Predicting Dark Energy Survey Results Within the Haug-Tatum Cosmology Model
Overview & Synopsis
The new Haug-Tatum cosmology model has very recently been used to propose solutions of the Hubble tension problem [1][2] in favor of the Planck Collaboration Hubble parameter value [3]. Our model gives much tighter confidence intervals on the Hubble parameter than the ΛCDM model. This is due to new and exact mathematical relationships recently discovered between the cosmic microwave background (CMB) temperature and the Hubble parameter. This brief letter shows what our model predicts for the final consensus regarding Dark Energy Survey (DESI) results to be reported in or around 2026.
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Document Information
| Document Title | Predicting Dark Energy Survey Results Within the Haug-Tatum Cosmology Model |
|---|---|
| Author / Organization | Eugene Tatum, Espen Gaarder Norwegian University of Life Sciences Haug |
| Subject & Discipline | Multidisciplinary Academic Open Research |
| Categories | Science & Mathematics |
| Publication Year | 2024 |
| License / Rights | Open Access / Creative Commons |
| Resource Verification | Listed PDF (Verification Pending) |
| Original Host Website |
HAL Open Science
(hal.science)
|
| File Format | application/pdf (Portable Document Format) |
| Language | EN |
| Catalog ID | DOC-81148 |
| Original Source Link | Visit Source Page on hal.science » |