A Noether symmetry ansatz yields exact scale-factor and vector-field solutions for a teleparallel cosmology, producing dark-energy-like acceleration and a possible phantom phase for chosen parameters.
Is it possible to know cosmological fine-tuning?
1 Pith paper cite this work. Polarity classification is still indexing.
abstract
Fine-tuning studies whether some physical parameters, or relevant ratios between them, are located within so-called life-permitting intervals of small probability outside of which carbon-based life would not be possible. Recent developments have found estimates of these probabilities that circumvent previous concerns of measurability and selection bias. However, the question remains if fine-tuning can indeed be known. Using a mathematization of the epistemological concepts of learning and knowledge acquisition, we argue that most examples that have been touted as fine-tuned cannot be formally assessed as such. Nevertheless, fine-tuning can be known when the physical parameter is seen as a random variable and it is supported in the nonnegative real line, provided the size of the life-permitting interval is small in relation to the observed value of the parameter.
citation-role summary
citation-polarity summary
fields
gr-qc 1years
2025 1verdicts
CONDITIONAL 1roles
background 1polarities
unclear 1representative citing papers
citing papers explorer
-
Exact Solutions for a Teleparallel Cosmological Model with Vector Field via Noether Symmetry
A Noether symmetry ansatz yields exact scale-factor and vector-field solutions for a teleparallel cosmology, producing dark-energy-like acceleration and a possible phantom phase for chosen parameters.