782 citations · 2.5k across the 51 of their papers we have counts for
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Can one measure the Cosmic Neutrino Background?
Amand Faessler, Rastislav Hodak, Sergey Kovalenko +1
The Cosmic Microwave Background (CMB) yields information about our Universe at around 380 000 years after the Big Bang (BB). Due to the weak interaction of the neutrinos with matte…
Search for the Cosmic Neutrino Background and KATRIN
Amand Faessler, Rastislav Hodak, Sergey Kovalenko +1
The spectrum of the Cosmic Microwave Background follows Planck's black body radiation formula and shows a remarkable constant temperature of T = 2.7. About 380 000 years after the…
Neutrino accompanied beta^-beta^-, beta^+beta^+, beta^+/EC and EC/EC processes within single state dominance hypothesis
P. Domin, S. Kovalenko, F. Simkovic +1
The systematic study of (anti-)neutrino accompanied beta^-beta^-, beta^+beta^+ decays and beta^+/EC, EC/EC electron captures is performed under the assumption of single intermediat…
Nuclear muon-positron conversion mediated by Majorana neutrinos
Pavol Domin, Amand Faessler, Sergey Kovalenko +1
We study lepton number violating (LNV) process of muon-positron conversion in nuclei mediated by the exchange of light and heavy Majorana neutrinos. Nuclear structure calculations…