Atomic and Nuclear Phenomena Flashcards

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1
Q

the photoelectric effect

A

the ejection of an electron from the surface of a metal in response to light, normally high frequency light

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2
Q

current

A

net charge flow per unit time

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3
Q

threshold frequency f(t)

A

the minimum light frequency necessary to eject an electron from a given metal; depends on the type of metal being exposed to the radiation

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4
Q

energy of a photon of light

A

E=hf

E=energy of the photon of light
h=Planck’s constant (6.626 x 10^-34 J s)
f= is the frequency of the light

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5
Q

maximum kinetic energy of an electron in the photoelectric effect

A

Kmax=hf-W

W=work function of the metal in question

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6
Q

work function

A

the minimum energy required to eject an electron and is related to threshold frequency of that metal

W=h(f(t))

f(t)= threshold frequency

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7
Q

fluorescence

A

occurs when a species absorbs high-frequency light and then returns to its ground state in multiple steps; each step has less energy than the absorbed light and is within the visible range of the electromagnetic spectrum

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8
Q

mass defect

A

the difference between the mass of the unbounded nucleons and the mass of the bonded nucleons within the nucleus; the amount of mass converted to energy during nuclear fusion

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9
Q

mass defect and energy

A

E=mc^2

E=energy
m=mass contributed by the binding energy of the nucleus
c=speed of light

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10
Q

nucleons

A

protons and neutrons

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11
Q

what is the most stable kind of nucleus?

A

intermediate in size are the most stable (Iron), in comparison to small or large nuclei

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12
Q

binding energy

A

the energy that originated from mass defect, the energy released from protons and neutrons bind together

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13
Q

fusion

A

occurs when small nuclei combine into larger nuclei

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14
Q

fission

A

occurs when a large nucleus splits into smaller nuclei

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15
Q

why is energy released in fission and fusion

A

the nuclei formed in both processes are more stable then the starting nuclei

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16
Q

radioactive decay

A

the loss of small particles from the nucleus

17
Q

alpha decay

A

the emission of an alpha particle which is a helium nucleus, has zero electrons, 2 protons and 2 neutrons; carries double the charge of a beta particle and is much bigger; does not penetrate shielding

18
Q

beta-negative decay

A

the decay of a neutron into a proton, with emission of an electron and an antineutrino; more penetrating then alpha particles

19
Q

beta-positive decay

A

also called positron emission, the decay of a proton into a neutron, with emission of a positron (a particle with the size of an electron but with a positive charge) and a neutrino; more penetrating then alpha particles

20
Q

Gamma decay

A

the emission of a gamma ray, which converts a high-energy nucleus into a more stable nucleus

21
Q

electron capture

A

the absorption of an electron from the inner shell that combines with a proton in the nucleus to form a neutron

22
Q

half-life (T 1/2)

A

the amount of time required for half of a sample of radioactive nuclei to decay

23
Q

exponential decay

A

the rate at which radioactive nuclei decay is proportional to the number of nuclei that remain

n= (no)e^-(lambda)t

no= the number of undecayed nuclei at time t=0

24
Q

rate of nuclear decay

A

delta n/ delta t= -lambda(n)

n=number of radioactive nuclei that have not yet decayed in a sample
lambda= decay constant

25
Q

decay constant (lambda)

A

lambda= ln2/T-half= 0.693/T-half