Zobrazeno 1 - 10
of 73
pro vyhledávání: '"M. M. Saez"'
The interaction of dark matter particles (weakly interacting massive particles (WIMPs)) with the odd-mass [Formula: see text]Ge and [Formula: see text]Xe target nuclei, that is, the recoil rates corresponding to the elastic scattering of WIMPs by the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::514f252988c0ff26d86289dc826a6462
http://arxiv.org/abs/2302.00879
http://arxiv.org/abs/2302.00879
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:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7dc5232b0ec39af51f6fe9d0c5c2eebf
http://arxiv.org/abs/2202.03887
http://arxiv.org/abs/2202.03887
The production of heavy-mass elements due to the rapid neutron-capture mechanism ([Formula: see text]-process) is associated with astrophysical scenarios, such as supernovae and neutron-star mergers. In the [Formula: see text]-process the capture of
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ed278b9976cb1f9147a2bf3df59eb408
http://arxiv.org/abs/2105.03202
http://arxiv.org/abs/2105.03202
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:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1d683e2cd573438227452c22beeb2285
http://arxiv.org/abs/2006.08043
http://arxiv.org/abs/2006.08043
Publikováno v:
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
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:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6cc1dedf1ab399fc06ce338bc4fa393d
Publikováno v:
SEDICI (UNLP)
Universidad Nacional de La Plata
instacron:UNLP
Universidad Nacional de La Plata
instacron:UNLP
In the present work, we discuss the effects of the inclusion of sterile–active neutrino oscillations during the production of primordial light-nuclei. We assume that the sterile neutrino mass-eigenstate might oscillate with the two lightest active
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6abc2f93938ead25d5af0865d7424dbb
http://www.worldscientific.com/doi/abs/10.1142/S0218301314500803
http://www.worldscientific.com/doi/abs/10.1142/S0218301314500803
Publikováno v:
International Journal of Modern Physics E: Nuclear Physics; Jan2023, Vol. 32 Issue 1, p1-18, 18p
Autor:
Maldonado, Maria
Publikováno v:
Biochemical Society Transactions; Aug2024, Vol. 52 Issue 4, p1647-1659, 13p
Publikováno v:
International Journal of Modern Physics E: Nuclear Physics; Mar2022, Vol. 31 Issue 3, p1-21, 21p
Publikováno v:
International Journal of Modern Physics E: Nuclear Physics; Apr2021, Vol. 30 Issue 04, pN.PAG-N.PAG, 15p