Zobrazeno 1 - 10
of 34
pro vyhledávání: '"de Séréville Nicolas"'
Autor:
Bastin Beyhan, Kiener Jürgen, Deloncle Isabelle, Coc Alain, Pospelov Maxim, Mrazek Jaromir, Lamia Livio, Ackermann Dieter, Adsley Philip, Bacri Charles-Olivier, Bourçois Jérôme, Burjan Vaclav, Cassisa Anastasia, D’agata Giuseppe, De France Gilles, Di Pietrio Alessia, Demane Yasmine, De Oliveira François, Donaldson Lindsay, Donzaud Corinne, Ducret Jean-Eric, Hamadache Clarisse, Hammache Fairouz, Jones Pete, La Cognata Marco, Laviron Adrien, Lewitowicz Marek, Malatji Kgashane, Massara Antonio, Pitrou Cyril, Pizzone Rosario Gianluca, Guardo Giovanni Luca, Płoszajczak Marek, Rapisarda Giuseppe, Rebeiro Bernadette, Roussèire Brigitte, Santonocito Domenico, de Séréville Nicolas, Sergi Maria Letizia, Simeckova Eva, Sorlin Olivier, Stodel Christelle, Tatischeff Vincent, Thomas Jean-Charles, Tumino Aurora
Publikováno v:
EPJ Web of Conferences, Vol 275, p 01012 (2023)
Several experiments around the world are looking for a new particle, named Dark Boson, which may do the link between the Ordinary Matter (which forms basically stars, planets, interstellar gas...) and the Hidden Sectors of the Universe. This particle
Externí odkaz:
https://doaj.org/article/53ece56ab0bd494283dc0bb1f7124442
Autor:
Harrouz Djamila-Sarah, de Séréville Nicolas, Adsley Philip, Hammache Faïrouz, Longland Richard, Bastin Beyhan, Faestermann Thomas, Hertenberger Ralf, La Cognata Marco, Lamia Livio, Meyer Anne, Palmerini Sara, Pizzone Rosario Gianluca, Romano Stefano, Tumino Aurora, Wirth Hans-Friedrich
Publikováno v:
EPJ Web of Conferences, Vol 260, p 01003 (2022)
Some observed abundances in globular clusters have suggested the existence of multiple generations of stars within the clusters as the observations require temperature ranges higher than current stars. The 30Si(p,γ)31P reaction plays a key role in t
Externí odkaz:
https://doaj.org/article/a3928abaa64741a1abd7135bb2dfc129
Autor:
de Séréville, Nicolas, Tatischeff, Vincent, Cristofari, Pierre, Gabici, Stefano, Diehl, Roland
The presence of live $^{60}$Fe nuclei (lifetime of 3.8~Myr) in cosmic rays detected by the ACE/CRIS instrument suggests a nearby nucleosynthesis source. $^{60}$Fe is primarily produced in core-collapse supernovae, and we aim to clarify whether the de
Externí odkaz:
http://arxiv.org/abs/2401.17660
Autor:
Gulino Marisa, Cherubini Silvio, Gabriele Rapisarda Giuseppe, Kubono Shigeru, Lamia Livio, La Cognata Marco, Gianluca Pizzone Rosario, Yamaguchi Hidetoshi, Hayakawa Seya, Wakabayashi Yasuo, Iwasa Naohito, Kato Seigo, Komatsubara Tetsuro, Teranishi Takashi, Coc Alain, de Séréville Nicolas, Hammache Fairouz, Kiss Gabor, Bishop Shawn, Nguyen Binh Dam, Roeder Brian, Trache Livius, Tribble Robert, Spartà Roberta, Indelicato Iolanda, Spitaleri Claudio
Publikováno v:
EPJ Web of Conferences, Vol 184, p 01008 (2018)
The Trojan Horse Method (THM) is an indirect method that allows to get information about a two body reaction cross-section even at very low energy, avoiding the suppression effects due to the presence of the Coulomb barrier. The method requires a ver
Externí odkaz:
https://doaj.org/article/ad7922e9eb2a489b940f6dd5bd791f11
Publikováno v:
EPJ Web of Conferences, Vol 165, p 01022 (2017)
It has been recently suggested that hydrogen ingestion into the helium shell of massive stars could lead to high 13C and 15N excesses when the blast of a core collapse supernova (ccSN) passes through its helium shell. This prediction questions the or
Externí odkaz:
https://doaj.org/article/cde886f45b69461e95bff378da0a0ee0
Autor:
Fruet Guillaume, Courtin Sandrine, Jenkins David G., Heine Marcel, Montanari Daniele, Morris Luke G., Adsley Philip, Beck Christian, Della Negra Serge, Haas Florent, Hammache Fairouz, Kirsebom Oliver S., Meyer Anne, Regan Patrick H., Rudiger Matthias, de Séréville Nicolas, Stodel Christelle
Publikováno v:
EPJ Web of Conferences, Vol 163, p 00018 (2017)
This contribution is focused on the STELLA project (STELlar LAboratory), which aims at the measurement of fusion cross sections between light heavy ions like 12C+12C, 12C+16O or 16O+16O at deep subbarrier energies. The gamma-particle coincidence tech
Externí odkaz:
https://doaj.org/article/3d7ed80e0cc14bb8b8b8449b30abae0c
Autor:
Palmerini, Sara, La Cognata, Marco, Hammache, Fairouz, Acosta, Luis, Alba, Rosa, Burjan, Vaclav, Chavez, Efrain, Cherubini, Silvio, Cvetinovic, Alexandra, D'Agata, Giuseppe, De Sereville, Nicolas, Di Pietro, Alessia, Figuera, Pierpaolo, Fullop, Zsolt, Rios, Karen De Los, Guardo, Giovanni Luca, Gulino, Marisa, Hayakawa, Seiya, Kiss, Gabor, La Commara, Marco, Lamia, Livio, Manicò, Concetta Maiolino Giulio, Matei, Catalin, Mazzocco, Marco, Mrazek, Jaromir, Parascandolo, Tina, Petruse, Teodora, Pierroutsakou, Dimitra, Pizzone, Rosario Gianluca, Rapisarsa, Giuseppe Gabriele, Romano, Stefano, Santonocito, Domenico, Sergi, Maria Letizia, Spartà, Roberta, Tumino, Aurora, Yamaguchi, Hidetoshi
The 27Al(p,a)24Mg reaction, which drives the destruction of 27Al and the production of 24Mg in stellar hydrogen burning, has been investigated via the Trojan Horse Method (THM) by measuring the 2H(27Al,a24Mg)n three-body reaction. The experiment cove
Externí odkaz:
http://arxiv.org/abs/2108.06145
Nuclear reaction rates are one of the most important ingredients in describing how stars evolve. The study of the nuclear reactions involved in different astrophysical sites is thus mandatory to address most questions in nuclear astrophysics. Direct
Externí odkaz:
http://arxiv.org/abs/2107.13228
Publikováno v:
A&A 642, A41 (2020)
Context. Monte Carlo methods can be used to evaluate the uncertainty of a reaction rate that arises from many uncertain nuclear inputs. However, until now no attempt has been made to find the effect of correlated energy uncertainties in input resonan
Externí odkaz:
http://arxiv.org/abs/2007.03802
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.