. (11) in the R W2 limit. In Eq. (12), weuse J3 to denote the limiting current density because tosimulate emission from an elliptical patch into a planargap would have required a three-dimensional particle-in-cell code.

    The scaling laws derived thus far predict the emissioncurrent density for the onset of the virtual cathode, whichoccurs at the center region of the emission area. If theavailable electrons are further increased (e.g., by raisingthe laser intensity in a photocathode [8]), a point maybe reached where the entire emitting area may becomespace-charge-limited and the electron emission becomes

    278301-2

  • VOLUME 87, NUMBER 27 P H Y S I C A L R E V I E W L E T T E R S 31 DECEMBER 2001

    saturated. This latter situation was recently analyzed inRefs. [5,9], and it was found that the current density peaksat the rim of the emitting region (i.e., the current densityprofile has a winglike structure). The most recent pho-tocathode experiments [8] seem to have confirmed boththe onset of virtual cathode and the saturated emission asthe laser intensity is raised, in a manner described in thisparagraph.

    While Eqs. (10) and (11) agree well with simulation datadown to relatively small values of W and R, it must bestressed that they do not give the correct limits when Wand R approach zero. One can prove that, as W approacheszero, J2J1 , ADWa for some constants A and awith a , 1. One can similarly prove that, as R approacheszero, J2J1 , BDRb for some constants B and bwith b , 2. It would be highly desirable to establish theasymptotic limits of J2J1 as W and R approach zero.

    In conclusion, a simple 2D Child-Langmuir law is es-tablished analytically for the first time. It is in excellentagreement with numerical simulations. It predicts the onsetof virtual cathode before the entire emitting region reachessaturation. The simple scaling laws are established fromfirst principles. They are independent of the cathode ma-terials, as in the 1D case.

    It is a pleasure to acknowledge stimulating discussionswith John Luginsland, Agust Valfells, Kevin Jensen, andRon Gilgenbach. This work was supported by DUSD(S&T) under the Innovative Microwave Vacuum Electron-

    ics MURI Program, managed by the Air Force Office ofScientific Research under Grant No. F49620-99-1-0297,and by the Northrop-Grumman Industrial AssociatesProgram.

    *Email address: [email protected][1] C. D. Child, Phys. Rev. 32, 492 (1911); I. Langmuir, ibid.

    21, 419 (1921).[2] C. K. Birdsall and W. B. Bridges, Electron Dynamics of

    Diode Regions (Academic, New York, 1966).[3] R. C. Davidson, Physics of Nonneutral Plasmas

    (Addison-Wesley, Redwood City, CA, 1990); R. B.Miller, An Introduction to the Physics of Intense ChargedParticle Beams (Plenum, New York, 1982).

    [4] P. T. Kirstein, G. S. Kino, and W. E. Waters, Space ChargeFlow (McGraw-Hill, New York, 1967).

    [5] R. J. Umstattd and J. W. Luginsland, Phys. Rev. Lett. 87,145002 (2001).

    [6] J. W. Luginsland, Y. Y. Lau, and R. M. Gilgenbach, Phys.Rev. Lett. 77, 4668 (1996). There is a misprint in this paper;the number 1 should be added to the right-hand side ofEq. (2) [see Phys. Rev. Lett. 78, 2680(E) (1997)].

    [7] J. W. Luginsland, Bull. Am. Phys. Soc. 46(8), 175 (2001).[8] A. Valfells, Bull. Am. Phys. Soc. 46(8), 175 (2001).[9] J. J. Watrous, J. W. Luginsland, and G. E. Sasser III, Phys.

    Plasmas 8, 289 (2001).

    278301-3278301-3