A note on the nonexistence of global solutions to the semilinear wave equation with nonlinearity of derivative-type in the generalized Einstein-de Sitter spacetime
Makram Hamouda, Mohamed Ali Hamza, Alessandro Palmieri

TL;DR
This paper proves that solutions to a specific semilinear wave equation in generalized Einstein-de Sitter spacetime cannot exist globally, identifying critical exponents that depend on space dimension and spacetime geometry.
Contribution
It introduces a new blow-up result for derivative-type nonlinear wave equations in this spacetime, using Yagdjian's integral transform to determine solution behavior.
Findings
Blow-up results for the wave equation in Einstein-de Sitter spacetime.
Identification of a Glassey-type critical exponent.
Dependence of the exponent on space dimension and spacetime metric.
Abstract
In this paper, we establish blow-up results for the semilinear wave equation in generalized Einstein-de Sitter spacetime with nonlinearity of derivative type. Our approach is based on the integral representation formula for the solution to the corresponding linear problem in the one-dimensional case, that we will determine through Yagdjian's Integral Transform approach. As upper bound for the exponent of the nonlinear term, we discover a Glassey-type exponent which depends both on the space dimension and on the Lorentzian metric in the generalized Einstein-de Sitter spacetime.
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