Seek a nonzero separated solution . Substitution into the heat equation and division by the product gives
The left side depends only on time, so set it to . Multiplication by then separates the angular dependence, with separation constant . The three ordinary differential equations are
The temporal solution is . With , the angular equation is the Legendre differential equation; regularity at both angular endpoints selects and , the Legendre polynomial. The radial equation has the Spherical Bessel functions and for . Regularity at , if imposed, excludes the singular second solution. For the radial powers are and . Without specified radial boundary conditions, no discrete set of is selected; is a convention for the temporal separation constant.
For spherical symmetry the angular mode is . Put . Direct differentiation gives
so the radial heat equation in three dimensions becomes the ordinary one-dimensional heat equation . Since , the zero endpoint temperatures become .
Write . The two initial sine modes already satisfy these Dirichlet boundary conditions; their squared wave numbers are and . Each therefore evolves independently with its corresponding exponential decay. Dividing back by gives
At the initial profile is recovered, and each sine is zero at both endpoints. The first mode decays four times more slowly in its exponential rate than the second. This is the two-mode instance of the spherical-shell heat equation via radial rescaling; uniqueness follows, for example, by applying the heat equation energy identity to the difference of two solutions.

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