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pro vyhledávání: '"Federico Maria Guercilena"'
Publikováno v:
The Astrophysical Journal Letters, Vol 962, Iss 2, p L24 (2024)
The recent detection of the live isotopes ^60 Fe and ^244 Pu in deep ocean sediments dating back to the past 3–4 Myr poses a serious challenge to the identification of their production site(s). While ^60 Fe is usually attributed to standard core-co
Externí odkaz:
https://doaj.org/article/604d46f2d6ca4a83bbc8bcca48988d57
Autor:
Alessandro Camilletti, Leonardo Chiesa, Giacomo Ricigliano, Albino Perego, Lukas Chris Lippold, Surendra Padamata, Sebastiano Bernuzzi, David Radice, Domenico Logoteta, Federico Maria Guercilena
GW190425 was the second gravitational wave (GW) signal compatible with a binary neutron star (BNS) merger detected by the Advanced LIGO and Advanced Virgo detectors. Since no electromagnetic counterpart was identified, whether the associated kilonova
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ff17267dc710a4fbae01f4df099c18b0
http://arxiv.org/abs/2204.05336
http://arxiv.org/abs/2204.05336
Autor:
Marco Cusinato, Federico Maria Guercilena, Albino Perego, Domenico Logoteta, David Radice, Sebastiano Bernuzzi, Stefano Ansoldi
Neutrinos are copiously emitted by neutron star mergers, due to the high temperatures reached by dense matter during the merger and its aftermath. Neutrinos influence the merger dynamics and shape the properties of the ejecta, including the resulting
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a5b52d345a7b2feaaf3ce7d6241b9730
http://hdl.handle.net/11390/1230007
http://hdl.handle.net/11390/1230007