PHB - Term 4 (E1, E3) Flashcards

(24 cards)

1
Q

Define Isotope

A

Nuclei that have the same number of protons but different numbers of neutrons

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2
Q

Define Binding Energy

A

The energy required to break a nucleus into its constituent protons and neutrons

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3
Q

Define Half-Life

A

The time taken for half the undecayed nuclei to decay or the activity of a source to decay by half

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4
Q

Thomson Model

A

Also known as the plum pudding model of the atom. Positive charge (dough) with negative electrons

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5
Q

Geiger-Marsden-Rutherford experiment

A

Alpha particles fired at a thin sheet of gold foil. Discovered the existence of the nucleus, small, dense, positive

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6
Q

eV to J

A

1eV to 1.6x10^-19 J

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7
Q

Change in energy in Atomic Transitions

A

ΔE = Ei - Ef

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8
Q

Define eV

A

The kinetic energy an electron gains when it accelerated across a potential difference of 1V

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9
Q

Discrete emission spectrum

A

Because energy levels are discrete, photons emitted by gases only have discrete energies equal to the differences between atomic energy levels. E=hc/λ

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10
Q

Define Photons

A

‘Packets’ of electromagnetic energy, discrete quantity

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11
Q

What does the frequency in E=hf show

A

The frequency of photons emitted when de-excitation occurs

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12
Q

Atomic Transitions in relation to the light spectrum

A

n=x -> n=1 is ultraviolet || n=x -> n=2 is visible light || n=x -> n=3 is infrared

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13
Q

The emission spectrum

A

Hydrogen gas is excited it will emit photons with specific energies/wavelengths. Consists of bright emission lines on dark backgrounds

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14
Q

The absorption spectrum

A

Shine a white light on hydrogen gas, absorbs the photons with energies that correspond to the possible atomic transitions. Consists of dark lines on a bright bg

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15
Q

What is Background Radiation

A

The ionising radiation present in the environemtn

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16
Q

Alpha Decay (4)

A

(4,2)α || High energy helium nucleus || emitted by Large unstable nucleus || Highly ionising, least penetrating

17
Q

Beta-Minus Decay (4)

A

(0,-1) β || High energy electron || emitted by unstable nuclei with too many neutrons || Neutrons turn into a proton with an anti neutrino

18
Q

Beta-Plus Decay (4)

A

(0,+1) β || High energy positron || emitted by unstable nuclei with too many protons || Proton turns into neutron with a positive neutrino

19
Q

Gamma Radiation (4)

A

(0,0)γ || High energy electromagnetic radiation || Emitted by nuclei that need to lose energy || Weakly ionising and highest penetrating

20
Q

Ionisation

A

Damages or Destroys Cells, increased exposure may cause illness or death

21
Q

Mass-Energy equivalence

A

E = mc^2
m = mass defect (kg)

22
Q

u –> kg

A

1u = 1.661x10^-27 kg

23
Q

Define Mass Defect

A

m = Total mass of individual nucleons(u) - mass of nucleus

24
Q

Strong force range

A

Strong Force < 0.5 fm ==> Repulsive
0.5 < Strong Force < 3 ==> Attractive
0.5 = Equilibrium