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Negative Energy Density: Pulsars and Kerr Rotating Black Holes

Publié
Serveur de preprints
Preprints.org
DOI
10.20944/preprints202503.0027.v1

This paper will explain how negative energy density, the same kind of negative energy density that is used in theoretical frameworks that explain wormholes, interact with rotating black holes in spacetime. Wormholes are particularly significant since they can be a route for time travel. As sci-fi as it seems, it is indeed a possibility, thanks to Kerr rotating black holes. Penrose process is key in understanding how negative energy density comes into play, and ergospheres in rotating black holes are also crucial. NASA data and Chandra telescope data were extracted to look at particle anomalies, which strongly suggest energy leakage and exotic matter. EHT (Event Horizon Telescope) data was also extracted, which solidifies the negative energy density argument. I will explain how this occurs using past theoretical models and real-world scientific observations. Jets, cone particles formed by hardons and other quark particles, leave the rotational black hole, from which it is produced, to create a forward force in space. Particles split, and the weaker one goes into the rotational black hole becoming negative, and the other one extracts energy from the black hole, making it exotic. These factors contribute to negative density since negative density fills the void left by the jets once they are carried away.

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