Zobrazeno 1 - 6
of 6
pro vyhledávání: '"La Cognata Marco"'
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
Autor:
Chieffi, Alessandro, Roberti, Lorenzo, Limongi, Marco, La Cognata, Marco, Lamia, Livio, Palmerini, Sara, Pizzone, Rosario Gianluca, Sparta', Roberta, Tumino, Aurora
We discuss how the new measurement of the $^{12}C+^{12}C$ fusion cross section carried out with the Trojan Horse Method (Tumino, A., Spitaleri, C., La Cognata, M., et al., 2018, Nature 57, 687) affects the compactness of a star, i.e. basically the bi
Externí odkaz:
http://arxiv.org/abs/2106.00013
Autor:
Pidatella, Angelo, Cristallo, Sergio, Galatà, Alessio, La Cognata, Marco, Mazzaglia, Maria, Perego, Albino, Spartà, Roberta, Tumino, Aurora, Vescovi, Diego, Mascali, David
Publikováno v:
IL NUOVO CIMENTO C 44, 65 (2021)
In the context of the INFN project PANDORA_Gr3 (Plasma for Astrophysics, Nuclear Decays Observation and Radiation for Archaeometry) and of multi-messenger astronomy, we propose a feasibility study for in-laboratory plasma's opacity investigation, in
Externí odkaz:
http://arxiv.org/abs/2101.05814
Autor:
Adsley, Philip, Battino, Umberto, Best, Andreas, Caciolli, Antonio, Guglielmetti, Alessandra, Imbriani, Gianluca, Jayatissa, Heshani, La Cognata, Marco, Lamia, Livio, Masha, Eliana, Massimi, Cristian, Palmerini, Sara, Tattersall, Ashley, Hirschi, Raphael
The competing $^{22}$Ne($\alpha,\gamma$)$^{26}$Mg and $^{22}$Ne($\alpha,n$)$^{25}$Mg reactions control the production of neutrons for the weak $s$-process in massive and AGB stars. In both systems, the ratio between the corresponding reaction rates s
Externí odkaz:
http://arxiv.org/abs/2005.14482
Autor:
Trippella, Oscar, La Cognata, Marco
The $^{13}{\rm C}(\alpha,n)^{16}{\rm O}$ reaction is considered to be the main neutron source responsible for the production of heavy nuclides (from ${\rm Sr}$ to ${\rm Bi}$) through slow $n$-capture nucleosynthesis ($s$-process) at low temperatures
Externí odkaz:
http://arxiv.org/abs/1702.01589
Autor:
Qun-Gang, Wen, Cheng-Bo, Li, Shu-Hua, Zhou, Irgaziev, Bakhadir, Yuan-Yong, Fu, Spitaleri, Claudio, La Cognata, Marco, Jing, Zhou, Qiu-Ying, Meng, Lamia, Livio, Lattuada, Marcello
Publikováno v:
Phys. Rev. C 93, 035803 (2016)
To explore a possible indirect method for $\rm ^8Be$ induced astrophysical reactions, the $\rm ^9Be=({}^8Be+\it n)$ cluster structure was studied via the Trojan Horse Method. It is the first time to study a super short life nucleus $\rm ^8Be$ via the
Externí odkaz:
http://arxiv.org/abs/1412.8577