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The vibrating string: modes and energy
Standing waves and harmonics on a finite string, energy conservation, and uniqueness from energy.
For a string fixed at both ends, \( u_{tt} = c^2u_{xx} \), \( u(0,t) = u(L,t) = 0 \), separation of variables gives the same spatial modes as the heat equation, but the time factor now solves \( T'' + c^2\lambda_n T = 0 \) and oscillates: \[ u(x,t) = \sum_{n=1}^\infty\Big(A_n\cos\frac{n\pi ct}{L} + B_n\sin\frac{n\pi ct}{L}\Big)\sin\frac{n\pi x}{L}. \] The initial position fixes \( A_n = \frac2L\int_0^L f\sin\frac{n\pi x}L\,dx \), and the initial velocity fixes \( \frac{n\pi c}{L}B_n = \frac2L\int_0^L g\sin\frac{n\pi x}L\,dx \). The frequencies \( n\pi c/L \) are whole-number multiples of the fundamental: the harmonics of a musical string.
The energy of the string is kinetic plus potential, \[ E(t) = \frac12\int_0^L\big(u_t^2 + c^2u_x^2\big)\,dx. \] Differentiate and integrate the second term by parts: \( E'(t) = \int_0^L u_t\big(u_{tt} - c^2u_{xx}\big)\,dx + \big[c^2u_xu_t\big]_0^L \). The integrand vanishes by the equation, and the boundary term vanishes because \( u_t = 0 \) at fixed ends. So \( E \) is constant. For the single mode \( u = \sin x\cos t \) on \( [0, \pi] \) with \( c = 1 \), \( E = \frac12\int_0^\pi(\sin^2x\sin^2t + \cos^2x\cos^2t)\,dx = \pi/4 \), using the integral the example computes.
Energy gives uniqueness with no formula at all. If \( u \) and \( v \) solve the same problem, \( w = u - v \) solves it with zero data, so \( E_w(0) = 0 \), hence \( E_w(t) = 0 \), hence \( w_t = w_x = 0 \) everywhere, so \( w \) is constant and the boundary condition makes it zero.
Picture it: a plucked string is a sum of standing waves, each node pinned, each loop swinging at its own frequency. Energy sloshes between stretching (at maximum displacement) and motion (as it passes through equilibrium), and the total never changes.
Think it: the energy argument used only integration by parts and the sign of each term, so it survives variable coefficients, curved domains and higher dimensions where no series exists. That portability is why energy methods, not formulas, are the working tools for nonlinear equations.
పనిరోజులు · integrate sin(x)^2 dx from 0 to pi
Integrate sin(x)^2 from 0 to pi
అడుగు ద్వారా
- \int_{0}^{\pi} \sin^{2}{\left(x \right)}\, dx
First find an antiderivative F, then evaluate F(b) − F(a).
- \sin^{2}{\left(x \right)} = \frac{1}{2} - \frac{\cos{\left(2 x \right)}}{2}
Rewrite the integrand into a friendlier form.
- \int \frac{1}{2} - \frac{\cos{\left(2 x \right)}}{2}\, dx = \int \frac{1}{2}\, dx + \int - \frac{\cos{\left(2 x \right)}}{2}\, dx
The integral of a sum is the sum of the integrals.
- \int \frac{1}{2}\, dx = \frac{x}{2}
The integral of a constant c is c·x.
- \int - \frac{\cos{\left(2 x \right)}}{2}\, dx = - \frac{1}{2} \int \cos{\left(2 x \right)}\, dx
Pull the constant - \frac{1}{2} out of the integral.
- u = 2 x,\quad du = 2\, dx
Substitute u = 2 x.
- \int \cos{\left(2 x \right)}\, dx = \int \frac{\cos{\left(u \right)}}{2}\, d_u
Rewrite the integral in terms of u.
- \int \frac{\cos{\left(u \right)}}{2}\, d_u = \frac{1}{2} \int \cos{\left(u \right)}\, d_u
Pull the constant \frac{1}{2} out of the integral.
- \int \cos{\left(u \right)}\, d_u = \sin{\left(u \right)}
Standard trigonometric antiderivative.
- = \frac{\sin{\left(2 x \right)}}{2}
Substitute back u = 2 x.
- F(\pi) - F(0) = \left(\frac{\pi}{2}\right) - \left(0\right)
Fundamental theorem of calculus: plug in the limits.
- = \frac{\pi}{2} \approx 1.5708
Simplify.
జవాబు వెల్లడి చేయండి
ఇప్పుడుమీరు ప్రతీ అడుగున, మీరు అడిగేంత వరకు దాక్కున్న జవాబు.
మీరు ఏ పాఠం నేర్చుకున్నారో, ఆ విషయం గురించి ఒక రిపోర్టులో మీరు తీసుకున్న సమస్యలను, మీ సమస్యలను ఒక స్థలంలో పరిష్కరించిన సమస్యలను, మీరు ఈ పేజీ గురించి అడగవచ్చు.
నమోదు చేసుకోండి ప్రవేశించుఇక్కడ వుపయోగించిన చిహ్నాలు
మొదటి శతాబ్దంలోని క్రైస్తవులు కూడా అదే విధంగా భావించారు.
ఎలా: The vibrating string: modes and energy
- Separate variables: spatial modes sin(nπx/L), temporal frequencies nπc/L.
- Expand the initial position in sines to get A_n.
- Expand the initial velocity in sines and divide by nπc/L to get B_n.
- For energy, compute (1/2)∫(u_t² + c² u_x²) dx; with orthogonal modes it is a sum over modes.
- To prove uniqueness, apply energy conservation to the difference of two solutions.
ప్రశ్నలు
Why does a violin string sound different from a flute at the same pitch?
The fundamental frequency is the same, but the coefficients A_n and B_n of the higher harmonics differ, and the ear hears that mix as timbre.
Is energy conserved with a free end?
Yes, if the free end means u_x = 0 there: the boundary term c² u_x u_t still vanishes. With damping or a forcing term the energy changes, and the same computation measures by how much.
What should I know before starting?
Partial derivatives, the divergence theorem and multiple integrals from multivariable calculus; linear second-order ODEs; eigenvalues from linear algebra; and enough analysis to be comfortable with uniform convergence and integrals over infinite intervals.
Why are there so few formulas for solutions?
Explicit solutions exist for linear equations with constant coefficients on simple domains. Almost everything else (curved domains, variable coefficients, nonlinear terms) has none, so the modern subject proves that a solution exists and estimates its size and smoothness without ever writing it down.
How does this course lead to the Navier-Stokes problem?
The Navier-Stokes equations are a heat equation for the velocity with a transport term and a pressure that is found from a Poisson equation. Reading the Millennium problem needs energy estimates, weak solutions, Sobolev spaces, local existence with a blow-up criterion, and the scaling argument that explains why three dimensions is hard. The last six lessons build those.
What do elliptic, parabolic and hyperbolic mean?
Elliptic equations (Laplace) describe equilibrium and smooth everything; parabolic equations (heat) describe diffusion forward in time; hyperbolic equations (waves) carry signals at finite speed and keep their sharp edges. The type decides which data make a sensible problem.
ఇంకా Partial Differential Equations
What a PDE is, and how to classify oneFirst-order linear equations and characteristicsNonlinear first-order equations and shocksThe heat equation: where it comes fromSeparation of variablesFourier series: coefficients, convergence and ParsevalThe heat equation on an intervalThe wave equation and d'Alembert's formulaLaplace's equation and harmonic functionsMaximum principles and uniquenessGreen's functions and the fundamental solutionThe Fourier transform and the heat kernelEnergy methods: uniqueness, stability and decayDistributions and weak derivatives