where δ(x) is Dirac delta function.
This fundamental solution enables the presentation of a general solution Equation (2.4) in the form of modified Duhamel integral, and in and of itself, it describes a wave impulse excited by an instantaneous point source. As Equation (2.4) is asymptotic at ω >> 1/τr, this model is applicable only near the wave impulse front during the time period or at a distance (C ∞ = 1) smaller than זr (which at accepted dimensionless units equals one).
The wave impulse front that emerged at the moment t = 0 and at the point x = 0 reaches the points +x and −x at the moment t = |x|. Solution of the problem Equations (2.4) and (2.5) represents the wave after this moment if to record t = |x| + τ and 0 ˂ τ ˂ τr=1:
where the function fα(ζ) may be represented through an inverse Laplace transform:
Its expansion in a series is
where H(ζ) is Heaviside step function. In a special case at α = ½, the series (2.8) converges to
Due to nonuniform convergence of the series Equation (2.8), may also be found asymptotic formula for fα(ζ). It is determined using the saddle point method:
This correlation becomes equal to the exact expression Equation (2.9) at α = 1/2.
The function fα(ζ) defined by the equality Equation (2.7) converges to δ(ζ) at λ → 0. There is the equivalent representation of the last term in expression Equation (2.6) for cores of Equation (2.3) type. The packing φα (ζ)* fα(ζ) may be computed explicitly for this case and the left part of Equation (2.6) may then be written in a form more convenient for computation as it no longer includes the second integral. The function t = (|x| + τ|x|) is smooth and is faster tending to zero with the approach to the front corresponding to τ = 0 than nay power of τ, remaining infinitely differentiable which is obvious from (2.10).
The trivariate Green function for the medium model under review represents a solution of the spherically symmetric Cauchy problem [30]:
where
The solution of Equations (2.11) and (2.12) has the following format:
where it is assumed that
(2.14)
The Green’s function (2.13) behind the front (τ ˂˂ αr) as presented in space-time has the following format:
According to the theory of generalized functions,
(2.16)
where
(2.17)
(2.18)
(2.19)