D Quantum Corrections

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    Inclusion of Tunneling and Size-Quantization Effects in Semi-

    Classical Simulators

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    Outline:

    What is Computational Electronics?

    Semi-Classical Transport Theory

    Drift-Diffusion Simulations

    Hydrodynamic Simulations

    Particle-Based Device Simulations

    Inclusion of Tunneling and Size-Quantization Effects in Semi-Classical Simulators

    Tunneling Effect: WKB Approximation and Transfer Matrix Approach

    Quantum-Mechanical Size Quantization Effect

    Drift-Diffusion and Hydrodynamics: Quantum Correction and QuantumMoment Methods

    Particle-Based Device Simulations: Effective Potential Approach

    Quantum Transport

    Direct Solution of the Schrodinger Equation (Usuki Method) and TheoreticalBasis of the Greens Functions Approach (NEGF)

    NEGF: Recursive Greens Function Technique and CBR Approach

    Atomistic SimulationsThe Future

    Prologue

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    Quantum Mechanical Effects

    There are three important manifestations

    of quantum mechanical effects in nano-

    scale devices:

    - Tunneling

    - Size Quantization

    - Quantum Interference Effects

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    Inclusion of Tunneling and Size-

    Quantization Effects

    Tunneling Effect: WKB Approximation and

    Transfer Matrix Approach

    Quantum-Mechanical Size Quantization EffectDrift-Diffusion and Hydrodynamics:

    Quantum Correction and

    Quantum Moment Methods

    Particle-Based Device Simulations: EffectivePotential Approach

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    Tunneling Currents vs. Technology

    Nodes and Tunneling Mechanisms

    10-16

    10-14

    10-12

    10-10

    10-8

    10-6

    10-4

    0 50 100 150 200 250

    Cu

    rrent(A/

    m)

    Technology Generation (nm)

    Ion

    IG

    Iof f

    For tox 40 , Fowler-Nordheim (FN) tunneling dominates For t

    ox< 40 , direct tunneling becomes important

    Idir

    > IFN

    at a given Vox

    when direct tunneling active For given electric field: - IFN independent of oxide thickness

    - Idir

    depends on oxide thickness

    B Vox>

    B

    Vox=

    B

    Vox<

    B

    FN FN/Direct Direct

    tox

    B Vox>

    B

    Vox=

    B

    Vox<

    B

    FN FN/Direct Direct

    tox

    This slide is courtesy of D. K. Schroder.

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    WKB Approximation to Tunneling

    Currents Calculation

    0

    EF

    B

    0

    EF

    B

    a

    No applied bias With applied bias

    - eEx

    x-axis

    The difference between the Fermi level and the top of the barrier isdenoted by B

    According to WKB approximation, the tunneling coefficient through thistriangular barrier equals to:

    a

    dxxT 0 )(2exp where: eExm

    x B 2*2

    )(

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    WKB Approximation to Tunneling

    Currents Calculation

    eE

    mT B

    3

    *24exp

    2/3

    Calculated and experimental tunnelcurrent characteristics for ultra-thin oxidelayers.

    (M. Depas et al., Solid State Electronics, Vol.38, No. 8, pp. 1465-1471, 1995)

    The final expression for theFowler-Nordheim tunnelingcoefficient is:

    Important notes:

    The above expressionexplains tunneling processonly qualitatively becausethe additional attraction ofthe electron back to the plateis not included

    Due to surfaceimperfections, the surface

    field changes and can makelarge difference in the results

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    Tunneling Current Calculation in Particle-

    Based Device Simulators

    If the device has a Schottky gate then one must

    calculate both the thermionic emission and the

    tunneling current through the gate

    WKB fails to account for quantum-mechanicalreflections over the barrier

    Better approach to use in conjunction with

    particle-based device simulations is the

    Transfer Matrix Approach

    W. R. Frensley, Heterostructure and Quantum Well Physics, ch. 1 in

    Heterostructure and Quantum Devices, a volume of VLSI Electronics:

    Microstructure Science, N. G. Einspruch and W. R. Frensley, eds.,

    (Academic Press, San Diego, 1994).

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    Transfer Matrix Approach

    Within the Transfer Matrix approach one

    can assume to have either

    Piece-wise constant potential barrier

    Piecewise-linear potential barrier

    D. K. Ferry, Quantum Mechanics for Electrical Engineers, Prentice Hall, 2000.

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    Piece-Wise Constant Potential Barrier

    (PCPBT Tool) installed on the nanoHUB

    www.nanoHUB.org

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    The Approach at a Glance

    Slide property of Sozolenko.

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    The Approach, Continued

    Slide property of Sozolenko.

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    Piece-Wise Linear Potential Barrier

    This algorithm is implemented in ASUs code formodeling Schottky junction transistors (SJT)

    It approximates real barrier with piece-wiselinear segments for which the solution of the 1D

    Schrodinger equation leads to Airy functions andmodified Airy functions

    Transfer matrix approach is used to calculate theenergy-dependent transmission coefficient

    Based on the value of the energy of the particleE, T(E) is looked up and a random number isgenerated. If r

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    The Approach at a Glance

    E

    ai-1 aiai+1

    Vi

    Vi+1

    Vi-1 V(x)

    1D Schrdingerequation:

    Solution for piecewiselinear potential:

    The total transmissionmatrix:

    T(E):

    ExVdx

    d

    m

    )(

    2 2

    22

    )()( )2()1( iiiii BCAC

    1 2 1........T FI N BI M M M M M M

    1

    2011

    1 NT

    kT

    K m

    ' '1 1

    0 0

    ' '1 1

    0 0

    ' '1 1

    ' '1 1

    1 1[ (0) (0)] [ (0) (0)]

    2 2

    1 1[ (0) (0)] [ (0) (0)]

    2 2

    ( ) ( ) ( ) ( )

    ( ) ( ) ( ) ( )

    i i i i

    FI

    i i i i

    N i N N i N N i N N i N

    BI

    n N i N N i N N i N N i N

    r rA A B B

    ik ik M

    r rA A B B

    ik ik

    r B ik B r B ik BM

    r r A ik A r A ik A

    '

    ' ''1 1

    ( ) ( )( ) ( )

    ( ) ( )( ) ( )

    i i i ii i i i i

    i

    i i i i i i ii i i i i

    A Br B B

    Mr r A r Br A A

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    Simulation Results for Gate Leakage in

    SJT

    10-7

    10-6

    10-5

    10-4

    10-3

    0.1 0.2 0.3 0.4 0.5 0.6 0.7

    Drain currentGate CurrentTunneling Current

    Current[A/u

    m]

    Gate Voltage [V]

    T. Khan, D. Vasileska and T. J.

    Thornton, Quantum-mechanical

    tunneling phenomena in metal-

    semiconductor junctions, NPMS 6-

    SIMD 4, November 30-December 5,

    2003, Wailea Marriot Resort, Maui,

    Hawaii.

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    Quantum-Mechanical Size Quantization

    Quantum-mechanical size quantization

    manifests itself as:

    - Effective charge set-back from the

    interface

    - Band-gap increase

    - Modification of the Density of Statesfunction

    D. Vasileska, D. K. Schroder and D.K. Ferry, Scaled silicon MOSFETs: Part II - Degradationof the total gate capacitance, IEEE Trans. Electron Devices44, 584-7 (1997).

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    Effective Charge Set-Back From The

    Interface

    Schrodinger-Poisson Solvers

    Quantum Correction Models

    Quantum Moment Models

    Substrate

    Gate

    ox

    oxox

    t

    C

    polyC

    invC deplC inv

    ox

    poly

    ox

    ox

    deplinv

    ox

    poly

    ox

    oxtot

    C

    C

    C

    C1

    C

    CC

    C

    C

    C1

    C

    C

    D. Vasileska, and D.K. Ferry, "The influence of poly-

    silicon gates on the threshold voltage, inversion layer

    and total gate capacitance in scaled Si-MOSFETs,"NanotechnologyVol. 10, pp.192-197 (1999).

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    Schrdinger-Poisson Solvers

    At ASU we have developed:

    1D SchrodingerPoisson Solvers (inversion

    layers and heterointerfaces)

    2D SchrodingerPoisson solvers (Sinanowires)

    3D SchrodingerPoisson solvers (Si quantum

    dots)

    S. N. Milii, F. Badrieh, D. Vasileska, A. Gunther, and S. M. Goodnick, "3D Modeling of

    Silicon Quantum Dots," Superlattices and Microstructures, Vol. 27, No. 5/6, pp. 377-382

    (2000).

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    Simulation Results Obtained With

    SCHRED

    0

    5 x019

    1x1020

    1.5x1020

    2x1020

    0 5 10 15 20 25 30 35 40

    n(z)[cm-3]

    Distance from the SiO2

    /Si interface []

    QM

    VG= 2.5 V

    SC0

    5

    10

    15

    20

    25

    1011 1012 1013

    QMSC

    zav

    []

    Ns [cm-2]

    Cinvreduces Ctotby about 10%

    Cpoly+ Cinvreduce Ctotby about 20%

    With poly-depletion Ctothas pronoun-

    ced gate-voltage dependence

    0.2

    0.4

    0.6

    0.8

    1.0

    -0.5 0.0 0.5 1.0 1.5 2.0 2.5

    Ctot

    [F/cm

    2]

    VG [V]

    Cox

    SCNP QMNP

    SCWPQMWP

    invoxpolytot CCCC

    1111

    The classical charge density peaks rightat the SC/oxide interface.

    The quantum-mechanically calculatedcharge density peaks at a finite distancefrom the SC/oxide interface, which leadsto larger average displacement of

    electrons from that interface.

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    Simulation Results Obtained With

    SCHRED

    0.2

    0.3

    0.4

    0.50.6

    0.7

    0.8

    0.91

    1 2 3 4 5 6 7 8 9 10

    classical M-B, metal gates

    classical F-D, metal gatesquantum, metal gates

    quantum, poly-gates ND=6x1019cm-3

    quantum, poly-gates ND=1020cm-3

    quantum, poly-gates ND=2x1020cm-3

    Ctot/

    Cox

    Oxide thickness tox

    [nm]

    T=300 K, NA

    =1018cm-3

    Degradation of the Total Gate Capacitance Ctot

    for Different Device Technologies

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    Simulation Results Obtained With

    SCHRED

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    Comparison With Experiments

    0

    10

    20

    30

    40

    50

    60

    0

    10

    20

    30

    40

    50

    60

    0 5x1011

    1x1012

    1.5x1012

    2x1012

    2.5x1012

    3x1012

    Exp. data [Kneschaurek et al.]V

    eff(z)=V

    H(z)+V

    im(z)+V

    exc(z)

    Veff

    (z)=VH(z)

    Veff

    (z)=VH(z)+V

    im(z)

    Exp. data [Kneschaurek et al.]V

    eff(z)=V

    H(z)+V

    im(z)+V

    exc(z)

    Veff

    (z)=VH(z)

    Veff

    (z)=VH(z)+V

    im(z)

    EnergyE10[meV] T = 4.2 K, Ndepl=10

    11 cm-2

    Ns [cm-2 ]

    Kneschaurek et al., Phys. Rev. B 14, 1610 (1976) Infrared Optical Absorption

    Experiment:

    far-ir

    radiation

    LED

    SiO2 Al-Gate

    Si-Sample

    Vg

    Transmission-Line Arrangement

    Infrared Optical Absorption

    Experiment:

    far-ir

    radiation

    LED

    SiO2 Al-Gate

    Si-Sample

    Vg

    far-ir

    radiation

    LEDLED

    SiO2 Al-Gate

    Si-Sample

    Vg

    Transmission-Line Arrangement

    D. Vasileska, PhD Thesis, 1995.

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    SCHRED Usage on the nanoHUB

    SCHRED has 92 citations in Scientific Research Papers,

    1481 users and 36916 jobs as of July 2009

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    3D Schrodinger-Poisson Solvers

    3D SchrodingerARPACK

    3D Poisson: BiCGSTAB method

    Aluminum

    Chrome

    PECVD SiO2

    Thermal SiO2

    p-type bulk silicon

    Na = 1016

    cm-3

    400 nm

    30 nm

    93 nm20 nm

    5 nm

    Built-in gates

    Aluminum

    Chrome

    PECVD SiO2

    Thermal SiO2

    p-type bulk silicon

    Na = 1016

    cm-3

    400 nm

    30 nm

    93 nm20 nm

    5 nm

    Built-in gates

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    3D Schrodinger-Poisson Solvers

    Left: The energy level spacing distribution as a function of s =E/(E)avg

    obtained by combining the results of a number of impurity configurations.

    Right: The 11th to 16th eigenstates of the silicon quantum dot.

    0 1 3 42

    s

    0.0

    0.8

    0.6

    0.4

    0.2

    1.0

    P(s) 11 12 13

    14 15 16

    S. N. Milicic, D. Vasileska, R. Akis, A. Gunther, and S. M Goodnick, "Discrete impurity effects in silicon

    quantum dots," Proceedings of the 3rd International Conference on Modeling and Simulation ofMicrosystems, San Diego, California, March 27-29, 2000, pp. 520-523 (Computational Publications, 2000).

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    Quantum Correction Models

    - Hansc and Van Dort Approach -

    These quantum-correction models try to incorporate thequantum-mechanical description of the carrier density in aMOSFET device structure via modification of certain deviceparameters:

    HANSC model - modifies the effective DOS function

    Van Dort model - modifies the intrinsic carrier density viamodification of the energy band-gap. Within this model, themodification of the surface potential is:

    2* /exp1 LAMBDAzNN CC

    CONVQMn

    CONVs

    QMs zzzzEq ,/

    Accounts for the band-gap wideningeffect because of the upward shift ofthe lowest allowed state

    Accounts for the larger displacementof the carriers from the interface andextra bend-bending needed for givenpopulation:

    94zqEn

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    With these modifications, the energy band-gap becomes:

    This results in modification of the intrinsic carrier density,which now, anywhere through the depth of the device, takes

    the form:

    The function F(y) is introduced to describe smooth transitionbetween classical and quantum description (pinch-off andinversion regions)

    3/23/1

    4

    ,

    9

    13

    E

    Tqk

    EE

    B

    SiCONVg

    QMg

    B.DORT (MODEL)

    QMi

    CONVii

    BCONV

    gQM

    gCONVi

    QMi

    nyFyFnn

    TkEEnn

    )()(1

    2/exp

    refyyaaayF /,2exp1/exp2)( 22

    N.DORT (MODEL)

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    The Van Dort model is activated by specifying N.DORT on theMODEL statement.

    E0

    E1

    distance

    Energy n(z)

    z

    z

    CONVz

    QMz

    Classical density

    Quantum-mechanicaldensity

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    Modification of the DOS Function

    The modification of the DOS function affects thescattering rates and must be accounted for inthe adiabatic approximation via solution of the1D/2D Schrodinger equation in slices along the

    channel of the device

    This is time consuming and for all practicalpurposes only charge set-back and modificationof the band-gap are to a very good accuracyaccounted for using eitherBohm potential approach to continuum modeling

    Effective potential approach in conjunction withparticle-based device simulators

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    Quantum Corrected Approaches

    Drift DiffusionDensity Gradient

    HydrodynamicQuantum Hydrodynamic

    Particle-based device simulations

    Effective Potential Approaches due to:

    - Ferry, and

    - Ringhofer and Vasileska

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    Bohm Theory

    The hydrodynamic formulation is initiated by substituting the wavefunc-

    tion into the time-dependent SWE:

    The resultant real and imaginary parts give:

    nRReiS ,/ t

    iVm

    22

    2

    qc ffQVdt

    dm

    mR

    RmtQ

    tQtVSmt

    tS

    S/mtRtSmt

    t

    v

    r

    eq.JacobiHamiltonrrr

    vrrr

    2/122/12

    22

    2

    2

    2

    1

    2),,(

    );,,(),(2

    1),()2(

    ;),(),(;01),(

    )1(

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    Effective Potential Approach Due to Ferry

    ieffi

    ii

    ii

    ii

    Vd

    Vdd

    dVd

    ndrVV

    )r()rr(r~

    'rrexp)'r('r)rr(r~

    )r'r(

    'rr

    exp'r)r(r~

    )r()r(

    2

    2

    2

    2

    In principle, the effective role of the potential can be rewritten in terms of thenon-local density as (Ferry et al.1):

    Classical densitySmoothed,

    effective potential

    Buil t-in potential

    for tr iangular po-

    tent ial approx ima-

    t ion.

    Effective potential

    approximation

    Quantization

    energy

    Set backof ch arge --

    quantum capacitance

    effects

    Buil t-in potential

    for tr iangular po-

    tent ial approx ima-

    t ion.

    Effective potential

    approximation

    Quantization

    energy

    Set backof ch arge --

    quantum capacitance

    effects

    1 D. K. Ferry, Superlatt. Microstruc.27, 59 (2000); VLSI

    Design, in press.

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    Parameter-Free Effective Potential

    The basic concept of the thermodynamic approach to effectivequantum potentials is that the resulting semiclassical transport

    picture should yield the correct thermalized equilibrium quantum

    state. Using quantum potentials, one generally replaces the

    quantum Liouville equation

    for the density matrix (x,y) by the classical Liouville equation

    for the classical density function f(x,k). Here, the relation betweenthe density matrix and the density function f is given by the Weyl

    quantization

    , 0it H

    12 *

    0t x x k mf k f V f

    ( , ) [ ] ( / 2, / 2)exp( )f x k W x y x y ik y dy

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    The thermal equilibrium density matrix in the quantum

    mechanical setting is given by eq = e-H, where =1/kBT is the

    inverse energy, and the exponential is understood as a matrix

    exponential.

    In the semi-classical transport picture, the thermodynamic

    equilibrium density function feq is given by the Maxwellian

    distribution function.

    Consequently, to obtain the quantum mechanically correctequilibrium states in the semiclassical Liouville equation with the

    effective quantum potential VQ, we set:

    22

    2 *

    ( , ) exp [ ] ( / 2, / 2)exp( )k Q eq H

    eq m

    f x k V W e x y x y ik y dy

    D. Vasileska and S. S. Ahmed, Modeling of Narrow-Width SOI Devices, Semicond.

    Sci. Technol., Vol. 19, pp. S131-S133 (2004).

    D. Vasileska and S. S. Ahmed, Narrow-Width SOI Devices: The Role of Quantum

    Mechanical Size Quantization Effect and the Unintentional Doping on the Device

    Operation, IEEE Transactions on Electron Devices, Volume 52, Issue 2, Feb. 2005Page(s):227236.

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    Different forms of the effective quantum potential arise from

    different approaches to approximate the matrix exponential e-H.

    In the approach presented in this paper, we represent e-Has theGreens function of the semigroup generated by the

    exponential.

    The logarithmic Bloch equation is now solved asymptotically,

    using the Born approximation, i.e. by iteratively inverting thehighest order differential operator (the Laplacian).

    This involves successive solution of a heat equation for which

    the Greens function is well known, giving

    2 2

    23 2

    1 2 *( , ) sinh exp ( )2 * 8 *2

    i x yQ

    Q QB H

    m kV x k V y e dyd m mk

    V V

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    The Barrier Potential

    The total potential is divided into Barrier and Hartree potential,where Barrier is a Heviside step function and Hartree is the

    solution to the Poisson equation.

    The barrier field is then calculated using:

    Note: It is evaluated only once at the beginning of the simulation!!!

    1 1

    1 1

    22 11

    1 1

    2 *sinh 2 *( , ) (1, 0, 0) exp2 8 *

    Q i xTx B

    p

    mB me V x p e d m p

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    The Hartree Field

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    Output Characteristics of DG Device

    Tox = 1 nm Tsi = 3 nmLG = 9 nm LT = 17 nmLsd = 10 nm Nsd = 2 x 10

    20 cm-3

    Nb = 0 g= 1 nm/decade

    G = 4.188 VG = 0.4 V

    1.E+10

    1.E+13

    1.E+16

    1.E+19

    1.E+22

    DopingDensity[cm-3]

    Source DrainSi Channel

    Substrate

    BOXBackGate

    FrontGate

    LG

    LT

    Tsi

    Lsd

    Tox = 1 nm Tsi = 3 nmLG = 9 nm LT = 17 nmLsd = 10 nm Nsd = 2 x 10

    20 cm-3

    Nb = 0 g= 1 nm/decade

    G = 4.188 VG = 0.4 V

    1.E+10

    1.E+13

    1.E+16

    1.E+19

    1.E+22

    DopingDensity[cm-3]

    Source DrainSi Channel

    Substrate

    BOXBackGate

    FrontGate

    LG

    LT

    Tsi

    Lsd

    Source DrainSi Channel

    Substrate

    BOXBackGate

    FrontGate

    LG

    LT

    Tsi

    Lsd

    Source DrainSi Channel

    Substrate

    BOXBackGate

    FrontGate

    LG

    LT

    Tsi

    Lsd

    0

    500

    1000

    1500

    2000

    0 0.2 0.4 0.6 0.8 1Drain Voltage [V]

    DrainCurrent[uA/um]

    0

    15

    30

    45

    %C

    hangeinC

    urrent

    W/o quant. (3nm)QM (3nm)NEGF (3nm)W/o quant. (1nm)

    QM (1nm)%Change

    3 nmVG= 0.4 V

    1 nm

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    Summary

    Tunneling that utilizes transfer matrix approach can quiteaccurately be included in conjunction with particle-baseddevice simulators

    Quantum-mechanical size-quantization effect can beaccounted in fluid models via quantum potential that is

    proportional to the second derivative of the log of thedensity

    Effective potential approach has been proven to includesize-quantization effects rather accurately in conjunctionwith particle-based device simulators

    Neither the Bohm potential nor the effective potential canaccount for the modification of the density of statesfunction, and, therefore, scattering rates modificationbecause of the low-dimensionality of the system, and,therefore, mobility and drift velocity