General Physics Review: Mechanics, Thermodynamics, Electromagnetism

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Comprehensive vocabulary flashcards detailing core principles, laws, definitions, and equations across mechanics, thermodynamics, electrostatics, and magnetism based on the general physics syllabus.

Last updated 1:04 PM on 10/18/26
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32 Terms

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Material Point (Point Mass)

An idealized physical body whose dimensions and spatial extent are negligible compared to the characteristic distances or geometric scale of its motion.

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Inertial Reference Frame

A coordinate reference system in which Newton's first law of motion is valid, meaning an isolated object remains at rest or moves with constant velocity without experiencing fictitious inertial forces.

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Non-Inertial Reference Frame

A reference frame that accelerates or rotates with respect to an inertial frame, requiring the introduction of fictitious inertial forces to satisfy Newton's dynamical laws.

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Tangential Acceleration

The component of linear acceleration directed tangent to the trajectory, defined as at=dvdta_t = \frac{dv}{dt}, which characterizes the time rate of change of the speed of a particle.

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Normal Acceleration

The component of linear acceleration perpendicular to the trajectory and directed toward the instantaneous center of curvature, defined as an=v2Ra_n = \frac{v^2}{R}, characterizing the time rate of change of the direction of the velocity vector.

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Total Acceleration

The vector sum of the tangential and normal accelerations, given by a=at+an\mathbf{a} = \mathbf{a}_t + \mathbf{a}_n, with magnitude a=at2+an2a = \sqrt{a_t^2 + a_n^2}.

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Angular Velocity Vector

A pseudovector ω\boldsymbol{\omega} aligned along the axis of rotation following the right-hand rule, with magnitude ω=dφdt\omega = \frac{d\varphi}{dt}, related to linear velocity by v=ω×r\mathbf{v} = \boldsymbol{\omega} \times \mathbf{r}.

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Angular Acceleration Vector

The time rate of change of the angular velocity vector, β=dωdt\boldsymbol{\beta} = \frac{d\boldsymbol{\omega}}{dt}, whose magnitude is related to tangential acceleration in circular motion by at=βRa_t = \beta R.

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Momentum Theorem

The principle stating that the time derivative of linear momentum equals the net external force acting on a particle: dpdt=F\frac{d\mathbf{p}}{dt} = \mathbf{F}, or in differential form dp=F dtd\mathbf{p} = \mathbf{F}\,dt.

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Impulse of a Force

The integral of an applied force over a specified time duration, defined as J=∫t1t2F dt\mathbf{J} = \int_{t_1}^{t_2} \mathbf{F}\,dt, which equals the resulting change in linear momentum Δp\Delta \mathbf{p}.

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Work-Energy Theorem for Kinetic Energy

The theorem stating that the net work WW performed on a particle by all external forces equals the variation in its kinetic energy: W=ΔK=12mv22−12mv12W = \Delta K = \frac{1}{2}m v_2^2 - \frac{1}{2}m v_1^2.

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Basic Equation of the Kinetic Theory of Gases

The fundamental relation expressing macroscopic gas pressure in terms of microscopic molecular motion: p=13nm0v2‾=23nEk‾p = \frac{1}{3} n m_0 \overline{v^2} = \frac{2}{3} n \overline{E_k}, where nn is molecular number density, m0m_0 is molecular mass, and Ek‾\overline{E_k} is average translational kinetic energy.

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Degrees of Freedom of a Molecule

The total number of independent coordinates required to uniquely identify the spatial location and spatial configuration of a molecule (i=3i = 3 for monatomic, i=5i = 5 for rigid diatomic, and i=6i = 6 for non-linear polyatomic molecules).

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Law of Equipartition of Energy

The thermodynamic principle stating that the mean kinetic energy of a molecule in thermal equilibrium is distributed equally among all its active degrees of freedom, each contributing an average energy of 12kBT\frac{1}{2} k_B T.

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Internal Energy of an Ideal Gas

The cumulative thermal kinetic energy of all constituent gas molecules, defined by U=i2mMRTU = \frac{i}{2} \frac{m}{M} R T, where ii is degrees of freedom, mm is mass, MM is molar mass, and RR is the universal gas constant.

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First Law of Thermodynamics

The statement of energy conservation for thermodynamic systems, given by Q=ΔU+A′Q = \Delta U + A', stating that heat QQ supplied to a system equals the increase in its internal energy ΔU\Delta U plus the work A′A' performed by the system on its surroundings.

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Work in an Isobaric Process

The mechanical work delivered by an ideal gas during a process occurring at constant pressure: A′=p (V2−V1)=mMR (T2−T1)A' = p\,(V_2 - V_1) = \frac{m}{M} R\,(T_2 - T_1).

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Work in an Isothermal Process

The mechanical work delivered by an ideal gas during a process occurring at constant temperature: A′=mMRTln⁡(V2V1)=mMRTln⁡(p1p2)A' = \frac{m}{M} R T \ln\left(\frac{V_2}{V_1}\right) = \frac{m}{M} R T \ln\left(\frac{p_1}{p_2}\right).

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Second Law of Thermodynamics (Kelvin-Planck Statement)

The assertion that it is impossible to construct a thermodynamic engine operating in a continuous cycle whose sole result is the absorption of heat from a single thermal reservoir and the complete conversion of that heat into work.

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Carnot Efficiency

The upper bound on thermal efficiency for any heat engine operating reversibly between a hot heat reservoir at temperature THT_H and a cold heat reservoir at temperature TCT_C, given by η=1−TCTH\eta = 1 - \frac{T_C}{T_H}.

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Electric Field Intensity Vector

A vector field quantity defined as the electrostatic force experienced per unit positive stationary test charge: E=Fq0\mathbf{E} = \frac{\mathbf{F}}{q_0}, with SI unit V/m\text{V/m}.

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Electric Potential

A scalar field quantity defined as the potential energy per unit positive test charge at a given location in an electrostatic field: V=Wq0V = \frac{W}{q_0}, measured in volts (V\text{V}).

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Conservative Nature of Electrostatic Fields

The characteristic whereby electrostatic work done on a moving charge depends only on its initial and final locations, resulting in zero circulation along any closed path: ∮E⋅dr=0\oint \mathbf{E} \cdot d\mathbf{r} = 0.

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Electrostatic Energy of a Charged Capacitor

The stored electric potential energy residing within the dielectric medium of a charged capacitor: We=12CV2=Q22C=12QVW_e = \frac{1}{2} C V^2 = \frac{Q^2}{2 C} = \frac{1}{2} Q V.

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Electrostatic Equilibrium of a Conductor

The physical state in which mobile charges in a conductor are stationary, causing the internal field to vanish (E=0\mathbf{E} = \mathbf{0}), the entire body to be equipotential, and net charges to reside exclusively on the exterior boundary.

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Electric Energy Density

The electrostatic energy stored per unit volume of an electric field in a medium of dielectric constant ε\varepsilon: we=12ε0εE2w_e = \frac{1}{2} \varepsilon_0 \varepsilon E^2, expressed in J/m3\text{J/m}^3.

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Magnetic Induction of an Infinite Straight Wire

The magnitude of the magnetic field generated at a perpendicular separation distance rr from an infinitely long straight wire carrying current II: B=μ0μI2πrB = \frac{\mu_0 \mu I}{2 \pi r}.

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Ampère's Magnetic Force Law

The magnetic force acting on an infinitesimal straight current-carrying segment IdlI d\mathbf{l} immersed in an external magnetic field B\mathbf{B}, expressed by dF=I (dl×B)d\mathbf{F} = I\,(d\mathbf{l} \times \mathbf{B}), with magnitude F=IBlsin⁡(α)F = I B l \sin(\alpha).

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Self-Induction

The electromagnetic induction process wherein a time-varying electric current within a conducting circuit induces an electromotive force (EMF) inside that same circuit via its own changing magnetic flux.

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Self-Induced Electromotive Force

The induced EMF produced in an inductive circuit directly proportional to the negative time rate of change of electric current: Etc=−LdIdt\mathcal{E}_{\text{tc}} = -L \frac{dI}{dt}, where LL is the inductance.

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Self-Inductance of a Solenoid

The self-induction coefficient of a solenoid of length ll, core area SS, and turn count NN: L=μ0μN2lS=μ0μn2VL = \mu_0 \mu \frac{N^2}{l} S = \mu_0 \mu n^2 V, where nn is turns per unit length.

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Magnetic Energy Density

The magnetic potential energy contained per unit volume of space occupied by a magnetic field: wm=12BH=B22μ0μ=12μ0μH2w_m = \frac{1}{2} B H = \frac{B^2}{2 \mu_0 \mu} = \frac{1}{2} \mu_0 \mu H^2, measured in J/m3\text{J/m}^3.