Classical and Modern Physics Equations and Concepts

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Vocabulary practice flashcards generated from classical mechanics, electrodynamics, optics, thermodynamics, quantum mechanics, and special relativity lecture formulas.

Last updated 8:12 PM on 9/18/26
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30 Terms

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Translational Kinetic Energy

12mv2\frac{1}{2} m v^2

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Rotational Kinetic Energy

The kinetic energy associated with the rotation of an object with moment of inertia II and angular velocity ω\text{ω}, expressed as 12Iω2\frac{1}{2} I \text{ω}^2.

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Parallel Axis Theorem

A theorem stating that the moment of inertia II about any axis parallel to and a distance rr from the center-of-mass axis is given by I=ICM+Mr2I = I_{\text{CM}} + M r^2.

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Lagrangian

The function L(q,q˙,t)=TUL(q, \dot{q}, t) = T - U, defined as the difference between kinetic energy TT and potential energy UU.

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Conjugate Momentum

The momentum pip_i conjugate to the generalized coordinate qiq_i, defined as pi=Lq˙ip_i = \frac{\partial L}{\partial \dot{q}_i}.

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Hamiltonian

The function H(p,q)=ipiq˙iLH(p, q) = \sum_i p_i \dot{q}_i - L, representing total energy H=T+UH = T + U when the potential energy UU does not depend explicitly on velocities or time.

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Reduced Mass

The effective two-body inertial mass used to simplify two-body mechanical problems, defined as μ=m1m2m1+m2\mu = \frac{m_1 m_2}{m_1 + m_2}.

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Gauss's Law (Electrostatics)

A fundamental field equation of electrostatics stating that the divergence of the electric field is proportional to volumetric charge density, E=ρϵ0∇ \cdot \mathbf{E} = \frac{\rho}{\epsilon_0}.

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Poisson's Equation

A second-order partial differential equation relating the electric scalar potential VV to spatial charge density ρ\rho, given by 2V=ρϵ0\nabla^2 V = -\frac{\rho}{\epsilon_0}.

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Laplace's Equation

The partial differential equation satisfied by the electric potential VV in charge-free region of space, given by 2V=0\nabla^2 V = 0.

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Parallel-Plate Capacitor

A configuration of two parallel conducting plates of area AA separated by distance dd, with capacitance defined as C=ϵ0AdC = \frac{\epsilon_0 A}{d}.

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Ampere's Law (Magnetostatics)

A fundamental relation in magnetostatics connecting the curl of magnetic field B\mathbf{B} to current density J\mathbf{J}, expressed as ×B=μ0J\nabla \times \mathbf{B} = \mu_0 \mathbf{J}.

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Cyclotron Radius

The radius RR of the circular path executed by a charge qq moving with velocity vv perpendicular to a uniform magnetic field BB, given by R=mvqBR = \frac{m v}{q B}.

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Faraday's Law of Induction

A fundamental Maxwell equation stating that a time-varying magnetic field induces a circulating electric field, expressed as ×E=Bt\nabla \times \mathbf{E} = -\frac{\partial \mathbf{B}}{\partial t}.

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Poynting Vector

A vector representing the directional energy flux density of an electromagnetic field, defined as S=1μ0(E×B)\mathbf{S} = \frac{1}{\mu_0}(\mathbf{E} \times \mathbf{B}).

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Phase Velocity

The rate at which the phase of a wave propagates in space, defined as vphase=ωkv_{\text{phase}} = \frac{\omega}{k}.

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Group Velocity

The velocity with which the overall shape or envelope of wave amplitudes propagates, defined as vgroup=dωdkv_{\text{group}} = \frac{d\omega}{dk}.

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Brewster's Angle

The angle of incidence at which light with a particular polarization is transmitted without reflection, given by θB=arctan(n2n1)\theta_B = \arctan\left(\frac{n_2}{n_1}\right).

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Snell's Law

The formula describing the relationship between angles of incidence and refraction for waves passing through an interface, n1sin(θ1)=n2sin(θ2)n_1 \sin(\theta_1) = n_2 \sin(\theta_2).

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Partition Function

A key sum over Boltzmann factors of quantum microstates used to derive thermodynamic parameters, given by Z=ieβEiZ = \sum_i e^{-\beta E_i}.

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Fundamental Thermodynamic Relation

An expression combining the First and Second Laws of Thermodynamics for a reversible process, written as dU=TdSPdVdU = T dS - P dV.

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Fermi-Dirac Distribution

The statistical distribution function describing the occupancy probability of quantum states by non-interacting fermions, given by FFD(E)=1e(Eμ)/(kBT)+1F_{\text{FD}}(E) = \frac{1}{e^{(E - \mu)/(k_B T)} + 1}.

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Bose-Einstein Distribution

The statistical distribution function describing the occupancy probability of quantum states by non-interacting bosons, given by FBE(E)=1e(Eμ)/(kBT)1F_{\text{BE}}(E) = \frac{1}{e^{(E - \mu)/(k_B T)} - 1}.

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Position and Momentum Operators

In one-dimensional quantum mechanics, position operator x^=x\hat{x} = x and linear momentum operator p^=ix\hat{p} = -i \hbar \frac{\partial}{\partial x}.

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Heisenberg Uncertainty Principle

The relation expressing the fundamental quantum precision limit for simultaneously measuring position and momentum, σxσp2\sigma_x \sigma_p \ge \frac{\hbar}{2}.

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Fine-Structure Constant

A dimensionless fundamental physical constant characterizing the strength of electromagnetic interaction, defined as α=e24πϵ0c1137\alpha = \frac{e^2}{4\pi \epsilon_0 \hbar c} \approx \frac{1}{137}.

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Lorentz Factor

The scaling factor in special relativity describing time dilation and length contraction, defined as γ=11v2/c2\gamma = \frac{1}{\sqrt{1 - v^2/c^2}}.

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Relativistic Energy-Momentum Relation

The relation connecting total relativistic energy EE, momentum pp, and rest mass mm, given by E2=p2c2+m2c4E^2 = p^2 c^2 + m^2 c^4.

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Compton Shift

The shift in photon wavelength when scattering off a stationary particle, given by Δλ=hmc(1cos(θ))\Delta \lambda = \frac{h}{m c}(1 - \cos(\theta)).

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Fermi Energy (3D Free Electron Gas)

The highest single-particle quantum energy level in a non-interacting Fermi gas at absolute zero temperature, given by EF=22m(3π2n)2/3E_F = \frac{\hbar^2}{2m}(3\pi^2 n)^{2/3}.