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Authors: Roberto C. M. Navacchia
This paper presents an alternative method of analysis for identifying pulsars using data from the High Time Resolution Universe Survey neutron star catalog and the construction of radial curves derived from statistical parameters of the observed radio signals, where, through a geometric approach, highlights their unique and distinct signature for each pulsar, which differs significantly from the curves produced by noise signals. The method seeks to offer the scientific community a complementary means of classification, opening up possibilities for the creation of a ‘Geometric Atlas of Pulsars’ useful in Astrophysics, Data Science, Quantum Mechanics, and especially in Analytical Geometry.
Comments: 8 Pages. In Portuguese; License: CC BY-NC (Note by viXra Admin: Please submit article written with AI assistance to ai.viXra.org)
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[v1] 2025-09-25 20:48:12
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