Particles Flashcards

1
Q

Alpha decay

A

The process of an unstable nucleus emitting an alpha particle to become more stable. Usually in nuclei that have too much mass.

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2
Q

Annihilation

A

The process of a particle and antiparticle colliding and being converted into energy. The energy is released in two photons moving in opposite directions to conserve momentum. The rest mass energy of the particle and antiparticle pair is converted into energy of the photons. Need to show particles convert to 2 photons of equal energy and the relationship, E=hf

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3
Q

Antiparticle

A

All particles have a corresponding antiparticle with the same mass but opposite charge and conservation numbers.

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4
Q

Baryon number

A

quantum number that is conserved in all particle interactions.
Baryons have a baryon number of +1 and non-baryons have a baryon number of 0.

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5
Q

Beta-Minus Decay

A

The process of a neutron inside a nucleus turning into a
proton, and emitting a beta-minus particle (an electron) and a antineutrino.

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6
Q

Beta-Plus Decay

A

The process of a proton inside a nucleus turning into a
neutron, and emitting a beta-plus particle (a positron) and a neutrino.

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7
Q

Electron Diffraction

A

The spreading of electrons as they pass through a gap
similar to the magnitude of their de Broglie wavelength. It is evidence of the
wave-like properties of particles.

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8
Q

Electron-volt (eV)

A

The work done to accelerate an electron through a potential difference of 1V. 1eV is equal to the charge of an electron (E=qv).

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9
Q

Energy Levels

A

Defined and distinct energies at which electrons can exist in an
atom. An electron cannot exist between energy levels.

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10
Q

Excitation

A

The process of an electron taking in exactly the right quantity of
energy to move to a higher energy level.

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11
Q

Gauge Boson

A

The exchange particles that transmit the four fundamental
interactions between particles.

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12
Q

Ground State

A

The most stable energy level that an electron can exist in.

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13
Q

Hadrons

A

A class of subatomic particle that experiences the strong nuclear
interaction.

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14
Q

Ionisation

A

The process of an atom losing an orbital electron and becoming
charged.

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15
Q

Isotope:

A

Same number of protons but different numbers of neutrons.

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16
Q

Isotopic Data

A

Data from isotopes that can be used for a purpose, such as carbon dating.

17
Q

Kaon

A

A type of meson that decays into pions.

18
Q

Lepton Number

A

A quantum number that is conserved in all particle interactions. Both electron lepton numbers and muon lepton numbers must be conserved

19
Q

Lepton

A

A group of elementary subatomic particles, consisting of electrons,
muons and neutrinos.

20
Q

Meson

A

A class of hadron that is made up of a quark and antiquark pair.

21
Q

Muon

A

A type of lepton that decays into electrons.

22
Q

Neutrino

A

A subatomic particle whose existence was hypothesised to maintain the conservation of energy in beta decay

23
Q

Nucleon Number (A)

A

The sum of the number of protons and neutrons in a given nucleus.

24
Q

Nucleon

A

A proton or neutron

25
Q

Pair Production

A

The process of a sufficiently high-energy photon converting into a particle and its corresponding antiparticle. To conserve momentum, this usually occurs near a nucleus.

26
Q

Photon

A

A packet of energy

27
Q

Pion

A

A type of meson and the exchange particle for the strong nuclear force.

28
Q

Positron

A

A positively charged particle that is the antiparticle of an electron.

29
Q

Proton Number (Z)

A

The number of protons present in the nucleus of a given
element.

30
Q

Stopping Potential

A

The minimum potential difference required to stop the
highest kinetic energy electrons from leaving the metal plate in the photoelectric effect.

31
Q

Strange Particles

A

Particles that are produced through the strong interaction but decay through the weak interaction.

32
Q

Strangeness

A

A quantum number that is conserved in strong interactions but not in weak interactions. This reflects that strange particles are always produced in pairs.

33
Q

Strong Nuclear Force

A

A force that acts between nucleons in a nucleus to keep it stable. It is attractive at distances of up to 3fm and repulsive at separations less than 0.5fm.

34
Q

Threshold Frequency

A

The minimum frequency of photons required for photoelectrons to be emitted from the surface of a metal plate through the
photoelectric effect. It is equal to the metal’s work function divided by Planck’s constant.

35
Q

Work Function

A

The minimum energy required to remove an electron from a
metal’s surface.