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P.Ravindran, FME-course on Ab initio Modelling of solar cell Materials 19 June 2015 Evolution of Band structure of Solids
http://folk.uio.no/ravi/MENA9520-15
Prof.P. Ravindran, Department of Physics, Central University of Tamil
Nadu, India
&Center for Materials Science and Nanotechnology,
University of Oslo, Norway
Evolution of Bands in Solids
1
P.Ravindran, FME-course on Ab initio Modelling of solar cell Materials 19 June 2015 Evolution of Band structure of Solids
Band Structure: KCl
We first depict the band structure of an ionic crystal, KCl. The bands are very
narrow, almost like atomic ones. The band gap is large around 9 eV. For alkali
halides they are generally in the range 7-14 eV.
P.Ravindran, FME-course on Ab initio Modelling of solar cell Materials 19 June 2015 Evolution of Band structure of Solids
Band Structure: silver (fcc)
P.Ravindran, FME-course on Ab initio Modelling of solar cell Materials 19 June 2015 Evolution of Band structure of Solids
Band Structure: tungsten (bcc)
P.Ravindran, FME-course on Ab initio Modelling of solar cell Materials 19 June 2015 Evolution of Band structure of Solids
Empirical pseudopotential method
Energy band of Si, Ge and Sn
Empirical pseudopotential
method
Si Ge Sn
P.Ravindran, FME-course on Ab initio Modelling of solar cell Materials 19 June 2015 Evolution of Band structure of Solids
6Band structure of semiconductor
Calculated energy band structure of
Silicon
Calculated energy band structure of
GaAs
- Interband transitions : The excitation or relaxation of electrons between
subbands
- Indirect gap : The bottom of the conduction band and the top of the
valence band do not occur at the same k
- Direct gap : The bottom of the conduction band and the top of the
valence band occur at the same k
P.Ravindran, FME-course on Ab initio Modelling of solar cell Materials 19 June 2015 Evolution of Band structure of Solids
DOS is Nanomaterials
In bulk (a), layered (b) and wire (c) materials, there are always states populated which do not contribute to gain. These are parasitic states and contribute to inefficiency.
In quantum dot (d) materials, the DOS is a set of discrete states. Theory predicts this type of material is ideal for the gain region of a laser because fewer parasitic states are occupied.
P.Ravindran, FME-course on Ab initio Modelling of solar cell Materials 19 June 2015 Evolution of Band structure of Solids
8
First Brillouin zone E vs. k band
diagram of zincblende semiconductors
One relevant conduction band is
formed from s- like atomic orbitals“unit cell” part of wavefunction is
approximately spherically symmetric.
The three upper valence bands are
formed from (three) p- like orbitalsand the spin-orbit interaction splits off
lowest, “split-off” hole (i. e., valence)
band. The remaining two hole bands
have the same energy (“degenerate”)at zone center, but their curvature is
different, forming a “heavy hole” (hh)
band (broad), and a “light hole” (lh)band (narrower)
P.Ravindran, FME-course on Ab initio Modelling of solar cell Materials 19 June 2015 Evolution of Band structure of Solids
SnO2: band structure
VBM
CBM
Density of States
P.Ravindran, FME-course on Ab initio Modelling of solar cell Materials 19 June 2015 Evolution of Band structure of Solids
10
P.Ravindran, FME-course on Ab initio Modelling of solar cell Materials 19 June 2015 Evolution of Band structure of Solids
11
How to get conduction in Si?
P.Ravindran, FME-course on Ab initio Modelling of solar cell Materials 19 June 2015 Evolution of Band structure of Solids
12
Doping Silicon with Donors (n-type)
P.Ravindran, FME-course on Ab initio Modelling of solar cell Materials 19 June 2015 Evolution of Band structure of Solids
13
Doping Silicon with Acceptors (p-type)
P.Ravindran, FME-course on Ab initio Modelling of solar cell Materials 19 June 2015 Evolution of Band structure of Solids
14
Atomic Density
for Si
P.Ravindran, FME-course on Ab initio Modelling of solar cell Materials 19 June 2015 Evolution of Band structure of Solids
15
Summary of n- and p-type Silicon
P.Ravindran, FME-course on Ab initio Modelling of solar cell Materials 19 June 2015 Evolution of Band structure of Solids
16
P.Ravindran, FME-course on Ab initio Modelling of solar cell Materials 19 June 2015 Evolution of Band structure of Solids
17
P.Ravindran, FME-course on Ab initio Modelling of solar cell Materials 19 June 2015 Evolution of Band structure of Solids
Introduction to Silicon
6
The appearance of Band Gap, separating CB and VB
The 6 CB minima are not located at the center of 1st
Brillouin zone, INDIRECT GAP
CB VB-H VB-L
1st Brillouin zone of Diamond
lattice
CB
VB
Anisotropy in surface of E
P.Ravindran, FME-course on Ab initio Modelling of solar cell Materials 19 June 2015 Evolution of Band structure of Solids
19
P.Ravindran, FME-course on Ab initio Modelling of solar cell Materials 19 June 2015 Evolution of Band structure of Solids
20
The Bandgap Problem of DFT
P.Ravindran, FME-course on Ab initio Modelling of solar cell Materials 19 June 2015 Evolution of Band structure of Solids
21
The Bandgap problem [Sham,Schluter, PRL, 51, 1888 (1983).
P.Ravindran, FME-course on Ab initio Modelling of solar cell Materials 19 June 2015 Evolution of Band structure of Solids
22
Baandgap Error in Semiconductors from LDA
P.Ravindran, FME-course on Ab initio Modelling of solar cell Materials 19 June 2015 Evolution of Band structure of Solids
23Calculated Badgap values of Si from various level of Calculation
P.Ravindran, FME-course on Ab initio Modelling of solar cell Materials 19 June 2015 Evolution of Band structure of Solids
24GWA calculation of Bandgap of Semiconductors
P.Ravindran, FME-course on Ab initio Modelling of solar cell Materials 19 June 2015 Evolution of Band structure of Solids
25
Graphite band structure (Semi Metal)
P.Ravindran, FME-course on Ab initio Modelling of solar cell Materials 03 June 2013 Various Aspects of Energy Issues
Fermi level
As Fermions are added to an energy band, they will fill the
available states in an energy band just like water fills a
bucket.
The states with the lowest energy are filled first, followed by
the next higher ones.
At absolute zero temperature (T = 0 K), the energy levels are
all filled up to a maximum energy, which we call the Fermi
level. No states above the Fermi level are filled.
P.Ravindran, FME-course on Ab initio Modelling of solar cell Materials 03 June 2013 Various Aspects of Energy Issues
22/3
2
( ) 3( )
8F
hc NE
mc V
FERMI ENERGY
P.Ravindran, FME-course on Ab initio Modelling of solar cell Materials 19 June 2015 Evolution of Band structure of Solids
Fermi surface sampling for metallic systems
The determination of the Fermi level might be delicate for metallic systems
Slightly different choices of k-points can lead to bands
entering or exiting the sum, depending if a given
eigenvalue is above or below the Fermi level.
Band structure of bulk Al
For this k-point, three
bands are occupied
For this k-point, two
bands are occupied
For this k-point, one
band is occupied
For a sufficiently dense Brillouin zone sampling, this should not be a problem
P.Ravindran, FME-course on Ab initio Modelling of solar cell Materials 19 June 2015 Evolution of Band structure of Solids
For the k-points close to the Fermi surface, the
highest occupied bands can enter or exit the sums
from one iterative step to the next, just because the
adjustement of the Fermi energy
Difficulties in the convergence of the self-consistence procedure
with metals: smearing the Fermi surface
Instability of the self-consistent procedure
Solution 1: Use small self-consistent mixing coefficients
Solution 2: Smear the Fermi surface introducing a distribution of occupation number
The occupations are not any longer 1 (if below EF) or 0 (if above EF)
Gaussians
Fermi functions
C. –L. Fu and K. –M. Ho, Phys. Rev. B 28, 5480 (1989)
P.Ravindran, FME-course on Ab initio Modelling of solar cell Materials 19 June 2015 Evolution of Band structure of Solids
Smearing the Fermi surface: the Electronic Temperature
is a broadening energy parameter that is adjusted to avoid instabilities
in the convergence of the self-consistent procedure. It is a technical
issue. Due to its analogy with the Fermi distribution, this parameter is
called the Electronic Temperature
For a finite , the BZ integrals converge faster but to incorrect values. After
self-consistency has been obtained for a relatively large value of Tc , this has to
be reduced until the energy becomes independent of it.
P.Ravindran, FME-course on Ab initio Modelling of solar cell Materials 19 June 2015 Evolution of Band structure of Solids
Comparing energies of structures having
different symmetries: take care of BZ samplings
The BZ sampling of all the structures must be sampled
with the same accuracy
Since for unit cells of different shapes it is not possible to
choose exactly the same k-point sampling, a usual strategy is
to try and maintain the same density of k-points
P.Ravindran, FME-course on Ab initio Modelling of solar cell Materials 03 June 2013 Various Aspects of Energy Issues
CONTACT POTENTIAL
1 2contactV
e
P.Ravindran, FME-course on Ab initio Modelling of solar cell Materials 03 June 2013 Various Aspects of Energy Issues
P.Ravindran, FME-course on Ab initio Modelling of solar cell Materials 03 June 2013 Various Aspects of Energy Issues
BZ integration, “FERMI”-methods Replace the “integral” of the BZ by a finite summation on a mesh of “k-points”
weights wk,n depend on k and bandindex n (occupation)
– for full “bands” the weight is given by “symmetry”
w(G)=1, w(x)=2, w(D)=4, w(k)=8
shifted “Monkhorst-Pack” mesh
– for partially filled bands (metals) one must find the
Fermi-energy (integration up to NE) and determine
the weights for each state Ek,n
linear tetrahedron method (TETRA, eval=999)
linear tetrahedron method + “Bloechl” corrections (TETRA)
“broadening methods”
– gauss-broadening (GAUSS 0.005)
– temperature broadening (TEMP/TEMPS 0.005)
– broadening useful to damp scf oszillations, but dangerous (magnetic moment)
kk
nk
nknknk
EE
n
wkdrFn
*
,
,
3
,
*
,)(
G D X
P.Ravindran, FME-course on Ab initio Modelling of solar cell Materials 19 June 2015 Evolution of Band structure of Solids
Relativistic treatment
Valence states
– Scalar relativistic
mass-velocity
Darwin s-shift
– Spin orbit coupling on demand by
second variational treatment
Semi-core states
– Scalar relativistic
– on demand
spin orbit coupling by second
variational treatment
Additional local orbital (see Th-6p1/2)
Core states
– Fully relativistic
Dirac equation
For example: Ti
P.Ravindran, FME-course on Ab initio Modelling of solar cell Materials 19 June 2015 Evolution of Band structure of Solids
Relativistic semi-core states in fcc Th
additional local orbitals for
6p1/2 orbital in Th
Spin-orbit (2nd variational method)
J.Kuneš, P.Novak, R.Schmid, P.Blaha, K.Schwarz,
Phys.Rev.B. 64, 153102 (2001)