Classical Mechanics, Electromagnetism, Waves, Thermodynamics, Quantum Mechanics, Relativity, and Laboratory Methods Flashcards

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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.

Last updated 4:20 AM on 8/23/26
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141 Terms

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Coefficient of static friction for a block on a ramp

The minimum coefficient of static friction μ\mu required to keep a block in place on a ramp inclined at angle θ\theta is μ=tan(θ)\mu = \tan(\theta).

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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.

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Massless string (GRE definition)

A string that carries the same tension at every point.

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Kinematics equations for 2D projectile motion

Equations giving position as a function of time under constant acceleration gg acting in the negative y-direction: x(t)=v0xt+x0x(t) = v_{0x}t + x_0 and y(t)=12gt2+v0yt+y0y(t) = -\frac{1}{2}gt^2 + v_{0y}t + y_0.

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One-dimensional constant acceleration formula

The formula relating initial velocity viv_i, final velocity vfv_f, constant acceleration aa, and displacement Δx\Delta x: vf2vi2=2aΔxv_f^2 - v_i^2 = 2a\Delta x.

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Radial acceleration (Uniform circular motion)

The inward radial acceleration experienced by a particle moving in a circular path of radius rr with constant speed vv, given by a=v2ra = \frac{v^2}{r}.

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Centripetal force

The net radially inward force required to keep an object of mass mm moving in a circular path of radius rr at constant speed vv, given by F=mv2rF = \frac{mv^2}{r}.

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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.

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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.

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Translational kinetic energy

Energy of linear motion given by 12mv2\frac{1}{2}mv^2.

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Rotational kinetic energy

Energy of rotational motion given by 12Iω2\frac{1}{2}I\omega^2, where II is the moment of inertia and ω\omega is angular velocity.

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Gravitational potential energy (Earth's surface)

Potential energy given by mghmgh, where mm is mass, gg is gravitational acceleration, and hh is height above a chosen zero reference level.

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Spring potential energy

Energy stored in a stretched or compressed spring with spring constant kk and displacement xx, given by 12kx2\frac{1}{2}kx^2.

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Potential energy change (ΔU\Delta U)

The change in potential energy between points aa and bb for a conservative force F\mathbf{F}, defined as ΔU=abFdl\Delta U = -\int_a^b \mathbf{F} \cdot d\mathbf{l}.

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Gravitational force magnitude

The attractive force between two masses m1m_1 and m2m_2 separated by distance rr, given by Fgrav=Gm1m2r2F_{\text{grav}} = \frac{Gm_1m_2}{r^2}.

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Gravitational potential energy (Two point masses)

Potential energy of a mass mm at distance rr from mass MM, defined with zero at infinity as U(r)=GmMrU(r) = -\frac{GmM}{r}.

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Force from potential energy

The relation computing force from a potential energy function UU, given by F=U\mathbf{F} = -\nabla U.

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Rolling without slipping condition

The kinematic relationship between linear velocity vv and angular velocity ω\omega for an object of radius RR rolling without slipping: v=Rωv = R\omega.

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Work-energy theorem

Principle relating initial energy, work done by nonconservative forces WotherW_{\text{other}}, and final energy: Einitial+Wother=EfinalE_{\text{initial}} + W_{\text{other}} = E_{\text{final}}, or W=ΔKEW = \Delta \text{KE}.

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Conservation of linear momentum

Principle stating that linear momentum is always conserved in a system in the absence of external forces.

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Elastic collision

A collision in which the total initial and final kinetic energies of the system are equal.

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Angular momentum (Point particle)

Vector quantity defined by L=r×p\mathbf{L} = \mathbf{r} \times \mathbf{p}, where r\mathbf{r} is the position vector from a reference point and p\mathbf{p} is linear momentum.

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Angular momentum (Extended body)

Quantity defined as L=IωL = I\omega, where II is the moment of inertia and ω\omega is angular velocity.

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Torque

Rotational analogue of force, defined by τ=r×F\boldsymbol{\tau} = \mathbf{r} \times \mathbf{F}, or scalar relation τ=dLdt\tau = \frac{dL}{dt}.

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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)\mathbf{F}_{\text{centrifugal}} = -m\boldsymbol{\Omega} \times (\boldsymbol{\Omega} \times \mathbf{r}) or magnitude mΩ2rm\Omega^2 r.

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Coriolis force

A fictitious force appearing in a rotating reference frame acting on a moving object, given by FCoriolis=2mΩ×v\mathbf{F}_{\text{Coriolis}} = -2m\boldsymbol{\Omega} \times \mathbf{v}.

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Moment of inertia (Point particle)

Measure of rotational inertia for a point particle of mass mm at radius rr from the rotation axis, given by I=mr2I = mr^2.

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Moment of inertia (Continuous mass distribution)

Integral definition I=r2dm=r2ρdVI = \int r^2 \, dm = \int r^2 \rho \, dV, where rr is the perpendicular distance from the axis of rotation to the mass element.

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Parallel axis theorem

Theorem stating that the moment of inertia II about any axis parallel to an axis through the center of mass is I=ICM+Mr2I = I_{\text{CM}} + Mr^2, where rr is the distance between the two axes and MM is total mass.

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Center of mass (Continuous object)

Position vector defined by rCM=rdmM\mathbf{r}_{\text{CM}} = \frac{\int \mathbf{r} \, dm}{M}.

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Lagrangian ($L$)

A scalar function describing a mechanical system, defined as L(q,q˙,t)=TUL(q, \dot{q}, t) = T - U, where TT is kinetic energy and UU is potential energy.

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Euler-Lagrange equations

Equations of motion derived from the Lagrangian LL for each generalized coordinate qq: ddt(Lq˙)=Lq\frac{d}{dt}\left(\frac{\partial L}{\partial \dot{q}}\right) = \frac{\partial L}{\partial q}.

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Conjugate momentum ($p_i$)

Momentum corresponding to generalized coordinate qiq_i, defined by piLq˙ip_i \equiv \frac{\partial L}{\partial \dot{q}_i}.

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Cyclic coordinate

A generalized coordinate qq that does not explicitly appear in the Lagrangian (Lq=0\frac{\partial L}{\partial q} = 0), implying its conjugate momentum pip_i is conserved.

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Hamiltonian ($H$)

Scalar function defined via Legendre transformation as H(p,q)=ipiq˙iLH(p, q) = \sum_i p_i \dot{q}_i - L, equal to total energy T+UT + U when UU is velocity- and time-independent.

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Hamilton's equations of motion

Coupled first-order differential equations of motion: p˙=Hq\dot{p} = -\frac{\partial H}{\partial q} and q˙=Hp\dot{q} = \frac{\partial H}{\partial p}.

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Central potential

A potential function U(r)U(r) that depends only on the radial distance rr between two interacting bodies.

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Effective potential (Orbital mechanics)

Equivalent 1D potential for radial motion in a central force field, given by V(r)=l22mr2+U(r)V(r) = \frac{l^2}{2mr^2} + U(r), where ll is angular momentum.

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Reduced mass (μ\mu)

Effective single-body mass for a two-body system, defined as μ=m1m2m1+m2\mu = \frac{m_1 m_2}{m_1 + m_2}.

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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).

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Kepler's Second Law

Statement that planetary orbits sweep out equal areas in equal times, expressing conservation of angular momentum (areal velocity).

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Kepler's Third Law

Statement that the square of the orbital period TT is proportional to the cube of the semi-major axis aa (T2a3T^2 \propto a^3).

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Hooke's Law

Restoring force equation for a spring displaced by xx from equilibrium: F=kxF = -kx.

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Natural angular frequency (Harmonic oscillator)

Angular frequency of oscillation for a mass mm on a spring with constant kk, given by ω0=km\omega_0 = \sqrt{\frac{k}{m}}.

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Normal modes

Independent collective modes of oscillation of a system where all parts oscillate at the same fixed normal frequency.

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Damped harmonic oscillator equation

Equation of motion mx¨+bx˙+kx=0m\ddot{x} + b\dot{x} + kx = 0, categorized into underdamped, critically damped, and overdamped regimes based on damping parameter β=b2m\beta = \frac{b}{2m} and natural frequency ω0=km\omega_0 = \sqrt{\frac{k}{m}}.

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Resonant frequency (Driven damped oscillator)

The driving frequency that maximizes steady-state amplitude, given by ωR=ω022β2\omega_R = \sqrt{\omega_0^2 - 2\beta^2}.

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Simple pendulum angular frequency

Small-angle oscillation frequency for a simple pendulum of length LL, given by ω=gL\omega = \sqrt{\frac{g}{L}}.

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Physical pendulum angular frequency

Small-angle oscillation frequency for an extended object of mass mm, moment of inertia II about pivot, and CM distance RR, given by ω=mgRI\omega = \sqrt{\frac{mgR}{I}}.

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Equivalent spring constants

For parallel springs, keq=k1+k2k_{\text{eq}} = k_1 + k_2; for series springs, 1keq=1k1+1k2\frac{1}{k_{\text{eq}}} = \frac{1}{k_1} + \frac{1}{k_2}.

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Bernoulli's principle

Statement that along a streamline of an incompressible fluid, v22+gz+pρ=constant\frac{v^2}{2} + gz + \frac{p}{\rho} = \text{constant}.

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Buoyant force (Archimedes' principle)

Upward force exerted on a submerged object equal to the weight of the displaced fluid: Fbuoyant=ρVgF_{\text{buoyant}} = \rho V g.

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Gauss's Law (Electrostatics)

Maxwell equation stating E=ρε0\nabla \cdot \mathbf{E} = \frac{\rho}{\varepsilon_0}, or in integral form SEdS=Qencε0\oint_S \mathbf{E} \cdot d\mathbf{S} = \frac{Q_{\text{enc}}}{\varepsilon_0}.

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Electric potential ($V$)

Scalar field defined such that E=V\mathbf{E} = -\nabla V, or V(b)V(a)=abEdlV(b) - V(a) = -\int_a^b \mathbf{E} \cdot d\mathbf{l}.

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Poisson's and Laplace's equations

Differential equations for electric potential VV: Poisson's equation is 2V=ρε0\nabla^2 V = -\frac{\rho}{\varepsilon_0}, and Laplace's equation (in empty space) is 2V=0\nabla^2 V = 0.

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Electric field of an infinite charged sheet

Uniform electric field produced by a flat sheet with surface charge density σ\sigma: E=σ2ε0E = \frac{\sigma}{2\varepsilon_0}, pointing normal to the sheet.

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Electric field of an infinite line charge

Radial electric field at distance rr from an infinite line of linear charge density λ\lambda: E=λ2πε0rE = \frac{\lambda}{2\pi\varepsilon_0 r}.

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Electrostatic boundary conditions

Conditions across a charged surface: parallel electric field is continuous (EoutEin=0E_{\parallel}^{\text{out}} - E_{\parallel}^{\text{in}} = 0), perpendicular electric field is discontinuous (EoutEin=σε0E_{\perp}^{\text{out}} - E_{\perp}^{\text{in}} = \frac{\sigma}{\varepsilon_0}), and potential VV is continuous.

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Ideal conductor properties

Potential VV is constant throughout, E=0\mathbf{E} = 0 inside, bulk charge density ρ=0\rho = 0, net charge resides on the surface, and E\mathbf{E} just outside is perpendicular to the surface.

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Method of images

Technique for solving electrostatic boundary value problems by replacing conducting surfaces with virtual image charges that reproduce the boundary conditions.

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Electrostatic field energy

Total energy stored in an electric field: UE=ε02E2d3rU_E = \frac{\varepsilon_0}{2} \int |\mathbf{E}|^2 \, d^3r.

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Capacitance ($C$)

Constant of proportionality relating charge and potential difference on conductors: Q=CVQ = CV.

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Parallel-plate capacitance

Capacitance of two plates of area AA separated by distance dd: C=ε0AdC = \frac{\varepsilon_0 A}{d}.

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Energy stored in a capacitor

Energy given by UC=12Q2C=12CV2U_C = \frac{1}{2}\frac{Q^2}{C} = \frac{1}{2}CV^2.

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Ampère's Law (Magnetostatics)

Maxwell equation stating ×B=μ0J\nabla \times \mathbf{B} = \mu_0 \mathbf{J}, or in integral form CBdl=μ0Ienc\oint_C \mathbf{B} \cdot d\mathbf{l} = \mu_0 I_{\text{enc}}.

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Magnetic vector potential (A\mathbf{A})

Vector field defined such that ×A=B\nabla \times \mathbf{A} = \mathbf{B}.

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Lorentz force law

Force on a test charge qq moving with velocity v\mathbf{v} in electric and magnetic fields: F=q(E+v×B)\mathbf{F} = q(\mathbf{E} + \mathbf{v} \times \mathbf{B}).

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Biot-Savart law

Formula for magnetic field produced by a current element: B(r)=μ0I4πdl×r^r2\mathbf{B}(\mathbf{r}) = \frac{\mu_0 I}{4\pi} \int \frac{d\mathbf{l} \times \hat{\mathbf{r}}'}{r'^2}.

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Magnetic field of an infinite straight wire

Field at distance rr from an infinite wire carrying current II: B=μ0I2πrB = \frac{\mu_0 I}{2\pi r}, directed azimuthally.

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Magnetic field of a solenoid

Uniform magnetic field inside an infinite solenoid with nn turns per unit length carrying current II: B=μ0nIB = \mu_0 n I.

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Magnetic field of a toroid

Field inside a toroid with NN total turns carrying current II at radius rr: B=μ0NI2πrB = \frac{\mu_0 N I}{2\pi r}.

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Magnetostatic boundary conditions

Normal magnetic field is continuous (BoutBin=0B_{\perp}^{\text{out}} - B_{\perp}^{\text{in}} = 0), parallel magnetic field is discontinuous (BoutBin=μ0K×n^B_{\parallel}^{\text{out}} - B_{\parallel}^{\text{in}} = \mu_0 |\mathbf{K} \times \hat{\mathbf{n}}|).

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Magnetostatic field energy

Energy stored in a magnetic field: UB=12μ0B2d3rU_B = \frac{1}{2\mu_0} \int |\mathbf{B}|^2 \, d^3r.

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Cyclotron radius and frequency

For a charge qq with mass mm moving at speed vv_{\perp} perpendicular to magnetic field BB: radius R=mvqBR = \frac{m v_{\perp}}{qB} and cyclotron frequency Ω=qBm\Omega = \frac{qB}{m}.

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Faraday's Law of Induction

Maxwell equation stating ×E=Bt\nabla \times \mathbf{E} = -\frac{\partial \mathbf{B}}{\partial t}, or in terms of electromotive force E=dΦBdt\mathcal{E} = -\frac{d\Phi_B}{dt}.

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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.

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Self-inductance ($L$)

Proportionality constant between magnetic flux and current in a circuit (ΦB=LI\Phi_B = LI), yielding induced emf E=LdIdt\mathcal{E} = -L \frac{dI}{dt}.

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Energy stored in an inductor

Energy stored in the magnetic field of an inductor: UL=12LI2U_L = \frac{1}{2} L I^2.

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Electric dipole moment (p\mathbf{p})

Vector defined for two equal and opposite charges ±q\pm q separated by displacement d\mathbf{d} as p=qd\mathbf{p} = q\mathbf{d}, pointing from negative to positive charge.

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Electric dipole torque and energy

In external field E\mathbf{E}: torque N=p×E\mathbf{N} = \mathbf{p} \times \mathbf{E} and potential energy U=pEU = -\mathbf{p} \cdot \mathbf{E}.

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Magnetic dipole moment (m\mathbf{m})

Vector for a planar loop carrying current II with area vector A\mathbf{A} defined by m=IA\mathbf{m} = I\mathbf{A}; torque in field B\mathbf{B} is N=m×B\mathbf{N} = \mathbf{m} \times \mathbf{B} and potential energy is U=mBU = -\mathbf{m} \cdot \mathbf{B}.

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Dielectric constant (κ\kappa)

Factor by which permittivity increases in a material: ε=κε0\varepsilon = \kappa \varepsilon_0, increasing capacitance of a parallel-plate capacitor to C=κε0AdC = \kappa \frac{\varepsilon_0 A}{d}.

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Speed of light in vacuum ($c$)

Constant relation defined by c=1ε0μ0c = \frac{1}{\sqrt{\varepsilon_0 \mu_0}}.

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Poynting vector (S\mathbf{S})

Vector representing energy flux (power per unit area) of an electromagnetic wave: S=1μ0(E×B)\mathbf{S} = \frac{1}{\mu_0}(\mathbf{E} \times \mathbf{B}).

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Larmor formula

Total power radiated by a nonrelativistic accelerating point charge qq with acceleration aa: P=q2a26πε0c3P = \frac{q^2 a^2}{6\pi \varepsilon_0 c^3}.

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Electric dipole radiation power

Time-averaged power radiated by an oscillating electric dipole p(t)=p0cos(ωt)z^p(t) = p_0 \cos(\omega t)\hat{\mathbf{z}}: PE=μ0p02ω412πc\langle P \rangle_E = \frac{\mu_0 p_0^2 \omega^4}{12\pi c}.

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Kirchhoff's Rules

Circuit laws: (1) Node rule (charge conservation): kIk=0\sum_k I_k = 0; (2) Loop rule (energy conservation): kVk=0\sum_k V_k = 0.

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RC and RL time constants

Characteristic response times: τRC=RC\tau_{RC} = RC for RC circuits, and τRL=LR\tau_{RL} = \frac{L}{R} for RL circuits.

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LC circuit resonant frequency

Natural angular frequency of an LC circuit: ω0=1LC\omega_0 = \frac{1}{\sqrt{LC}}.

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One-dimensional wave equation

Differential equation 2ft2=v22fx2\frac{\partial^2 f}{\partial t^2} = v^2 \frac{\partial^2 f}{\partial x^2}, with general solutions f(x±vt)f(x \pm vt).

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Phase velocity and Group velocity

For a wave with dispersion relation ω(k)\omega(k), phase velocity is vphase=ωkv_{\text{phase}} = \frac{\omega}{k} and group velocity is vgroup=dωdkv_{\text{group}} = \frac{d\omega}{dk}.

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Malus's Law

Transmitted intensity of polarized light passing through a polarizer at angle θ\theta relative to its polarization direction: I=I0cos2(θ)I = I_0 \cos^2(\theta).

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Brewster's angle (θB\theta_B)

Angle of incidence at which reflected light is completely polarized perpendicular to the incident plane: θB=arctan(n2n1)\theta_B = \arctan\left(\frac{n_2}{n_1}\right).

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Double-slit interference conditions

For slit distance dd and angle θ\theta: maxima at dsin(θ)=mλd \sin(\theta) = m\lambda and minima at dsin(θ)=(m+12)λd \sin(\theta) = \left(m + \frac{1}{2}\right)\lambda.

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Single-slit diffraction minima

Minima occur at asin(θ)=mλa \sin(\theta) = m\lambda for m=1,2,3,m = 1, 2, 3, \dots, where aa is slit width.

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Optical path length

Equivalent path length in vacuum for light traveling distance dd in medium of index nn: OPL=nd\text{OPL} = nd.

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Thin-film reflection phase shift rules

Reflection off a boundary with n2>n1n_2 > n_1 undergoes a phase shift of π\pi; reflection off a boundary with n2<n1n_2 < n_1 undergoes no phase shift.

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Rayleigh criterion (Circular aperture)

Resolution limit for a circular aperture of diameter DD: first minimum occurs at Dsin(θ)=1.22λD \sin(\theta) = 1.22\lambda.

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Bragg diffraction condition

Condition for constructive interference of x-rays scattered from crystal planes separated by distance dd at incidence angle θ\theta: 2dsin(θ)=nλ2d \sin(\theta) = n\lambda.

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Thin lens equation

Relation between object distance ss, image distance ss', and focal length ff: 1s+1s=1f\frac{1}{s} + \frac{1}{s'} = \frac{1}{f}.