Spectroscopy (Topics 8,10,12,14,15) Flashcards
What does the de Broglie relation allow us to conclude?
Particles with low linear momentum have long wavelengths and vice versa
Which type of transitions in a molecule is likely to be induced by photons with a wavelength in the microwave region?
Vibrational
What is spectoscopy?
the study of the interaction of electromagnetic
radiation with matter
How and why things scatter, absorb, or emit light
Exchange of energy between radiation and matter
Electromagnetic radiation is
Light
Oscillating electric and magnetic fields that propagate as a wave
c =
speed of light : 2.998 x 10^8 ms^-1
๐ (wavelength (m)) x ๐ (frequency (Hz = s^-1)
๐ =
The wavelength at which a substance has itโs strongest photon absorption
โ (6.626 x 10^-34 Js) / ๐ (mass(kg)) x ๐ฃ (velocity (ms^-1))
angular frequency ๐
2 ๐ ๐ (frequency (s^-1)
2 ๐ / T (s)
๐ (1D)
๐๐/2๐ฟ
1 / 2๐ (๐๐ / ๐๐๐๐)^1/2
๐~ (wavenumber (cm^-1) =
๐ (s^-1) / c (2.998 x 10^8 ms^-1)
1 / 2๐c (๐๐ / ๐๐๐๐)^1/2
๐ (1D) =
2๐ฟ๐/๐
๐๐ฅ^2 + ๐๐ฆ^2 + ๐๐ง^2 (3D)
4๐ฟ^2๐^2 / C^2
Infrared radiation frequency
n ~10^12 โ 10^13 s-1
Visible light radiation frequency
n ~10^14 s-1
Planck Constant โ =
โ =
6.626 x 10^-34 Js
โ / 2 pi
Planck-Einstein Relation:
๐ธ (J) = โ (6.626 x 10^-34 Js) x ๐ (frequency (s^-1))
๐ธ = ๐๐^2
๐ธ^2 =
So for a photon, ๐ธ =
๐ธ^2 = (๐๐^2)^2 + (๐๐)^2
๐ธ = ๐๐
๐ธ (energy (J))
๐ (mass (kg))
๐ (momentum (kg m s^-1)
๐ (speed of light (2.998 x 10^8 ms^-1))
Einstein mass-energy relation
E = mc^2
de Broglie Wavelength
lambda (wavelength (m)) = โ (6.626 x 10^-34 Js or kg m^2 s^-1 / ๐ (mass(kg)) ๐ฃ (velocity(m s^-1))
How do you define a peak?
Peak position
Peak intensity
Peak breadth
delta E =
E1 - E0
Bohr condition
Photon energy โ๐ must be equal to delta E in order for a transition to occur
๐ (excited state lifetime)=
1 / A1->0
Peak intensity information
Population
Transition Probability
State Degeneracy
Experimental: Path length of sample
Boltzmann expression
๐(๐ฝ) / ๐= ๐(๐ฝ) ๐^โ (๐ธ(๐ฝ) ๐๐)
๐ธ(๐ฝ) = ๐ต~โ๐๐ฝ(๐ฝ + 1)
๐(๐ฝ) = 2๐ฝ + 1
(J) subscript
N upper / N lower =
๐โ^(โ๐ธ ๐๐)
At room temp (298K), kT =
200 cm^-1
Most critical factor in determining selection rules and line intensities
Transition dipole moment
Measure of the electric dipole moment associated with movement of
charge from its initial state (state 0) to its final state (state n)
Gross Selection rule
In order for a transition to occur,
it must have a nonzero transition dipole moment
In order for an atom or molecule to
absorb/emit a photon at a specific frequency, it must possess
(at least transiently) a dipole oscillating at that frequency
๐ด = ๐๐ฟ๐ units
Absorbance (unit less) = molar extinction coefficient (M^-1 cm^-1) x sample thickness (often 1cm) x concentraTion (M)
Commonly used versions of Beer-Lambert Law
๐ด = ๐๐ฟ๐
log (๐ผ0/๐ผ) = ๐๐ฟ๐
log (๐ผ0/๐ผ) = ๐๐ฟ[๐] = ๐ผ๐ฟ
๐ผ = transmitted light intensity
๐ = molar extinction coefficient (M^-1 cm^-1)
๐ฟ = sample thickness (often 1cm)
๐ = concentration (M)
๐ = absorption cross section
[๐] = Concentration (molecule cm^-3)
๐ผ = absorption coefficient