AAPT NCPT (Level 1) flashcards
AAPT NCPT (Level 1) · Build recall with a focused review session.
33 cards. Read the term and the definition here. The deck at the top of this page is optional.
- Newton's second law
- The net force on an object equals its mass times its acceleration. It holds only in inertial reference frames and relates force, mass, and acceleration vectorially.
- Centripetal acceleration
- An object moving in a circle of radius r at speed v has acceleration v²/r directed toward the center. Speed may be constant while velocity changes direction.
- Conservation of momentum
- If the net external impulse on a system is zero, total momentum stays constant. This applies component by component and underlies collision analysis.
- Elastic collision
- A collision in which both momentum and kinetic energy are conserved. Objects bounce apart; in perfectly inelastic collisions they stick and lose maximum kinetic energy.
- Simple harmonic motion
- Oscillation with restoring acceleration proportional to displacement and opposite in direction, a = −ω²x. Angular frequency is √(k/m) for springs and √(g/L) for pendulums.
- First law of thermodynamics
- The change in internal energy equals heat added to the system minus work done by the system: ΔU = Q − W, with signs defined by the chosen convention.
- Ideal gas law
- Relates pressure, volume, and temperature: PV = nRT = NkT. It assumes negligible molecular volume and no intermolecular forces.
- Root-mean-square speed
- The typical molecular speed v_rms = √(3kT/m). At equal temperatures, lighter molecules have higher rms speeds than heavier ones.
- Adiabatic process
- A process with no heat exchange, Q = 0, so ΔU = −W. For an ideal gas, PV^γ remains constant, with γ = C_p/C_v.
- Carnot efficiency
- The maximum possible efficiency of a heat engine operating between hot and cold reservoirs: η = 1 − T_c/T_h, using absolute temperatures. No real engine exceeds it.
- Wave speed relation
- For any periodic wave, speed equals frequency times wavelength, v = fλ. On a stretched string, v also equals √(T/μ).
- Standing waves on a string
- A string fixed at both ends supports frequencies f_n = nv/(2L). The fundamental has one antinode; each higher harmonic adds one more antinode.
- Snell's law
- Refraction obeys n₁ sinθ₁ = n₂ sinθ₂. Light bends toward the normal entering a higher-index medium and away from it entering a lower-index medium.
- Total internal reflection
- Occurs when light travels from higher to lower refractive index at angles beyond the critical angle, where sinθ_c = n₂/n₁. No refracted ray emerges.
- Thin lens equation
- Relates focal length, object distance, and image distance: 1/f = 1/d_o + 1/d_i. Magnification is m = −d_i/d_o; negative m indicates an inverted image.
- Double-slit interference
- Bright fringes occur where path difference d sinθ = mλ. Fringe spacing on a distant screen is approximately λL/d.
- Coulomb's law
- The force between point charges is kq₁q₂/r², directed along the line joining them. Like charges repel, opposite charges attract.
- Electric field definition
- Electric field is force per unit charge, E = F/q, pointing in the direction a positive test charge would be pushed. Field lines never cross.
- Ohm's law and power
- For ohmic resistors, V = IR. Power dissipated can be written P = IV = I²R = V²/R, useful when one quantity is fixed.
- Series and parallel resistors
- Series resistances add: R_eq = ΣR, with common current. Parallel conductances add: 1/R_eq = Σ1/R, with common voltage across branches.
- Kirchhoff's rules
- The junction rule states charge is conserved at nodes; the loop rule states total voltage change around any closed loop is zero. Together they solve circuits.
- Magnetic force on moving charge
- A charge q moving at velocity v in field B feels force qvB sinθ, perpendicular to both v and B. It does no work and cannot change speed.
- Faraday's law of induction
- An induced emf equals the negative rate of change of magnetic flux, −dΦ_B/dt. Lenz's law sets the induced current direction to oppose the flux change.
- Photon energy
- A photon carries energy E = hf = hc/λ. Using hc ≈ 1240 eV·nm quickly gives photon energies for visible and ultraviolet light.
- Photoelectric effect
- Electrons eject from a metal when light exceeds a threshold frequency. Maximum kinetic energy is K_max = hf − φ, where φ is the work function.
- de Broglie wavelength
- Matter has an associated wavelength λ = h/p. Higher momentum means shorter wavelength, observable for electrons but negligible for macroscopic objects.
- Radioactive half-life
- The time for half of a sample to decay, t₁/₂ = ln2/λ ≈ 0.693/λ. Activity follows N = N₀e^(−λt) and decreases by half each half-life.
- Mass-energy equivalence
- Mass and energy are related by E = mc². Nuclear reactions convert small mass differences into energy, with 1 u equivalent to about 931.5 MeV.
- Bohr energy levels
- Hydrogen levels follow E_n = −13.6 eV/n². A transition emits or absorbs a photon whose energy equals the level difference.
- Accuracy versus precision
- Accuracy measures closeness to the true value; precision measures repeatability among trials. Systematic errors hurt accuracy, while random errors limit precision.
- Propagation of uncertainty
- For sums, absolute uncertainties add in quadrature. For products and quotients, fractional uncertainties add in quadrature to give the result's fractional uncertainty.
- Standard error of the mean
- The spread of an average is s/√N, where s is the sample standard deviation and N the number of trials. Averaging reduces random error by √N.
- Systematic error
- A consistent bias that shifts measurements in one direction, such as miscalibration or zero offset. It is not reduced by repeated trials and requires correction or recalibration.