2.3.3 Shockley-Read-Hall Recombination

In this chapter we take a closer look at the generation and recombination of carriers. Even the simple treatments given so far – cf. the formulas for the p-n junction – made it clear that generation and recombination are the major parameters that govern device characteristics and performance.
First, we will treat in more detail the band-to-band recombination in direct semiconductors, next the recombination via defects in indirect semiconductors, and for this we introduce and use the "Shockley -Read- Hall Recombination" or SRH model.
However, we will just sort of scratch the subject. In an advanced module some finer points to recombination are treated; here we will stick to fundamentals.
First a few basic remarks. Generally, we do not only have to maintain energy and momentum conservation for any generation/recombination process, we also have to assure that we keep the minimum of the free enthalpy, or in other words, we have also to consider the entropy of these processes. These requirements transform into the conditions
1. kk' = g as an expression of the (crystal) momentum conservation.
2. E eE h = D E something else for energy conservation.
We have ECEV = DE something else because the electrons and holes recombining are always close to the band edges for energy conservation.
DE something else refers to the unavoidable condition that "something else" has to provide the energy needed for generation, or must take away the energy released during recombination.
3. Now we look at the entropy. Recombination reduces the entropy of the system (empty bands are more orderly than bands with a few wildly moving holes and electrons). The "something else" that takes energy out of the system may in addition take some entropy out of it, too. However, no easy law can be formulated.
The first two points determine if a recombination/generation event – which we from now on are going to call an R/G-event – can take place at all, i.e. if it is allowed; the third point comes in – in principle – when we discuss the probability of an allowed R/G-event to take place. This insight, however, will only be used in an indirect way in what follows.
The major quantities are the recombination rate R and the generation rate G.
The recombination rate R is the more important one of the two. It is related to the carrier density ne,h by
 =  R
It is always directly given by the rate at which the carrier density decreases (the minus sign thus makes R a positive quantity) and it does not matter which carrier type we are looking at because dn e /dt = dnh/dt as long as the carriers disappear in pairs by recombination.
Note that the equilibrium condition of constant carrier density does not mean that there is no dynamics anymore in the charge carrier population (i.e. that the carriers remain where they are): When n remains constant, this just means that as many carriers recombine as are generated, since n is an average quantity. (That this is not unlike the drift velocity of electrons which can be zero despite large thermal velocities of the individual electrons.)

Recombination and Generation in Direct Semiconductors

If we first look at recombination in direct semiconductors, we need holes and electrons at the same position in the band diagram; i.e. in k-space. However, that does not imply that they are at the same position in real space. For a recombination event they have to find each other; i.e., we also need them to be at about the same position in real space.
The recombination rate R thus must be proportional to the two densities, ne and nh, because the probability of finding a partner scales with the carrier density. We thus can write down the recombination rate R as
R  =  r · ne · nh  =  r · Neff h  · Neffe  · exp –  ECEFe
· exp –  EF hEV
With r = proportionality constant, having the dimensions of volume/time; we will come back to this later. We also only assume only local equilibrium as evidenced by the use of quasi Fermi energies.
We can rewrite this equation as follows
R  =  r · Neffh  · Neff e  · exp – EC + E FeEFh + EV
  =  r · Neff h · Neffe · exp – ECEV
· exp –  EFhEF e
Using our old relation for the intrinsic carrier density ni
ni 2  =  Neffh  · Neff e  · exp –  ECEV
we finally obtain
R  =  r · ni2 ·  exp  EFeEF h
Note again that we have not invoked total equilibrium, but only local equilibrium in the bands – we use the quasi Fermi energies EFe,h. That is essential; after all it is recombination and generation that restore equilibrium between the bands and the SRH theory only makes sense for non-equilibrium.
If we were to consider total thermal equilibrium, we know that the generation rate G must be identical to the recombination rate R; both quasi Fermi energies are identical (= EF) and R = r · ni2 applies.
Note that we did not assume intrinsic conditions; the Fermi energy can have any value, i.e. the semiconductor may be doped.
In essence, we see the following:
The recombination rate in non-equilibrium depends very much on the actual carrier density!
So far it was easy and straigth-forward. Now comes an important point.
In contrast to the recombination rate R, the generation rate G does not depend (very much) on the carrier density; it is just a reflection on the thermal energy contained in the system and therefore pretty much constant. In other words, under most conditions we have
G = Gtherm   »  constant ¹ R(n) 
We may, from the above consideration, equate G under all conditions with the recombination rate for equilibrium, i.e.
G = Gtherm  =  r · ni2  
In non-equilibrium, which will be the normal case for devices under operation, the difference (R – G) is no longer zero, but has some value
U  =  R  –  G
Since R is mostly (but not always) larger than G under non-equilibrium conditions, U is the net rate of recombination (or, on special occasions, the net generation rate).
Using the expressions derived so far, we obtain
U  =  R  –  Gtherm   =  r · (ne · nh –  n i2)  =  r · ni2 · æ
exp  EF eEFh
  –   1 ö
This equation tells us, for example, how fast a non-equilibrium carrier density will decay, i.e. how fast full equilibrium will be reached, or, if we keep the non-equilibrium density fixed for some reason, what kind of recombination current we must expect.
This is so because U, the difference between recombination and generation, times the charge is nothing but a net current flowing from the conduction band to the valence band (for positive U).
Determining the Proportionality Constant r
We still need to determine the proportionality constant r.
This is not so easy, but we can make a few steps in the right direction. We assume in a purely classical way that an electron (or hole) moves with some average velocity v through the lattice, and whenever it encounters a hole (or electron), it recombines.
The problem is the word "encounters ". If the particles were to be small spheres with a diameter dp, "encountering" would mean that parts of such a sphere would be found in the cylinder with diameter dp formed by another moving sphere because that would cause a physical contact.
Our particles are not spheres, but for the purpose of scattering theory we treat them as such, except that the diameter of the cylinder that characterizes its "scattering size" is called scattering cross section s and has a numerical value that need not be identical to the particle size.
One electron now covers a volume v · s per second and all Ne electrons of the whole sample (a number, not a density) probe per second the volume
Vprobed  = N e · v · s
Any time an electron encounters a hole in the volume it probes, it recombines. The absolute recombination rate Rabs then is simply the number of encounters per second, occurring in the whole sample.
How many holes are "hit" per second? In other words, how many are to be found in the volume probed? That is easy: The number Nh of holes encountered in the volume probed by electrons, and thus the recombination rate is
Nh =  nh ·  Vprobed  =  nh · Ne · v · s  =  Rabs
Here, nh is simply the density of holes in the sample. You many wonder if this is correct, considering that the holes move around, too, but simply realize that the density of holes is nevertheless constant.
The formula is a bit unsatisfying, because it contains the volume density of holes, but the absolute number of electrons.
That is easily remedied, however, if we express N e, the number of electrons, by their density ne via Ne = ne · V with V = sample volume. Using the latter for normalizing the absolute recombination rate to the sample volume, this gives us
R =  Rabs
 =    Recombinations per
s and cm 3
   =   ne · nh · v · s
In other words, if we use the density of the electron and holes, we obtain a recombination rate density , i.e. recombination events per s and per cm3 – as it should be. As always, we are going to be a bit sloppy about keeping densities and numbers apart. But there is no real problem: Just look at the dimensions you get, and you know what it is.
A comparison with the formula from above yields
r  =  v · s
This leaves us with finding the proper value for s. Whereas this is difficult (in fact, the equation above is more useful for determining s from measurements of R than to calculate r), we are still much better off than with r alone:
Whereas we had no idea about a rough value for r, we do know something about v (it is the group velocity of the carriers considered), and we know at least the rough order of magnitude for s: We would expect it to be in the general range of atomic dimensions (give or take an order of magnitude).
You might wonder now why we assume that any "meeting" of the elctrons and holes leads to recombination, given that we have to preserve momentum, too. You are right, but remember:
We are treating direct semiconductors here! Since we only consider the mobile electrons and holes, we only consider the ones at the band edges – and those have the same k-vector in the reduced band diagram!
Useful Approximations and the Lifetime t
We now consider non-equilibrium, but describe it in terms of deviations from equilibrium. Then it is sensible to rewrite the carrier densities (or numbers, take whatever you like) in terms of the equilibrium density ne,h(equ) plus/minus some delta:
ne,h  =  ne,h(equ)  +  Dne,h
This is one of the decisive "tricks" to get on with the basic equations, because it permits to specify particular cases (e.g. Dne,h << ne,h(equ) or whatever), and then resort to approximations. We will encounter this "trick" fairly often.
We obtain after some shuffling of the terms form the equation for the net recombination rate U
U   =    v · s · æ
{n e(equ) + Dne} · {nh(equ) + Dnh} – ne(equ) · nh(equ) ö
So far everything is still correct. But now we consider a first special, but still rather general case:
We assume that Dne = Dnh = Dn, i.e. that only additional electron–hole pairs were created in non-equilibrium. We then may simplify the equation to
U   =   r · æ
Dn · {ne (equ) + nh(equ)} + Dn 2 ö
We can simplify even more. For the extrinsic case where one carrier density – let's say for example nh – is far larger than ne or Dn (i.e. we have a p-doped semiconductor), we may neglect the terms Dn · ne(equ) and Dn2 and obtain
U   »   r · nh · D n
U was the difference between the recombination and the generation rate. We are now looking at an approximation where only some Dn in the density of the minority carriers is noticeably different from equilibrium conditions (where we always have U = 0).
We thus may write
U  =  R(equ) + R(D) – G(equ) = R(D)
Here, R(D) denotes the additional recombination due to the excess minorities. Remembering the basic definition of R we see that now we have
d(Dne )
 =  U  =  r · nh · Dne  = – v · s · nh · Dne
This is a differential equation for Dne(t), it has the simple solution
Dne(t)  =  Dne(t = 0) · exp –    t   
The quantity demanded by the general solution is, of course, the life time of the minority carriers. We now have a formula for this prime parameter, it comes out to be
t  =  1 
v · s · nh
  =   1 
v · s · nmaj
The last equality generalizes for both types of carriers – it is always the density of the majority carriers that determine the lifetime of the minority carriers. This is clear enough considering the "hit and recombine" scenario that we postulated at the beginning
Substituting r · n h with 1/t in the equation for U yields
U  =  D n
In other words: The recombination rate in excess of the recombination rate in equilibrium is simply given by the excess density of minority carriers divided by their life time.
In yet other words:
The net current flowing from the band containing the minority carriers to the other band is given by U (times the elementary charge, of course, and times the total sample volume), because U gives the net amount of carriers "flowing" from here to there! And that is the definition of a current!
This result not only justifies our earlier approach, it gives us the minority carrier life time in more basic quantities including (at least parts) of its temperature dependence via the thermal velocity v and the majority carrier density nh – the T-dependence of which we already know.
Since 1/nh is more or less proportional to the resistivity, we expect t to increase linearly with the resistivity which it does as illustrated before, at least for resistivities that are not too low.
A rough order of magnitude estimate gives indeed a good value for many direct semiconductors:
s  »  10–15 cm2         Þ         t  »  10–9 s  =  1 ns
v  =  107 cm/s
n h  =  1017 cm–3
Recombination and Generation in Indirect Semiconductors
In indirect semiconductors, direct recombination is theoretically impossible or, being more realistic, very improbable.
In general, a recombination event needs a third partner to provide conservation of energy and crystal momentum.
Under most (but not all) circumstances, this third partner is a lattice defect, most commonly an impurity atom, with an energy state "deep" in the band gap, i.e. not close to the band edges.
Recombination then is determined by these "deep states" or deep levels, and is no longer an intrinsic or just doping dependent property.
How the recombination and generation depends on the properties of deep levels is the subject of the proper Shockley–Read–Hall theory (what we did so far was just a warming-up exercise). It is a lengthy theory with long formulas; here we will just give an outline of the important results. More topics will be covered in an even more advanced module.
First we look at the situation in a band diagram that shows the relevant energy levels plus the mid-band energy level EMB, which will come in handy later on.
Deep level
Besides the energy level of the "deep level" defect, we now need four transition rates instead of just one recombination rate:
  • Red, the rate with which electrons from the conductance band transit from the conduction band to the deep level, or more simply put, occupy the deep level with the energy EDL – in short: the rate with which they are going down to the deep level.
  • Reu , the rate with which electrons occupying the deep level state go up to the conduction band.
  • Rhu, the rate with which holes from the valence band go up to the deep level – or better: the electrons in the deep level go down to the valence band, and finally
  • Rhd, the rate with which holes from the deep level go down to the valence band – or better: electrons up to the deep level.
The equilibrium density of electrons (and holes) on the deep level is, as always, given by the Fermi distribution. We have
nDL = NDL · f(EDL, T) = density of negatively charged deep levels with one electron sitting on it, and
n0DL = NDL · [1 – f(EDL, T)] = density of deep levels with no electron sitting on it. NDL , of course, is the density of deep level states, e.g. the density of impurity atoms. It's written with capital N (otherwise used for absolute numbers) to avoid confusion with the carrier densities.
To make life easier, we assumed that the deep level is normally neutral, i.e. does not contain an unalterable fixed charge, and it can only accommodate one additional electron.
We may now write down formulas for the transition rates in direct analogy to the consideration of the recombination rate in direct semiconductors as given above. For Red we have
Re d  =  r · ne · n0DL  =  v · se · ne · NDL · [1 – f(EDL, T)]
With se = scattering cross section (also called capture cross section) of the deep level for electrons.
For the other transition rate Reu we have to think a little harder. For the electron trapped at the deep level to go up to the conduction band it needs a free place up there, hence:
Re u  =  r' · (Neffe  – ne) · n DL
With r' = some proportionality constant, principally different from r, and Neff ene = density of free places (which, please remember, aren't holes!) in the conduction band.
Since ne is much smaller than Neffe, we may approximate this equation by
Reu  »  r' · Neffe · NDL · f(E DL, T)
We have not invoked some cross section and thermal velocity here, because the electron now is localized and doesn't move around. We also used a different proportionality constant r' because the situation is not fully symmetric to the reverse process. It is common to call the quantity ee = r' · Neffe the emission probability for electrons from the deep level.
The emission probability contains the information about the generation of carriers from the deep level; in this it is comparable to the generation rate from the valence band for the simple recombination theory considered above.
Now , if we assume that the transitions of conduction band electrons to the deep level and their re-emission to the conduction band are in local equilibrium (which does not necessarily entail total equilibrium), we have Re u = Red.
From this we get – after a minimal shuffling of the terms – for the emission probability ee in local equilibrium:
ee  =  v · s e · ne · [1 – f(E DL, T)]
f(EDL, T)
Again, as in the case of the generation rate G for direct semiconductors, we may assume that the emission probability ee is pretty much constant and this is a crucial point for what follows.
Since we want to find quantities like life times as a function of the density and energy level of the deep level, it is useful to use the mid-band energy level as a reference, and to rewrite the equation for ee in terms of this mid-band level EMB via the relations
1  –  f(EDL, T)
f(EDL , T)
 = exp –  EF  –  EDL


ni   =  Neffe  · exp –  ECEMB
These equations may need a little thought. The first one came up before in a similar way, the second simply defines mid band-gap, and the last one uses the fact that the Fermi energy for intrinsic semiconductors is in mid band gap (at least in a good approximation).
Using these equations, we first rewrite the formula for the density of electrons in the conduction band and obtain
ne  =  N effe  · exp – E CEF
  = Neffe  · exp –  ECEMB
· exp –  EMBEF
  =  ni · exp  EFEMB
Putting everything together, we get for the emission probability
ee  =  v · se · ni · exp EDLEMB
This is the best we can do to describe the traffic of electrons between the deep level and the conduction band.
Next, we do the matching calculation for the transitions rates with the valence band, Rhu and Rh d.
Except, we won't do it. Too boring – everything is quite similar. As the final result for the emission probability for the holes, e h, we obtain exactly what we should expect anyway:
eh  =  v · sh · ni · exp EMBEDL
The Net Interband Recombination
We captured the electron and hole traffic betwen a deep level and the conduction or valence band, respectively, with these equations – always for local equilibrium of the deep level with the respective band. Now we consider the interband generation and recombination rates, G and R .
This is exactly the same thing as the money traffic form one major bank to another one via an intermediate bank. Each bank can deposit and withdraw money from all three accounts, while the total amount of all the money must be kept constant. If it would be your money, you sure like hell would want to and be able to keep track of it. So let's do it with electrons and holes, too.
With G we still denote the rate of electron–hole pair generation taking place directly between the bands; by thermal or other energies, e.g. by illumination. It is thus the rate with which electrons and holes are put directly into the conduction or valence band, no matter what goes on between the deep level and the bands.
We may, for some added clarity, decompose G into Gperfect, the generation always going on even in a hypothetical perfect semiconductor, and Gne for whatever is added in non-equilibrium (e.g. the generation by light). We have G = Gperfect + Gne .
After all, before we put in "our " deep levels or switched on the light, the hypothetically perfect crystal already must have had some generation and recombination, too (for which Rperfect = Gperfect must hold). However, we can expect that Rperfect is rather small in a perfect indirect semiconductor, which makes Gperfect rather small, too.
The rate of change of the electron and hole density in their bands is then the sum total of all processes withdrawing and depositing electrons or holes, i.e.
 =  G perfect  +  Gne   –   Rperfect   + Reu  –  Red  =  Gne  –  (Red  –  Reu)

 =  Gperfect  +  Gne   –   Rperfect   +  Rhd  –  Rhu  = Gne  –  (Rhu  –  Rhd)
Note that G perfect – R perfect = 0 by definition.
Local equilibrium between the bands and the deep level, still not necessarily implying total equilibrium, now demands that both dne/dt and dnh /dt must be zero.
That means that the density of electrons in the conduction band and the density of the holes in the valence band do not change with time anymore. However, that does not mean that they have their global equilibrium value, only that we have a so-called steady state (in global non-equilibrium) which, on the time scales considered, appears to keep things at a constant value.
As an example, a piece of semiconductor under constant illumination conditions will achieve a steady state in global non-equilibrium conditions. The carrier densities in the bands will be constant, but not at their equilibrium values if light generates electron–hole pairs all the time.
This gives us the simple equation
Re d   –  Reu   =   Gne   =   Rhu  –  Rhd
Essentially, this says that the total electron or hole traffic or current [= difference of the partial rates (times elementary charge)] from the conduction or valence band, respectively, to the deep level are identical and equal to the extra band-to-band generation current produced in non-equilibrium for the given material and situation.
But steady state also implies that there must be an additional recombination exactly equal to Gne and that is of course exactly what the terms Red  –  Reu or Rhu  –  Rhd denote: They are identical to the additional recombination rates needed for balancing the additional generation Gne, or simply
We thus have
Red  –  R eu  = R  –  R perfect  = R  –  Gperfect   =: UDL
The quantity UDL is exactly analogous to the difference (R – G) defined for direct semiconductors.
UDL is also the difference between the recombination to a deep level and the emission from it. For the example considered so far (additional generation via illumination) it must be positive, there is more recombination than generation
However, our treatment is completely general; UDL can have any value – if it is negative, we would have more generation via deep levels than recombination.
Of course, UDL makes only sense for global non-equilibrium conditions, because for global equilibrium UDL must be zero!
All we have to do now is to express the Re's with the formulas from above. Inserting the equations for the various R's, the emission probabilities, and setting se = sh = s for the sake of simplicity, we get, after some shuffling of the terms, the final equation
UDL  =  

v · s · NDL · (ne · nh  –  ni 2)

ne   +  nh  +  2ni · cosh EDLE MB
The cosh (= hyperbolic cosine) comes from the sum of the two exponential functions. Its value is 1 for EDL = EMB ; it increases symmetrically for deviations of EDL from the mid-level energy EMB.
A chain hanging down from two posts has exactly a cosh(x) shape – that's the way to memorize the general shape of a cosh curve. If you want to look more closely at the cosh function, activate the link.
The equation for UDL is quite similar to the one we had for direct semiconductors, as far as the numerator is concerned. We will explore a little more what it implies.
For global equilibrium, the mass action law ne · nh = ni2 applies, and UDL = 0. In other words, there is no net recombination, i.e. recombination in excess of what is always going on.
Without deep levels UDL = 0! The recombination rate then is fixed and simply Rperfect.
The recombination rate – everything else being constant – is directly proportional to the density of the deep levels and their scattering cross section (or capture cross section as it is called in this case).
Since the recombination rate is highest for deep levels exactly in mid-band (look at the cosh function), defects with levels near mid-band are more efficient in recombining carriers than those with levels farther off the mid-band position.
Approximations and the Lifetime t
As before, let's look at some special case. Again, we write the carrier densities as ne,h = n e,h(equ) + Dn assuming equal D 's for electron and holes.
This gives us
U v · s ·N DL ·   [ne(equ)  +  Dn] · [nh(equ)  + D n]  –  ni2
ne(equ)  +  nh(equ)  +  2 Dn  +  2ni · cosh[(E DLEMB) / (kT)]
Looking at a p-doped semiconductor and only considering the large densities nh as in the example before, we obtain
U  =  v · s · NDL · n h(equ) · Dne
n h(equ)  +  2ni · cosh[(E DLEMB) / (kT)]
Since ni is also much smaller than nh(equ) , we may neglect the whole cosh term, too – as long as cosh[(EDLEMB)/(kT)] is not large, i.e. for deep levels around mid-band.
As a consequence, nh(equ) cancels and we are left with
U  =  v · s · NDL · D ne
Again, as before, the change in excess minority carrier density is given by d(Dne)/dt = –U, giving
d(D ne)
 =  – v · s · NDL · D ne
The solution of the differential equation now becomes trivial and we have
D n e(t)  =  Dne (t = 0) · exp –    t   
with t = minority life time or better recombination life time in indirect semiconductors defined by

t   =    1
v · s · NDL

This is the same equation as before except that the density of the majority carriers (holes in the valence band for the example) now is replaced by the density of (mid-band) deep levels.
That this formula is a useful approximation is shown in the two illustrations below:
recOmbinatiOn life time
Life time with Au
Dependence of the life time on the deep level position relative to the mid level – it is fairly constant (and small) as long as the deep level is approximately in mid band. Dependence of life time on deep level density – it is linear as predicted. (The red curve is for p-Si, of course.)
The picture on the right illustrates a sad fact hidden in all these equations: it doesn't take much dirt (or contamination, to use the proper word) to considerably degrade the life time. Interstitial gold atoms obviously are felt at 1014 cm–3 , i.e. at concentrations well below ppb.
More to Shockley–Read–Hall recombination can be found in an advanced module.

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© H. Föll (Semiconductors - Script)