Ultraviolet–visible spectroscopy or ultraviolet-visible spectrophotometry (UV-Vis or UV/Vis) refers to absorption spectroscopy or reflectance spectroscopy in the ultraviolet-visible spectral region. This means it uses light in the visible and adjacent ranges.
Introduction,Instrumentation, Classification of electronic transitions, Substituent and solvent effects, Classification of electronic transitions
Substituent and solvent effects
Applications of UV Spectroscopy
UV spectral study of alkenes
UV spectral study of poylenes
UV spectral study of α, β-unsaturated carbonyl
UV spectral study of Aromatic compounds
Empirical rules for calculating λmax.
Applications of UV Spectroscopy, Empirical rules for calculating λmax.
INTRODUCTION TO UV-VISIBLE SPECTROSCOPYJunaid Khan
UV-visible spectroscopy is the classical and the most reliable technique for qualitative and quantitative analysis of organic compounds. It involves detection of light absorbed by the sample and correlates it with concentration of the solute.
Introduction,Instrumentation, Classification of electronic transitions, Substituent and solvent effects, Classification of electronic transitions
Substituent and solvent effects
Applications of UV Spectroscopy
UV spectral study of alkenes
UV spectral study of poylenes
UV spectral study of α, β-unsaturated carbonyl
UV spectral study of Aromatic compounds
Empirical rules for calculating λmax.
Applications of UV Spectroscopy, Empirical rules for calculating λmax.
INTRODUCTION TO UV-VISIBLE SPECTROSCOPYJunaid Khan
UV-visible spectroscopy is the classical and the most reliable technique for qualitative and quantitative analysis of organic compounds. It involves detection of light absorbed by the sample and correlates it with concentration of the solute.
various parts of mAss spectroscopy, applications, principle, peaks, rules, typical mass spectra, various combinations, Fragmentation, rules of fragmentation and useful points which can help Chemical and analytical students and structural elucidation.
this ppt contain all basic information related to the mass spectrometry like introduction, principle of MS, type of ions, fragmentation processes eg. mcLafferty rearrangement, alpha clevage, sigma bond clevage, retro-diels-alder reaction
Quadrupole and Time of Flight Mass analysers.Gagangowda58
Description about important mass analysers Quadrupole and TOF: Principle, Construction and Working, Advantages and Disadvantages and their Applications.
Nuclear magnetic resonance (NMR) spectroscopyVK VIKRAM VARMA
SPECTROSCOPY
NMR SPECTROSCOPY
HISTORY
THEORY
PRINCIPLE
INSTRUMENTATION
SOLVENTS USED IN NMR(PROTON NMR)
CHEMICAL SHIFT
FACTORS AFFECTING CHEMICAL SHIFT
RELAXATION PROCESS
SPIN-SPIN COUPLING
푛+1 RULE
NMR SIGNALS IN VARIOUS COMPOUNDS
COUPLING CONSTANT
NUCLEAR MAGNETIC DOUBLE RESONANCE/ SPIN DECOUPLING
FT-NMR
ADVANTAGES & DISADVANTAGES
APPLICATIONS
REFERENCE
spectrofluorometer is the instrument for recording fluorescence emission and absorption spectra When a beam of light is incident on certain substances they emit visible light or radiations. This is known as fluorescence. Fluorescence starts immediately after the absorption of light and stops as soon as the incident light is cut off. The substances showing this phenomenon are known as flourescent substances.
A method of obtaining an Infrared spectrum by measuring the interferogram of a sample using an interferometer, then performing a Fourier Transform upon the interferogram to obtain the spectrum.
various parts of mAss spectroscopy, applications, principle, peaks, rules, typical mass spectra, various combinations, Fragmentation, rules of fragmentation and useful points which can help Chemical and analytical students and structural elucidation.
this ppt contain all basic information related to the mass spectrometry like introduction, principle of MS, type of ions, fragmentation processes eg. mcLafferty rearrangement, alpha clevage, sigma bond clevage, retro-diels-alder reaction
Quadrupole and Time of Flight Mass analysers.Gagangowda58
Description about important mass analysers Quadrupole and TOF: Principle, Construction and Working, Advantages and Disadvantages and their Applications.
Nuclear magnetic resonance (NMR) spectroscopyVK VIKRAM VARMA
SPECTROSCOPY
NMR SPECTROSCOPY
HISTORY
THEORY
PRINCIPLE
INSTRUMENTATION
SOLVENTS USED IN NMR(PROTON NMR)
CHEMICAL SHIFT
FACTORS AFFECTING CHEMICAL SHIFT
RELAXATION PROCESS
SPIN-SPIN COUPLING
푛+1 RULE
NMR SIGNALS IN VARIOUS COMPOUNDS
COUPLING CONSTANT
NUCLEAR MAGNETIC DOUBLE RESONANCE/ SPIN DECOUPLING
FT-NMR
ADVANTAGES & DISADVANTAGES
APPLICATIONS
REFERENCE
spectrofluorometer is the instrument for recording fluorescence emission and absorption spectra When a beam of light is incident on certain substances they emit visible light or radiations. This is known as fluorescence. Fluorescence starts immediately after the absorption of light and stops as soon as the incident light is cut off. The substances showing this phenomenon are known as flourescent substances.
A method of obtaining an Infrared spectrum by measuring the interferogram of a sample using an interferometer, then performing a Fourier Transform upon the interferogram to obtain the spectrum.
The detailed information of UV Visible Spectroscopy, it includes the information regarding electronic transitions, Electromagnetic radiations, Various shifts.
UV - Visible Spectroscopy detailed information is included .The Spectroscopy study provide the information and the absorbance as well the concentration of the drugs is studied.
Infrared Spectroscopy and UV-Visible spectroscopyPreeti Choudhary
Instrumentation of Infrared Spectroscopy and UV-Vis spectroscopy
Discuss the fundamentals and concepts behind Infrared and UV-Vis spectroscopy.
I hope this presentation helpful for you.
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Richard's entangled aventures in wonderlandRichard Gill
Since the loophole-free Bell experiments of 2020 and the Nobel prizes in physics of 2022, critics of Bell's work have retreated to the fortress of super-determinism. Now, super-determinism is a derogatory word - it just means "determinism". Palmer, Hance and Hossenfelder argue that quantum mechanics and determinism are not incompatible, using a sophisticated mathematical construction based on a subtle thinning of allowed states and measurements in quantum mechanics, such that what is left appears to make Bell's argument fail, without altering the empirical predictions of quantum mechanics. I think however that it is a smoke screen, and the slogan "lost in math" comes to my mind. I will discuss some other recent disproofs of Bell's theorem using the language of causality based on causal graphs. Causal thinking is also central to law and justice. I will mention surprising connections to my work on serial killer nurse cases, in particular the Dutch case of Lucia de Berk and the current UK case of Lucy Letby.
Earliest Galaxies in the JADES Origins Field: Luminosity Function and Cosmic ...Sérgio Sacani
We characterize the earliest galaxy population in the JADES Origins Field (JOF), the deepest
imaging field observed with JWST. We make use of the ancillary Hubble optical images (5 filters
spanning 0.4−0.9µm) and novel JWST images with 14 filters spanning 0.8−5µm, including 7 mediumband filters, and reaching total exposure times of up to 46 hours per filter. We combine all our data
at > 2.3µm to construct an ultradeep image, reaching as deep as ≈ 31.4 AB mag in the stack and
30.3-31.0 AB mag (5σ, r = 0.1” circular aperture) in individual filters. We measure photometric
redshifts and use robust selection criteria to identify a sample of eight galaxy candidates at redshifts
z = 11.5 − 15. These objects show compact half-light radii of R1/2 ∼ 50 − 200pc, stellar masses of
M⋆ ∼ 107−108M⊙, and star-formation rates of SFR ∼ 0.1−1 M⊙ yr−1
. Our search finds no candidates
at 15 < z < 20, placing upper limits at these redshifts. We develop a forward modeling approach to
infer the properties of the evolving luminosity function without binning in redshift or luminosity that
marginalizes over the photometric redshift uncertainty of our candidate galaxies and incorporates the
impact of non-detections. We find a z = 12 luminosity function in good agreement with prior results,
and that the luminosity function normalization and UV luminosity density decline by a factor of ∼ 2.5
from z = 12 to z = 14. We discuss the possible implications of our results in the context of theoretical
models for evolution of the dark matter halo mass function.
THE IMPORTANCE OF MARTIAN ATMOSPHERE SAMPLE RETURN.Sérgio Sacani
The return of a sample of near-surface atmosphere from Mars would facilitate answers to several first-order science questions surrounding the formation and evolution of the planet. One of the important aspects of terrestrial planet formation in general is the role that primary atmospheres played in influencing the chemistry and structure of the planets and their antecedents. Studies of the martian atmosphere can be used to investigate the role of a primary atmosphere in its history. Atmosphere samples would also inform our understanding of the near-surface chemistry of the planet, and ultimately the prospects for life. High-precision isotopic analyses of constituent gases are needed to address these questions, requiring that the analyses are made on returned samples rather than in situ.
Professional air quality monitoring systems provide immediate, on-site data for analysis, compliance, and decision-making.
Monitor common gases, weather parameters, particulates.
Multi-source connectivity as the driver of solar wind variability in the heli...Sérgio Sacani
The ambient solar wind that flls the heliosphere originates from multiple
sources in the solar corona and is highly structured. It is often described
as high-speed, relatively homogeneous, plasma streams from coronal
holes and slow-speed, highly variable, streams whose source regions are
under debate. A key goal of ESA/NASA’s Solar Orbiter mission is to identify
solar wind sources and understand what drives the complexity seen in the
heliosphere. By combining magnetic feld modelling and spectroscopic
techniques with high-resolution observations and measurements, we show
that the solar wind variability detected in situ by Solar Orbiter in March
2022 is driven by spatio-temporal changes in the magnetic connectivity to
multiple sources in the solar atmosphere. The magnetic feld footpoints
connected to the spacecraft moved from the boundaries of a coronal hole
to one active region (12961) and then across to another region (12957). This
is refected in the in situ measurements, which show the transition from fast
to highly Alfvénic then to slow solar wind that is disrupted by the arrival of
a coronal mass ejection. Our results describe solar wind variability at 0.5 au
but are applicable to near-Earth observatories.
(May 29th, 2024) Advancements in Intravital Microscopy- Insights for Preclini...Scintica Instrumentation
Intravital microscopy (IVM) is a powerful tool utilized to study cellular behavior over time and space in vivo. Much of our understanding of cell biology has been accomplished using various in vitro and ex vivo methods; however, these studies do not necessarily reflect the natural dynamics of biological processes. Unlike traditional cell culture or fixed tissue imaging, IVM allows for the ultra-fast high-resolution imaging of cellular processes over time and space and were studied in its natural environment. Real-time visualization of biological processes in the context of an intact organism helps maintain physiological relevance and provide insights into the progression of disease, response to treatments or developmental processes.
In this webinar we give an overview of advanced applications of the IVM system in preclinical research. IVIM technology is a provider of all-in-one intravital microscopy systems and solutions optimized for in vivo imaging of live animal models at sub-micron resolution. The system’s unique features and user-friendly software enables researchers to probe fast dynamic biological processes such as immune cell tracking, cell-cell interaction as well as vascularization and tumor metastasis with exceptional detail. This webinar will also give an overview of IVM being utilized in drug development, offering a view into the intricate interaction between drugs/nanoparticles and tissues in vivo and allows for the evaluation of therapeutic intervention in a variety of tissues and organs. This interdisciplinary collaboration continues to drive the advancements of novel therapeutic strategies.
Introduction:
RNA interference (RNAi) or Post-Transcriptional Gene Silencing (PTGS) is an important biological process for modulating eukaryotic gene expression.
It is highly conserved process of posttranscriptional gene silencing by which double stranded RNA (dsRNA) causes sequence-specific degradation of mRNA sequences.
dsRNA-induced gene silencing (RNAi) is reported in a wide range of eukaryotes ranging from worms, insects, mammals and plants.
This process mediates resistance to both endogenous parasitic and exogenous pathogenic nucleic acids, and regulates the expression of protein-coding genes.
What are small ncRNAs?
micro RNA (miRNA)
short interfering RNA (siRNA)
Properties of small non-coding RNA:
Involved in silencing mRNA transcripts.
Called “small” because they are usually only about 21-24 nucleotides long.
Synthesized by first cutting up longer precursor sequences (like the 61nt one that Lee discovered).
Silence an mRNA by base pairing with some sequence on the mRNA.
Discovery of siRNA?
The first small RNA:
In 1993 Rosalind Lee (Victor Ambros lab) was studying a non- coding gene in C. elegans, lin-4, that was involved in silencing of another gene, lin-14, at the appropriate time in the
development of the worm C. elegans.
Two small transcripts of lin-4 (22nt and 61nt) were found to be complementary to a sequence in the 3' UTR of lin-14.
Because lin-4 encoded no protein, she deduced that it must be these transcripts that are causing the silencing by RNA-RNA interactions.
Types of RNAi ( non coding RNA)
MiRNA
Length (23-25 nt)
Trans acting
Binds with target MRNA in mismatch
Translation inhibition
Si RNA
Length 21 nt.
Cis acting
Bind with target Mrna in perfect complementary sequence
Piwi-RNA
Length ; 25 to 36 nt.
Expressed in Germ Cells
Regulates trnasposomes activity
MECHANISM OF RNAI:
First the double-stranded RNA teams up with a protein complex named Dicer, which cuts the long RNA into short pieces.
Then another protein complex called RISC (RNA-induced silencing complex) discards one of the two RNA strands.
The RISC-docked, single-stranded RNA then pairs with the homologous mRNA and destroys it.
THE RISC COMPLEX:
RISC is large(>500kD) RNA multi- protein Binding complex which triggers MRNA degradation in response to MRNA
Unwinding of double stranded Si RNA by ATP independent Helicase
Active component of RISC is Ago proteins( ENDONUCLEASE) which cleave target MRNA.
DICER: endonuclease (RNase Family III)
Argonaute: Central Component of the RNA-Induced Silencing Complex (RISC)
One strand of the dsRNA produced by Dicer is retained in the RISC complex in association with Argonaute
ARGONAUTE PROTEIN :
1.PAZ(PIWI/Argonaute/ Zwille)- Recognition of target MRNA
2.PIWI (p-element induced wimpy Testis)- breaks Phosphodiester bond of mRNA.)RNAse H activity.
MiRNA:
The Double-stranded RNAs are naturally produced in eukaryotic cells during development, and they have a key role in regulating gene expression .
2. Spectroscopy is the tool for study of atomic &
molecular structure.
It deals with interaction of electronic radiation with
matter involving the measurement & interpretation of
the extension of absorption or emission of
electromagnetic radiation by molecule.
ALOK SHARMA Asst. Professor, Mahakal Institute of Pharmaceutical Studies, Ujjain (M.P.)
UV-Visible Spectroscopy
3. Most important consequence of such interaction is
the energy is absorbed or emitted by the matter in
discrete amount called as quanta.
UV radiation starts at blue end of visible light(4000Å)
& ends at 2000A.
It divided into two spectral region-
Near UV region- 2000Å-4000Å.
Far or vacuum UV region- below 2000Å.
UV-spectroscopy involved with electronic excitation.
ALOK SHARMA Asst. Professor, Mahakal Institute of Pharmaceutical Studies, Ujjain (M.P.)
UV-Visible Spectroscopy
4. Absorption And Emission spectra:-
Spectroscopy mainly concerned with interaction of
electromagnetic radiation with matter.
After interaction they may variation in intensity of EMR
with frequency.
Instrument which record this variation in intensity
known as spectrophotometer
Two way in which interaction may observed-
Sample itself emits radiation Called as emission spectra
Absorbs radiation from continuous source Called as absorption spectra
ALOK SHARMA Asst. Professor, Mahakal Institute of Pharmaceutical Studies, Ujjain (M.P.)
UV-Visible Spectroscopy
5. Wavelength(λ):-
distance between two successive maxima of one
electromagnetic wave. express in Angstron units or (mu)
Frequency(ν):-
Number of wavelength passing through a given point. per
sec.
Unit:- Hertz or cycles per second
Wave number:-
Number of waves per centimeter in vacuum.
Reciprocal of wavelength, express as per (cm).
relation between frequency, velocity & wave number
ν=(1/λ)c=(c/v)λ=(v/c)
ALOK SHARMA Asst. Professor, Mahakal Institute of Pharmaceutical Studies, Ujjain (M.P.)
UV-Visible Spectroscopy
7. Ultra violet absorption spectra arises from transition of electron
or electrons within molecule.
UV emission spectra arises from reverse type of transition.
Electron undergoes transition from lower to higher energy level,
this energy difference given by,
E=hν erg
But actually energy difference between ground & excited states
of electrons
E1-E0=hν
Total energy of the molecule is sum of electronic, vibrational,
rotational energy.
E=Eele +Evib +Erot
ALOK SHARMA Asst. Professor, Mahakal Institute of Pharmaceutical Studies, Ujjain (M.P.)
UV-Visible Spectroscopy
8. UV-visible spectroscopy is the measurement of absorbance or
transmittance of radiation in the ultra-violet &visible region of
the spectrum.
It arises from transition of electron.
Stage -1
M + hν M*
Stage -2
M* new species
Excitation of species by absorption of
photon with the limited life time.
Relaxation by converting M* to
the new species by
photochemical reaction
ALOK SHARMA Asst. Professor, Mahakal Institute of Pharmaceutical Studies, Ujjain (M.P.)
UV-Visible Spectroscopy
9. σ-electrons-
Involved in the saturated bonds.
Found in the carbon, hydrogen in the paraffin.
Energy required to excite σ-produced is electron more
than the produced by the UV-light.
π- electrons-
Involved in unsaturated hydrocarbon.
Present in trienes & aromatic compounds.
n-electrons-
It does not evolved in the bonding of the molecules.
ALOK SHARMA Asst. Professor, Mahakal Institute of Pharmaceutical Studies, Ujjain (M.P.)
UV-Visible Spectroscopy
10. transition
σ-σ*
n-σ* usually
allowed
n-π*
π-π* forbidden
Allowed transition:- having ε max 104 or more.This transition due to π-π* transition.
In 1,3-butadiene exhibits absorption at 217 nm & has εmax 21000 represent allowed transition.
Forbidden transition:- transition having εmax less than 104 .Occurs due to n-π*transition.
ALOK SHARMA Asst. Professor, Mahakal Institute of Pharmaceutical Studies, Ujjain (M.P.)
UV-Visible Spectroscopy
11. Transition Region Wavelength
σ-σ*
π-π*
Far UV- region <200 nm
n-σ* Ultra-violet =200 nm
n-π* Near UV &
visible
300- 600 nm
Energy required for various transitions are in the order
σ-σ*> n-σ* > π-π*> n-π*
Thus, n-π*transition required less energy than a π-π* or σ-σ* transition.
ALOK SHARMA Asst. Professor, Mahakal Institute of Pharmaceutical Studies, Ujjain (M.P.)
UV-Visible Spectroscopy
15. fig.-Schematic representation of
single beam UV-spectrophotometer
Fig.-schematic representation of
double beam UV- spectrophotometer
ALOK SHARMA Asst. Professor, Mahakal Institute of Pharmaceutical Studies, Ujjain (M.P.)
UV-Visible Spectroscopy
16. Distribution of energy through spectrum is function of
temperature.
For Visible region-
Tungsten filament lamp
Use for region 350nm to 2000nm.
Problem-
Due to evaporation of tungsten life period
decreases.
It is overcome by using tungsten-halogen lamp.
Halogen gas prevents evaporation of tungsten.
ALOK SHARMA Asst. Professor, Mahakal Institute of Pharmaceutical Studies, Ujjain (M.P.)
UV-Visible Spectroscopy
17. For ultra violet region-
Hydrogen discharge lamp
consist of two electrode contain in deuterium filled
silica envelop.
gives continuous spectrum in region 185-380nm.
above 380nm emission is not continuous.
UV-Vis spectrophotometer have both deuterium &
tungsten lamps.
Selection of lamp is made by moving lamp mounting or
mirror to cause the light fall on monochromator.
ALOK SHARMA Asst. Professor, Mahakal Institute of Pharmaceutical Studies, Ujjain (M.P.)
UV-Visible Spectroscopy
18. Deuterium lamps:-
Radiation emitted is 3-5 times more than the hydrogen
discharge lamps.
Xenon discharge lamp:-
Xenon stored under pressure in 10-30 atmosphere.
It possesses two tungsten electrode separated by 8
cm.
Intensity of UV radiation more than hydrogen lamp.
Mercury arc:-
Mercury vapour filled under the pressure .
Excitation of mercury atom by electric discharge
ALOK SHARMA Asst. Professor, Mahakal Institute of Pharmaceutical Studies, Ujjain (M.P.)
UV-Visible Spectroscopy
19. Provides a beam of radiant energy of a given nominal
wavelength and spectral bandwidth.
Parts of a monochramator
1. An entrance slit
2. A collimator
3. A grating
4. A collimator*
5. An exit slit
ALOK SHARMA Asst. Professor, Mahakal Institute of Pharmaceutical Studies, Ujjain (M.P.)
UV-Visible Spectroscopy
20. Filters –
a) Glass filters-
Made from pieces of colored glass which transmit limited
wavelength range of spectrum.
Color produced by incorporation of oxide of vanadium,
chromium, iron, nickel, copper.
Wide band width 150nm.
b) Gelatin filters-
Consist of mixture of dyes placed in gelatin &
sandwiched between glass plates.
Band width 25nm.
c) Inter ferometric filters-
Band width 15nm.
ALOK SHARMA Asst. Professor, Mahakal Institute of Pharmaceutical Studies, Ujjain (M.P.)
UV-Visible Spectroscopy
21. Prisms-
Prism bends the monochromatic light.
Amount of deviation depends on wavelength.
Quartz prism used in UV-region.
Glass prism used in visible region spectrum.
Function –
They produce non linear dispersion.
ALOK SHARMA Asst. Professor, Mahakal Institute of Pharmaceutical Studies, Ujjain (M.P.)
UV-Visible Spectroscopy
22. Fig.-mechanism of working of prism.
ALOK SHARMA Asst. Professor, Mahakal Institute of Pharmaceutical Studies, Ujjain (M.P.)
UV-Visible Spectroscopy
23. Grating-
Large number of equispaced lines on a glass blank
coated with aluminum film.
Blaze angle
Normal surface
vector
Normal to
groove face
ALOK SHARMA Asst. Professor, Mahakal Institute of Pharmaceutical Studies, Ujjain (M.P.)
UV-Visible Spectroscopy
24. Spectroscopy requires all materials in the beam path
other than the analyte should be as transparent to the
radiation as possible.
The geometries of all components in the system should
be such as to maximize the signal and minimize the
scattered light.
The material from which a sample cuvette is fabricated
controls the optical window that can be used.
ALOK SHARMA Asst. Professor, Mahakal Institute of Pharmaceutical Studies, Ujjain (M.P.)
UV-Visible Spectroscopy
25. Some typical materials are:
Optical Glass - 335 - 2500 nm
Special Optical Glass – 320 - 2500 nm
Quartz (Infrared) – 220 - 3800 nm
Quartz (Far-UV) – 170 - 2700 nm
•Keep the cuvette clean.
•Don’t clean with paper products.
•Store dry.
•Don’t get finger prints on them.
•Store carefully and gently
ALOK SHARMA Asst. Professor, Mahakal Institute of Pharmaceutical Studies, Ujjain (M.P.)
UV-Visible Spectroscopy
26. Three common types of detectors are used
Barrier layer cells
Photocell detector
Photomultiplier
Photo voltaic cells or barrier layer cells :-
They are primarily used for measurement of radiation
in visible region.
Maximum sensitivity-550nm.
It consist of flat Cu or Fe electrode on which
semiconductor such as selenium is deposited.
on the selenium a thin layer of silver or gold is
sputtered over the surface.
ALOK SHARMA Asst. Professor, Mahakal Institute of Pharmaceutical Studies, Ujjain (M.P.)
UV-Visible Spectroscopy
27. Barrier layer cells
A barrier exist between the selenium & iron which
prevents the electron flowing through iron.
Therefore electrons are accumulated on the silver
surface.
These electrons are produced voltage.
- terminal
Silver surface
selenium
+ terminal
fig.-Barrier layer cell
ALOK SHARMA Asst. Professor, Mahakal Institute of Pharmaceutical Studies, Ujjain (M.P.)
UV-Visible Spectroscopy
28. Photocell detector:-
It consist of high sensitive cathode in the form of a half
cylinder of metal which is evacuated.
Anode also present which fixed along the axis of the
tube
Photocell is more sensitive than photovoltaic cell.
+ -
light
Fig.- photocell detector
ALOK SHARMA Asst. Professor, Mahakal Institute of Pharmaceutical Studies, Ujjain (M.P.)
UV-Visible Spectroscopy
29. Photomultiplier tube:-
It is generally used as detector in UV-spectrophotometer.It
is the combination of photodiode & electron multiplier. It
consist of evacuated tube contains photo-cathode. 9-16
electrodes known as dynodes.
Fig.-photomultiplier tube
ALOK SHARMA Asst. Professor, Mahakal Institute of Pharmaceutical Studies, Ujjain (M.P.)
UV-Visible Spectroscopy
30. Signal from detector received by the recording system
The recording done by recorder pan.
ALOK SHARMA Asst. Professor, Mahakal Institute of Pharmaceutical Studies, Ujjain (M.P.)
UV-Visible Spectroscopy
31. Important to reposition the cuvettes properly
To clean the cuvettes, lens paper soaked in
spectrograde methanol, which is held by a hemostat is
used.
When cuvettes are cleaned the methanol film left
evaporates quickly leaving cuvette surface free of
contaminants
For maximum precision syringes are used to change
the solution leaving the cuvettes in the same place.
ALOK SHARMA Asst. Professor, Mahakal Institute of Pharmaceutical Studies, Ujjain (M.P.)
UV-Visible Spectroscopy
32. Single beam spectrophotometer:-
Double beam spectrophotometer:-
Advantage of double beam spectrophotometer:-
It is not necessary to continually replace the blank with
the sample or to adjust the auto zero.
The ratio of the powers of the sample & reference is
constantly obtained.
It has rapid scanning over the wide wavelength region
because of the above two factors.
ALOK SHARMA Asst. Professor, Mahakal Institute of Pharmaceutical Studies, Ujjain (M.P.)
UV-Visible Spectroscopy
33. Lamberts Law:-
Intensity of beam of parallel monochromatic radiation
decreases exponentially as it passes through medium
of homogeneous thickness.
Absorption is proportional to the thickness (path
length) of solution.
I0/It=KC
k=“absorption coefficient” defined as reciprocal of the
thickness which required to reduced to light to 1/10 of
its intensity
ALOK SHARMA Asst. Professor, Mahakal Institute of Pharmaceutical Studies, Ujjain (M.P.)
UV-Visible Spectroscopy
34. Beers law:-
Intensity of a beam of parallel monochromatic radiation
decreases exponentially with the number of absorbing
molecule.
Absorption is proportional to concentration.
Combination of two law yields beers- lamberts law.
A=Io/It=abc
Where,
A=absorbance
Io-intensity of incident light
It-transmitted light
C-concentration
B-thickness
ALOK SHARMA Asst. Professor, Mahakal Institute of Pharmaceutical Studies, Ujjain (M.P.)
UV-Visible Spectroscopy
35. Deviation from beer’s law:-
From the beer’s law plot the absorbance against the
conc.
A straight line passing through origin is obtained.
Deviation is due to the following factors:-
A foreign substance having colour particle may affect the
absorption & extinction coefficient.
Deviation also occur if colored solute ionized or dissociates
in the solution.
for e.g.- benzyl alcohol in chloroform
Due to the presence of impurities that fluoresce or absorb at
the absorption wave length.
If monochromatic light is not used deviation may occurs.
If width of the slit is not proper.
If the solution species undergoes polymerisation
ALOK SHARMA Asst. Professor, Mahakal Institute of Pharmaceutical Studies, Ujjain (M.P.)
UV-Visible Spectroscopy
36. Transmittance (T)= Io/It
% transmittance (%T)= It/Io ˣ 100
Absorbance (A) = log (It/Io)
Absorbance also term as,
Extinction coefficient(E)
Optical density (D)
A= log (Io/It) =abc
when concentration is in moles/lit. the constant called
as molar absorptivity (ε) molar extinction coefficient.
Specific absorbance-
absorbance of a specific concentration in a cell of
specific pathlength.
ALOK SHARMA Asst. Professor, Mahakal Institute of Pharmaceutical Studies, Ujjain (M.P.)
UV-Visible Spectroscopy
37. Most common form in p’ceutical analysis A1cm
1% is
absorbance of 1g/100ml (1%w/v) solution in 1cm cell.
ε = A 1cm
1%
ˣ mole.wt.
10
ALOK SHARMA Asst. Professor, Mahakal Institute of Pharmaceutical Studies, Ujjain (M.P.)
UV-Visible Spectroscopy
38. It is used for calculating the absorption maxima
Woodward (1941) gives certain rule for correlating λmax with the
molecular structure
These rules are modified by Scott & Feiser.
This rule for calculating λmax in conjugated dienes, trienes,
polyenes.
Homoannular dienes:-
cyclic dienes having conjugated double bonds in the same ring.
e.g. CH3
CH3
ALOK SHARMA Asst. Professor, Mahakal Institute of Pharmaceutical Studies, Ujjain (M.P.)
UV-Visible Spectroscopy
39. Hateroannuler dienes:-
Cyclic dienes in which double bonds in conjugation are present
in the different ring.
Endocyclic double bonds:-
It is the double bond present in ring as shown.
Exocyclic double bonds:-
Double bond in which one of the double bonded atom is the part
of ring system.
CH2
CH2
e.g. Heteroannuler dienes
Endocyclic
double bond
Exocyclic
double bond
ALOK SHARMA Asst. Professor, Mahakal Institute of Pharmaceutical Studies, Ujjain (M.P.)
UV-Visible Spectroscopy
41. Problems:-1) 1,4- dimethyl cyclohex-1,3,-diene
Parent value for Homoannular diene = 253 nm
Two alkyl substituent's 2 ˣ 5 = 10 nm
Two ring residues 2ˣ 5 = 10 nm
Calculated value = 273 nm
Observed value = 265 nm
2)
Parent value for Heteroannuler diene = 215 nm
Four ring residue 4 ˣ 5 = 20 nm
Calculated value = 235 nm
Observed value = 236 nm
CH3 CH3
ALOK SHARMA Asst. Professor, Mahakal Institute of Pharmaceutical Studies, Ujjain (M.P.)
UV-Visible Spectroscopy
42. a)Parent values:-
1.α,β-unsaturated acyclic or six membered ring ketone 215 nm
2.α,β-unsaturated five membered ring ketone 202nm
3.α,β-unsaturated aldehyde 207nm
b)increments:-
1.Each alkyl substituent or ring residue
at α, position 10nm
at β,position 12nm
at γ,position 18nm
2.Each Exocyclic double bond 5nm
3.Double bond extending conjugation 30nm
4.Homoannular conjugatated dienes 39nm
5.Auxochromes. Positions
α β γ
-OH 35 30 50
-OR 35 30 17
-SR - 85 -
-OCOCH3 6 6 6
ALOK SHARMA Asst. Professor, Mahakal Institute of Pharmaceutical Studies, Ujjain (M.P.)
UV-Visible Spectroscopy
43. Problems:- O
CH3-C-C=CH3
CH3
1) Parent value = 215 nm
2) One alkyl substituent in α position = 10 nm
3) Calculated value = 225 nm
4) Observed value = 220 nm
Parent value for α,β- unsaturated 6 membered cyclic ketone=215 nm
One ring residue at α position = 10 nm
2 ring residue at β- position 2* 12 =24 nm
Double bond Exocyclic to 2 ring 2* 5 =10 nm
Calculated value = 259nm
Observed value =
A α,β- unsaturated
acyclic ketone
O
ALOK SHARMA Asst. Professor, Mahakal Institute of Pharmaceutical Studies, Ujjain (M.P.)
UV-Visible Spectroscopy
44. R-C6H4-COG λmax (nm)
parent chromophore:-
G=alkyl/ring residue
G=H & R=H
G=OH or O alkyl
246
250
230
Add for R:
Alkyl or ring residue o,m 3
p 10
-OH, OMe, -O-Alkyl o,m 7
p 25
O- o 11
m 20
p 78
Cl o,m 0
p 10
Br o,m 2
P 15
NH2 o,m 13
p 58
NMe2 o,m 20
p 85
ALOK SHARMA Asst. Professor, Mahakal Institute of Pharmaceutical Studies, Ujjain (M.P.)
UV-Visible Spectroscopy
45. 1) Para chloroacetophenone
Basic value = 246 nm
Cl substitution at p- position = 10 nm
Calculated value = 256 nm
Observed value = 254nm
Cl
C CH3
O
ALOK SHARMA Asst. Professor, Mahakal Institute of Pharmaceutical Studies, Ujjain (M.P.)
UV-Visible Spectroscopy
46. Extent of conjugation
Distinction between conjugated and non conjugated compound
Detection of chromophore in an unknown compound
Identification of a chromophore (functional group)
Study of strain
Study of geometric isomerism
Study of tautomerism
Study of structural features in different solvents
As an analytical tool
ALOK SHARMA Asst. Professor, Mahakal Institute of Pharmaceutical Studies, Ujjain (M.P.)
UV-Visible Spectroscopy
47. Willard H. et.al.; Instrumental Methods Of Analysis.
Gurdeep R. chatwal; Sham K. Anand; Instrumental Methods Of Chemical Analysis.
Y. Anjaneyulu; K. Chandrasekhar; Valli Manickam; Text book of analytical chemistry.
Y. R.Sharma; Elementary organic spectroscopy.
P.S.Kalsi; Spectroscopy of organic compound.
B.K.Sharma; Instrumental methods of chemical analysis.
ALOK SHARMA Asst. Professor, Mahakal Institute of Pharmaceutical Studies, Ujjain (M.P.)
UV-Visible Spectroscopy
48. Queries
ALOK SHARMA Asst. Professor, Mahakal Institute of Pharmaceutical Studies, Ujjain (M.P.)
UV-Visible Spectroscopy