Classical Mechanics: Fundamental Concepts and Principles

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Vocabulary practice flashcards defining core concepts, equations, and principles in Classical Mechanics.

37 Terms

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Principle of relativity

The fundamental principle that observers moving at a constant velocity relative to each other obey the same laws of mechanics. There’s no way to tell which object is truly at rest if both move at a constant relative velocity.

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Inertial frame

A non-accelerating, non-rotating reference frame where Newton’s first law holds and objects in motion remain at rest or in uniform motion unless acted upon by an external force.

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Newton's first law

A body acted on by no forces moves with uniform velocity in a straight line, which physically establishes the existence of inertial frames of reference.

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Newton's second law

The equation of motion specifying that the time rate of change of momentum of a body is equal to the total force acting on it, dpdt=ma=F\frac{d\bf{p}}{dt} = m\bf{a} = \bf{F}.

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Newton's third law

The dynamical law asserting that mutual forces of action and reaction between two bodies are equal in magnitude and opposite in direction, satisfying Fji=−Fij\bf{F}_{ji} = -\bf{F}_{ij}.

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Equivalence principle

The physical law derived from experimental observation stating that inertial mass in Newton's second law is proportional to gravitational mass.

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Conservative force

Conservative Force: A force field depending only on position whose curl vanishes (∇×F=0\nabla \times \bf{F} = \bf{0}), enabling it to be represented as the negative gradient of a potential energy function, F(r)=−∇V(r)\bf{F}(\bf{r}) = -\nabla V(\bf{r}), and ensuring total mechanical energy is conserved.

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Work done

The line integral of force over an infinitesimal displacement, defined in three dimensions by dW=F×drdW = \bf{F} \times d\bf{r}, which measures the amount of energy converted into kinetic energy.

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Simple harmonic oscillator

A system executing motion near a stable equilibrium point under a linear restoring force F=−kxF = -kx, described by the differential equation d2xdt2+kmx=0\frac{d^2x}{dt^2} + \frac{k}{m}x = 0.

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Superposition principle

The property of linear differential equations stating that any linear combination of linearly independent solutions is also a solution to the equation.

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Relaxation time

The characteristic time interval 1γ=2mλ\frac{1}{\gamma} = \frac{2m}{\lambda} during which the amplitude of an underdamped oscillator diminishes by a factor of e−1e^{-1}.

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Quality factor (QQ)

A dimensionless parameter of an oscillator defined by Q=m×km1/2λ=ω02γQ = \frac{m\times\frac{k}{m}^{1/2}}{\lambda} = \frac{\omega_0}{2\gamma}, characterizing the sharpness of resonance and the persistence of stored mechanical energy.

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Critical damping

The boundary damping condition occurring when γ=ω0\gamma = \omega_0, providing the most rapid return of an oscillator to equilibrium without any oscillatory overshoot.

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Transient

The portion of the general solution of a driven damped oscillator that corresponds to the complementary function and decays exponentially with time, leaving only steady-state forced oscillations.

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Resonance

The physical phenomenon occurring when the angular frequency of a periodic driving force approaches the natural frequency of an undamped oscillator (ω1≈ω0\omega_1 \approx \omega_0), generating maximum response amplitude.

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Half-width of resonance

The parameter γ\gamma specifying the frequency deviation from resonance (ω1=ω0±γ\omega_1 = \omega_0 \pm \gamma) at which the amplitude of forced oscillation drops to 12\frac{1}{\sqrt{2}} of its resonance peak.

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Impulse

The definite time integral of a force delivered over a short duration, I=∫tt+ΔtF dtI = \int_{t}^{t+\Delta t} F\,dt, which equals the resultant change in linear momentum Δp\Delta p.

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Green's function

The response function G(t−t′)G(t - t') representing the displacement at time tt of an oscillator at rest induced by an impulsive blow of unit impulse applied at time t′t'.

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Elastic collision

A collision between bodies in which total mechanical kinetic energy is conserved before and after impact, reversing the relative velocity between the colliding bodies.

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Coefficient of restitution (ee)

The ratio of relative separation speed to relative approach speed between two colliding bodies, defined by v2−v1=e(u1−u2)v_2 - v_1 = e(u_1 - u_2).

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Moment of a force

The vector product G=r×F\bf{G} = \bf{r} \times \bf{F} of the position vector and applied force, which equals the time rate of change of angular momentum.

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Angular momentum

The moment of linear momentum about a reference origin, defined for a body by J=r×p=m(r×drdt)\bf{J} = \bf{r} \times \bf{p} = m(\bf{r} \times \frac{d\bf{r}}{dt}).

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Axial vector

A vector quantity, such as angular momentum or torque, whose assigned direction is determined by a right-hand screw convention rather than spatial inversion invariance.

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Central force

A force that is always directed radially toward or away from a fixed point, having zero moment (r×F=0\bf{r} \times \bf{F} = \bf{0}) and therefore conserving angular momentum.

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Kepler's second law

The law stating that the radius vector of a particle moving under a central force sweeps out equal areas in equal times, satisfying dAdt=J2m=constant\frac{dA}{dt} = \frac{J}{2m} = \text{constant}.

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Euler-Lagrange equation

The second-order differential equation ∂f∂y−ddx(∂f∂y′)=0\frac{\partial f}{\partial y} - \frac{d}{dx}\left(\frac{\partial f}{\partial y'}\right) = 0 that a function y(x)y(x) must satisfy for the integral I=∫x0x1f(y,y′) dxI = \int_{x_0}^{x_1} f(y, y')\,dx to achieve a stationary value.

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Lagrangian function (LL)

The characteristic dynamical function defined as the difference between the kinetic energy and potential energy of a conservative system, L=T−VL = T - V.

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Hamilton's principle

The foundational principle stating that the actual trajectory followed by a conservative dynamical system renders the action integral I=∫t0t1L dtI = \int_{t_0}^{t_1} L\,dt stationary under arbitrary variations that vanish at the boundaries.

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Generalized momentum

The conjugate momentum variable corresponding to a generalized coordinate qiq_i, defined in analytical mechanics by pi=∂L∂q˙ip_i = \frac{\partial L}{\partial \dot{q}_i}.

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Effective potential energy

The composite radial potential function U(r)=J22mr2+V(r)U(r) = \frac{J^2}{2mr^2} + V(r) that combines the actual potential energy with the repulsive centrifugal potential term.

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Impact parameter (bb)

The perpendicular distance from the center of force to the asymptotic straight line along which an incident particle approaches from infinity.

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Semi-latus rectum (ll)

The geometric scale factor of a conic orbit under an inverse square law, defined by l=J2m∣k∣l = \frac{J^2}{m|k|}, which gives the radial distance at right angles to perihelion.

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Kepler's third law

The astronomical law stating that the square of the orbital period of a body orbiting a primary mass MM is directly proportional to the cube of its semi-major axis, satisfying (τ2π)2=a3GM\left(\frac{\tau}{2\pi}\right)^2 = \frac{a^3}{GM}.

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Differential cross-section

The ratio of the number of particles scattered into a unit solid angle per unit time to the incident particle flux per unit area, denoted by dσdΩ\frac{d\sigma}{d\Omega}.

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Mean free path

The average straight-line distance λ=1nσ\lambda = \frac{1}{n\sigma} traversed by a particle through a scattering medium with particle number density nn and total collision cross-section σ\sigma before colliding.

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Rutherford scattering cross-section

The differential cross-section for Coulomb scattering of a charged particle by a central charge, given by dσdΩ=a24(sin⁡(12θ))4\frac{d\sigma}{d\Omega} = \frac{a^2}{4\left(\sin\left(\frac{1}{2}\theta\right)\right)^4}.

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Angular velocity vector

The axial vector ω=ωn\bf{\omega} = \omega\bf{n} oriented along the axis of rotation by the right-hand screw rule, relating the position vector to velocity by v=ω×r\bf{v} = \bf{\omega} \times \bf{r}.