In solid-state physics, the Poole–Frenkel effect (also known as Frenkel–Poole emission[1]) is a model describing the mechanism of trap-assisted electron transport in an electrical insulator. It is named after Yakov Frenkel, who published on it in 1938,[2] extending the theory previously developed by H. H. Poole.
Electrons can move slowly through an insulator by the following process. The electrons are generally trapped in localized states (loosely speaking, they are "stuck" to a single atom, and not free to move around the crystal). Occasionally, random thermal fluctuations will give an electron enough energy to leave its localized state, and move to the conduction band. Once there, the electron can move through the crystal, for a brief amount of time, before relaxing into another localized state (in other words, "sticking" to a different atom). The Poole–Frenkel effect describes how, in a large electric field, the electron doesn't need as much thermal energy to be promoted into the conduction band (because part of this energy comes from being pulled by the electric field), so it does not need as large a thermal fluctuation and will be able to move more frequently.On theoretical grounds, the Poole–Frenkel effect is comparable to the Schottky effect, which is the lowering of the metal-insulator energy barrier due to the electrostatic interaction with the electric field at a metal-insulator interface. However, the conductivity arising from the Poole–Frenkel effect is detected in presence of bulk-limited conduction (when the limiting conduction process occurs in the bulk of a material), while the Schottky current is observed when the conductivity is contact-limited (when the limiting conduction mechanism occurs at the metal-insulator interface).
\sigma
105V/cm
103V/cm
\sigma=\sigma0\exp{(\alphaE)}
\sigma0
\alpha
E is the applied electric field.In this model the conduction is supposed to be carried by a free electron system moving in a self-consistent periodic potential.On the contrary, Frenkel derived his formula describing the dielectric (or the semiconductor) as simply composed by neutral atoms acting as positively charged trap states (when empty, i.e. when the atoms are ionized). For localized trap states with Coulomb potentials, the barrier height that an electron must cross to move from one atom to another is the depth of the trap potential well. Without any externally applied electric field, the maximum value of the potential is zero and is located at infinite distance from the trap center.[3] When an external electric field is applied, the height of the potential barrier is reduced on one side of the trap by the amount[2]
\DeltaU=qEr0+
q2 | |
4\pi\epsilonr0 |
q is the elementary charge
\epsilon
r0
q2/(4\pi\epsilon
2 | |
r | |
0) |
=qE
r0=\sqrt{q/(4\pi\epsilonE)}
\DeltaU=qE\sqrt{
q | |
4\pi\epsilonE |
\exp\left(
-q\phiB | |
kBT |
\right)
\phiB
kB
T is the temperaturethen, in presence of an external electric field the electrical conductivity will be proportional to[2]
\exp\left(
-q\left(\phiB-\sqrt{qE/(\pi\epsilon) | |
\right |
)}{kBT}\right)
\sigma=\sigma0\exp\left(
q\sqrt{qE/(\pi\epsilon) | |
E
J\proptoE\exp\left(
-q\left(\phiB-\sqrt{qE/(\pi\epsilon) | |
\right |
)}{kBT}\right)
J\proptoV\exp\left(
q | |
kBT |
\left(2\sqrt{qV/(4\pi\epsilond)}-\phiB\right)\right)
For materials such as Si3N4, Al2O3, and SiO2, at high temperature and high field regimes, the current J is likely due to Poole–Frenkel emission.[1] The detection of Poole–Frenkel emission as the limiting conduction process in a dielectric is usually made studying the slope in the so-called Poole–Frenkel plot, where the logarithm of the current density divided by the field (
ln(J/E)
\sqrt{E}
ln(J/E)
\sqrt{E}
\kappa=\epsilon/\epsilon0
\epsilon0
\kappa
\kappa=n2
n
Although many progresses have been made on the topic since the classical work of Frenkel,the Poole–Frenkel formula has been spreadly used to interpret several non-ohmic experimental currents observed in dielectrics and also semiconductors.[8] [9] The debate about the underlying assumptions of the classical Poole–Frenkel model has given life to several improved Poole–Frenkel models. These hypotheses are presented in the following.
Only electron (single-carrier) conduction is considered, assuming the existence of ohmic contacts capable to refill detrapped electrons at the electrodes, and space charge effects are neglected, supposing that the field is uniform. A revisitation of this latter assumption can be found, for example, in the “theory of space charge limited current enhanced by Frenkel effect” developed by Murgatroyd.
The carriers mobility is assumed to be field-independent. Neglecting every kind of diffusion process for the de-trapped carriers, the pre-exponential factor in the Poole–Frenkel formula is thus proportional to
E
E-1/2
E1/2
E1/2
E-3/2
E-3/4
In the classical Poole–Frenkel theory a Coulombic trap potential is assumed, but steeper potentials belonging to multipolar defects or screened hydrogenic potentials are considered as well.
Regarding the typology of traps, the Poole–Frenkel effect is described to occur for positively charged trap sites, i.e. for traps that are positive when empty and neutral when filled, in order for the electron to experience a Coulombic potential barrier due to the interaction with the positively charged trap. Donors or acceptors sites and electrons in the valence band will also exhibit the Poole–Frenkel effect as well. On the contrary, a neutral trap site, i.e. a site that is neutral when empty and charged (negatively for electrons) when filled, will not exhibit Poole–Frenkel effect.Among the others, Simmons has proposed an alternative to the classical model with shallow neutral traps and deep donors, capable to exhibit a bulk-limited conduction with a Schottky electric field dependence, even in presence of a Poole–Frenkel conduction mechanism, thus explaining the "anomalous Poole–Frenkel effect" revealed by Ta2O5 and SiO films.Models there exist that consider the presence of both donor and acceptor trap sites, in a situation called compensation of traps.The model of Yeargan and Taylor, for example, extends the classical Poole–Frenkel theory including diverse degrees of compensations: when only one kind of trap is considered, the slope of the curve in a Poole–Frenkel plot reproduces that obtained from Schottky emission, in spite of the barrier lowering being twice that for Schottky effect; the slope is twice larger in presence of compensation.[13]
As a further assumption a single energy level for the traps is assumed. However, the existence of further donor levels is discussed, even if they are supposed to be entirely filled for every field and temperature regime, and thus to not furnish any conduction carrier (this is equivalent to state that the additional donor levels are placed well below the Fermi level).
The calculation made for the trap depth reduction is a one-dimensional calculation, resulting in an overestimation of the effective barrier lowering.In fact, only in the direction of the external electric field the potential well height is lowered as much estimated accordingly to the Poole–Frenkel expression. More accurate calculation, performed by Hartke[14] making an average of the electron emission probabilities with respect to any direction, shows that the growth of the free carriers concentration is about an order of magnitude less than that predicted by Poole–Frenkel equation. The Hartke equation is equivalent to
J\proptoE\exp\left(
-q\phiB | |
kBT |
\right)\left(
1 | |
2 |
+
1 | |
\beta2E |
\left(1+\left(\beta\sqrt{E}-1\right)\exp(\beta\sqrt{E})\right)\right)
\beta=
q | |
kBT |
\sqrt{
q | |
\pi\epsilon |
}
Poole–Frenkel saturation occurs when all the trap sites become ionized, resulting in a maximum of the number of conduction carriers.The corresponding saturation field is obtained from the expression describing the vanishing of the barrier:
\phiB-\sqrt{
qEs | |
\pi\epsilon |
}=0
Es
Es=
\pi\epsilon{\phiB | |
2}{q} |
In charge trap flash memories, charge is stored in a trapping material, typically a silicon-nitride layer, as current flows through a dielectric. In the programming process, electrons are emitted from the substrate towards the trapping layer due to a large positive bias applied to the gate. The current transport is the result of two different conduction mechanisms, to be considered in series: the current through the oxide is by tunneling, the conduction mechanism through the nitride is a Poole–Frenkel transport. The tunneling current is described by a modified Fowler-Nordheim tunneling equation, i.e. a tunneling equation that takes into account that the shape of the tunneling barrier is not triangular (as assumed for the Fowler-Nordheim formula derivation), but composed of the series of a trapezoidal barrier in the oxide, and a triangular barrier in the nitride. The Poole–Frenkel process is the limiting mechanism of conduction at the beginning of the memory programming regime due to the higher current provided by tunneling. As the trapped electron charge raises, beginning to screen the field, the modified Fowler-Nordheim tunneling becomes the limiting process. The trapped charge density at the oxide-nitride interface is proportional to the integral of the Poole–Frenkel current flowed across it.With an increasing number of memory write and erase cycles, retention characteristics worsen due to the increasing bulk conductivity in the nitride.