Maximal non-Kochen-Specker sets and a lower bound on the size of Kochen-Specker sets
Physical Review A American Physical Society (APS) 111:1 (2025) 012223
Searching for a dark matter induced galactic axion gradient
Physical Review D American Physical Society (APS) 111:1 (2025) 015006
Evaporating Primordial Black Holes, the String Axiverse, and Hot Dark Radiation
Physical Review Letters American Physical Society (APS) 133:26 (2024) 261003
Computation of quark masses from string theory
Nuclear Physics B Elsevier 1010 (2024) 116778
Abstract:
We present a numerical computation, based on neural network techniques, of the physical Yukawa couplings in a heterotic string theory compactification on a smooth Calabi-Yau threefold with non-standard embedding. The model belongs to a large class of heterotic line bundle models that have previously been identified and whose low-energy spectrum precisely matches that of the MSSM plus fields uncharged under the Standard Model group. The relevant quantities for the calculation, that is, the Ricci-flat Calabi-Yau metric, the Hermitian Yang-Mills bundle metrics and the harmonic bundle-valued forms, are all computed by training suitable neural networks. For illustration, we consider a one-parameter family in complex structure moduli space. The computation at each point along this locus takes about half a day on a single twelve-core CPU. Our results for the Yukawa couplings are estimated to be within 10% of the expected analytic result. We find that the effect of the matter field normalisation can be significant and can contribute towards generating hierarchical couplings. We also demonstrate that a zeroth order, semi-analytic calculation, based on the Fubini-Study metric and its counterparts for the bundle metric and the bundle-valued forms, leads to roughly correct results, about 25% away from the numerical ones. The method can be applied to other heterotic line bundle models and generalised to other constructions, including to F-theory models.Search for dark matter from the center of the Earth with ten years of IceCube data
ArXiv 2412.12972 (2024)