chapter 3: vocab and definitions Flashcards

1
Q

electromagnetic radiation

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

wave

A

regular oscillation in some particular property (position in the case of ocean waves)

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

frequency

A

number of waves crests passing a point in space in one second

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

wavelength

A

distance between successive wave crests

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

speed of light (c)

A

2.9979 * 10^8 m/s

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

photoelectric effect

A

electrons ejected from metal when light of sufficient energy hits it

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

photon

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

E of a photon

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

Planck’s constant

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

continuous spectrum

A

contains all wavelengths of visible light

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

line spectrum

A

each line corresponds to a discrete wavelength

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

rydberg-balmer equation

A

predicts the series of lines in an emission

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

the bohr model of the hydrogen atom

A

structural model in which an electron moves around the nucleus only in circular orbits, each with a specific allowed radius

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

what equation do you use to calculate the energy level of an electron transitioning from one energy level to another?

A

E = -2.178 * 10^18 J (1/nfinal^2 - 1/ninitial^2)

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

absorption spectra

A

observed when sample irradiated with electromagnetic radiation transitions when electrons jump from low to higher energy states

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

dual nature of light

A

wave properties and particulate properties

17
Q

heisenberg’s uncertainty principle

A

momentum and position of particle-wave cannot be simultaneously known; the position of a moving electron cannot be precisely defined because they’re delocalized (spread out waves)

18
Q

3d waves

A

orbitals (3 dimensional volume)

19
Q

shape of an orbital represents

A

region of electron density around the nucleus

20
Q

each orbital can hold

A

2 electrons max

21
Q

n - principle quantum number

A

describes orbital energy and indicates distance of e- from nucleus

22
Q

l - secondary quantum number

A

describes energy and shape of orbital; ranges from 0 to n-1

23
Q

m of l - magnetic quantum number

A

describes orientation of orbital; ranges from +l to -l

24
Q

m of s - spin quantum number

A

designates spin orientation of electron, “up” or “down”; can be +1/2 or -1/2

25
Q

pauli exclusion principle

A

in a given atom no two electrons can have the same set of four quantum numbers; electrons in an orbital have opposite spins

26
Q

polyelectronic atoms

A

atoms with more than one electron

27
Q

variations in nuclear charge and number of electrons

A

change the magnitudes of the electrical forces that hold electrons in their orbitals

28
Q

higher nuclear charge

A

higher attraction

29
Q

shielding and penetration effect

A

electrons are shielded from nuclear charge by repulsion of other electrons

30
Q

electron configuration

A
31
Q

aufbau principle

A

as protons are added one by one to nucleus to build up elements, electrons similarly added to hydrogen–like orbitals

32
Q

guidelines for atomic ground states

A
  1. each electron in an atom occupies most stable available orbital
  2. no two electrons can have identical descriptions
  3. orbital capacities are as follow
    s - 2 electrons p - 6 electrons d - 10 electrons f - 14 electrons
  4. higher n, less stable orbital
  5. for equal n, the higher l, the less stable orbital
33
Q

hund’s rule

A

the lowest energy configuration for an atom is the one having the maximum number of unpaired electrons allowed by Pauli principle in a particular set of degenerate orbitals

34
Q

valence electrons

A

electrons in the outermost principal quantum level of atom

35
Q

continuous spectrum

A

electromagnetic radiation given off in an unbroken series of wavelengths

36
Q

standing wave

A

localized wave phenomenon characterized by discrete wavelengths determined by the boundary conditions used to generate the waves; standing waves are inherently quantized