Zobrazeno 1 - 10
of 31
pro vyhledávání: '"Saez, M. M."'
Abstract: The interaction of dark matter particles (WIMPs) with the odd-mass $^{73}$Ge and $^{131}$Xe target nuclei ,{ {that is the recoil rates corresponding to the elastic scattering of WIMPs by these nuclei}}, is analysed in the context of the min
Externí odkaz:
http://arxiv.org/abs/2302.00879
Publikováno v:
International Journal of Modern Physics E, Volume 30, Issue 12, id. 2150107, (2021)
Dark Matter particles can be detected directly via their elastic scattering with nuclei. Next generation experiments can eventually find physical evidences about dark matter candidates. With this motivation in mind, we have calculated the expected si
Externí odkaz:
http://arxiv.org/abs/2202.03887
Neutrinos play an important role in core-collapse supernova events since they are a key piece to understand the explosion mechanisms. The analysis of the neutrino fluxes can bring answers to neutrino's related problems e.g.: mass hierarchy, spectral
Externí odkaz:
http://arxiv.org/abs/2109.06244
The production of heavy-mass elements due to the rapid neutron-capture mechanism (r-process) is associated with astrophysical scenarios, such as supernovae and neutron-star mergers. In the r-process the capture of neutrons is followed by $\beta$-deca
Externí odkaz:
http://arxiv.org/abs/2105.03202
Publikováno v:
International Journal of Modern Physics E 2020
A possible mechanism for the formation of heavy-mass elements in supernovae is the rapid neutron-capture-mechanism (r-process). It depends upon the electron-fraction $Y_e$, a quantity which is determined by beta-decay-rates. In this paper, we focus o
Externí odkaz:
http://arxiv.org/abs/2006.08043
Publikováno v:
Boletin de la Asociacion Argentina de Astronomia. Volumen 60. 2018
The inclusion of massive neutrinos affects the cross sections involved in the formation of heavy nuclei, modifying their abundances. Rapid neutron capture processes (r-process) are often associated with explosive events such as core-collapse supernov
Externí odkaz:
http://arxiv.org/abs/1809.01063
Publikováno v:
International Journal of Modern Physics D. volume = {27}, number = {12}, pages = {1850116}, year = {2018}
Neutrino induced reactions are a basic ingredient in astrophysical processes like star evolution. The existence of neutrino oscillations affects the rate of nuclear electroweak decays which participates in the chain of events that determines the fate
Externí odkaz:
http://arxiv.org/abs/1808.03249
Publikováno v:
International Journal of Modern Physics E. 31
Neutrinos play an important role in core-collapse supernova events since they are a key piece to understand the explosion mechanisms. The analysis of the neutrino fluxes can bring answers to neutrino's related problems e.g.: mass hierarchy, spectral
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