Physics 30 Diploma study materials
Physics 30 Diploma study resources

Physics 30 Diploma flashcards

Physics 30 Diploma · Build recall with a focused review session.

32 cards. Read the term and the definition here. The deck at the top of this page is optional.

Momentum
The product of an object's mass and velocity, p = mv. It is a vector quantity pointing in the direction of motion, measured in kg·m/s.
Impulse
The product of net force and the time interval over which it acts, J = FΔt. Impulse equals the change in momentum, measured in N·s.
Conservation of momentum
In an isolated system with no net external force, the total vector momentum before an interaction equals the total vector momentum after it.
Elastic collision
A collision in which both total momentum and total kinetic energy are conserved. Objects separate after impact with no permanent deformation or thermal energy loss.
Perfectly inelastic collision
A collision in which the objects stick together and move with one common velocity. Momentum is conserved but maximum kinetic energy is lost.
Work–energy theorem
The net work done on an object equals its change in kinetic energy: W_net = ΔKE = ½mv_f² − ½mv_i².
Coulomb's law
The electrostatic force between two point charges is F = kq1q2/r², proportional to the product of charges and inversely proportional to the square of their separation.
Electric field strength
The force per unit positive charge at a point, E = F/q, a vector pointing in the direction of force on a positive test charge.
Electric potential energy
The energy stored in a system of charges due to their positions; for two point charges, PE = kq1q2/r, negative for opposite charges.
Magnetic force on moving charge
A charge moving in a magnetic field experiences force F = qvB sinθ, perpendicular to both velocity and field; zero when motion is parallel to the field.
Magnetic force on a wire
A current-carrying conductor in a magnetic field experiences force F = BIL sinθ, maximum when the current is perpendicular to the field.
Electromagnetic induction
A changing magnetic flux through a loop induces an emf in the loop, described by Faraday's law; the induced current opposes the change by Lenz's law.
Magnetic flux
The product of magnetic field strength and the perpendicular area it passes through, Φ = BA cosθ, measured in webers (T·m²).
Faraday's law
The induced emf in a loop equals the negative rate of change of magnetic flux through it: ε = −NΔΦ/Δt.
Lenz's law
An induced current flows in a direction whose magnetic field opposes the change in flux that produced it, consistent with conservation of energy.
Accelerating voltage
A charge q accelerated through potential difference V gains kinetic energy qV; for electrons, qV = ½mv² determines final speed.
Millikan oil-drop experiment
Balanced charged oil droplets between horizontal plates so electric force equaled gravitational force, allowing measurement of the elementary charge e = 1.60 × 10⁻¹⁹ C.
Photon energy
The energy of a photon is E = hf = hc/λ, where h = 6.63 × 10⁻³⁴ J·s; shorter wavelength means higher energy.
Photoelectric effect
Light above a threshold frequency ejects electrons from a metal surface; maximum kinetic energy is K_max = hf − W, independent of intensity.
Work function
The minimum energy needed to remove an electron from a metal surface, W = hf₀, where f₀ is the threshold frequency.
de Broglie wavelength
Moving particles have wave character with wavelength λ = h/p = h/(mv), explaining electron diffraction and quantized atomic energy levels.
Bohr model transitions
An electron dropping from a higher to lower energy level emits a photon of energy E = E_i − E_f = hf; absorption requires a matching energy.
Line spectra
Atoms emit or absorb only specific photon energies, producing discrete spectral lines that serve as fingerprints of each element.
Mass–energy equivalence
Mass and energy are interchangeable through E = mc²; mass defect in a nucleus appears as released binding energy.
Binding energy
The energy required to separate a nucleus into its individual nucleons; it equals the mass defect times c², measured in MeV.
Alpha decay
A nucleus emits an alpha particle (helium-4 nucleus), decreasing mass number by 4 and atomic number by 2: (A,Z) → (A−4, Z−2) + α.
Beta negative decay
A neutron converts to a proton, emitting an electron and antineutrino; mass number unchanged, atomic number increases by one.
Gamma decay
An excited nucleus releases a high-energy photon without changing its mass number or atomic number; it accompanies other decays.
Half-life
The time for half the nuclei in a radioactive sample to decay; after n half-lives, remaining fraction is (½)ⁿ.
Activity
The decay rate of a radioactive sample, A = ΔN/Δt, measured in becquerels (decays per second); activity halves each half-life.
Refraction and Snell's law
Light bends when crossing between media: n₁ sinθ₁ = n₂ sinθ₂, where n = c/v is the index of refraction of the medium.
Total internal reflection
When light travels from denser to less dense medium beyond the critical angle θ_c = sin⁻¹(n₂/n₁), it reflects entirely back into the denser medium.