MSCE Physics flashcards
MSCE Physics · 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.
- SI base units
- Seven base units: meter, kilogram, second, ampere, kelvin, mole, candela. All other SI units derive from these by multiplication or division without numerical factors.
- Random versus systematic error
- Random error scatters readings unpredictably and shrinks with averaging. Systematic error shifts all readings in one direction and is corrected by calibration, not by more trials.
- Precision versus accuracy
- Precision is how closely repeated measurements agree with each other. Accuracy is how close a measurement is to the accepted or true value. They are independent qualities.
- Falsifiability
- A scientific hypothesis must make predictions that could be shown false by observation or experiment. Claims that cannot be tested in principle fall outside empirical science.
- Kinematic equations
- For constant acceleration: v = v0 + at, x = x0 + v0t + ½at², and v² = v0² + 2a(x − x0). These fail when acceleration changes with time.
- Newton's second law
- The net force on an object equals its mass times acceleration, ΣF = ma. Acceleration points along the net force and is inversely proportional to mass.
- Static versus kinetic friction
- Static friction adjusts up to a maximum μsN and prevents sliding. Kinetic friction equals μkN and opposes motion once sliding begins, usually smaller than the static maximum.
- Centripetal acceleration
- An object moving in a circle at constant speed accelerates toward the center with magnitude v²/r. A net inward force, such as tension or gravity, must supply it.
- Work-energy theorem
- The net work done on an object equals its change in kinetic energy, W_net = ½mv² − ½mv0². Work is Fd cos θ, zero when force is perpendicular to displacement.
- Conservation of momentum
- If no net external force acts on a system, its total momentum stays constant. Momentum is a vector, so conservation applies separately to each spatial axis.
- Elastic collision
- A collision in which both momentum and kinetic energy are conserved. Billiard-ball collisions approximate this; objects separate after impact rather than sticking together.
- Impulse-momentum theorem
- Impulse equals the change in momentum, J = FΔt = Δp. Extending collision time with the same impulse lowers the peak force, as in airbags and crumple zones.
- Wave speed relation
- Wave speed equals frequency times wavelength, v = fλ. Frequency is fixed by the source; crossing into a new medium changes speed and wavelength but not frequency.
- Doppler effect
- Observed frequency increases when source and observer approach and decreases when they recede. The shift depends on relative motion along the line joining them.
- Snell's law
- n1 sin θ1 = n2 sin θ2, where n = c/v is the refractive index. Light entering a higher-index medium bends toward the normal and slows down.
- Total internal reflection
- Occurs only when light travels from higher to lower refractive index and the incidence angle exceeds the critical angle θc = arcsin(n2/n1). No light refracts out.
- Thin lens equation
- 1/f = 1/do + 1/di with magnification m = −di/do. Positive di gives a real image; negative di gives a virtual image on the same side as the object.
- Coulomb's law
- The electric force between two point charges is F = kq1q2/r², directed along the line joining them. Like charges repel and opposite charges attract.
- Series versus parallel circuits
- Series elements share one current and their resistances add. Parallel elements share one voltage and their conductances add, giving a smaller equivalent resistance.
- Kirchhoff's rules
- Junction rule: charge conservation, currents into a node sum to currents out. Loop rule: energy conservation, voltage changes around any closed loop sum to zero.
- Lenz's law
- An induced current flows in the direction that opposes the change in magnetic flux that produced it. This is the negative sign in Faraday's law.
- Magnetic force on a charge
- A charge moving in a magnetic field feels F = qvB sin θ, perpendicular to both velocity and field. A charge moving parallel to the field feels no force.
- Ideal gas law
- PV = nRT relates pressure, volume, moles, and absolute temperature; R ≈ 8.314 J/(mol·K). It assumes negligible molecular volume and no intermolecular forces.
- First law of thermodynamics
- ΔU = Q − W, where W is work done by the system. Internal energy changes by heat added minus work performed; it is a statement of energy conservation.
- Carnot efficiency
- The maximum possible efficiency of a heat engine is e = 1 − Tc/Th, using absolute temperatures. No real engine operating between those reservoirs can exceed it.
- Root-mean-square speed
- v_rms = √(3kT/m) = √(3RT/M), the typical molecular speed in an ideal gas. It rises with temperature and falls for heavier molecules.
- Time dilation
- A clock moving relative to an observer runs slow by Δt = γΔt0, where γ = 1/√(1 − v²/c²). The proper time Δt0 is measured in the clock's rest frame.
- Photoelectric effect
- Light ejects electrons only above a threshold frequency. Maximum kinetic energy is K_max = hf − φ, independent of intensity, supporting photon quantization.
- de Broglie wavelength
- Any particle with momentum p has wavelength λ = h/p. It is measurable for electrons and explains electron diffraction, but negligible for everyday objects.
- Half-life
- The time for half of a radioactive sample to decay, N = N0(1/2)^(t/T½). Decay is random per nucleus but statistically predictable for large numbers of nuclei.
- Binding energy per nucleon
- The energy holding a nucleus together divided by its nucleon count. It peaks near iron-56, so fusion releases energy for lighter nuclei and fission for heavier ones.
- Formative versus summative assessment
- Formative assessment monitors learning during instruction and guides feedback. Summative assessment evaluates achievement at the end of a unit or course.
- Laser safety classes
- Class 1 is safe under normal use. Class 2 visible lasers are protected by the blink reflex. Class 3B and 4 need wavelength-matched eye protection and controlled access.