Georgia Unified Physics flashcards
Georgia Unified Physics · 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.
- Centripetal acceleration
- For an object moving in a circle of radius r at speed v, acceleration has magnitude v²/r and points toward the center; it changes direction, not speed.
- Impulse-momentum theorem
- The impulse delivered to an object equals its change in momentum: FΔt = Δp. A longer collision time with the same impulse means a smaller average force.
- Conservation of mechanical energy
- When only conservative forces act, KE + PE stays constant. Falling objects trade gravitational potential energy mgh for kinetic energy ½mv², so v = √(2gh) from rest.
- Static versus kinetic friction
- Static friction adjusts up to μ_sN to prevent sliding; kinetic friction equals μ_kN while sliding. Because μ_s exceeds μ_k, starting motion takes more force than keeping it.
- Torque
- Torque about a pivot is τ = rF sinθ, where θ is the angle between the lever arm and the force. Maximum torque occurs when force is perpendicular to the lever arm.
- First law of thermodynamics
- ΔU = Q − W, where Q is heat added to the system and W is work done by the system. For an isochoric process W = 0, so ΔU equals Q.
- Carnot efficiency limit
- No heat engine operating between reservoirs at T_H and T_C can exceed e = 1 − T_C/T_H. Temperatures must be in kelvin, and real engines fall below this ceiling.
- Latent heat
- Energy absorbed or released during a phase change at constant temperature is Q = mL, where L is the specific latent heat. No temperature change occurs during melting or boiling.
- Adiabatic process
- A process with no heat exchange, Q = 0, so the first law gives ΔU = −W. Compressing a gas adiabatically raises its temperature; expanding it adiabatically cools it.
- Standing waves on a string
- Both ends fixed gives nodes at each end, so wavelengths are λ = 2L/n and frequencies f = nv/(2L). The n = 1 mode is the fundamental.
- Total internal reflection
- Occurs when light travels from a higher to a lower index and the incident angle exceeds the critical angle θ_c = sin⁻¹(n₂/n₁). The interface then reflects all light.
- Snell's law
- n₁sinθ₁ = n₂sinθ₂, with n = c/v for each medium. Entering a higher-index medium slows light and bends it toward the normal.
- Thin lens equation
- 1/f = 1/d_o + 1/d_i with magnification m = −d_i/d_o. A negative image distance for a lens means a virtual image on the object side.
- Double-slit interference
- Constructive interference occurs at d sinθ = mλ for integer m, producing bright fringes. Increasing slit separation d decreases fringe spacing on the screen.
- Ohm's law
- V = IR for an ohmic conductor at constant temperature. Power dissipated follows P = IV = I²R = V²/R, so doubling current quadruples resistive power loss.
- Parallel resistors
- The reciprocal of equivalent resistance is the sum of reciprocals: 1/R_eq = 1/R₁ + 1/R₂. Equivalent resistance is always less than the smallest individual resistor.
- Kirchhoff's loop rule
- Around any closed loop, the sum of potential changes is zero. This expresses energy conservation: charges returning to a point must have the same potential.
- Magnetic force on a charge
- F = qvB sinθ, perpendicular to both velocity and field. Because force is perpendicular to motion, magnetic fields do no work and cannot change speed.
- Faraday's law of induction
- Induced emf equals the negative rate of change of magnetic flux through a loop: ε = −NΔΦ/Δt. Faster flux change or more turns yields larger emf.
- Electric field of a point charge
- E = kq/r², directed away from positive charge and toward negative charge. Field magnitude falls off as the inverse square of distance.
- Photoelectric effect
- Electrons are ejected only when photon energy hf exceeds the work function φ. Maximum kinetic energy is K_max = hf − φ; intensity affects count, not energy.
- de Broglie wavelength
- Any particle with momentum p has wavelength λ = h/p. Electrons at typical laboratory speeds have wavelengths comparable to atomic spacing, enabling diffraction.
- Half-life
- The time for half of a radioactive sample to decay. After n half-lives, the remaining fraction is (1/2)ⁿ, and activity decreases by the same factor.
- Mass defect and binding energy
- A nucleus is lighter than its separated nucleons by Δm; the binding energy is Δm·c². Binding energy per nucleon peaks near iron-56, the most stable region.
- Alpha decay
- A nucleus emits a helium-4 nucleus, decreasing mass number by 4 and atomic number by 2. The daughter element sits two places left in the periodic table.
- Hydrogen energy levels
- E_n = −13.6 eV/n², with n = 1 the ground state. A photon is emitted when an electron drops to a lower level, carrying exactly the energy difference.
- Percent error
- Percent error = |measured − accepted|/|accepted| × 100, comparing a result to an accepted value. It is not the same as percent difference between two measurements.
- Linearizing a graph
- Plot a transformed variable so the relationship becomes a straight line, then use the slope to extract a constant. Example: T² versus L for a pendulum gives slope 4π²/g.
- Random versus systematic error
- Random error scatters readings in both directions and shrinks with averaging. Systematic error shifts all readings in one direction and is not reduced by averaging.
- Propagating uncertainty
- For adding or subtracting, add absolute uncertainties. For multiplying or dividing, add fractional uncertainties, then convert back to an absolute uncertainty.
- Significant figures in operations
- Multiplication and division results keep the fewest significant figures among inputs. Addition and subtraction results keep the fewest decimal places among inputs.
- Control of variables
- Only the independent variable is changed while all others are held constant, so any effect on the dependent variable can be attributed to the independent variable.