Heat Equation with Non-Zero Temperature Boundaries — Question 10

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Question 10

Let ut=κuxxu_t=\kappa u_{xx} on 0<x<L0<x<L, with fixed endpoint temperatures A,BA,B, κ,L>0\kappa,L>0, and stationary field S=A+(B−A)x/LS=A+(B-A)x/L. For smooth compatible data define the error energy Ev=12∫0L(u−S)2dxE_v=\tfrac 12\int_0^L(u-S)^2\,dx and the raw quadratic quantity Eu=12∫0Lu2dxE_u=\tfrac 12\int_0^L u^2\,dx. You may use the zero-endpoint Poincare inequality ∫vx2≥(π/L)2∫v2\int v_x^2\ge(\pi/L)^2\int v^2 and the parabolic maximum principle.

Tasks

  1. Derive the energy identities for EvE_v and EuE_u, retaining all boundary terms. Prove the sharp bound Ev(t)≤e−2λtEv(0)E_v(t)\le e^{-2\lambda t}E_v(0), where λ=κπ2/L2\lambda=\kappa\pi^2/L^2.

  2. For A=B=1A=B=1 and u(x,0)=1−εsin⁡(πx/L)u(x,0)=1-\varepsilon\sin(\pi x/L), 0<ε≤10<\varepsilon\le 1, construct the solution. Prove that its raw quadratic quantity increases while its error energy decreases.

  3. If |u(x,0)−S(x)|≤Csin⁡(πx/L)|u(x,0)-S(x)|\le C\sin(\pi x/L), C>0C>0, use comparison to prove a pointwise error bound for all later times. Give a sufficient time for uniform temperature error at most δ\delta, where 0<δ<C0<\delta<C.

  4. Give a sufficient time for reducing error energy to a fraction η∈(0,1)\eta\in(0,1) of its initial value, and explain why neither total heat nor raw quadratic energy alone measures distance from a maintained nonzero equilibrium.

Original worksheet page 1: question and worked solution for 9-6-010
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Question 10 – Solution

Strategy. Dissipation applies naturally to deviations from the maintained equilibrium; the boundary reservoirs can increase the unshifted quantities.

Step 1: Identify which energy has no boundary work. For v=u−Sv=u-S, the endpoints vanish and vt=κvxxv_t=\kappa v_{xx}. Therefore Ev′=−κ∫0Lvx2dx≤−2λEv,Ev(t)≤e−2λtEv(0).E_v'=-\kappa\int_0^L v_x^2\,dx\le-2\lambda E_v, \qquad E_v(t)\le e^{-2\lambda t}E_v(0). A first-sine error attains equality, so the rate is sharp. For the raw quantity, Eu′=κ[uux]0L−κ∫0Lux2dx.\boxed{E_u'=\kappa[u u_x]_0^L-\kappa\int_0^L u_x^2\,dx.} The first term need not vanish with nonzero maintained boundary values.

Step 2: Exhibit simultaneous raw growth and error decay. The stated initial data give u=1−εe−λtsin⁡(πx/L)u=1-\varepsilon e^{-\lambda t}\sin(\pi x/L). Then Eu=L2−2εLπe−λt+ε2L4e−2λt,Ev=ε2L4e−2λt.E_u=\frac L2-\frac{2\varepsilon L}{\pi}e^{-\lambda t} +\frac{\varepsilon^2 L}{4}e^{-2\lambda t},\qquad E_v=\frac{\varepsilon^2 L}{4}e^{-2\lambda t}. Writing z=εe−λt∈(0,1]z=\varepsilon e^{-\lambda t}\in(0,1] gives Eu′=λLz(2/π−z/2)>0E_u'=\lambda Lz(2/\pi-z/2)>0, since 2/π>1/22/\pi>1/2. Meanwhile Ev′=−2λEv<0E_v'=-2\lambda E_v<0. Heating by the reservoirs moves this field closer to equilibrium while increasing its raw quadratic quantity.

Step 3: Establish a pointwise stopping criterion. The barriers ±Ce−λtsin⁡(πx/L)\pm C e^{-\lambda t}\sin(\pi x/L) solve the homogeneous zero-endpoint heat equation and bound the initial error. Applying comparison to their differences with vv on any finite time interval gives |u−S|≤Ce−λtsin⁡(πx/L)≤Ce−λt.\boxed{|u-S|\le C e^{-\lambda t}\sin(\pi x/L)\le C e^{-\lambda t}.} Thus t≥λ−1log⁡(C/δ)t\ge\lambda^{-1}\log(C/\delta) suffices for uniform error at most δ\delta. This conclusion uses the supplied pointwise initial bound, not merely an initial L2L^2 norm.

Step 4: Distinguish the two stopping criteria. The energy inequality gives Ev(t)/Ev(0)≤ηE_v(t)/E_v(0)\le\eta once t≥(2λ)−1log⁡(1/η)t\ge(2\lambda)^{-1}\log(1/\eta) for nonzero initial error; zero error is already at equilibrium. The factor of two comes from squaring a decaying amplitude. Total heat can conceal spatial differences, and raw energy includes the maintained background and boundary work. Neither is a substitute for an explicit norm of u−Su-S when measuring equilibration.

Original worksheet page 2: question and worked solution for 9-6-010

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