19 장 Fundamentals of Spectrophotometry Fundamentals of Spectrophotometry –19-1Properties of...
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Transcript of 19 장 Fundamentals of Spectrophotometry Fundamentals of Spectrophotometry –19-1Properties of...
19 장 Fundamentals of Spectrophotometry
• Fundamentals of Spectrophotometry– 19-1 Properties of Light– 19-2 Absorption of Light– 19-3 The Spectrophotometer– 19-4 Beer’s Law in Chemical Analysis– 19-5 What happens when a molecule absorbs
light?– 19-6 Luminescence
Spectrophotometry
• Any procedure that uses light to measure the concentration of a chemical species
• Light is composed of perpendicular, oscillating electric and magnetic fields
Electric fieldy
z
x (t)
Magnetic field
Fig. 19-1
Properties of Light
• Wavelength (): crest-to-crest (or trough-to-trough) distance between waves, generally measured in nm
• Light described as “waves”
y
x
Properties of Light
• Frequency (): number of complete oscillations the wave makes each second (1/s, s-1, Hz)
= c
c speed of light (in vacuum) = 2.998 x 108 m/s
• Units for above equation:
(s-1)(m) = (m/s)
Properties of Light
• Refractive index (n): measure of angle at which light is bent
• Speed of light in a medium other than a vacuum
c/n(n = 1 in a vacuum)
Properties of Light
• Photons (h): energetic particles of light
E = h E = hc/ = hc
h Planck’s constant = 6.626 x 10-34 Js
wavenumber (1/)
• Light described as “particles”
~
~
Electromagnetic Spectrum
• Compare energy of red and blue light:
E = hc/red > blue so Ered < Eblue
Cosmic -rays X-rays UV IR -wave Radio
Vis
ible
(Hz)
(m)
1020 1018 1016 1014 1012 108
10-12 10-11 10-8 10-6 10-3 10-1
(nm): 400 500 600 700 800
Fig. 19-2
19-2. Absorption of light
• Molecules absorb photons with energy (E)
E = h• Molecules gain that energy (E) when they
absorb photons
• M is promoted from the ground state to an excited state
Ground state
Excited states
Ene
rgy
Mh
Absorption of light
• Molecules gain energy when they absorb photons
• Molecules lose energy when they emit photons
Ground state
Excited states
Ene
rgy
Absorption
gain hEmission
lose h
Fig. 19-3
Types of electromagnetic radiation (light)
• X-ray light– promotes core e-s to higher energy orbitals– breaks chemical bonds and ionizes
molecules
• Ultraviolet and visible light (UV-VIS)– promotes valence e-s to higher energy
orbitals
• Infrared light (IR)– stimulates vibrations of molecules
• Microwaves– stimulates rotational motion of molecules
E
N
E
R
G
Y
Energy levels
• Quantized: discrete levels, not continuous
• Energy states are “quantized”
rotational levels
vibrational levels
v2
v1
S0
S1
E = h
electronic levels
Example Problem
• By how many kJ per mole is the energy of O2 increased when it absorbs UV radiation with a of 147 nm?
• New energy: E2
• Original energy: E1
E2 – E1 = energy of photon absorbed
hchE
Example Problem
hchE
m
nm10
nm147
)s/m10998.2)(sJ10626.6(E
9834
molecule/J1035.1 18
J1000
kJ1
mol
molecules10022.6
molecule
J1035.1 2318
mol/kJ814
Reminder
• Prefixes of SI units
pico nano micro milli centi kilo mega
p n m c k M
10-12 10-9 10-6 10-3 10-2 103 106
• Example:
nm10
m1or
nm
m109
9
Measuring Absorption of Light
selects that analyte
will absorb
sample
absorbs
radiation
bsource may
contain
many s
Light
SourceMonochromator DetectorSample
P0 P
detector
looks for
amount of
radiation
not
absorbed
Measuring Absorption of Light
• Detector measures P
• Amount of light transmitted through sample is what is measured
• Transmittance (T): fraction of original light that passes through sample– Absorbance is measured INDIRECTLY
0P
PT radiant power not absorbed by sample
incident radiant power=
T100T%
Sept. 19 – Ch. 19
• Fundamentals of Spectrophotometry19-1 Properties of Light– 19-2 Absorption of Light– 19-3 The Spectrophotometer– 19-4 Beer’s Law in Chemical Analysis– 19-5 What happens when a molecule absorbs
light?– 19-6 Luminescence
Ch. 19-2
• Fundamentals of Spectrophotometry19-1 Properties of Light– 19-2 Absorption of Light– 19-3 The Spectrophotometer– 19-4 Beer’s Law in Chemical Analysis– 19-5 What happens when a molecule absorbs
light?– 19-6 Luminescence
Measuring Absorption of Light
• Detector measures P
• Amount of light transmitted through sample is what is measured
• Transmittance (T): fraction of original light that passes through sample– Absorbance is measured INDIRECTLY
0P
PT radiant power not absorbed by sample
incident radiant power=
T100T%
Measuring Absorption of Light
0 < T < 1
0 < %T < 100
• Absorbance is related to T:
T
1log
P
PlogA 0
TlogA
Tlog1logA
Absorbance vs. Transmittance
• When P decreases, A increases– less radiant power (light) is reaching the
detector because the sample is absorbing light
• T and A are dimensionless (although some- times “absorbance units” are mentioned)
P/P0 %T A
1 100 00.1 10 10.01 1 2
Absorbance vs. Reflection• When a molecule absorbs different s of
white (visible) light, our eyes see the reflected s (the non-absorbed s)
of Max.Absorption
380-420420-440440-470470-500500-520520-550550-580580-620620-680680-780
ColorAbsorbed
violetviolet-blue
blueblue-green
greenyellow-green
yelloworange
redpurple
ColorObserved
green-yellowyelloworange
redpurpleviolet
violet-blueblue
blue-greengreen
Table
19-1
Blue Blocker Sunglasses
• The infomercial claims that “harmful blue light” is blocked from damaging your eyes.
• Why are they orange?
Measuring Absorption of Light
P(for absorption by sample) = P0 – P(reflected) – P( scattered)
• Reference blank: solution containing all components of a sample except analyte
A(analyte) = A(measured) – A(reference blank)
DetectorSampleP0
P
scattering
reflections
Absorbance• Spectrophotometry: Any procedure that uses
light to measure the concentration of a chemical species
• Beer’s Law:
A = bc
Molar absorptivity (or extinction coefficient)
b pathlength light travels through cuvet
c concentration of analyte
• Absorbance is directly proportional to concentration
Beer’s Law
• Best applied when c 0.01 M– when c > 0.01 M, solute molecules influence
one another because they are closer together– physical properties of molecules change when
they are close together
– physical property that will change relevant to
our discussion of Beer’s Law:
Beer’s Law
• Molar absorptivity (): characteristic of a substance that tells how much light is absorbed at a particular wavelength ( is -dependent AND analyte-dependent
because different analytes absorb different amounts of light at different s
• Pathlength (b): width of cuvet; dependent on instrumental setup
A = bc = (M-1 cm-1)(cm)(M)
A is dimensionless
Example Problem
• A 3.15 x 10-6 M solution of a colored complex exhibited an absorbance of 0.267 at 635 nm in a 1.000-cm cuvet. A blank solution had an absorbance of 0.019. Find the molar absorptivity of the colored complex.
bcA
)M1015.3)(cm000.1(
)019.0267.0(
bc
A6
114 cmM1087.7
Double-beam Scanning Spectrophotometer
• Alternately measuring P0 and P by diverting light beam through reference cuvet
lightsource
monochromator detector
amplifier
computer/recorder
samplecuvet
referencecuvet
mirrormirror/
beam chopper
mirrormirror
mirror/beam chopper
Fig 19-6
P0
P
P0’
Spectrophotometers• Single-beam spectrophotometer
– insert reference blank once at beginning of exp’t– only measure absorbance of EITHER sample OR
reference blank at a time
• Double-beam spectrophotometer– continuously checks reference blank to account
for changes in• source intensity (P0)
• detector response
– if absorbance measurement from reference blank changes, spectrophotometer corrects for that change to find true absorbance of analyte
Using a spectrophotometer
• Picking the (the source of the light)– Choose the at which the analyte absorbs the
most (max)
• measurement is most sensitive at max
• Keep samples clean and dust free
• Analyte solution should absorb in the range of 0.4 < A < 0.9– dilute solution if it is too concentrated
• reduce c to reduce A
– use cuvet with longer pathlength• increase b to increase A
Why should 0.4 < A < 0.9?
• Consider when A < 0.4– P is almost as large as P0
– difficult to see a small difference between two large numbers
• Consider when A > 0.9– P is very very small– difficult to see a small amount of light– stray light reaching the detector could compete
with P
• Adjust experimental parameters to keep A in an intermediate region
What happens when amolecule absorbs light?
• Consider Molecular Orbital (MO) Theory– describes the distribution of electrons in the
molecular orbitals of a molecule
• Electronic transition– e- from one MO moves to another MO
• Ex: Formaldehyde– 4 bonds– 1 bond– 1 lone pair (the other lone pair is mixed with the
bond orbitals)– refer to Figure 19-11
CHH
O
What happens when amolecule (Formaldehyde) absorbs light?
1
2
3
4
n
singlet
or
1
2
3
4
n
triplet
E
1
2
3
4
n
Ground
State
Electronic
States
Moleculeabsorbslight ()
n *transition
What happens when amolecule (Formaldehyde) absorbs light?
• Difference between 2 excited states is spin of e-
• Singlet– spin still opposite from
e- it was originally paired with
• Triplet– spin parallel with spin of
e- it was originally paired with
• In general, T1 < S1
1
2
3
4
n
singlet (S1)
or
1
2
3
4
n
triplet (T1)
Electronic
States
Processes that occur whena molecule absorbs light
• The above “state state” transitions are only examples– S T or T S: different spins– S S: same spins
Absorbance S0 S1
Fluorescence S1 S0
Phosphorescence T1 S0
Radiational
Transitions
Internal Conversion S1 S0
Intersystem Crossing T1 S0
Relaxations (within a state)
Radiationless
Transitions
Jablonski diagram
S1
S0
T1
A
Absorbance
F
Fluorescence
P
Phosphorescence
IC
Internal Conversion
ISC
ISC
Intersystem Crossing
R
Relaxation
Fig. 19-14
Processes that occur whena molecule absorbs light
• Internal conversions (IC) and intersystem crossings (ISC)– no gain or loss in energy– IC: S S– ISC: S T or T S
• Fluorescence (F) and phosphorescence (P) are rare processes– molecule emits photons (loss in energy)– F: S S– P: T S– examples of Luminescence (section 19-6)