IB Physics Topic 5 Definitions

This page contains our IB Physics definitions for topic 5. By learning each one of these definitions, you will fully cover the content for IB Physics 'Nuclear & Quantum Physics'.
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absorption spectrum

It is the wavelengths of electromagnetic waves an atom can absorb

Antiparticles

This particle has the same mass as a normal particle but opposite charge and quantum number

Background radiation

It is the daily radiation one can be exposed to

Binding energy per nucleon

It is the ratio of nuclear binding energy to number of nucleons in a nucleus

Chandrasekhar Limit

The maximum mass of a white dwarf star (approximately 1.4 solar masses), beyond which it will collapse into a neutron star or black hole

Conditioning

The final step in nuclear waste management, involving encapsulating or solidifying waste in materials like cement, bitumen, or glass, and storing it in corrosion-resistant containers

Control Rods

Retractable rods that absorb neutrons to control the rate of the nuclear chain reaction

Emission spectrum

It is the wavelengths of electromagnetic waves an atom emits

Exchange particle

It is a particles that mediates a fundamental force

Fission

It is the splitting of a large nucleus into two smaller nuclei, releasing energy

Formation of an absorption spectrum

It is formed from the absorption of electromagnetic waves by electrons to jump to a higher energy level

Fusion

It is the joining of two nuclei to form a larger nucleus, releasing energy

Half-life

It is the amount of time for half of the atoms to decay

Hydrostatic Equilibrium

A balance between the outward radiation pressure from fusion reactions and the inward gravitational pull of the gases in a star

Ionizing radiation

It is radiation that it removes electrons from exposed matter

Ions

These are nuclides that have lost or gained electrons, gaining a positive or negative charge

Isotopes

These are nuclides with different numbers of neutrons, and thus different mass numbers

Jeans Criterion

A criterion determining when a cloud of gas will collapse to form a star, dependent on the mass, temperature, and density of the cloud

Mass defect

It is the difference in the mass of a nucleus and the sum of its constituent masses

Moderator

A material within the reactor that slows down neutrons to optimize their speed for successful nuclear reactions

Neutron Bombardment

The process of bombarding fuel rods with neutrons to initiate a fission reaction

Nuclear binding energy

It is the energy released by the production of a nucleus from its constituent nucleons

Nucleon

It is a particle in the nucleus

Nuclides

These are atoms of one element

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Photoelectric effect

It is the emission of electrons from a metal surface when UV light shines on it

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Quantum tunnelling

It is a particle's ability to escape its potential barrier without sufficient energy

Radiation

It is the emission of electromagnetic waves from an atom by electrons

Radioactive decay

It is the process of decomposition of unstable nuclei into lighter nuclei and emission of radiation

Radioactivity

It is the number of decays occurring per second

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Rutherford scattering

It is the prediction of the intensity of alpha particles from the angle of scattering at low energies

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Stable orbit

It is an orbit whereing the angular momentum is a multiple of h/2π

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Stopping potential

It is the voltage at which there is no electron emission

Supernova

A powerful explosion that occurs when a massive star exhausts its nuclear fuel and its core collapses

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Threshold frequency

It is the frequency of absorbed photon below which no electron is emitted

Unified atomic mass unit

It is defined as one twelfth the mass of a Carbon-12 atom

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Wave-particle duality

It is the property of sometimes behaving as a wave and sometimes behaving as a particle

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Work function

It is the minimum energy that electrons need to escape the metal surface

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