Planetary Nebulae 1989
DOI: 10.1007/978-94-009-0865-9_88
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Abundances of C, N and O in Planetary Nebulae

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“…Some of these solutions, e.g., (18), (21) with µ = 1 and c 2 1 + c 2 2 > 1, describe the wave propagation with the group velocity higher then the velocity of light. Moreover, these solutions are smooth and bounded functions which correspond to positive definite and bounded energy density [14]. In spite of that these solutions are causal since their energy velocity does not exceed the velocity of light [14].…”
Section: Discussionmentioning
confidence: 98%
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“…Some of these solutions, e.g., (18), (21) with µ = 1 and c 2 1 + c 2 2 > 1, describe the wave propagation with the group velocity higher then the velocity of light. Moreover, these solutions are smooth and bounded functions which correspond to positive definite and bounded energy density [14]. In spite of that these solutions are causal since their energy velocity does not exceed the velocity of light [14].…”
Section: Discussionmentioning
confidence: 98%
“…It has been proven in [14] that the maximal continuous invariance group of system (2), (3) with arbitrary function F (θ) is the group P (1,3). The corresponding Lie algebra p(1,3) is spanned on the following basis elements:…”
Section: Group Classification Of System (2) (3)mentioning
confidence: 99%
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