New DUT Simulation Technology Challenges ΛCDM with High-Redshift Galaxies

A recent preprint by Joel Almeida, a cosmology researcher and CEO of ExtractoDAO, introduces a groundbreaking computational simulation that reproduces the properties of high-redshift galaxies observed by the James Webb Space Telescope (JWST). This simulation, based on the Dead Universe Theory (DUT), presents a radical challenge to the standard ΛCDM cosmological model, proposing that the universe may not be expanding but retracting within a non-singular black hole structure.

The DUT simulator achieves an impressive accuracy rate of under 5% in its estimations of stellar mass, size, and formation timescales for galaxies at redshifts greater than 8, including notable examples such as CEERS-1019 and GLASS-z13. According to Almeida, these galaxies, which possess stellar masses exceeding 10¹⁰ solar masses and compact cores smaller than 1 kiloparsec, present a conundrum for traditional cosmological models, which struggle to account for their early formation in the universe.

"The simulations demonstrate that the universe does not need to have emerged from a singular point or be undergoing infinite expansion. Instead, JWST data can be interpreted as evidence of asymmetric gravitational retraction within a larger, stable, non-singular cosmic structure," Almeida explains. This perspective aligns with the DUT model, which posits that our observable universe constitutes an entropic bubble nested within the core of a structural black hole governed by a regularized oscillatory gravitational potential.

The DUT simulations mark a significant advancement in computational cosmology. Utilizing DarkStructSim™, a fully auditable and reproducible tool, researchers can simulate the universe offline, with future integrations planned for quantum computing platforms. This innovative approach not only provides a potential pathway for understanding high-redshift galaxies but also offers falsifiable predictions; if no galaxies with redshifts greater than 12 and masses exceeding 10¹⁰ solar masses are observed by the end of 2024, the DUT will be considered refuted.

The implications of this research extend beyond theoretical constructs, challenging established paradigms in cosmology. As Almeida notes, the DUT framework refutes the necessity of cosmic inflation and exotic dark matter, proposing instead a model that accommodates the rapid star formation rates observed in high-redshift galaxies within a coherent gravitational framework.

This research, available on Research Square, opens new avenues for exploration in cosmology. Researchers interested in the DUT simulator can access the code and documentation through ExtractoDAO's platform, enabling reproducibility and collaboration across the scientific community. The findings are poised to ignite debates in cosmological theories, potentially reshaping our understanding of the universe's formation and evolution.

In summary, Almeida's innovative work represents a pivotal moment in cosmology, as it not only questions the validity of the ΛCDM model but also provides tangible tools for further investigation into the mysteries of high-redshift galaxy formation. As the scientific community delves into these new simulations, the future of cosmological research may well hinge on the outcomes of these bold assertions.