ULTRAVIOLET-VISIBLE SPECTROSCOPY (UV-VIS) - PowerPoint PPT Presentation

1 / 9
About This Presentation
Title:

ULTRAVIOLET-VISIBLE SPECTROSCOPY (UV-VIS)

Description:

ULTRAVIOLET-VISIBLE SPECTROSCOPY (UV-VIS) UV-VIS Relative Transition Energies UV-VIS UV-VIS UV-VIS Spectrum UV-VIS Spectrum UV-VIS Spectrum END ULTRAVIOLET-VISIBLE ... – PowerPoint PPT presentation

Number of Views:674
Avg rating:3.0/5.0
Slides: 10
Provided by: ban15
Category:

less

Transcript and Presenter's Notes

Title: ULTRAVIOLET-VISIBLE SPECTROSCOPY (UV-VIS)


1
ULTRAVIOLET-VISIBLESPECTROSCOPY(UV-VIS)
2
UV-VIS
Absorbance of energy in the UV-Vis region results
in the movement of an electron from the ground
state to an excited state. Bonded electrons are
either in a s or a p bonding orbital. Unshared
electrons are nonbonding (n) es. Excited
electrons reside in antibonding orbitals. Common
electronic transitions are n ? p p ?
p n ? s Difficult electronic transitions
are s ? p p ? s s ? s
3
Relative Transition Energies
s
p
n
p
s
4
UV-VIS
Peaks from electronic transitions are broad
because they encompass a large number of
vibrational and rotational states. These
absorbances follow Beers Law A ecl A
Absorbance, A.U. e molar
extinction coefficient, cm2/mmol c
concentration, M l pathlength,
cm Spectra are usually characterized by ?max,
the wavelength of maximum absorbance, and e at
this wavelength.
5
UV-VIS
UV absorbances normally occur in the 200-350 nm
region of the spectrum (mµ is also used). The
visible region is typically from 350-700 nm. The
energy of the transition is indicated by ?max.
The intensity of the absorbance (e) is related
to the probability of the transition. The n ? p
transition requires less energy and occurs at
longer wavelength. The p ? p transition is
more generally more probable so has a greater
extinction coefficient.
6
UV-VIS Spectrum
F
F
F
F
7
UV-VIS Spectrum
8
UV-VIS Spectrum
9
ENDULTRAVIOLET-VISIBLESPECTROSCOPY(UV-VIS)
Write a Comment
User Comments (0)
About PowerShow.com