Electronic Vocab 5 Flashcards

1
Q

Relatively small scale (0 – 100 cm-1) energy transitions corresponding to wavelengths in the microwave region of the spectrum; only shown by molecules possessing a permanent electrical dipole moment; pure rotational spectra are observed for gas phase molecules where it is possible to distinguish transitions between rotational quantum energy levels.

A

rotational energy transitions

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2
Q

Medium scale (100 – 3000 cm-1) energy transitions corresponding to wavelengths in the infrared region of the spectrum; shown by molecules in which a change in the permanent dipole moment occurs during the vibrational motion; also seen in Raman spectra where a ∂Q
deformation of the overall polarizability of the molecule occurs during the vibrational motion

A

vibrational energy transitions

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3
Q

Large scale (10,000 – 50,000 cm-1) energy transitions corresponding to wavelengths in the UV/Vis spectral regions; seen in all molecules since changes in electron distribution are always accompanied by a dipole change.

A

electronic energy transitions

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4
Q

Since the energies of electronic transitions are so large, vibrational and rotational transitions are also excited by electronic energy transitions; therefore, for molecules in the gas phase, vibrational transitions appear as “coarse structure” and rotational transitions appear as “fine structure” on top of electronic spectra

A

rotational-vibrational fine structure

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5
Q

Defined as the region of the electromagnetic spectrum less than 200 nm; corresponds to electronic energy transitions greater than 50,000 cm-1.

A

far or vacuum ultra-violet spectral region

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6
Q

Defined as the region of the electromagnetic spectrum between 200 – 400 nm; corresponds to electronic energy transitions between 50,000 – 25,000 cm-1.

A

near ultra-violet spectral region

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7
Q

Defined as the region of the near ultra-violet between 315 – 400 nm.

A

UV-A spectral region

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8
Q

Defined as the region of the near ultra-violet between 280 – 315 nm.

A

UV-B spectral region

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9
Q

Defined as the region of the near ultra-violet between 200 – 280 nm

A

UV-C spectral region

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10
Q

Defined as the region of the electromagnetic spectrum between 400 – 780 nm; corresponds to electronic energy transitions between 25,000 – 12,821 cm-1.

A

visible spectral region

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11
Q

The molecular orbital that acts as an electron donor, since it is the outermost, i.e., highest energy, frontier orbital containing an electron.

A

HOMO

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12
Q

The molecular orbital that acts as an electron acceptor, since it is the innermost, i.e., lowest energy, frontier orbital that has room to accept electrons.

A

LUMO

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13
Q

These electrons form single covalent bonds between atoms, e.g. C – C, C – H, O – H, etc.; the strongest type of covalent bonds due to the direct overlap of orbitals; electrons are the most firmly bound to nuclei and require the most energy to undergo electronic transitions.

A

σ - Electrons

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14
Q

These electrons form multiple covalent chemical bonds, e.g. C = C, C = N, etc.; result from overlap of atomic orbitals that are in contact through two areas of overlap; are more diffuse than sigma bonds

A

π - electrons

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15
Q

These electrons are non-bonding electrons that can populate non-bonding molecular orbitals; occur in atoms to the right of C in the periodic table, e.g. N, O, and halogens.

A

n - electrons

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16
Q

group of atoms, with their associated electrons, in a molecule that produces an electronic absorption.

A

chromophore

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17
Q

Substituent groups attached to the basic chromophore structure that change the position and/or intensity of the chromophore’s absorption band; typical examples include methyl, hydroxyl, alkoxyl, halogen, and amino groups

A

auxochromophore

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18
Q

A shift in the absorption maximum to longer wavelength or lower energy, i.e. a red shift

A

bathochromic shift

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19
Q

A shift in the absorption maximum to shorter wavelength or higher energy, i.e. a blue shift

A

hypsochromic shift

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20
Q

An increase in band intensity

A

hyperchromic shift

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21
Q

A decrease in band intensity.

A

hypochromic shift

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22
Q

a transition in which a bonding s electron is excited to an anti bonding sigma orbital; not generally analytically useful since their energies fall outside the normal UV-Vis spectral range

A

σ - σ* transition

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23
Q

Insertion of a group containing n-electrons; common for O, N, S, and halogen containing chromophores

A

n - σ* transition

24
Q

Promotion of an electron from a non-bonding molecular orbital to an anti-bonding orbital; common for heteroatom-containing molecules, e.g. O, N.

A

n - π* transition

25
Q

Promotion of one electron from a p bonding molecular orbital to a π* antibonding orbital; common in unsaturated molecules, e.g. C = C

A

π - π* transition

26
Q

a first approximation, the electronic, vibrational, and rotational energies of a molecule may be considered to be completely independent of one another

A

Born-Oppenheimer Approximation

27
Q

An electronic transition in a molecule takes place much more rapidly than does the vibrational motion of the nuclei in a bond vibration. Therefore, the internuclear distance in the vibrating molecule can be regarded as fixed, i.e. it does not change, during an electronic transition. Alternate definition: An electronic transition is more probable if it begins in the middle of the v”=0 level and terminates toward either end of an excited v’ vibrational level.

A

Frank-Condon Principle

28
Q

An excited state de-excitation process that results in the emission of radiation at a longer wavelength than that of the initial absorption; the initial excitation is caused by photons.

A

Photoluminescence

29
Q

An excited state de-excitation process that results in the emission of radiation at a longer wavelength than that of the initial excitation; the initial excitation is caused by high-energy particles.

A

radioluminescence

30
Q

An excited state de-excitation process that results in the emission of radiation at a longer wavelength than that of the initial excitation; the initial excitation is caused by a chemical process.

A

chemiluminescence

31
Q

The quantification of the amount of unpaired electron spin; equivalent to the total spin angular momentum

A

multiplicity

32
Q

The case for uncharged organic molecules in which all electrons are paired; in this case S, the total spin angular momentum quantum number is 0

A

singlet state

33
Q

The case for organic molecules in which an excited state electron has reversed its spin; in this case S, the total spin angular momentum quantum number is 1

A

triplet state

34
Q

singlet multiplicity defined as

A

2S + 1 = 2 x 0 + 1 = 1

35
Q

triplet state multiplicity defined as

A

2S + 1 = 2 x 1 + 1 = 3

36
Q

An energy diagram that illustrates the electronic states of a molecule and the transitions between them; the states are arranged vertically by increasing energy and grouped horizontally by spin multiplicity.

A

Jablonski Diagram

37
Q

A non-radiative means of dissipating excess vibrational energy in an excited electronic state; the excess energy is usually released as heat following collision with solvent molecules

A

vibrational relaxation

38
Q

A non-radiative process by which an excited state molecule passes from its original excited state to a lower energy excited state of the same multiplicity

A

internal conversion

39
Q

The radiative emission of energy from the first excited singlet state to the ground singlet state; i.e. the process of photon emission for de-excitation from S1 to S0 ; due to Boltzmann factors, the emission primarily occurs from the v’=0 vibrational level of S1; the time scale is 10-9 s.

A

fluorescence

40
Q

The electronic transition between the lowest vibrational levels of the ground and excited electronic states that has the same energy in both absorption and fluorescence; i.e. it is the transition between the v”=0 level in S0 and the v’=0 level in S1.

A

“0 - 0” transition

41
Q

A non-radiative de-excitation process that involves energy transfer between the excited state molecule and the solvent or other solute molecule.

A

external conversion

42
Q

A non radiative process in which the molecule in an excited electronic state changes its spin multiplicity from a singlet state to a triplet state that is lower in energy than the initial singlet state.

A

intersystem crossing

43
Q

The radiative emission of energy from the first excited triplet state to the ground singlet state; i.e. the process of photon emission for de-excitation from T1 ® S0 ; due to Boltzmann factors, the emission primarily occurs from the v’=0 vibrational level of T1; the time scale is much longer than that of fluorescence due to the long-lived, “spin-forbidden” T1 ® S0 transition, it can be on the order of 10-3 – 10 s

A

phosphorescence

44
Q

Any non-radiative de-excitation process that depopulates the S1 or T1 excited states and competes with fluorescence or phosphorescence;

A

quenching

45
Q

The difference in wavelength or energy between the position of the band maximum of the absorption band and the maximum of the fluorescence emission spectra; it is a measure of the change in geometry of the equilibrium configurations of the ground and excited states.

A

stokes loss or stokes shift

46
Q

The fraction of the total number of photons absorbed that result in fluorescence emission; can be considered a conversion factor between the rate of photon absorption and the rate of fluorescence emission.

A

fluorescence quantum yield

47
Q

The fluorescence spectrum that is observed as a function of scanning the excitation wavelength, with the emission wavelength held constant.

A

excitation spectrum

48
Q

The fluorescence spectrum that is observed as a function of scanning the emission wavelength, with the excitation wavelength held constant.

A

emission spectrum

49
Q

Fluorescence spectrum is observed as a three-dimensional representation or contour plot; shows the fluorescence signal as a function of both excitation and emission; also known as a total luminescence spectrum.

A

excitation-emission matrix

50
Q

The fluorescence spectrum that is observed by simultaneously scanning both the excitation and emission monochromators with a small wavelength difference between them.

A

synchronous spectrum

51
Q

i.e., excited state dimers; formed by the interaction of an excited singlet state with a ground state of an identical molecule; concentration increases as the monomer concentration increases; emission is red-shifted relative to monomer emission.

A

excimer

52
Q

i.e. excited state complexes; formed by the interaction of an excited singlet state with the ground state of a non-identical molecule

A

exciplex

53
Q

Quenching of fluorescence due to dynamic solution diffusion of quencher and collision with excited state fluorophore, thereby decreasing its excited state lifetime; examples include O2, H2O2, I2, NO, BrO4-, etc.

A

dynamic or collisional quenching

54
Q

Quenching of fluorescence due to formation of a ground state non-fluorescent complex between fluorophore and quencher; when this complex absorbs light, it returns to ground state without emission of fluorescence; examples include stacking interactions in purine and pyrimidine nucleotides

A

static quenching

55
Q

Quantitative linear relationship describing dynamic collisional quenching

A

Stern-Volmer equation