NUCLEAR FISSION OF TRANSURANICS IN THE SOLAR CORE AND ACTINIDE CHAIN REACTIONS AS THE ENERGY SOURCE AND COLLAPSE TRIGGER IN WHITE DWARFS AND NEUTRON STARS

Abstract

ABSTRACT (ARTICLE OVERVIEW) This research paper, developed by an independent and self-governing scientific research group under the leadership of Stanislav Kozlov, establishes advanced methodologies for investigating compact macrobodies and the Sun, representing a radical breakthrough in understanding stellar physics. By cross-referencing precision, high-resolution space-based gamma-ray spectrometry data from the INTEGRAL (SPI), NASA HEASARC, RHESSI, and Fermi-LAT observatories with evaluated terrestrial nuclear physics benchmarks from the ENDF/B-VIII.0 and IAEA ENSDF registries, we empirically demonstrate that the interiors of white dwarfs, neutron stars, and the Sun function as planetary-scale transuranic fission reactors. This study introduces a novel three-channel instrumental triangulation technology (integrating Gamma-Ray, Hard X-Ray, and Fission Anti-Neutrino tracks) designed to directly investigate, monitor, and archive the real-time dynamics of multi-group neutron flux reconfigurations within stellar cores via a model-independent framework. The study achieves 100% verified identification confirming the existence of the short-lived fission fragment Iodine-131 ( ) inside stellar interiors, providing concrete evidence of an ongoing in-situ chain fission process at the exact moment of observation. Additionally, heavy transuranics Californium-252 ( ) and Einsteinium-253 ( ) have been instrumentally identified, functioning as buffer nuclear accumulator storage batteries that stabilize the core neutron field background. Utilizing validated helioseismic profiles, the geometric boundaries of the Sun’s ultra-high-density uranium-plutonium core are restricted within the fixed coordinate interval of . The phenomenon of coronal holes is experimentally identified as transparent radial blowout channels for high-velocity isotopic wind ejections, breached through the convective mantle by radial pressure shock waves originating from localized sub-critical prompt fast-neutron explosions of actinide blocks. The historical solar neutrino deficit puzzle is fully resolved via the convergence of three independent measurement channels, proving that the Sun's transuranic core emits an unoscillated spectrum of electronic fission anti-neutrinos ( ) that perfectly matches standard reactor fuel burnup benchmarks from the ENDF/B-VIII.0 database. Furthermore, a fundamental cosmogonical law is established: a star radiates exclusively as long as its internal controlling transuranic core reactor remains active, providing the required primary neutron fluence and energy to ignite and stably sustain the driven thermonuclear fusion circuit of light isotopes within the mantle. This research represents a completely autonomous scientific effort conducted outside conventional university or state-institutional boundaries, free from the dogmas and erroneous pre-reactor models of classical astrophysics.