ch 9 - Atomic and Nuclear Phenomena Flashcards

1
Q

photoelectric effect

A

when light of high frequency (blue to ultraviolet light) is incident on a metal in a vacuum, the metal atoms emit electrons; an “all or nothing” response

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

current

A

created by electrons liberated from the metal by the photoelectric effect that produce a net charge flow per unit time

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

threshold frequency (f sub T)

A

minimum frequency of light that causes ejection of electrons and depends on the type of metal being exposed to radiation

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

f

A

if frequency of incident photon is less than the threshold frequency then no electron will be ejected because the photons do not have sufficient energy to dislodge the e- from its atom

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

f>f sub T

A

If the frequency of incident photon is greater than the threshold frequency then an e- will be ejected and the maximum kinetic energy of the ejected e- will be equal to the difference between hf and hf sub T (also called the work function)

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

energy of photon equation

A

E=hf; where E is energy of the photon of light, h is Planck’s constant (6.626 x 10^-34 Jxs); f = frequency of the light

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

nanometer

A

1 nm = 10^-9 m

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

angstroms

A

1 A = 10^-10 m

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

max kinetic energy of the ejected e- equation

A

K sub max = hf - W; where h = Planck’s constant, f = frequency of the light, W = work function of the metal in question

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

work function related to threshold frequency of a certain metal, equation

A

work function is the min energy required to eject an electron and is related to the threshold frequency by W = hf sub T; where W = work function of the metal in question; h = Planck’s constant; f sub T = threshold frequency

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

infrared (IR) spectroscopy

A

used to determine chemical structure because different bonds will absorb different wavelengths of light

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

UV-Vis spectroscopy

A

looks at the absorption of light in the visible and ultraviolet range

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

note about indicators

A

most contain large organic compounds that have very different absorption patterns based solely on the protonation state of the compound. often have conjugated double bonds or aromatic ring systems which permit the absorption of light from photons in the visible range

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

fluorescence

A

if a fluorescent substance is excited (such as a ruby, emerald or phosphors in fluorescent lights) with uv radiation, it will begin to glow with visible light; it is a stepwise photon emission in which an excited e- returns to the ground state through one or more intermediate excited states in which each step emits a photon

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

mass defect

A

difference between the weight of the sum of protons and neutrons inside a nucleus and the actual weight of the nucleus which is slightly smaller

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

equation embodying mass defect

A

E = mc^2; E = energy; m = mass and c = the speed of light; this is a result of matter that has been converted to energy

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

strong nuclear force

A

force attaching protons and neutrons together to form the nucleus; strong enough to more than compensate for the repulsive electromagnetic force between the protons; acts over very short distances only

18
Q

binding energy

A

energy that is radiated away from the nucleus in the form of heat, light or other electromagnetic radiation before the mass defect becomes apparent; allows the nucleons to bind together in the nucleus

19
Q

weak nuclear force

A

also contributes to stability of the nucleus, but is one-millionth as strong as the strong nuclear force

20
Q

Four fundamental forces of nature

A

strong nuclear force, weak nuclear force, electrostatic forces and gravitation

21
Q

isotopic notation

A

notation in which elements are preceded by their atomic number as a subscript and mass number as a superscript

22
Q

atomic number (Z)

A

corresponds to number of protons in nucleus

23
Q

mass number (A)

A

corresponds to number of protons plus neutrons

24
Q

fusion

A

occurs when small nuclei combine to form a larger nucleus

25
Q

Fission

A

process by which a large nucleus splits into smaller nuclei; powers most nuclear power plants

26
Q

radioactive decay

A

naturally occurring spontaneous decay of certain nuclei accompanied by emission of specific particles

27
Q

Example of isotope decay arithmetic and nucleon conservation

A

X represents parent nucleus, Y represents daughter nucleus: (superscript A, subscript Z)X -> superscript A’, subscript Z’)Y + emitted decay particle; when balancing, sum of atomic numbers and mass numbers (separately) must be the same on both sides

28
Q

Alpha decay

A

emission of an alpha-particle which is a (superscript 4, subscript 2)He nucleus that consists of two protons, two neutrons, and zero electrons; carries double charge of beta-particle and is much bigger; interact with matter very easily and do not penetrate shielding very extensively

29
Q

balanced equation example of alpha decay

A

(superscript A, subscript Z)X -> (superscript A-4, subscript Z - 2)Y + (superscript 4, subscript 2)alpha

30
Q

Beta decay

A

emission of the beta-particle which is an electron and is given the symbol e- or beta-; electrons do not reside in nucleus but are emitted by the nucleus when a neutron decays into a proton, a beta-particle, and an antineutrino (v with a line over it); more penetrating and much smaller (electron is 1836 times smaller than proton) than alpha-particle

31
Q

positron emission

A

induced decay

32
Q

positron

A

has mass of an electron but is positively charged: symbol is e+ or beta+; a neutrino (v) is emitted in positron decay

33
Q

balanced equation example of beta- decay

A

(superscript A, subscript Z)X -> (superscript A, subscript Z + 1)Y + beta-; neutron is converted to electron so atomic number will be one more

34
Q

example equation of beta+ decay

A

proton is converted into a neutron and beta+ particle is emitted: (superscript A, subscript Z)X -> (superscript A, subscript Z-1)Y + beta+

35
Q

gamma decay

A

emission of gamma-rays which are high-energy (high-frequency) photons which carry no charge and simply lower the energy of the parent nucleus without changing the mass number or atomic number

36
Q

expression equation of gamma decay

A

(superscript A, subscript Z)X -> (superscript A, subscript Z)X + gamma

37
Q

electron capture

A

certain unstable radionuclides are capable of capturing an inner electron that combines with a proton to form a neutron, while releasing a neutrino. Atomic number is one less than the original but mass number remains the same; rare process best thought of as the reverse of beta- decay

38
Q

expression of electron capture

A

(superscript A, subscript Z)X + e- -> (superscript A, subscript Z-1)Y

39
Q

half-life (T sub 1/2)

A

in a sample of radioactive particles this is the time it takes for half of the sample to decay, in each subsequent half-life, one-half of the remaining sample decays so that the remaining amount asymptotically approaches zero

40
Q

exponential decay equation

A

delta n/delta t = -(sign for wavelength)n; sign for wavelength = known as decay constant; solution tells us how the number of radioactive nuclei changes with time

41
Q

exponential decay equation

A

n = n sub 0 x e (to the power of -wavelength sign (decay constant) x t); n sub 0 = number of undecayed nuclei at time t = 0

42
Q

decay constant is related to the half-life by this equation

A

decay constant (upside down y) = (ln2)/(T sub 1/2) = (0.693)/(T sub 1/2)