DSM Alves, N Weiner - Journal of High Energy Physics, 2018 - Springer
A bstract The QCD axion is one of the most compelling solutions of the strong CP problem. There are major current efforts into searching for an ultralight, invisible axion, which is …
The QCD axion remains experimentally viable in the mass range of O (10 MeV) if (i) it couples predominantly to the first generation of SM fermions;(ii) it decays to e+ e-with a short …
Y Giomataris, JD Vergados - Nuclear Instruments and Methods in Physics …, 2004 - Elsevier
The purpose of the present paper is to study the neutrino properties as they may appear in the low-energy neutrinos emitted in triton decay:[Formula: see text] with maximum neutrino …
The coherent contribution of all neutrons in neutrino nucleus scattering due to the neutral current offers a realistic prospect of detecting supernova neutrinos. As a matter of fact for a …
To the eyes of the average person and the trained scientist, the night sky is dark, even though the universe is populated by myriads of bright galaxies. Why this happens is a …
R Horvat, M Krčmar, B Lakić - Physical Review D, 2004 - APS
We explore the potential of the CERN Axion Solar Telescope (CAST) for testing the presence of large extra dimensions. The CAST experiment has originally been proposed to …
JD Vergados, Y Giomataris - Physics of Atomic Nuclei, 2007 - Springer
Supernova neutrinos can easily be detected by a spherical gaseous TPC detector measuring very low energy nuclear recoils. The expected rates are quite large for a neutron …
The coherent contribution of all neutrons in neutrino nucleus scattering due to the neutral current offers a realistic prospect of detecting supernova neutrinos. For a typical supernova …
“CRESST” employs scintillating CaWO4 crystals to search for Dark Matter (DM) induced nuclear recoils. The detector response to a nuclear recoil is described by the quenching …