Experimental methods to investigate the optical properties ... 2010-11/mep jdg_intro... ·...
Transcript of Experimental methods to investigate the optical properties ... 2010-11/mep jdg_intro... ·...
IPEQ - ICMP - SB - EPFLStation 3CH - 1015 LAUSANNE
J-D GaniereEPFL - SB - ICMP - IPEQCH - 1015 Lausanne
Credit: www.national.com
Experimental Methods in Physics
[2010-2011]
Experimental methods to investigate the optical properties of solids
1
J-D Ganiere MEP/2010-2011
Outline ...
• Definition of "spectroscopy"
• "EM" spectrum - orders of magnitude
• Frequency or wavelength ?
linewidth
• Units
• Radiometry versus Photometry
• How to obtain the optical signature of a EM signal
2
J-D Ganiere MEP/2010-2011
Spectroscopy
Spectroscopy is the study of the interaction between radiation (electromagnetic radiation, or light, as well as particle radiation) and matter.
excitationprobe
signal
energy filter
signaldetector
excitationsource
specimen
3
J-D Ganiere MEP/2010-2011
Spectroscopy
The objective in spectroscopy is typically to measure the intensity of a signal as a function of the energy of a proposed event occuring in the sample
name probe signal
PL Photons Photons
CL Electrons Photons
EDS Electrons X-photons
AES X-rays Electrons
EELS Electrons Electrons
4
J-D Ganiere MEP/2010-2011
An example : X-ray fluorescence
X-ray tube
sample
detector slit
Detector
crystal
5
J-D Ganiere MEP/2010-2011
Spectroscopy
excitation(probe) sample
emission
reflection
electronsneutronsmolecules
atomsphotons
...
gasliquidsolid
biologicsemiconductor
...
absorption
transmission
scattering
6
J-D Ganiere MEP/2010-2011
Optical Spectroscopy
• The optical spectroscopy of semiconductor is only a pretext to approach various important subjects in MEP.
• nothing too specific.
• Also useful in other domains (life science, chemistry, ...).
Raman map showing a horitzontal section of a carrot root. Based on miscoloured pictures the concentration profiles of betacarotin in plant tissue can be clearly illustrated.
Credit: IPA [Institute of Plant Analysis, www.bafz.de]
7
J-D Ganiere MEP/2010-2011
Optical spectroscopy - motivation
Better understanding of the physics !
Important for the realization of efficient device (lasers,detectors, ..)
To study the dynamic processes in materials or chemical compounds
To obtain information on the electronic structure
ground state
excited
triplet state
excited
singulet state
S1
S2
T1
internal conversion
vibrational relaxation
10 fs - 100 ps
absorption - 10 fs
fluorescence
100 fs - 100 ns
phosphorescence
1 ms - 10 ms
intersystem
Crossing
non-radiative
relaxation
8
J-D Ganiere MEP/2010-2011
Reminder
9
J-D Ganiere MEP/2010-2011
kT
At room temperature
kT = 25 meV
10
J-D Ganiere MEP/2010-2011
What you should know ...!
It is difficult to measure directly the frequency, that is why we use mostly the wavelength λ .
From the theoretical point of view, it is the frequency which plays a fundamental role, that is why we introduce a new unit, the wave number, σ, who expresses itself in
cm-1. The wave number is measured with the same precision as the wavelength !
v =m1= co
E = ho
11
J-D Ganiere MEP/2010-2011
Some useful equivalences
Wavelength Wavenumber Frequency Photon energy
Symbol
Fact
or o
f co
nver
sion
Exam
ples
m [nm] v [cm-1] o [Hz] Ep [eV]
Ep
m
v
o
107 /m 3 $ 1017 /m 1224/m
107 /v 3 $ 1010 $ v 1.22 $ 10-4v
3 $ 1017 /o 3.33 $ 1011o 4.1 $ 10-15o
1224/Ep 8197 $ Ep 2.44 $ 1014Ep
200
500
1000
5 $ 104
2 $ 104
104
1.5 $ 1015
6 $ 1014
3 $ 1014
6.12
2.45
1.224
12
J-D Ganiere MEP/2010-2011
cm-1, eV and/or nm ?
cm-1 (Vibrational and Rotational Transitions)
eV (semiconductors)
nm (photometry)
13
J-D Ganiere MEP/2010-2011
Linewidth nm or eV ?
o=mc
do=-m2cdm
odo=-
mdm
14
J-D Ganiere MEP/2010-2011
Units
Unit of length meter
Unit of mass kilogram
Unit of time second
Unit of electric current ampere
Unit of thermodynamic! temperature kelvin
Unit of amount of substance mole
Unit of luminous intensity candela
The candela was first defined as 1/60 the luminous intensity, in the perpendicular direction, of a1 cm2 blackbody radiator at the freezing temperature of platinum (about 2042 K) and a pressure of 1 atmosphereThe candela was first defined as 1/60 the luminous intensity, in the perpendicular direction, of a1 cm2 blackbody radiator at the freezing temperature of platinum (about 2042 K) and a pressure of 1 atmosphere
The candela is the luminous intensity, in a given direction, of a source that emits monochromatic radiation of frequency 540 x 1012 hertz and that has a radiant intensity in that direction of 1/683 watt per steradian. The candela is the luminous intensity, in a given direction, of a source that emits monochromatic radiation of frequency 540 x 1012 hertz and that has a radiant intensity in that direction of 1/683 watt per steradian.
15
J-D Ganiere MEP/2010-2011
Radiometry, Photometry
Radiometry the measurement of optical radiation over the entire spectrum from the ultra-violet to the infra-red.
Photometry the measurement of visible light as it appears to the human eye.
optical system
object image
16
J-D Ganiere MEP/2010-2011
Radiometry, Photometry
Although describing fundamentally similar parameters,namely flux, energy, intensity, power per unit area a different system of units is used to distinguishbetween radiometric and photometric quantities.
incoherent radiation optical geometric laws apply no diffraction ...
The assumptions (radiometry and photometry)
17
J-D Ganiere MEP/2010-2011
Data sheets ... photometric or radioemtric units ?
18
J-D Ganiere MEP/2010-2011
A useful table ...
Radiant Energy Luminous Energy
Total amount of light emitted from source
Qe
Qv
JJ
Radiant Flux Luminous Flux
Rate of energy emitted or transferred from source
Φe
Φvϕ=dQ/dt
Wlm
Radiant IntensityLuminous Intensity
Flux emitted from a point source per unit solid angle
Ie
IvI=dϕ/dΩΩ W sr-1
lm sr-1 = cd
Radiant Emittance Luminous Emittance
Flux emitted per surface unit area of extended source
Me
MvM=dϕ/dA
W m-2
lm m-2 = lx
RadianceLuminance
Flux emitted per unit surface area of extended source, per unit solid angle at angle normal to surface n
Le
Lv
L=d2ϕ/
(dAdΩΩcosθ)W m-2 sr-1
lm m-2 sr-1 = cd m-2
IrradianceIlluminance
Flux arriving at a surface per unit surface area at an angle normal to the surface
Ee
EvE=dϕ/dA
W m-2
lm m-2 = lx
Radiant Energy DensityLuminous Energy Density
Energy emitted per unit volume of source w w= dQ/dV J m-3
J m-3
19
J-D Ganiere MEP/2010-2011
Photometry
Photometric unitsPhotometric unitsPhotometric unitsPhotometric units
Photometry UnitsUnitsUnits
Photometry MKS CGS British
Luminous energy TalbotTalbotTalbot
Luminous power LumenLumenLumen
Illuminance Lux Phot Footcandle
Luminance NitApostilb, Blondel
StilbLambert Footlambert
Luminous intensity Candela (Candle, Candlepower, Carcel, Hefner)Candela (Candle, Candlepower, Carcel, Hefner)Candela (Candle, Candlepower, Carcel, Hefner)
Thus one nit is one lux per steradian is one candela per square meter is one lumen per square meter per steradian. Got it ? James Kajiya
20
J-D Ganiere MEP/2010-2011
To be pragmatic
A particular algebraic symbol is used to describe the optical parameter, be it radiometric or photometric, the subscript "e" added to denote a radiometric quantity (e, like energetic) , the subscript "v" to denote a photometric quantity (v, like visual).
radiant flux is a radiometric quantity denoted by ϕe
luminous flux is a photometric quantity denoted by ϕv
21
J-D Ganiere MEP/2010-2011
To be pragmatic
Note that radiometric and photometric parameters relate to the total amount of radiation emitted over all wavelengths (EM spectrum or visible). Sometimes need to define a parameter over a specific frequency or wavelength interval.
For example, spectral radiance is the flux per unit area per unit solid angle per unit frequency interval denoted as Lv(λ)
or Le(λ)
22
J-D Ganiere MEP/2010-2011
An example
Characteristics of light sources
23
J-D Ganiere MEP/2010-2011
Radiance
The radiance (luminance), L(x,ω), is the intensity
per unit area leaving a surface:
L(x,~) = dAdI(x,~)
= d~dAd2U(x,~)
Unit of radiance is: sr m2W; E
24
J-D Ganiere MEP/2010-2011
Conservation of radiance
Conservation of radiance (formerely called “brightness theorem”)
In an optical system the radiance measured in the direction of propagation is an invariant (in fact, this is the quantity L/n2 which is an invariant)
In an optical system the radiance of the image is equal to the radiance of the source
optical system
object image
25
J-D Ganiere MEP/2010-2011
Maximization of the radiant flux
In an optical system we will try to maximize the amount of radiant flux, ΩΩ, transferred from the source to the detector. If the system is aberration free and has no internal aperture, we verify the relation:
G= AsXs= AiXi= cste
The quantity, G, which is the same for the source and for the image is called the geometrical extent
Credit: http:www.newport.com
26
J-D Ganiere MEP/2010-2011
Maximization of the radiant flux
If the optical system has a cylindrical symmetry, the 1D version of the optical extent ia applicable:
G= h1i1 = h2i2= cste
Credit: http:www.newport.com
27
J-D Ganiere MEP/2010-2011
A practical case ...
excitation
sample
monochromator
the lowest geometrical extent of any component in an optical system limits system throughput. Generally the monochromator is the component with the lowest geometrical extent. The geometrical extent of the monochromator is the product of the entrance slit width and the angle of acceptance.
28
J-D Ganiere MEP/2010-2011
The index of refraction
The index of refraction, n, of a material is a dimensionless number defined by the relationship:
where c and v are the speeds of the light in the vaccum and in the material respectively
n= vc
c=299'792'458 m $ s-15 ?
29
J-D Ganiere MEP/2010-2011
The index of refraction
In the transparent materials, the index of refraction n, is equal or greater to 1 (réfringent material) :
n$1
http://ctd.grc.nasa.gov/organization/branches/eodb/metamateriallens.htmlmetamaterials: n ! 1
30
J-D Ganiere MEP/2010-2011
Conventionnal spectroscopy
How to obtain the optical signature of a EM signal ?
Prism spectrometer Grating spectrometer Interferential spectrometer Fourier transform interferometer…
31
J-D Ganiere MEP/2010-2011
Dispersive system
Dispersive SystemsPrism
Grating
Interferential
Spectrometer
Spectroscope
Spectrograph
Monochromator Image sensor, [CCD, CMOS, ...]
Flux detectors [PM, PD, ...
Optical filter
Light source
Spectral signature
32
J-D Ganiere MEP/2010-2011
Time resolved spectroscopy
• Fermat principle still applies
• Heisenberg principle also ... !
DE $ Dt$'
33
J-D Ganiere MEP/2010-2011
light sources sample
light analyzers
light detectors
crystallogenesis
epitaxy
cryogenic
magnetic field
sample
incoherent light sources- blackbody types- arc lamps- LED
coherent light sources - laser
synchrotron light
light source
monochromator (eg prism , grating type)
PF analyzer
light analyzer
quantum detectors (eg photographic plate, PM. PD, CCD, ...)
Thermal detectors (eg photoacoustic, ...)
light detector
34
J-D Ganiere MEP/2010-2011
Imaging Spectroscopy - CL mapping
35
J-D Ganiere MEP/2010-2011
Imaging Spectroscopy - CL mapping
SEM: Secondary electrons SEM: Cathodoluminescence mode
36