Atomic and Nuclear Phenomena Flashcards

You may prefer our related Brainscape-certified flashcards:
1
Q

photoelectric effect

A
  • when a sufficiently high frequency light (usually blue-UV) is incident on a metal in a vacuum, the metal atoms emit electrons
  • these freed electrons will then produce a net charge flor per unit time, a current
  • greater light beam intensity (amplitude) above threshold produce larger current, greater photons fall in electrode and greater liberated electrons
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
2
Q

threshold frequency

A
  • fT
  • depends on metal type
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
3
Q

energy of a photon

A

E = hf

h: 6.626 x 10^-34 J•s

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

kinetic energy of ejected electrons

A

Kmax = hf - W

  • only achieved when all possible energy from the photon is transferred to the ejected electron
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
5
Q

Work function of an electron

A

W = hfT

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

fluorescence

A
  • upon excitation of a fluorescent substance w UV radiation it will begin to glow in visible light
  • when electrons returns to original state in 2 or more steps, each step involves less energy and thus the photon emitted has lower frequency than UV absorbed
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
7
Q

mass defect of the nucleus

A

E = mc^2

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

mass defect is the result of…

A
  • matter that has been converted to energy
  • a very small amount of mass will yield a huge amount of energy
  • 1 TJ = 10^12 J
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
9
Q

nucleons and strong nuclear force

A

protons + neutrons

  • attracted to one another by a strong nuclear force, compensates for the repulsive electromagnetic force between protons
  • acts over extremely short distances
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
10
Q

binding energy

A
  • bonded system at a lower energy level than unbonded
  • allows the nucleons to bind together in the nucleus
  • the amount of mass that is transformed into dissipated energy will be a measurable fraction of the initial total mass
  • binding energy per nucleon peaks at iron (most stable nucleus)
  • intermediate sized nuclei are more stable than very large or small nuclei
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
11
Q

weak nuclear force

A
  • also contributes to the stability of the nucleus
  • but it’s about one millionth a strong as the strong nuclear force
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
12
Q

fusion

A
  • small nuclei combine to form a larger nucleus
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
13
Q

fission

A
  • large nucleus split into smaller nuclei
  • rarely occurs spontaneously
  • absorption of low energy neutron, fission can be induced in certain nuclei
  • of special interest are fission reactions that release more neutrons because these other neutrons will cause a chain reaction in which other nearby atoms can undergo fission; this in then releases more neutrons, continuing the chain rxn
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
14
Q

radioactive decay

A
  • spontaneous decay of certain nuclei accompanied by the emission of specific particles
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
15
Q

balancing nuclear reactions…

A

sum if atomic numbers must be same on both sides

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

alpha decay

A
  • emission of an a-particle, which is
    4
    2 He
  • do not penetrate shielding
  • very massive compared to beta particle and carrie’s double the charge
17
Q

beta decay

A
  • emission of a B-particle
  • an electron e-
  • emitted when a neutron decays into a p+, a B-particle, and an antineutrino

(A Z) X ~> (A [Z+1]) Y + B-

  • in some cases of induced decay (positron emission), positron released e+ as well as a neutrino

(A Z) X ~> (A [Z-1]) Y + B+

18
Q

gamma decay

A
  • emission of gamma rays (high freq photons)
  • carry no charge
  • simply lower energy of parent nucleus

(A Z) X* ~> (A Z) X + g

19
Q

electron capture

A
  • reverse of B- decay
  • unstable radionuclides are capable of capturing an inner electrons that combines with a proton to form a neutron
    (A Z) X + e- ~> (A [Z-1]) Y
20
Q

half-life T1/2

A
  • time it takes for half of a radioactive sample to decay

half life 4 years, 12 years later
12/4 = 3
(1/2)^3 = 1/8 of the sample remains

21
Q

rate of nuclei decay

A

delta n/delta t = - (decay constant) • n

n: number of radioactive nuclei that have not yet decayed in a sample

22
Q

exponential decay

A

n = n0 e ^ (- decay constant • t)

e: 2.72

23
Q

exponential decay rearranged to give decay constant

A

decay constant = ln2/half-life = 0.693/half-life