Classical Physics Comprehensive Exam Flashcards

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Comprehensive vocabulary flashcards covering the full curriculum of a classical physics lecture series, from mechanics and thermodynamics to modern physics and relativity.

Last updated 8:57 PM on 6/20/26
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123 Terms

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Right-handed coordinate system

A convention for x, y, and z axes where curling right-hand fingers from positive x toward positive y results in the thumb pointing toward positive z, ensuring consistent cross products like x^×y^=z^\hat{x} \times \hat{y} = \hat{z}.

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Cartesian coordinates

A rectilinear system specifying points by perpendicular distances (x, y, z) from a fixed origin, ideal for rectangular geometries.

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Polar coordinates

A curvilinear 2D system describing a point by its radial distance rr from the origin and the angle θ\theta from the positive x-axis.

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Scalar quantity

A quantity described by a single real number and a unit, possessing magnitude but no direction, such as mass or temperature.

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Vector quantity

A quantity requiring both magnitude and direction for complete specification, such as velocity or force.

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Dot product (scalar product)

A vector operation result in a scalar defined as AB=ABcos(θ)\mathbf{A} \cdot \mathbf{B} = |A||B|\cos(\theta), representing the projection of one vector onto another.

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Cross product (vector product)

A vector operation resulting in a vector perpendicular to both inputs, defined as A×B=ABsin(θ)n^\mathbf{A} \times \mathbf{B} = |A||B|\sin(\theta) \mathbf{\hat{n}}.

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Instantaneous velocity

The limit of average velocity as the time interval reaches zero, mathematically defined as the derivative of position: v(t)=drdt\mathbf{v}(t) = \frac{d\mathbf{r}}{dt}.

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Instantaneous acceleration

The limit of average acceleration as the time interval reaches zero, defined as a(t)=dvdt=d2rdt2\mathbf{a}(t) = \frac{d\mathbf{v}}{dt} = \frac{d^2\mathbf{r}}{dt^2}.

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Unit vector

A dimensionless vector with a magnitude of exactly 11 used to specify a direction, such as x^\mathbf{\hat{x}}, y^\mathbf{\hat{y}}, and z^\mathbf{\hat{z}} in Cartesian space.

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Inertial reference frame

A non-accelerating coordinate system in which Newton's First Law holds true.

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Uniform circular motion

Motion along a circular path at constant speed, resulting in a continuously changing velocity direction and a center-seeking acceleration.

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Centripetal acceleration

Acceleration directed toward the center of a circular path, with magnitude ac=v2r=ω2ra_c = \frac{v^2}{r} = \omega^2 r.

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Radian

The SI unit of angle defined as the ratio of arc length to radius (θ=sr\theta = \frac{s}{r}), where one full revolution equals 2π2\pi rad.

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Non-contact forces (field forces)

Forces that act over a distance mediated by fields, such as gravity, electrostatics, and magnetism.

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Newton's First Law (Inertia)

An object at rest remains at rest and an object in motion continues at constant velocity unless acted upon by a net external force.

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Newton's Second Law

The net force on an object equals the rate of change of its linear momentum, or F=ma\sum \mathbf{F} = m\mathbf{a} for constant mass.

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Newton's Third Law

For every action force, there is an equal and opposite reaction force acting simultaneously on a different object.

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Inertia

The intrinsic tendency of matter to resist changes in its state of motion, quantitatively measured by inertial mass.

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Normal force

The contact force exerted by a surface perpendicular to itself, arising from electromagnetic repulsion between atoms at the interface.

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Atwood's machine

A device with two masses connected by a string over a pulley, used to study uniform acceleration with the formula a=(m2m1)gm1+m2a = \frac{(m_2 - m_1)g}{m_1 + m_2}.

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Static friction (fsf_s)

A reactive contact force that prevents surfaces from sliding, reaching a maximum of fs,max=μsNf_{s,max} = \mu_s N.

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Kinetic friction (fkf_k)

A contact force opposing relative motion between sliding surfaces, equal to fk=μkNf_k = \mu_k N, where μk<μs\mu_k < \mu_s.

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Normal (Gaussian) distribution

A symmetric bell-shaped probability distribution defined by mean μ\mu and standard deviation σ\sigma, following the 68-95-99.7 rule.

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Extrapolation

The process of estimating a function's value at a point outside the range of measured data, assuming the established trend continues.

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Least squares method

A mathematical technique to find the best-fit model for data by minimizing the sum of the squares of the residuals (errors).

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Centrifugal force

A fictitious (pseudo) force in a rotating reference frame directed radially outward from the axis of rotation.

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Conical pendulum

A pendulum bob revolving in a horizontal circle such that the string traces a cone, where the period is T=2πLcos(θ)gT = 2\pi \sqrt{\frac{L\cos(\theta)}{g}}..

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Banked curve

A roadway tilted toward the center of a curve to provide an inward component of the normal force to assist centripetal acceleration.

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Drag force

A resistive force from a fluid directed opposite to motion, often defined as Fdrag=12ρCdAv2F_{drag} = \frac{1}{2} \rho C_d A v^2 for high-speed flows.

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Terminal velocity

The constant speed reached by a falling object when the upward drag force equals the downward force of gravity (vt=2mgρCdAv_t = \sqrt{\frac{2mg}{\rho C_d A}}).

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Universal Gravitation

Newton's law stating every particle attracts every other particle with a force F=Gm1m2r2F = \frac{G m_1 m_2}{r^2}, where G=6.674×1011Nm2/kg2G = 6.674 \times 10^{-11} N \cdot m^2/kg^2.

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Shell Theorem

A theorem stating a uniform spherical mass attracts external objects as if all its mass were at its center and exerts zero net gravitational force on objects inside.

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Geostationary orbit

A circular equatorial orbit with a period of 24 hours, keeping a satellite above a fixed point on Earth at approximately 35,78635,786 km altitude.

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Weightlessness

The condition of microgravity experienced in free fall, where no normal contact forces are present despite the presence of gravity.

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Kepler's Second Law

A line joining a planet and the Sun sweeps out equal areas in equal time intervals due to conservation of angular momentum.

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Kepler's Third Law (Harmonic Law)

The square of a planet's orbital period is proportional to the cube of its semi-major axis: T2a3T^2 \propto a^3.

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Lagrange Point L1

An unstable equilibrium point between two primary masses where the gravitational and centrifugal forces on a smaller object balance.

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Gauss's Law for Gravity

An integral law stating the gravitational flux through a closed surface is proportional to the enclosed mass: gdA=4πGMenc\oint \mathbf{g} \cdot d\mathbf{A} = -4\pi G M_{enc}.

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Work

The scalar energy transfer to an object by a force acting over a displacement, defined as W=Fd=Fdcos(θ)W = \mathbf{F} \cdot \mathbf{d} = |F||d|\cos(\theta) for constant force.

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Hooke's Law

The linear relationship for springs stating the restoring force is proportional and opposite to displacement: Fs=kxF_s = -kx.

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Kinetic Energy (KEKE)

The energy of an object due to its motion, defined as KE=12mv2KE = \frac{1}{2} m v^2 for translation.

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Work-Energy Theorem

The net work done on a particle equals the change in its kinetic energy: Wnet=ΔKEW_{net} = \Delta KE.

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Gravitational potential energy (UgravU_{grav})

The energy stored based on position in a gravitational field, given as mghmgh near Earth or GMmr-\frac{GMm}{r} for large distances.

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Elastic potential energy (UelasticU_{elastic})

The energy stored in a deformed elastic object, defined for a spring as U=12kx2U = \frac{1}{2} k x^2.

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Conservative force

A force where the work done between two points is path-independent and the work around a closed loop is zero, such as gravity or spring forces.

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Mechanical energy

The sum of the kinetic and potential energies of a system (Emech=KE+UE_{mech} = KE + U).

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Escape velocity

The minimum speed required for an object at the surface of a planet to escape its gravitational pull, defined as vesc=2GMRv_{esc} = \sqrt{\frac{2GM}{R}}.

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Power

The rate at which energy is transferred or work is done, measured in Watts (W=J/sW = J/s) and defined as P=dWdt=FvP = \frac{dW}{dt} = \mathbf{F} \cdot \mathbf{v}.

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Linear momentum (p\mathbf{p})

A vector quantity defined as the product of an object's mass and velocity: p=mv\mathbf{p} = m\mathbf{v}.

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Elastic collision

A collision where both the total linear momentum and total kinetic energy of the system are conserved.

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Perfectly inelastic collision

A collision where momentum is conserved but the maximum possible kinetic energy is lost as the objects stick together.

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Tsiolkovsky Rocket Equation

An equation relating rocket velocity change to exhaust velocity and the ratio of initial to final mass: Δv=veln(M0Mf)\Delta v = v_e \ln\left(\frac{M_0}{M_f}\right).

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Impulse (\mathbf{J})

The integral of force over time, equal to the change in an object's linear momentum: J=Fdt=Δp\mathbf{J} = \int \mathbf{F} dt = \Delta \mathbf{p}.

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Ballistic pendulum

A device used to measure bullet speed using momentum conservation during the inelastic collision and energy conservation during the subsequent swing.

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Center of mass (CM)

The unique point representing the average position of all the mass in a system, which moves as if all external forces were applied there.

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Angular velocity (ω\omega)

The rate of change of angular position, measured in rad/s: ω=dθdt\omega = \frac{d\theta}{dt}.

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Torque (\mathbf{\tau})

The rotational analog of force measuring the tendency to cause rotation, defined as τ=r×F\mathbf{\tau} = \mathbf{r} \times \mathbf{F}.

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Moment of inertia (II)

The measure of an object's resistance to angular acceleration, defined for a collection of particles as miri2\sum m_i r_i^2.

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Parallel Axis Theorem

A theorem used to find the moment of inertia about any axis parallel to one through the center of mass: I=Icm+Md2I = I_{cm} + Md^2.

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Rolling without slipping

A condition linking translation and rotation where the contact point is at rest relative to the surface (vcm=Rωv_{cm} = R\omega).

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Angular momentum (\mathbf{L})

The rotational analog of linear momentum, defined for a rigid body as L=Iω\mathbf{L} = I\mathbf{\omega} and for a point mass as r×p\mathbf{r} \times \mathbf{p}.

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Fictitious forces

Apparent forces in non-inertial frames such as centrifugal, Coriolis, and Euler forces, which are proportional to the object's mass.

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Coriolis force

A fictitious force in a rotating frame acting on a moving object, given by Fc=2m(Ω×v)\mathbf{F}_c = -2m(\mathbf{\Omega} \times \mathbf{v}'), causing deflections in paths.

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Static equilibrium

A state where both the net external force and net external torque on a rigid body are zero (F=0\sum \mathbf{F} = 0 and τ=0\sum \mathbf{\tau} = 0).

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Young's Modulus (EE)

The measure of a material's stiffness under tension or compression, defined as the ratio of tensile stress to longitudinal strain: E=F/AΔL/LE = \frac{F/A}{\Delta L/L}.

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Bulk Modulus (BB)

The measure of a material's resistance to uniform compression, defined as B=VdPdVB = -V \frac{dP}{dV}.

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Pascal's Principle

A pressure change applied to an enclosed static fluid is transmitted undiminished to every point in the fluid and the container walls.

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Archimedes' Principle

The upward buoyant force on an object submerged in a fluid equals the weight of the fluid it displaces (FB=ρfluidVdispgF_B = \rho_{fluid} V_{disp} g).

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Viscosity (η\eta)

The measure of a fluid's internal resistance to flow (friction between layers), typically decreasing with temperature in liquids and increasing in gases.

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Equation of Continuity

A statement of mass conservation for fluids: ρ1A1v1=ρ2A2v2\rho_1 A_1 v_1 = \rho_2 A_2 v_2, which for incompressible fluids simplifies to A1v1=A2v2A_1 v_1 = A_2 v_2.

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Bernoulli's Equation

Conservation of energy for an ideal fluid along a streamline: P+12ρv2+ρgh=constantP + \frac{1}{2} \rho v^2 + \rho gh = \text{constant}.

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Torricelli's Theorem

The speed of fluid exiting a small hole at depth hh from a large tank is v=2ghv = \sqrt{2gh}, equivalent to free-fall speed.

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Magnus effect

The generation of a sideward force on a spinning object moving through air due to pressure differences created by asymmetric airflow.

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Surface tension (\gamma)

The force per unit length trying to minimize a liquid's surface area due to unbalanced cohesive forces at the interface.

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Capillary action

The spontaneous rise or fall of a liquid in a narrow tube driven by the competition between adhesion and cohesion.

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Brownian motion

The random jiggling of microscopic particles in a fluid caused by unbalanced molecular bombardment, providing proof of atoms.

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Wien's Displacement Law

The blackbody law stating the wavelength of maximum emission is inversely proportional to absolute temperature: λmaxT=2.898×103mK\lambda_{max} T = 2.898 \times 10^{-3} m \cdot K.

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Stefan-Boltzmann Law

The law stating the total power radiated by a blackbody is proportional to the fourth power of its absolute temperature: P=σAT4P = \sigma A T^4.

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Ideal gas

A theoretical gas consisting of point-like molecules with zero volume that undergo perfectly elastic collisions and have no intermolecular forces.

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Kinetic theory of gases

A framework relating macroscopic properties like pressure and temperature to microscopic molecular motion, showing avg KE=32kBT\text{avg } KE = \frac{3}{2} k_B T.

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Maxwell-Boltzmann distribution

A probability distribution characterizing the speeds of molecules in a gas at a specific temperature.

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Triple point

The specific temperature and pressure at which the solid, liquid, and gas phases of a substance coexist in equilibrium.

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Fick's First Law

The principle that diffusion flux is proportional to the negative concentration gradient: J=DdCdxJ = -D \frac{dC}{dx}.

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Conduction

Heat transfer via direct molecular interaction without bulk matter motion, governed by Fourier's Law (dQdt=kAdTdx\frac{dQ}{dt} = -kA \frac{dT}{dx}).

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Specific heat capacity (cc)

The amount of heat required to raise the temperature of 1 kg of a substance by 1 K without a phase change (Q=mcΔTQ = mc\Delta T).

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Latent heat (LL)

The heat required per unit mass to change the phase of a substance at constant temperature (Q=mLQ = mL).

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Internal energy (UU)

The total microscopic energy of a system, including all molecular kinetic and potential energies, depending only on temperature for ideal gases.

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Zeroth Law of Thermodynamics

A fundamental law stating that if two systems are each in thermal equilibrium with a third, they are in equilibrium with each other, defining temperature.

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First Law of Thermodynamics

The conservation of energy for thermodynamic systems: ΔU=QW\Delta U = Q - W, where QQ is heat added and WW is work done by the system.

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Second Law of Thermodynamics

The law stating the total entropy of an isolated system never decreases, defining the direction of spontaneous processes.

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Entropy (SS)

A state function quantifying disorder or microscopic configurations, defined as dS=δQrevTdS = \frac{\delta Q_{rev}}{T} or S=kBln(Ω)S = k_B \ln(\Omega).

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Carnot efficiency

The maximum possible efficiency for a heat engine operating between two temperatures: η=1TCTH\eta = 1 - \frac{T_C}{T_H}..

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Equipartition theorem

The principle that each active quadratic degree of freedom in a molecules contributes 12kBT\frac{1}{2} k_B T to the internal energy.

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Simple Harmonic Motion (SHM)

Periodic oscillation where the restoring force is directly proportional to displacement (F=kxF = -kx), resulting in sinusoidal motion.

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Damped oscillations

Oscillatory motion where a dissipative force like friction causes the amplitude to decay exponentially over time.

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Resonance

The phenomenon where a system oscillates with maximum amplitude when driven at its natural frequency.

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Transverse wave

A wave where the medium oscillates perpendicular to the direction of energy propagation, such as waves on a string or light.

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Longitudinal wave

A wave where the medium oscillates parallel to the direction of propagation, such as sound waves.

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Principle of Superposition

The rule that the resultant displacement of two overlapping waves is the algebraic sum of their individual displacements.