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PreprintCC BY 4.0arXiv

Heat flow and the fundamental solution of the Baouendi-Grushin operator

Abstract

For the Baouendi-Grushin operator ℒγ= Δx + |x|2γΔy in Rm+k, with γ>0, we prove that the time integral of the heat kernel with pole at the origin equals Cγ,Q Nγ2−Q, where Nγ is the gauge and Q the homogeneous dimension. When γnot=1 no closed form of the heat kernel is known. After a partial Fourier transform in y, the time integral of the heat kernel becomes the Green function of an anharmonic oscillator, which solves a generalized modified Bessel equation, and the gauge appears when the inverse Fourier transform is computed as a Hankel transform. In particular, the heat flow provides a new proof that Cγ,Q Nγ2−Q is a fundamental solution of −ℒγ with pole at the origin.

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BibTeX
@misc{garofalo2026heat,
  title = {{Heat flow and the fundamental solution of the Baouendi-Grushin operator}},
  author = {Nicola Garofalo},
  howpublished = {arXiv},
  year = {2026},
  month = nov,
  doi = {10.48550/arxiv.2611.01336},
  eprint = {2611.01336},
  archivePrefix = {arXiv},
  url = {https://arxiv.org/abs/2611.01336},
  note = {CC BY 4.0},
}
RIS
TY  - UNPB
TI  - Heat flow and the fundamental solution of the Baouendi-Grushin operator
AU  - Nicola Garofalo
PY  - 2026
DA  - 2026/11/01
PB  - arXiv
DO  - 10.48550/arxiv.2611.01336
UR  - https://arxiv.org/abs/2611.01336
AB  - For the Baouendi-Grushin operator ℒ_γ= Δ_x + |x|^2γΔ_y in R^m+k, with γ>0, we prove that the time integral of the heat kernel with pole at the origin equals C_γ,Q N_γ^2−Q, where N_γ is the gauge and Q the homogeneous dimension. When γnot=1 no closed form of the heat kernel is known. After a partial Fourier transform in y, the time integral of the heat kernel becomes the Green function of an anharmonic oscillator, which solves a generalized modified Bessel equation, and the gauge appears when the inverse Fourier transform is computed as a Hankel transform. In particular, the heat flow provides a new proof that C_γ,Q N_γ^2−Q is a fundamental solution of −ℒ_γ with pole at the origin.
ER  -