Let be continuous and suppose that the displayed improper integral converges separately at both infinite endpoints for some . Absolute convergence is not required. Then its heat-kernel solution exists, is smooth and solves the heat equation for , and tends to as at each fixed .
To prove the smoothing claim, take a primitive of . The assumed convergence makes bounded. For , integration by parts givesThe endpoint term vanishes. The coefficient of in the exponent of is . Its derivatives therefore have Gaussian decay on every compact subset of , justifying differentiation under the integral sign in the absolutely convergent right-hand expression. Since , it satisfies the heat equation.
For the initial limit, apply the same construction to and split at . Continuity controls the local part by its small oscillation times the unit kernel mass. On each remaining tail, is monotone for sufficiently small : its maximum lies at , approaching . If the relevant primitive has absolute bound , integration by parts bounds that tail by times the value of at its finite endpoint. For either endpoint , that value tends to zero like times a fixed constant. Both tails vanish, proving the limit. Separate endpoint convergence matters here; merely assuming a symmetric Cauchy principal value does not provide the bounded primitive used in this proof.
Past exam of the mathematics course of the University of Cambridge 2021 ib Paper 4 14C Solution Created 2026-09-24 Updated 2026-09-25
Its total mass is found from the Gaussian integral:The unit-mass solution converging to the Dirac delta function as is therefore the heat kernel
For the second initial condition, the heat-kernel solution is the convolutionWith and the definition of the error function, this becomesThis is the heat equation with interval-indicator initial data for .
Past exam of the mathematics course of the University of Cambridge 2023 ib Paper 4 14A a Solution Created 2026-09-24 Updated 2026-09-25
Take the Fourier transform in . Since , the transformed heat equation isThereforeThe given transform pair and the convolution theorem yield the heat-kernel solution
Insert the linear initial profile into the transformed integral from (b):The constant part integrates to . The other part is an absolutely integrable odd function, so its integral vanishes. HenceAs a direct check, and . Thus a linear temperature profile is stationary on the whole line. More generally, every affine function is preserved by this heat-kernel solution.
The convolution theorem turns the product into a spatial convolution. Its kernel isComplete the square:After rescaling the variable, the supplied translated Gaussian integral givesThis is the heat-kernel solution for diffusivity one. Its kernel integrates to one, preserving the total temperature integral, and approaches a Dirac delta function as . Its variance is ; the factor is appropriate to , rather than the alternative convention with diffusivity .
For the Gaussian initial data for the heat equation, substitute the initial profile into the heat-kernel solution. Completing the square in givesThe remaining Gaussian integral yieldsThe centre stays at and the squared width grows linearly with time.
For the interval pulse, the convolution reduces to . Using and the error function givesThis is the translated and scaled heat equation with interval-indicator initial data. At its jump points the limits are ; away from them the initial data are recovered pointwise.
For fixed at late time, both error function arguments are small. Since ,The estimate is uniform for . Equivalently, on this fixed interval the Gaussian in the convolution is .
The spreading distance is more apparent on the growing spatial scale. For the Gaussian pulse the exponent is order one when . For the interval pulse, set with and fixed . Uniformly for bounded , its convolution givesThus both nonzero pulses spread over a distance , while their heights are and their total integrals remain constant. More quantitatively, the variances of their normalized profiles are and , respectively, confirming the same width law.
Gaussian and interval initial profiles broaden under the heat equation while conserving their integrals
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