Spectroscopy (Topics 8,10,12,14,15) Flashcards

(77 cards)

1
Q

What does the de Broglie relation allow us to conclude?

A

Particles with low linear momentum have long wavelengths and vice versa

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
2
Q

Which type of transitions in a molecule is likely to be induced by photons with a wavelength in the microwave region?

A

Vibrational

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
3
Q

What is spectoscopy?

A

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

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
4
Q

Electromagnetic radiation is

A

Light
Oscillating electric and magnetic fields that propagate as a wave

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
5
Q

c =

A

speed of light : 2.998 x 10^8 ms^-1
πœ† (wavelength (m)) x 𝜈 (frequency (Hz = s^-1)

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
6
Q

πœ† =

A

The wavelength at which a substance has it’s strongest photon absorption
β„Ž (6.626 x 10^-34 Js) / π‘š (mass(kg)) x 𝑣 (velocity (ms^-1))

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
7
Q

angular frequency πœ”

A

2 πœ‹ 𝜈 (frequency (s^-1)
2 πœ‹ / T (s)

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
8
Q

𝜈 (1D)

A

𝑛𝑐/2𝐿
1 / 2πœ‹ (π‘˜π‘“ / π‘šπ‘’π‘“π‘“)^1/2

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
9
Q

𝜈~ (wavenumber (cm^-1) =

A

𝜈 (s^-1) / c (2.998 x 10^8 ms^-1)
1 / 2πœ‹c (π‘˜π‘“ / π‘šπ‘’π‘“π‘“)^1/2

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
10
Q

𝑛 (1D) =

A

2𝐿𝜈/𝑐

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
11
Q

𝑛π‘₯^2 + 𝑛𝑦^2 + 𝑛𝑧^2 (3D)

A

4𝐿^2𝜈^2 / C^2

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
12
Q

Infrared radiation frequency

A

n ~10^12 – 10^13 s-1

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
13
Q

Visible light radiation frequency

A

n ~10^14 s-1

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
14
Q

Planck Constant β„Ž =
ℏ =

A

6.626 x 10^-34 Js
ℏ / 2 pi

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
15
Q

Planck-Einstein Relation:

A

𝐸 (J) = β„Ž (6.626 x 10^-34 Js) x 𝜈 (frequency (s^-1))

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
16
Q

𝐸 = π‘šπ‘^2
𝐸^2 =
So for a photon, 𝐸 =

A

𝐸^2 = (π‘šπ‘^2)^2 + (𝑝𝑐)^2
𝐸 = 𝑝𝑐
𝐸 (energy (J))
π‘š (mass (kg))
𝑝 (momentum (kg m s^-1)
𝑐 (speed of light (2.998 x 10^8 ms^-1))

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
17
Q

Einstein mass-energy relation

A

E = mc^2

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
18
Q

de Broglie Wavelength

A

lambda (wavelength (m)) = β„Ž (6.626 x 10^-34 Js or kg m^2 s^-1 / π‘š (mass(kg)) 𝑣 (velocity(m s^-1))

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
19
Q

How do you define a peak?

A

Peak position
Peak intensity
Peak breadth

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
20
Q

delta E =

A

E1 - E0

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
21
Q

Bohr condition

A

Photon energy β„Žπœˆ must be equal to delta E in order for a transition to occur

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
22
Q

𝝉 (excited state lifetime)=

A

1 / A1->0

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
23
Q

Peak intensity information

A

Population
Transition Probability
State Degeneracy
Experimental: Path length of sample

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
24
Q

Boltzmann expression

A

𝑁(𝐽) / 𝑁= 𝑔(𝐽) 𝑒^βˆ’ (𝐸(𝐽) π‘˜π‘‡)
𝐸(𝐽) = 𝐡~β„Žπ‘π½(𝐽 + 1)
𝑔(𝐽) = 2𝐽 + 1
(J) subscript

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
25
N upper / N lower =
π‘’βˆ’^(βˆ†πΈ π‘˜π‘‡)
26
At room temp (298K), kT =
200 cm^-1
27
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)
28
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
29
𝐴 = πœ€πΏπ‘ units
Absorbance (unit less) = molar extinction coefficient (M^-1 cm^-1) x sample thickness (often 1cm) x concentraTion (M)
30
Commonly used versions of Beer-Lambert Law 𝐴 = πœ€πΏπ‘
log (𝐼0/𝐼) = πœ€πΏπ‘ log (𝐼0/𝐼) = 𝜎𝐿[𝑁] = 𝛼𝐿 𝐼 = transmitted light intensity πœ€ = molar extinction coefficient (M^-1 cm^-1) 𝐿 = sample thickness (often 1cm) 𝑐 = concentration (M) 𝜎 = absorption cross section [𝑁] = Concentration (molecule cm^-3) 𝛼 = absorption coefficient
31
Heisenberg Uncertainty Δ𝐸Δ𝑑 >/=
β„Ž / 2πœ‹
32
Microwave wavelength
1cm - 100 um
33
Infra-red wavelength
1um - 100 um
34
Visible light wavelength
400 - 700 nm
35
Order of energies for 3 spectroscopies
Delta E elec >> Delta E vib >> Delta E rot
36
Rotational energies are in ... region of electromagnetic spectrum (microwave)
1 – 100 cm^-1
37
𝐼 (moment of inertia) =
Sum of (𝑖) π‘šπ‘–π‘Ÿπ‘–^2 𝑖 is subscript πœ‡π‘Ÿ^2
38
𝐹𝐽 = 𝐽 is subscript 𝐹~(𝐽) = (rotational energy levels)
𝐡𝐽(𝐽 + 1) 𝐡~𝐽 (𝐽 + 1) or 𝐡~𝐽 (𝐽 + 1) - 𝐷~(𝐽)𝐽^2(𝐽 + 1)^2 (𝐽) is subscript
39
𝐡 (cm^-1)= 𝐡~ (rotational constant (cm^-1) =
ℏ^2 / 2𝐼 ℏ / 4πœ‹π‘πΌ β„Ž / 8πœ‹^2c𝐼
40
𝜈~ (wavenumber (cm^-1) (𝐽 + 1 ← 𝐽) =
2𝐡~(𝐽 + 1) 2𝐡~(𝐽 + 1) - 4𝐷~(𝐽) (𝐽 + 1)^3 First J subscript
41
What will will result in a "red shift"
Increase in the wavelength of a wave with respect to the detector Decrease in the wavenumber of a wave with respect to the detector Decrease in the frequency of a wave with respect to the detector
42
For the Doppler broadening of a peak, what affects the width of the observed peak?
The temperature and the peak position
43
What function can be used to describe a peak in a spectrum?
Gaussian function
44
What will cause deviationes in the linearity of the Beer-Lambert law?
Changes in the refractive index at high analyte concentration Fluorescence or phosphorescence of the sample Scaterring of light due to particulates in the sample
45
The lifetime broadening of a spectral line arises from
The Heisenberg uncertainty principle
46
What are considered absorption and emission processes in spectroscopy
Spontaneous emission and stimulated absorption
47
The intensity of the spectroscopy transition can be predicted from
The population of the initial state and degeneracy
48
In the Beer-Lambert law, the graphical representation of -log(10) of transmittance versus concentration of a solution can be fitted using
a linear regression
49
𝑉 (Potential energy (J))
𝑉 = 1/2 π‘˜π‘“ π‘₯^2 π‘˜π‘“ = spring force constant (Nm^-1) 𝑓 is subscript π‘₯ = π‘Ÿ βˆ’ π‘Ÿπ‘’ π‘Ÿπ‘’ = distance away from equilibrium (m) 𝑒 is subscript
50
𝐺~(v) = (vibrational energy levels)
(v + 1/2) 𝜈~ (v + 1/2) 𝜈~ - (v + 1/2)^2 π‘₯𝑒 𝜈~ (anharmonic) π‘₯𝑒 = Unitless anharmonicity constant, 𝑒 subscript
51
𝐸v = (vibrational energy)
(v + 1 / 2) β„πœ”
52
πœ” =
(π‘˜π‘“ / π‘šπ‘’π‘“π‘“)^1/2
53
Gross Selection Rule
Dipole must change with displacement
54
From selection rules, transitions are only allowed for... (P, Q, R)
𝚫𝐯 = ±𝟏 𝚫J = ±𝟏 P: 𝚫 J = –1 Q: 𝚫 J = 0 R: 𝚫 J = +1
55
𝑆~ (v, 𝐽 ) = (transition energy levels)
𝐺~(v) + 𝐹~(𝐽) = (v + 1/2) 𝜈~ + 𝐡~𝐽(𝐽 + 1)
56
Δ𝑆~𝑃 (v, 𝐽) 𝑃 is subscript
𝜈~𝑃(𝐽) = 𝜈~ - 2𝐡~𝐽 𝑃 is subscript 𝜈~ βˆ’ (𝐡~1 + 𝐡~0)𝐽 + (𝐡~1 - 𝐡~0)𝐽^2
57
Δ𝑆~𝑄 (v, 𝐽) 𝑄 is subscript
𝜈~𝑄(𝐽) = 𝜈~ 𝑄 is subscript 𝜈~ + (𝐡~1 - 𝐡~0)𝐽(𝐽 + 1)
58
Δ𝑆~𝑅 (v, 𝐽) 𝑅 is subscript
𝜈~𝑅 (𝐽) = 𝜈~ + 2𝐡~(𝐽 + 1) 𝑅 is subscript 𝜈~ + (𝐡~1 + 𝐡~0)(𝐽 + 1) + (𝐡~1 - 𝐡~0)(𝐽 + 1)^2
59
Rotational spectroscopy rotors
rigid rotor and non-rigid rotor
60
Vibrational spectroscopy oscillators
harmonic oscillators and anharmonic oscillators
61
𝐡v =
𝐡e βˆ’ 𝛼e(v + 1/2) e subscript 𝐡e: Rotational constant at the equilibrium structure 𝛼: Constant, reflects shape of potential energy curve
62
Combination difference to the same J level
𝜈~𝑅 (𝐽-1) - 𝜈~𝑃(𝐽+1) = 4 𝐡~0 (𝐽 + 1/2)
63
Combination difference from the same J level
𝜈~𝑅 (𝐽) - 𝜈~𝑃(𝐽) = 4 𝐡~1 (𝐽 + 1/2)
64
Number of vibrational normal nodes
3N – 5 for a linear molecule and 3N – 6 for a nonlinear molecule
65
Ξ”G~ v = 0 β†’ 1 (fundamental):
𝐺~(v + 1) - 𝐺~(v) = (v + 3/2) 𝜈~ - (v + 3/2)^2 π‘₯𝑒 𝜈~ - (v + 1/2) 𝜈~ + (v + 1/2)^2 π‘₯𝑒 𝜈~ (using G~ equation) = 𝜈~ - 2(v + 1) π‘₯𝑒 𝜈~
66
Ξ”G~ v = 0 β†’ 2 (1st overtone)
𝐺~(v + 2) - 𝐺~(v) = (v + 5/2) 𝜈~ - (v + 5/2)^2 π‘₯𝑒 𝜈~ - (v + 1/2) 𝜈~ + (v + 1/2)^2 π‘₯𝑒 𝜈~ (using G~ equation) = 2𝜈~ - 2(2v + 3) π‘₯𝑒 𝜈~
67
Which one of the following functions best describes the simple harmonic oscillator?
y = Ax^2
68
At which frequency is the R(0) transition located?
𝜈 + 2B
69
In the simple harmonic oscillator model for a diatomic molecule, steeper slopes of the parabola indicates
stronger bond between the atoms in the molecule
70
The first P-branch transition is
P(0)
71
Parameters that can affect the full-width-at-half-maximum of an observed optical transition in a spectrum?
Temperature The lifetime in an excited state The phase of the medium Atomic mass of the species
72
Parameters that can affect the intensity (height) of an observed peak in a microwave spectrum?
The instrument resolution The degeneracy of the rotational energy levels involved in the transition The temperature The rotational transition dipole moment
73
𝐡~𝑒
Rotational constant for the equilibrium bond length of the molecule. It corresponds to the rotational constant when the molecule is in its lowest vibrational state, assuming no vibrational excitation. It provides the most fundamental measure of the molecule's moment of inertia in its equilibrium configuration
74
𝐡~0
the rotational constant for the molecule when it is in its vibrational ground state (v=0). It accounts for the slight increase in bond length due to zero-point vibrational motion even in the ground state. The value of 𝐡~0 is typically slightly less than 𝐡~𝑒 because the average bond length is longer due to the vibrations
75
𝐡~1
This is the rotational constant for the first vibrational excited state (v=1). The bond length further increases when the molecule is vibrationally excited, leading to an even larger moment of inertia and thus a smaller rotational constant compared to 𝐡~0
76
Fundamental band
the transition from the ground vibrational state (v=0) to the first excited vibrational state (v=1) in a molecule. This is the most basic and usually the most intense absorption band observed in vibrational spectroscopy.
77
Hot bands
transitions that originate from vibrationally excited states higher than the ground state. These transitions occur when a molecule that is already in an excited vibrational state (v=1, v=2, etc.) absorbs additional energy and transitions to an even higher vibrational state (v=2β†’v=3, v=3β†’v=4, etc.) energy difference of hΞ½