Scale-invariant bounds on the space-time derivatives of the heat kernel #
On a finite-dimensional real inner product space E of dimension n, the heat kernel
K_t(x) = (4πt)^(-n/2) exp(-‖x‖² / (4t)) has the parabolic scaling
D^m K_t(x) = t^(-(n + m) / 2) D^m K_1(t^(-1/2) x). This file turns that scaling into estimates
whose constants do not depend on the time, as needed for the Hölder estimates of heat potentials:
- for all orders
jin time andmin space,‖∂ₜ^j D^m K_t(x)‖ ≤ C t^(-(n + m + 2j) / 2) exp(-‖x‖² / (8t))for allt > 0; - equivalently for
j = 0,‖D^m K_t(x)‖ ≤ C t^(-m / 2) K_{2t}(x); - rescaling the case
t = 1 / 4, the derivatives of the Gaussianexp(-c ‖x‖²)satisfy‖D^m exp(-c ‖x‖²)‖ ≤ C c^(m / 2) exp(-c ‖x‖² / 2)uniformly inc ≥ 0; ‖D^m K_t(x)‖ ‖x‖^α ≤ C t^((α - m) / 2) K_{4t}(x)forα ≥ 0;- consequently
∫ ‖D^m K_t(x)‖ ‖x‖^α dx ≤ C t^((α - m) / 2), in particular∫ ‖D^m K_t‖ ≤ C t^(-m / 2); - for time differences,
∫ ‖D^m K_b(x) - D^m K_a(x)‖ ‖x‖^α dx ≤ C (b - a) a^((α - m - 2) / 2)when0 < a ≤ b ≤ 2a, by the mean value theorem in time; ∫ D^m K_t = 0form ≥ 1.
Every time derivative of D^m K_s(x) at s = t again has the scaling form s^(-b) Ψ(s^(-1/2) x)
for a profile Ψ all of whose derivatives decay like exp(-‖y‖² / 8), so the time bound
reduces to a bound on the profile. The vanishing integral follows by integrating by parts against
the constant function 1.
Main declarations #
TauCeti.iteratedFDeriv_heatKernel_eq_rpow_smul: parabolic scaling of the derivatives.TauCeti.differentiableAt_iteratedFDeriv_heatKernel: the spatial derivatives are differentiable in time.TauCeti.exists_norm_iteratedDeriv_iteratedFDeriv_heatKernel_le: Gaussian bounds on the space-time derivatives.TauCeti.exists_norm_iteratedFDeriv_heatKernel_le_rpow_mul_exp: the case of spatial derivatives.TauCeti.exists_norm_iteratedFDeriv_exp_neg_mul_norm_sq_le: the derivatives of the Gaussianexp(-c ‖ξ‖²)areO(c^{k/2} exp(-c ‖ξ‖² / 2)), uniformly inc ≥ 0.TauCeti.exists_norm_iteratedFDeriv_heatKernel_le_mul_rpow_mul_heatKernel: the bound byC t^(-m / 2) K_{2t}(x).TauCeti.exists_norm_iteratedFDeriv_heatKernel_mul_rpow_le: the weighted bound byC t^((α - m) / 2) K_{4t}(x).TauCeti.integrable_norm_iteratedFDeriv_heatKernel_mul_rpow: integrability of the weighted derivatives.TauCeti.integrable_norm_rpow_mul_heatKernel: integrability of the weight‖x‖^α K_t(x).TauCeti.heatKernelMoment: the absolute moment∫ ‖y‖^α K_1(y) dy.TauCeti.exists_integral_norm_iteratedFDeriv_heatKernel_mul_rpow_le: the weightedL¹bound.TauCeti.exists_integral_norm_iteratedFDeriv_heatKernel_le: theL¹bound.TauCeti.exists_norm_iteratedFDeriv_heatKernel_sub_mul_rpow_le,TauCeti.exists_integral_norm_iteratedFDeriv_heatKernel_sub_mul_rpow_le: the weighted bounds on time differences.TauCeti.integral_iteratedFDeriv_heatKernel_eq_zero: the derivatives have integral zero.
References #
- A. Friedman, Partial Differential Equations of Parabolic Type, Chapter 1 (Gaussian bounds on the derivatives of the fundamental solution).
- A. Lunardi, Linear and nonlinear diffusion problems, Chapter 4 (weighted kernel estimates for heat potentials).
Parabolic scaling of the derivatives of the heat kernel. For t > 0,
D^m K_t(x) = t^(-(n + m) / 2) D^m K_1(t^(-1/2) x), where n = dim E.
Time derivatives #
By parabolic scaling, D^m K_s(x) = s^(-a) Ψ(s^(-1/2) x) with a = (n + m) / 2 and
Ψ = D^m K_1. Differentiating such an expression in s gives one of the same shape,
s^(-(a + 1)) Ψ'(s^(-1/2) x) with Ψ'(y) = -a Ψ(y) - (1/2) DΨ(y) y. Since Ψ has Gaussian
decay at rate 1 / 8 and that class is closed under Ψ ↦ Ψ'
(exists_gaussianDecay_iteratedDeriv_rpow_smul), every time derivative has a Gaussian bound.
Gaussian bounds on the space-time derivatives of the heat kernel. For all orders j in
time and m in space there is a constant C, independent of the time, such that
‖∂ₜ^j D^m K_t(x)‖ ≤ C t^(-(n + m + 2j) / 2) exp(-‖x‖² / (8t)) for all t > 0 and all x,
where n = dim E.
For t > 0, the spatial derivative D^m K_s(x) of the heat kernel is differentiable in the
time s at s = t.
Scale-invariant Gaussian bounds on the derivatives of the heat kernel. For every order
m there is a constant C, independent of the time, such that
‖D^m K_t(x)‖ ≤ C t^(-(n + m) / 2) exp(-‖x‖² / (8t)) for all t > 0 and all x, where
n = dim E.
Derivatives of a Gaussian. For every order k there is a constant C such that, for
every c ≥ 0, ‖D^k exp(-c ‖ξ‖²)‖ ≤ C c^{k/2} exp(-c ‖ξ‖² / 2).
Scale-invariant Gaussian bounds on the derivatives of the heat kernel, against the heat
kernel at the doubled time. For every order m there is a constant C > 0, independent of the
time, such that ‖D^m K_t(x)‖ ≤ C t^(-m / 2) K_{2t}(x) for all t > 0 and all x.
Scale-invariant weighted Gaussian bounds on the derivatives of the heat kernel. For every
order m and every α ≥ 0 there is a constant C > 0, independent of the time, with
‖D^m K_t(x)‖ ‖x‖^α ≤ C t^((α - m)/2) K_{4t}(x) for all t > 0 and all x.
Time differences of the derivatives of the heat kernel. For every order m and every
α ≥ 0 there is a constant C > 0, independent of the times, such that
‖D^m K_b(x) - D^m K_a(x)‖ ‖x‖^α ≤ C (b - a) a^((α - m - 2)/2) K_{4b}(x) whenever
0 < a ≤ b ≤ 2a. One time derivative costs a factor a⁻¹ compared with
TauCeti.exists_norm_iteratedFDeriv_heatKernel_mul_rpow_le.
For t > 0 and α ≥ 0, the weighted derivative x ↦ ‖D^m K_t(x)‖ ‖x‖^α of the heat kernel
is integrable.
For t > 0 and α ≥ 0, the weight x ↦ ‖x‖^α K_t(x) is integrable.
The absolute moment M_α = ∫ ‖y‖^α K_1(y) dy of order α of the heat kernel at time one.
It is the constant in the Hölder estimates of heat potentials.
Instances For
The defining formula of TauCeti.heatKernelMoment.
Weighted L¹ bounds on the derivatives of the heat kernel. For every order m and every
α ≥ 0 there is a constant C > 0, independent of the time, with
∫ ‖D^m K_t(x)‖ ‖x‖^α dx ≤ C t^((α - m)/2) for all t > 0. Combined with the cancellation
∫ D^m K_t = 0, this is the kernel estimate behind Hölder bounds for heat convolutions.
Weighted L¹ bounds on time differences of the derivatives of the heat kernel. For every
order m and every α ≥ 0 there is a constant C > 0, independent of the times, with
∫ ‖D^m K_b(x) - D^m K_a(x)‖ ‖x‖^α dx ≤ C (b - a) a^((α - m - 2)/2) whenever 0 < a ≤ b ≤ 2a.
This is the kernel estimate behind temporal Hölder bounds for heat convolutions.
Scale-invariant L¹ bounds on the derivatives of the heat kernel. For every order m
there is a constant C, independent of the time, such that ‖D^m K_t‖_{L¹} ≤ C t^(-m / 2) for
all t > 0.
The derivatives of the heat kernel have integral zero. For every order m ≥ 1 and every
t > 0, ∫ D^m K_t = 0.