Zobrazeno 1 - 10
of 17
pro vyhledávání: '"Stephane Goriely"'
Publikováno v:
Galaxies, Vol 12, Iss 5, p 66 (2024)
Asymptotic giant branch (AGB) stars can experience proton ingestion events (PIEs), leading to a rich nucleosynthesis. During a PIE, the intermediate neutron capture process (i-process) develops, leading to the production of trans-iron elements. It is
Externí odkaz:
https://doaj.org/article/0f62a99c77fa431db71a543b64665540
Autor:
Chiaki Kobayashi, Ilya Mandel, Krzysztof Belczynski, Stephane Goriely, Thomas H. Janka, Oliver Just, Ashley J. Ruiter, Dany Vanbeveren, Matthias U. Kruckow, Max M. Briel, Jan J. Eldridge, Elizabeth Stanway
Publikováno v:
The Astrophysical Journal Letters, Vol 943, Iss 2, p L12 (2023)
Comparing Galactic chemical evolution models to the observed elemental abundances in the Milky Way, we show that neutron star mergers can be a leading r-process site only if at low metallicities such mergers have very short delay times and significan
Externí odkaz:
https://doaj.org/article/fed8bcd160d74876b079f92dadbea49d
Autor:
Felix Weber, Thomas E. Albrecht-Schönzart, Saleh O. Allehabi, Sebastian Berndt, Michael Block, Holger Dorrer, Christoph E. Düllmann, Vladimir A. Dzuba, Julie G. Ezold, Victor V. Flambaum, Vadim Gadelshin, Stephane Goriely, Ashley Harvey, Reinhard Heinke, Stephane Hilaire, Magdalena Kaja, Tom Kieck, Nina Kneip, Ulli Köster, Jeremy Lantis, Christoph Mokry, Danny Münzberg, Steven Nothhelfer, Stephan Oberstedt, Sophie Péru, Sebastian Raeder, Jörg Runke, Volker Sonnenschein, Matou Stemmler, Dominik Studer, Petra Thörle-Pospiech, Hideki Tomita, Norbert Trautmann, Shelley Van Cleve, Jessica Warbinek, Klaus Wendt
Publikováno v:
Physical Review C. 107
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::403a82dbe87b4f827a4dc2879515209c
https://doi.org/10.1103/physrevc.107.034313
https://doi.org/10.1103/physrevc.107.034313
Autor:
Stephane Goriely, Ina Kullmann
Publikováno v:
Handbook of Nuclear Physics ISBN: 9789811588181
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::f6a61f606aafd2f3d847bba31bdb71a3
https://doi.org/10.1007/978-981-15-8818-1_91-1
https://doi.org/10.1007/978-981-15-8818-1_91-1
Autor:
Anu Kankainen, Stephane Goriely
Publikováno v:
The Euroschool on Exotic Beams, Vol. VI ISBN: 9783031107504
Nuclear astrophysics aims to understand the origin of elements and the role of nuclear processes in astrophysical events. Nuclear reactions and reaction rates depend strongly on nuclear properties and on the astrophysical environment. Nuclear inputs
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::506ac6cb074c2d79ebe1d0fb739f1795
http://urn.fi/URN:NBN:fi:jyu-202212135575
http://urn.fi/URN:NBN:fi:jyu-202212135575
Models based on nuclear energy density functionals can provide access to a multitude of observables for thousands of nuclei in a single framework with microscopic foundations. Such models can rival the accuracy of more phenomenological approaches, bu
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3d6020f3557182aca9db1721094e498a
Publikováno v:
Handbook of Nuclear Physics ISBN: 9789811588181
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::a5655df8e4dc4f63b9987fdf09cbbc7b
https://doi.org/10.1007/978-981-15-8818-1_101-1
https://doi.org/10.1007/978-981-15-8818-1_101-1
Publikováno v:
EPJ Web of Conferences. 279:07001
The intermediate neutron-capture process is thought to arise when protons are mixed in a convective helium-burning zone. This can happen during the early Thermally-Pulsing (TP) Asymptotic Giant Branch (AGB) phase of low-mass, low-metallicity stars. A
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e8ab5a01f2ec62aa1395cee8f015dd31
https://doi.org/10.1051/epjconf/202327907001
https://doi.org/10.1051/epjconf/202327907001
Publikováno v:
Eur.Phys.J.A
Eur.Phys.J.A, 2021, 57 (12), pp.333. ⟨10.1140/epja/s10050-021-00642-1⟩
Eur.Phys.J.A, 2021, 57 (12), pp.333. ⟨10.1140/epja/s10050-021-00642-1⟩
The modeling of nuclear reactions and radioactive decays in astrophysical or earth-based conditions requires detailed knowledge of the masses of essentially all nuclei. Microscopic mass models based on nuclear energy density functionals (EDFs) can be
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::41b9f0b5293a6effcdca82570f24d493
http://arxiv.org/abs/2011.07904
http://arxiv.org/abs/2011.07904
Autor:
Chamel, Nicolas, Pearson, John Michael, Potekhin, Alexander Y., Fantina, Anthea F., Ducoin, Camille, Dutta, Anup, ´, Stephane Goriely, Perot, Loïc
Publikováno v:
AIP Conference Proceedings; 7/30/2019, Vol. 2127 Issue 1, p020021-1-020021-13, 13p