K Subramanian - Reports on Progress in Physics, 2016 - iopscience.iop.org
The universe is magnetized on all scales probed so far. On the largest scales, galaxies and galaxy clusters host magnetic fields at the micro Gauss level coherent on scales up to ten …
BS Acharya, I Agudo, I Al Samarai, R Alfaro, J Alfaro… - 2019 - air.uniud.it
Names: CTA Consortium (Organization) Title: Science with the Cherenkov Telescope Array/by The CTA Consortium. Description: New Jersey: World Scientific, 2018.| Includes …
R Durrer, A Neronov - The Astronomy and Astrophysics Review, 2013 - Springer
We review the possible mechanisms for the generation of cosmological magnetic fields, discuss their evolution in an expanding Universe filled with the cosmic plasma and provide a …
We provide a pedagogical review article on fundamentals and applications of the quantum dynamics in strong electromagnetic fields in QED and QCD. The fundamentals include the …
G Endrődi - Progress in Particle and Nuclear Physics, 2024 - Elsevier
This review provides a comprehensive summary of results on the physics of strongly interacting matter in the presence of background electromagnetic fields, obtained via …
Vector bosons heavier than 10-22 eV can be viable dark matter candidates with distinctive experimental signatures. Ultralight dark matter generally requires a nonthermal origin to …
Observational cosmology in the next decade will rely on probes of the distribution of matter in the redshift range between $0< z< 3$ to elucidate the nature of dark matter and dark …
One of the most promising ways to probe intergalactic magnetic fields (IGMFs) is through gamma rays produced in electromagnetic cascades initiated by high-energy gamma rays or …
The isotropy and homogeneity of the cosmic microwave background (CMB) favors “scalar driven” early Universe inflationary models. However, gauge fields and other non-scalar …