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Vocabulary flashcards covering core physics concepts, key formulas, constants, and theoretical principles across classical mechanics, electrodynamics, quantum mechanics, thermodynamics, relativity, and laboratory methods.
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Coefficient of static friction for a block on a ramp
The minimum coefficient of static friction μ required to keep a block in place on a ramp inclined at angle θ is μ=tan(θ).
Free-body diagram
A diagram where each individual block and only the forces acting on it are drawn, preventing double-counting and ensuring proper application of Newton's third law.
Massless string (GRE definition)
A string that carries the same tension at every point.
Kinematics equations for 2D projectile motion
Equations giving position as a function of time under constant acceleration g acting in the negative y-direction: x(t)=v0xt+x0 and y(t)=−21gt2+v0yt+y0.
One-dimensional constant acceleration formula
The formula relating initial velocity vi, final velocity vf, constant acceleration a, and displacement Δx: vf2−vi2=2aΔx.
Radial acceleration (Uniform circular motion)
The inward radial acceleration experienced by a particle moving in a circular path of radius r with constant speed v, given by a=rv2.
Centripetal force
The net radially inward force required to keep an object of mass m moving in a circular path of radius r at constant speed v, given by F=rmv2.
Conservation of energy
Principle stating that if an object is acted on only by conservative forces, the sum of its kinetic and potential energies is constant along its path.
Conservative force
A force for which the work done is independent of the path taken between starting and ending points, allowing an associated time-independent potential energy.
Translational kinetic energy
Energy of linear motion given by 21mv2.
Rotational kinetic energy
Energy of rotational motion given by 21Iω2, where I is the moment of inertia and ω is angular velocity.
Gravitational potential energy (Earth's surface)
Potential energy given by mgh, where m is mass, g is gravitational acceleration, and h is height above a chosen zero reference level.
Spring potential energy
Energy stored in a stretched or compressed spring with spring constant k and displacement x, given by 21kx2.
Potential energy change (ΔU)
The change in potential energy between points a and b for a conservative force F, defined as ΔU=−∫abF⋅dl.
Gravitational force magnitude
The attractive force between two masses m1 and m2 separated by distance r, given by Fgrav=r2Gm1m2.
Gravitational potential energy (Two point masses)
Potential energy of a mass m at distance r from mass M, defined with zero at infinity as U(r)=−rGmM.
Force from potential energy
The relation computing force from a potential energy function U, given by F=−∇U.
Rolling without slipping condition
The kinematic relationship between linear velocity v and angular velocity ω for an object of radius R rolling without slipping: v=Rω.
Work-energy theorem
Principle relating initial energy, work done by nonconservative forces Wother, and final energy: Einitial+Wother=Efinal, or W=ΔKE.
Conservation of linear momentum
Principle stating that linear momentum is always conserved in a system in the absence of external forces.
Elastic collision
A collision in which the total initial and final kinetic energies of the system are equal.
Angular momentum (Point particle)
Vector quantity defined by L=r×p, where r is the position vector from a reference point and p is linear momentum.
Angular momentum (Extended body)
Quantity defined as L=Iω, where I is the moment of inertia and ω is angular velocity.
Torque
Rotational analogue of force, defined by τ=r×F, or scalar relation τ=dtdL.
Centrifugal force
A fictitious apparent force in a uniformly rotating frame that pushes objects away from the axis of rotation, given by Fcentrifugal=−mΩ×(Ω×r) or magnitude mΩ2r.
Coriolis force
A fictitious force appearing in a rotating reference frame acting on a moving object, given by FCoriolis=−2mΩ×v.
Moment of inertia (Point particle)
Measure of rotational inertia for a point particle of mass m at radius r from the rotation axis, given by I=mr2.
Moment of inertia (Continuous mass distribution)
Integral definition I=∫r2dm=∫r2ρdV, where r is the perpendicular distance from the axis of rotation to the mass element.
Parallel axis theorem
Theorem stating that the moment of inertia I about any axis parallel to an axis through the center of mass is I=ICM+Mr2, where r is the distance between the two axes and M is total mass.
Center of mass (Continuous object)
Position vector defined by rCM=M∫rdm.
Lagrangian ($L$)
A scalar function describing a mechanical system, defined as L(q,q˙,t)=T−U, where T is kinetic energy and U is potential energy.
Euler-Lagrange equations
Equations of motion derived from the Lagrangian L for each generalized coordinate q: dtd(∂q˙∂L)=∂q∂L.
Conjugate momentum ($p_i$)
Momentum corresponding to generalized coordinate qi, defined by pi≡∂q˙i∂L.
Cyclic coordinate
A generalized coordinate q that does not explicitly appear in the Lagrangian (∂q∂L=0), implying its conjugate momentum pi is conserved.
Hamiltonian ($H$)
Scalar function defined via Legendre transformation as H(p,q)=∑ipiq˙i−L, equal to total energy T+U when U is velocity- and time-independent.
Hamilton's equations of motion
Coupled first-order differential equations of motion: p˙=−∂q∂H and q˙=∂p∂H.
Central potential
A potential function U(r) that depends only on the radial distance r between two interacting bodies.
Effective potential (Orbital mechanics)
Equivalent 1D potential for radial motion in a central force field, given by V(r)=2mr2l2+U(r), where l is angular momentum.
Reduced mass (μ)
Effective single-body mass for a two-body system, defined as μ=m1+m2m1m2.
Kepler's First Law
Statement that planets move in elliptical orbits with the Sun at one focus (or more precisely, orbiting their mutual center of mass).
Kepler's Second Law
Statement that planetary orbits sweep out equal areas in equal times, expressing conservation of angular momentum (areal velocity).
Kepler's Third Law
Statement that the square of the orbital period T is proportional to the cube of the semi-major axis a (T2∝a3).
Hooke's Law
Restoring force equation for a spring displaced by x from equilibrium: F=−kx.
Natural angular frequency (Harmonic oscillator)
Angular frequency of oscillation for a mass m on a spring with constant k, given by ω0=mk.
Normal modes
Independent collective modes of oscillation of a system where all parts oscillate at the same fixed normal frequency.
Damped harmonic oscillator equation
Equation of motion mx¨+bx˙+kx=0, categorized into underdamped, critically damped, and overdamped regimes based on damping parameter β=2mb and natural frequency ω0=mk.
Resonant frequency (Driven damped oscillator)
The driving frequency that maximizes steady-state amplitude, given by ωR=ω02−2β2.
Simple pendulum angular frequency
Small-angle oscillation frequency for a simple pendulum of length L, given by ω=Lg.
Physical pendulum angular frequency
Small-angle oscillation frequency for an extended object of mass m, moment of inertia I about pivot, and CM distance R, given by ω=ImgR.
Equivalent spring constants
For parallel springs, keq=k1+k2; for series springs, keq1=k11+k21.
Bernoulli's principle
Statement that along a streamline of an incompressible fluid, 2v2+gz+ρp=constant.
Buoyant force (Archimedes' principle)
Upward force exerted on a submerged object equal to the weight of the displaced fluid: Fbuoyant=ρVg.
Gauss's Law (Electrostatics)
Maxwell equation stating ∇⋅E=ε0ρ, or in integral form ∮SE⋅dS=ε0Qenc.
Electric potential ($V$)
Scalar field defined such that E=−∇V, or V(b)−V(a)=−∫abE⋅dl.
Poisson's and Laplace's equations
Differential equations for electric potential V: Poisson's equation is ∇2V=−ε0ρ, and Laplace's equation (in empty space) is ∇2V=0.
Electric field of an infinite charged sheet
Uniform electric field produced by a flat sheet with surface charge density σ: E=2ε0σ, pointing normal to the sheet.
Electric field of an infinite line charge
Radial electric field at distance r from an infinite line of linear charge density λ: E=2πε0rλ.
Electrostatic boundary conditions
Conditions across a charged surface: parallel electric field is continuous (E∥out−E∥in=0), perpendicular electric field is discontinuous (E⊥out−E⊥in=ε0σ), and potential V is continuous.
Ideal conductor properties
Potential V is constant throughout, E=0 inside, bulk charge density ρ=0, net charge resides on the surface, and E just outside is perpendicular to the surface.
Method of images
Technique for solving electrostatic boundary value problems by replacing conducting surfaces with virtual image charges that reproduce the boundary conditions.
Electrostatic field energy
Total energy stored in an electric field: UE=2ε0∫∣E∣2d3r.
Capacitance ($C$)
Constant of proportionality relating charge and potential difference on conductors: Q=CV.
Parallel-plate capacitance
Capacitance of two plates of area A separated by distance d: C=dε0A.
Energy stored in a capacitor
Energy given by UC=21CQ2=21CV2.
Ampère's Law (Magnetostatics)
Maxwell equation stating ∇×B=μ0J, or in integral form ∮CB⋅dl=μ0Ienc.
Magnetic vector potential (A)
Vector field defined such that ∇×A=B.
Lorentz force law
Force on a test charge q moving with velocity v in electric and magnetic fields: F=q(E+v×B).
Biot-Savart law
Formula for magnetic field produced by a current element: B(r)=4πμ0I∫r′2dl×r^′.
Magnetic field of an infinite straight wire
Field at distance r from an infinite wire carrying current I: B=2πrμ0I, directed azimuthally.
Magnetic field of a solenoid
Uniform magnetic field inside an infinite solenoid with n turns per unit length carrying current I: B=μ0nI.
Magnetic field of a toroid
Field inside a toroid with N total turns carrying current I at radius r: B=2πrμ0NI.
Magnetostatic boundary conditions
Normal magnetic field is continuous (B⊥out−B⊥in=0), parallel magnetic field is discontinuous (B∥out−B∥in=μ0∣K×n^∣).
Magnetostatic field energy
Energy stored in a magnetic field: UB=2μ01∫∣B∣2d3r.
Cyclotron radius and frequency
For a charge q with mass m moving at speed v⊥ perpendicular to magnetic field B: radius R=qBmv⊥ and cyclotron frequency Ω=mqB.
Faraday's Law of Induction
Maxwell equation stating ∇×E=−∂t∂B, or in terms of electromotive force E=−dtdΦB.
Lenz's law
Principle stating that induced currents flow in a direction such that the magnetic field they produce opposes the change in magnetic flux.
Self-inductance ($L$)
Proportionality constant between magnetic flux and current in a circuit (ΦB=LI), yielding induced emf E=−LdtdI.
Energy stored in an inductor
Energy stored in the magnetic field of an inductor: UL=21LI2.
Electric dipole moment (p)
Vector defined for two equal and opposite charges ±q separated by displacement d as p=qd, pointing from negative to positive charge.
Electric dipole torque and energy
In external field E: torque N=p×E and potential energy U=−p⋅E.
Magnetic dipole moment (m)
Vector for a planar loop carrying current I with area vector A defined by m=IA; torque in field B is N=m×B and potential energy is U=−m⋅B.
Dielectric constant (κ)
Factor by which permittivity increases in a material: ε=κε0, increasing capacitance of a parallel-plate capacitor to C=κdε0A.
Speed of light in vacuum ($c$)
Constant relation defined by c=ε0μ01.
Poynting vector (S)
Vector representing energy flux (power per unit area) of an electromagnetic wave: S=μ01(E×B).
Larmor formula
Total power radiated by a nonrelativistic accelerating point charge q with acceleration a: P=6πε0c3q2a2.
Electric dipole radiation power
Time-averaged power radiated by an oscillating electric dipole p(t)=p0cos(ωt)z^: ⟨P⟩E=12πcμ0p02ω4.
Kirchhoff's Rules
Circuit laws: (1) Node rule (charge conservation): ∑kIk=0; (2) Loop rule (energy conservation): ∑kVk=0.
RC and RL time constants
Characteristic response times: τRC=RC for RC circuits, and τRL=RL for RL circuits.
LC circuit resonant frequency
Natural angular frequency of an LC circuit: ω0=LC1.
One-dimensional wave equation
Differential equation ∂t2∂2f=v2∂x2∂2f, with general solutions f(x±vt).
Phase velocity and Group velocity
For a wave with dispersion relation ω(k), phase velocity is vphase=kω and group velocity is vgroup=dkdω.
Malus's Law
Transmitted intensity of polarized light passing through a polarizer at angle θ relative to its polarization direction: I=I0cos2(θ).
Brewster's angle (θB)
Angle of incidence at which reflected light is completely polarized perpendicular to the incident plane: θB=arctan(n1n2).
Double-slit interference conditions
For slit distance d and angle θ: maxima at dsin(θ)=mλ and minima at dsin(θ)=(m+21)λ.
Single-slit diffraction minima
Minima occur at asin(θ)=mλ for m=1,2,3,…, where a is slit width.
Optical path length
Equivalent path length in vacuum for light traveling distance d in medium of index n: OPL=nd.
Thin-film reflection phase shift rules
Reflection off a boundary with n2>n1 undergoes a phase shift of π; reflection off a boundary with n2<n1 undergoes no phase shift.
Rayleigh criterion (Circular aperture)
Resolution limit for a circular aperture of diameter D: first minimum occurs at Dsin(θ)=1.22λ.
Bragg diffraction condition
Condition for constructive interference of x-rays scattered from crystal planes separated by distance d at incidence angle θ: 2dsin(θ)=nλ.
Thin lens equation
Relation between object distance s, image distance s′, and focal length f: s1+s′1=f1.