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Semiconductor Device Noise Models Based on Semiclassical Transport 51153

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Title: Semiconductor Device Noise Models Based on Semiclassical Transport 51153


1
Semiconductor Device Noise Models Based on
Semiclassical Transport 5115-3
  • Can E. Korman
  • Department of ECE
  • The George Washington University
  • Washington, DC 20052
  • Collaborators
  • A. Piazza (Applied Wave Research, Inc.)
  • I. D. Mayergoyz (University of Maryland)

Noise Information in Nanoelectronics, Sensors
Standards SPIE's First International Symposium on
Fluctuations and Noise - Santa Fe, NM - June 1-4,
2003
2
Outline of the Talk
  • Introduction
  • Semiclassical Transport Theory
  • Stochastic Differential Equations Theory
  • Terminal Current Spectral Density Computation
  • Numerical Results
  • Numerical Techniques
  • Conclusion

3
1- Introduction
  • Motivation
  • Noise characterization of devices
  • Goal Connecting Electron Kinetics to Terminal
    Noise Characteristics
  • Related noise calculation techniques

4
Motivation
  • Low power low voltages and currents
  • Low voltage or current noise becomes critical
    problem
  • Accurate noise modeling is an essential element
    in modern device simulators

5
Noise Characterization of DevicesTerminal Noise
Spectral Density
  • Thermal noise
  • GR noise
  • Flicker or 1/f noise
  • Shot noise

6
Connecting Electron Kinetics to Terminal Noise
Characteristics
  • Comprehensive approach for device noise
    characterization Electron kinetics is described
    by the Semiclassical Transport Theory
  • Develop noise models in the framework of
    Semiclassical Transport Theory suitable for
    efficient numerical simulation and CAD

7
Connecting Electron Kinetics to Terminal Noise
Characteristics
8
Related Noise Calculation Techniques
  • Probabilistic approach reasonable assumption on
    the underlying microscopic process
  • Langevin Method add random source to
    deterministic differential equation
  • Monte Carlo Method Direct simulation of random
    electron kinetics - computationally intensive
  • SDE theory based model Connect electron
    scattering characteristics to terminal noise
    spectral density

9
2- Semiclassical Transport Theory
  • The adiabatic principle allows to separate
    crystal vibration from electron motion
  • The independent electron approximation treats
    electron-electron interactions by one electron
    effective potential
  • Each electron moves independently in a perfectly
    periodic potential due to lattice and all other
    electrons
  • Scattering mechanisms describe interaction of
    electrons with the lattice

10
2- Semiclassical Transport Theory (cont.)
  • Semiclassical Transport Theory predicts how, in
    the absence of collisions, the position and wave
    vector of each electron evolve in the presence of
    macroscopic electric and magnetic fields
  • Maxwells Equations describe the macroscopic
    fields
  • Electron position and wave vector correspond to a
    wave packet of Bloch electrons
  • Scattering causes random sudden jumps in the
    electron wave vector

11
2- Semiclassical Transport Theory (cont.)
  • Electron scattering from one wave vector to
    another is characterized by the transition
    probability function
  • Paulis exclusion principle limits the scattering
    rates
  • Such a process can be described in terms of
    occupation probability that satisfies Boltzmann
    transport equation (BTE)

12
Motion of wave packet of Bloch electrons
  • All distinct electron states are confined to a
    unit cell in reciprocal space first Brillouin
    zone
  • Velocity of wave packet
  • Force due to External Fields - Wave packet
    behaves classically

13
Macroscopic External Fields Poissons Equation
  • Electrostatic potential ?
  • Electric field E
  • Conduction valance band electron distributions
    f C and fV
  • Ionized impurity densities of donors acceptors
    ND and NA

14
Random Force Electron Scattering
  • Almost instantaneous changes in the value of the
    electron wave vector
  • Phonons deformation potential
  • Thermal generation-recombination Shockley Read
    Hall generation-recombination model
  • Ionized impurities screened Coulomb potential
  • Phonon scattering elastic, inelastic, isotropic,
    unisotropic, intervalley, intravalley, etc

15
Scattering Transition in k-space
  • Scattering probability per unit time
  • Transition rate Born-Von Karman boundary
    conditions

16
Paulis Exclusion Principle Scattering
transition from k to k
  • Transition into an occupied level is forbidden
  • Transition rate into partially filled group of
    level
  • Steady-state transition rate
  • f0 steady-state electron disribution function

17
Electron motion in reciprocal-space
18
Boltzmann Transport Equation (BTE) in terms of
electron occupation probability f0
LHS denotes flux in phase space
  • RHS denotes flux due to scattering events

19
Summary of Semiclassical Transport Model
  • Electrons drift due to macroscopic electrostatic
    field
  • Electrons scatter due to deviations from perfect
    periodicity of potential
  • Paulis exclusion principle limits scattering
    rates
  • Semiclassical transport embedded in Poissons and
    Boltzmann transport equations

20
Electron Kinetics Stochastic Differential
Equation (SDE) Electron motion can be
interpreted as a differential equation driven by
inhomogeneous randomly weighted Poisson process
SDE
  • Scattering rate (Poisson)
  • Transition rate

21
3 - Stochastic Differential Equations (SDE) Theory
  • Differential equations describing processes
    driven by random excitation
  • Wiener processes (continuous in time) - diffusion
  • Poisson processes (discontinuous in time) -
    scattering
  • These are continuous-state Markov processes
  • Process is completely characterized by its
    transition probability density function
  • Focker-Planck Equation
  • Kolmogoroff-Feller equations

22
Stochastic Differential Equation General Case
  • Differential equation driven by stochastic
    process j(y,t)
  • Stochastic process j(y,t) is characterized by
  • Intensity function (scattering rate)
  • Transition rate

23
Forward Kolmogoroff-Feller Equation (KFE)
General Case
  • The stochastic process y is characterized by the
    transition probability density function

24
Kolmogoroff-Feller Equation for Electron Motion
Described by Semiclassical Transport Theory
The electron transition probability density
function ? satisfies
25
3- Summary of SDE
  • Electron motion corresponds to Markov process
  • Process completely characterized by transition
    probability r
  • Transition probability function satisfies KFE
  • KFE identical to linear BTE
  • All stochastic information on electron kinetics
    is embedded in KFE or equivalently, linear BTE

26
4 - Terminal Current Spectral Density Computation
Goal compute spectral density of the terminal
current
  • Calculate the transition probability function r
  • Relate electron motion in phase-space state to
    the induced current at the device terminals
    Ramo-Schockley theorem
  • Combine the results of Steps (1) and (2) to
    calculate the autocovariance function or
    spectral density of induced terminal noise.

27
Ramo-Shockley Theorem
  • The extension of Ramos theorem by Cavalleri et
    al establishes a connection between induced
    terminal currents and motion of carriers inside a
    device
  • The model admits arbitrary mobile charge
    distribution and conduction current density

28
Ramo-Shockley Theorem (cont.)
  • The model shows that for terminal potentials Vj
    and terminal currrents Ij

E(0) is the electrostatic field due exclusively
to the applied potentials at the terminals j1,
, n
29
Ramo-Shockley Theorem (cont.)
  • At contact j the induced terminal current due to
    each electron with position x and wave vector k
    is

30
Autocovariance function computation of terminal
current
By definition, the autocovariance function of the
observed terminal current is
In terms of the Ramo-Shockley function ij and an
auxiliary function g it can be shown that the
autocovariance function of terminal current j is
as follows
where ? is the transition probability density
function and f is the steady-state electron
distribution function
31
Autocovariance function computation(cont.)
  • Terminal current autocovariance function
  • Auxiliary function g satisfies the transient BTE
  • Subject to the following special initial
    conditions

32
Current Spectral Density Computation
  • The spectral density is defined as the Fourier
    transform of the autocovariance function
  • Employing this definition it can be shown that
    the spectral density can be calculated in terms
    of an auxiliary function G
  • G satisfies the Fourier transform of the
    transient BTE


33
4 Summary of Terminal Current Spectral Density
Computation
  • Key computations for the terminal current
    spectral density function are reduced to solution
    of Kolmogorov-Feller Equation or Boltzmann
    Transport Equation
  • Ramo-Schockley theorem directly connects electron
    motion to current induced at the device terminals
  • A computationally efficient approach in terms of
    the effective distribution function G(x,k,w) was
    presented

34
5 Sample Numerical Results
  • Calculations for n-doped bulk silicon device
  • Thermal noise
  • Generation-Recombination noise
  • Employ Spherical harmonics technique for
    numerical calculations

35
Spectral Density Thermal Noise
36
Autocovariance Thermal Noise
37
Autocovariance Thermal Noise
38
Spectral Density GR Noise
39
Spectral Density GR Thermal Noise
40
5 - Summary
  • Simulation results are presented for bulk n-type
    silicon as a function of
  • Electric field
  • Temperature
  • Electron capture cross section
  • Results for thermal and Generation-Recombination
    noise are presented
  • Numerical results are in agreement with measured
    data
  • Results are obtained using computationally
    efficient Spherical Harmonic technique

41
6 - Numerical Implementation
  • Problem Steady state solution of Poisson and
    non-linear Boltzmann transport equations
  • Problem Transient solution of linear BTE with
    special initial condition in frequency domain
  • The BTE/KFE is a non-linear 7D equation (3D
    space, 3D momentum and 1D time)
  • Spherical harmonics technique is employed to
    reduce the number of dimensions in momentum space

42
Mathematical techniques
  • Poissons and non-linear Boltzmann transport
    equations are consistently solved employing
    Gummel block iteration method
  • BTE is iteratively solved in real-space
  • At a given point in real space, 3D non-linear
    equation in reciprocal-space is solved using
    spherical harmonics
  • No time iteration is required equation is solved
    in frequency domain

43
Spherical Harmonics Polynomials
  • Scattering involves transitions between spheres
  • Spherical harmonics give a more efficient
    representation of the distribution function

44
Gummel Iteration
start
Poissons equation
BTE
stop
n
y
45
Real-space iteration
start
BTE at xi
i0
i i1
n
stop
Last i
y
n
y
46
6 Summary of Numerical Techniques
  • The approach requires the numerical solution of
  • the steady-state Poisson equation
  • the steady-state non-linear Boltzmann transport
    equation
  • the transient linear Boltzmann transport equation
  • Gummel iteration used to decouple Poisson and
    Boltzmann transport equations
  • BTE solved in space iteratively
  • BTE solved in reciprocal-space using spherical
    harmonics
  • Transient solution performed in frequency domain

47
7 - Conclusion
  • Unified approach to model noise in the framework
    of semiclassical transport theory and stochastic
    differential equations
  • Noise is exclusively due to electron scattering
  • Model accounts for Paulis exclusion principle
  • Random electron motion in phase-space directly
    connected to induced terminal current Ramos
    theorem
  • Adapted spherical harmonics technique to solve
    transient BTE equation in frequency domain
  • Numerical solution approach based on well
    established techniques practical for CAD

48
Thank you for your attention
  • Questions?

49
Reference Publications and Presentations
  • C. E. Korman and I. D. Mayergoyz, Semiconductor
    Noise in the Framework of Semiclassical
    Transport,'' Phys. Rev. B, Vol. 54, No. 24, pp.
    17620-17627, 15 December, 1996.
  • A. J. Piazza, C. E. Korman and Amro M. Jaradeh,
    A Physics Based Semiconductor Noise Model
    Suitable for Efficient Numerical Implementation,
    IEEE Tran. On CAD of Integrated Circuits and
    Systems, Vol. 18, No. 12, pp. 1730-1740, December
    1999.
  • A. J. Piazza and C. E. Korman, Semiconductor
    Noise Computation Based on the Deterministic
    Solution of Poisson and Boltzmann Transport
    Equations, VLSI Design, 1998, vol. 8, Nos. (1-4),
    pp. 381-385.

50
Reference Publications and Presentations (cont.)
  • C. E. Korman and A. J. Piazza, Computation of
    Semiconductor Noise for Semiclassical Transport,
    proceedings of the International Semiconductor
    Device Research Symposium, Charlottesville,
    Virginia, 1995.
  • A. J. Piazza and C. E. Korman, Computation of the
    Spectral Density of Noise in Bulk Silicon Based
    on the Solution of the Boltzmann Transport
    Equation, VLSI Design, 1998, Vol. 6, Nos. (1-4),
    pp. 185-189.
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