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(1)

UV-VIS SPECTROSCOPY

(2)

X-ray:

core electron excitation

Nuclear spin states (in a magnetic feldd

(3)
(4)

Spectroscopic Techniques and Chemistry they Probe

UV-vis UV-vis region bonding electrons

Atomic Absorption UV-vis region atomic transitions (val. e-)

FT-IR IR/Microwave vibrations, rotations

Raman IR/UV vibrations

FT-NMR Radio waves nuclear spin states

X-Ray Spectroscopy X-rays inner electrons, elemental

(5)

Spectroscopic Techniques and Common Uses

UV-vis UV-vis region analysis/Beer’s LawQuantitative

Atomic Absorption UV-vis region

Quantitative analysis Beer’s Law

FT-IR IR/Microwave Functional Group Analysis

Raman IR/UV

Functional Group Analysis/quant

FT-NMR Radio waves Structure determination

X-Ray Spectroscopy X-rays Elemental Analysis

(6)

Different Spectroscopies

UV-vis – electronic states of valence

e/d-orbital transitions for solvated transition

metals

Fluorescence – emission of UV/vis by certain

molecules

FT-IR – vibrational transitions of molecules

FT-NMR – nuclear spin transitions

(7)

Why should we learn this stuf?

After all, nobody solves structures with

UV any longer!

Many organic molecules have chromophores that absorb UV

UV absorbance is about 1000 x easier to detect per mole than NMR

Still used in following reactions where the chromophore changes. Useful because timescale is so fast, and sensitivity so high. Kinetics, esp. in

biochemistry, enzymology.

Most quantitative Analytical chemistry in organic chemistry is conducted using HPLC with UV detectors

(8)

Uses for UV, continued

Knowing UV can help you know when to be skeptical of quant results. Need to calibrate response factors

Assessing purity of a major peak in HPLC is improved by “diode array” data, taking UV spectra at time points across a peak. Any diferences could suggest a unresolved component. “Peak Homogeneity” is key for purity analysis.

Sensitivity makes HPLC sensitive

e.g. validation of cleaning procedure for a production vessel

But you would need to know what compounds could and could not be detected by UV detector! (Structure!!!d

One of the best ways for identifying the presence of acidic or basic groups, due to big shifts in  for a chromophore containing a phenol, carboxylic acid, etc.

(9)

The UV Absorption process

•   * and   * transitions: high-energy,

accessible in vacuum UV (max <150 nmd. Not usually observed in molecular UV-Vis.

• n  * and   * transitions: non-bonding

electrons (lone pairsd, wavelength (maxd in the 150-250 nm region.

• n  * and   * transitions: most common transitions observed in organic molecular UV-Vis, observed in compounds with lone pairs and multiple bonds with max = 200-600 nm.

• Any of these require that incoming photons match in energy the gap corrresponding to a transition from ground to excited state.

(10)

What are the

nature of these

absorptions?

Example:   * transitions responsible for ethylene UV absorption at ~170 nm

calculated with ZINDO semi-empirical excited-states methods (Gaussian 03Wd:

HOMO u bonding molecular orbital LUMO g antibonding molecular orbital

h 170nm photon

(11)

How Do UV spectrometers work?

Two photomultiplier inputs, diferential voltage drives amplifer.

Matched quartz cuvettes

Sample in solution at ca. 10-5 M.

System protects PM tube from stray light

D2 lamp-UV

Tungsten lamp-Vis

Double Beam makes it a diference technique

(12)

Diode Array Detectors

Diode array alternative puts grating, array of photosens.

Semiconductors after the light goes through the sample.

Advantage, speed, sensitivity,

The Multiplex advantage

Disadvantage,

resolution is 1 nm, vs 0.1 nm for normal UV

(13)

Experimental details

What compounds show UV spectra?

Generally think of any unsaturated compounds as good candidates. Conjugated double bonds are strong absorbers Just heteroatoms are not enough but C=O are reliable

Most compounds have “end absorbance” at lower frequency. Unfortunately solvent cutofs preclude observation.

You will fnd molar absorbtivities  in L•cm/mol, tabulated. Transition metal complexes, inorganics

Solvent must be UV grade (great sensitivity to impurities with double bondsd

(14)

An Electronic Spectrum

Wavelength, , generally in nanometers (nmd 0.0

extinction 

Make solution of

concentration low enough that A≤ 1

(Ensures Linear Beer’s law behaviord

Even though a dual beam goes through a solvent blank, choose solvents that are UV transparent.

Can extract the  value if conc. (Md and b (cmd are known

UV bands are much

broader than the photonic transition event. This is because vibration levels

(15)

Solvents for UV (showing high

(16)

Organic compounds (many of

themd have UV spectra

From Skoog and West et al. Ch 14 One thing is clear

Uvs can be very non-specifc Its hard to interpret except at a cursory level, and to say that the spectrum is consistent with the structure

Each band can be a superposition of many transitions

(17)

An Example--Pulegone

Frequently plotted as

log of

molar

extinction

So at 240 nm, pulegone has a molar

extinction of 7.24 x 103

Antilog of 3.86

(18)

Can we calculate UVs?

Elec tronic Spectra

Wavelength (nm) Molar Absorptivity (l/mol-cm)

220 230 240 250 260 270 280 290 300

0

Wavelengt h (nm) Molar Absorptivity (l/mol-cm)

220 230 240 250 260 270 280 290 300 0

Nacety lindol

Semi-empirical (MOPACd at AM1, then ZINDO for

(19)

The orbitals involved

Electronic Spectra

Wavelength (nm) Molar Absorptivity (l/mol-cm)

200 210 220 230 240 250 260 270 280 290 300 0

atoms whose MO’s

(20)

The Quantitative Picture

Transmittance:

T = P/P

0

B(path through sample)

P0

(power ind P (power outd

Absorbance:

A = -log

10

T = log

10

P

0

/P

The Beer-Lambert Law (a.k.a. Beer’s Lawd:

A =

e

bc

Where the absorbance A has no units, since A = log10 P0 / P

e is the molar absorbtivity with units of L mol-1 cm-1

b is the path length of the sample in cm

(21)

Beer-Lambert Law

Linear absorbance with increased concentration--directly proportional

Makes UV useful for quantitative analysis and in HPLC detectors

(22)

Quantitative Spectroscopy

Beer’s Law

A

l1

= e

l1

bc

e is molar absorptivity (unique for a

given compound at l

1

)

(23)

Beer’s Law

A = -logT = log(P

0

/P) = ebc

T = P

solution

/P

solvent

= P/P

0

Works for monochromatic light

Compound x has a unique e at different

wavelengths

cuvette source slit

(24)

Characteristics of

Beer’s Law Plots

One wavelength

Good plots have a range of

absorbances from 0.010 to 1.000

Absorbances over 1.000 are not that

valid and should be avoided

(25)

Standard Practice

Prepare standards of known

concentration

Measure absorbance at

l

max

Plot A vs. concentration

Obtain slope

(26)

Typical Beer’s Law Plot

y = 0.02x

0 0.2 0.4 0.6 0.8 1 1.2

0.0 20.0 40.0 60.0

concentration (uM)

(27)

UV-Vis Spectroscopy

UV-

organic molecules

Outer electron bonding transitions

conjugation

Visible – metal/ligands in solution

d-orbital transitions

(28)

Characteristics of UV-Vis spectra of

Organic Molecules

Absorb mostly in UV unless highly

conjugated

Spectra are broad, usually to broad for

qualitative identification purposes

Excellent for quantitative Beer’s

Law-type analyses

(29)

Molecules have quantized energy levels: ex. electronic energy levels.

en Q: Where do these quantized energy levels come from?

A: The electronic confgurations associated with bonding.

Each electronic energy level (confgurationd has

(30)

Broad spectra

Overlapping vibrational and rotational

peaks

(31)

Molecular Orbital Theory

(32)

2s 2s

s s*

s

s*

p*

p

(33)

C C

Absorptions having max < 200 nm are difcult to observe because

everything (including quartz glass and air) absorbs in this spectral region.

(34)

C C

Example: ethylene absorbs at longer wavelengths: max = 165 nm = 10,000



=

hv

(35)

The n to pi* transition is at even lower wavelengths but is not as strong as pi to pi* transitions. It is said to be “forbidden.”

Example:

(36)
(37)

C C

HOMO LUMO

Conjugated systems:

Preferred transition is between Highest Occupied Molecular Orbital (HOMO) and Lowest Unoccupied Molecular Orbital (LUMO).

Note: Additional conjugation (double bondsd lowers the HOMO-LUMO energy gap:

Example:

(38)

O

O

O

Similar structures have similar UV spectra:

(39)

Lycopene:

max = 114 + 5(8d + 11*(48.0-1.7*11d = 476 nm

(40)

Polyenes, and Unsaturated

Carbonyl groups;

an Empirical triumph

R.B. Woodward, L.F. Fieser and others

Predict max for π  * in extended conjugation systems to within ca. 2-3 nm.

Homoannular, base 253 nm

heteroannular, base 214 nm Acyclic, base 217 nm

Attached group increment, nm Extend conjugation +30 Addn exocyclic DB +5

(41)

Similar for Enones

215 202 227 239

Base Values, add these increments…

Extnd C=C +30

Add exocyclic C=C +5

Homoannular diene +39

alkyl +10 +12 +18 +18

Cl/Br +15/+25 +12/+30

 b g d,+

(42)

Some Worked Examples

O

Base value 217 2 x

alkyl subst. 10 exo

DB 5 total

232 Obs. 237

Base value 214 3 x

alkyl subst. 15 exo

DB 5 total

234 Obs. 235

Base value 215 2 ß

alkyl subst. 24

total 239 Obs.

(43)

Distinguish Isomers!

HO

2C

HO

2C

Base value 214 4 x

alkyl subst. 20 exo

DB 5 total

239 Obs. 238

Base value 253 4 x

alkyl subst. 20 total

(44)

Generally, extending conjugation

leads to red shift

“particle in a box” QM theory; bigger box

Substituents attached to a chromophore that cause a red shift are called “auxochromes”

Strain has an efect…

(45)

Interpretation of UV-Visible Spectra

• Transition metal

complexes; d, f electrons.

• Lanthanide

complexes – sharp lines caused by

“screening” of the f electrons by other orbitals

• One advantage of this

is the use of holmium oxide flters (sharp linesd for wavelength calibration of UV

(46)

Benzenoid

aromatics

From Crewes, Rodriguez, Jaspars, Organic Structure Analysis

UV of

Benzene in heptane

Group K band () B band() R band

Alkyl 208(7800d 260(220d

---OH 211(6200d 270(1450d

-O- 236(9400d 287(2600d

-OCH3 217(6400d 269(1500d

NH2 230(8600d 280(1400d

-F 204(6200d 254(900d -Cl 210(7500d 257(170d -Br 210(7500d 257(170d

-I 207(7000d 258/285(610/180 d

-NH3+ 203(7500d 254(160d

-C=CH2 248(15000d 282(740d

-CCH 248(17000d 278(6500

-C6H6 250(14000d

-C(=OdH 242(14000d 280(1400d 328(55d

-C(=OdR 238(13000d 276(800d 320(40d

-CO2H 226(9800d 272(850d

-CO2- 224(8700d 268(800d

-CN 224(13000d 271(1000d

(47)

Substituent efects don’t really add up

Can’t tell any thing about substitution geometry

Exception to this is when adjacent substituents can interact, e.g hydrogen bonding.

E.g the secondary benzene band at 254 shifts to 303 in salicylic acid

(48)

Heterocycles

Nitrogen heterocycles are pretty similar to the benzenoid anaologs that are isoelectronic.

(49)

Quantitative

analysis

Great for non-aqueous titrations Example here gives detn of

Single clear point, can exclude intermediate state, exclude light scattering and Beer’s law applies

(50)

More Complex Electronic Processes

• Fluorescence: absorption of

radiation to an excited state, followed by emission of

radiation to a lower state of the same multiplicity

• Phosphorescence: absorption of

radiation to an excited state, followed by emission of

radiation to a lower state of diferent multiplicity

• Singlet state: spins are paired,

no net angular momentum (and no net magnetic feldd

• Triplet state: spins are unpaired,

(51)

Metal ion transitions

Degenerate D-orbitals of naked Co

D-orbitals

of hydrated Co2+

Octahedral Confguration

(52)

Co2+

H2O H2O

H2O H2O

H2O

H2O

(53)

Instrumentation

Fixed wavelength instruments

Scanning instruments

(54)

Fixed Wavelength Instrument

LED serve as source

Pseudo-monochromatic light source

No monochrometer necessary/ wavelength selection

occurs by turning on the appropriate LED

4 LEDs to choose from

photodyode sample

beam of light

(55)

Scanning Instrument

cuvette Tungsten

Filament (vis)

slit

Photomultiplier tube

monochromator

Deuterium lamp Filament (UV)

(56)

sources

Tungten lamp (350-2500 nm)

Deuterium (200-400 nm)

(57)

Monochromator

Braggs law, nl = d(sin i + sin r)

Angular dispersion

,

d

r/

dl

= n / d(cos rd

Resolution, R

=

l

/

Dl

=

nN, resolution is

(58)

Sample holder

(59)

Single beam vs. double beam

(60)

Diode array Instrument

cuvette Tungsten

Filament (vis)

slit

Diode array detector 328 individual detectors

monochromator Deuterium lamp

Filament (UV)

(61)

Advantages/disadvantages

Scanning instrument

High spectral resolution (63000),

l

/

Dl

Long data acquisition time (several

minutes)

Low throughput

Diode array

Fast acquisition time (a couple of

seconds), compatible with on-line

separations

(62)

Referensi

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