Blow-up for a fully fractional heat equation
Abstract
We study the existence and behaviour of blowing-up solutions to the fully fractional heat equation M u=up, x∈RN,\;0<t<T with p>0, where M is a nonlocal operator given by a space-time kernel M(x,t)=cN,σt- N2-1-σe-|x|24t1\t>0\, 0<σ<1. This operator coincides with the fractional power of the heat operator, M=(∂t-)σ defined through semigroup theory. We characterize the global existence exponent p0=1 and the Fujita exponent p*=1+2σN+2(1-σ), and study the rate at which the blowing-up solutions below p* tend to infinity, \|u(·,t)\|∞ (T-t)-σp-1.
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