Zobrazeno 1 - 10
of 137
pro vyhledávání: '"Guardo G.L."'
Publikováno v:
EPJ Web of Conferences, Vol 297, p 00001 (2024)
Externí odkaz:
https://doaj.org/article/4181aaddb77f45c3aa62ae374d0617aa
Autor:
La Cognata M., Kiss G. G., Yarmukhamedov R., Tursunmakhatov K. I., Wiedenhöver I., Baby L. T., Cherubini S., Cvetinović A., D’Agata G., Figuera P., Guardo G.L., Gulino M., Hayakawa S., Indelicato I., Lamia L., Lattuada M., Mudò F., Palmerini S., Pizzone R.G., Rapisarda G.G., Romano S., Sergi M. L., Spartà R., Spitaleri C., Trippella O., Tumino A., Anastasiou M., Kuvin S. A., Rijal N., Schmidt B., Igamov S. B., Sakuta S. B., Fülöp Zs., Gyürky Gy., Szücs T., Halász Z., Somorjai E., Hons Z., Mrázek J., Tribble R. E., Mukhamedzhanov A. M.
Publikováno v:
EPJ Web of Conferences, Vol 279, p 11001 (2023)
The p - p-chain reaction 3He(α, γ)7Be can sensitively influence the prediction of the 7Be and 8B neutrino fluxes. Despite its importance, the knowledge of its reaction cross section at energies of the core of the Sun (15 keV 30 keV) is limited and
Externí odkaz:
https://doaj.org/article/35441615cd0c4307a522d4b4a7dbca39
Autor:
Spampinato C., Pizzone R.G., Spartà R., Couder M., Tan W., Burian V., Chae K.Y., D’Agata G., Guardo G.L., Indelicato I., Cognata M. La, Lamia L., Lattuada D., Mrazek J., Oliva A., Palmerini S., Prajapati P.M., Rapisarda G.G., Romano S., Sergi M.L., Spitaleri C., Tumino A., Wiescher M., Anguilar S., Bardyan D., Blankstein D., Boccioli L., Callahan L., Clark A., Frentz B., Hall M., Gula A., Henderson S., Kelmar R., Liu Q., Long J., Majumdar A., McGuinness S., Nelson A., O’Malley P., Seyymour C., Skulski M., Wilkinson J.
Publikováno v:
EPJ Web of Conferences, Vol 227, p 02013 (2020)
In the network of reactions present in the Big Bang nucleosynthesis, the 3He(n, p)3H has an important role which impacts the final 7Li abundance. The Trojan Horse Method (THM) has been applied to the 3He(d, pt)H reaction in order to extract the astro
Externí odkaz:
https://doaj.org/article/06bbca1ae6f3443fa3c99858b8c6a6b1
Autor:
Dell‘Aquila D., Lombardo I., Verde G., Vigilante M., Acosta L., Agodi C., Cappuzzello F., Carbone D., Cavallaro M., Cherubini S., Cvetinovic A., D‘Agata G., Francalanza L., Guardo G.L., Gulino M., Indelicato I., La Cognata M., Lamia L., Ordine A., Pizzone R.G., Puglia S.M.R., Rapisarda G.G., Romano S., Santagati G., Spartà R., Spadaccini G., Spitaleri C., Tumino A.
Publikováno v:
EPJ Web of Conferences, Vol 184, p 01005 (2018)
The αdecay path of the Hoyle state in 12C (Ex = 7:654MeV) represents one ofthe most challenging questions of modern nuclear physics. Its knowledge can help in theunderstanding of cluster configurations in light nuclei and the possible existence of B
Externí odkaz:
https://doaj.org/article/4cf3a7439256424390994afe2c4d166c
Autor:
Xu Y., Goriely S., Balabanski D.L., Chesnevskaya S., Guardo G.L., La Cognata M., Lan H.Y., Lattuada D., Luo W., Matei C.
Publikováno v:
EPJ Web of Conferences, Vol 178, p 04007 (2018)
The astrophysical p-process is an important way of nucleosynthesis to produce the stable and proton-rich nuclei beyond Fe which can not be reached by the s- and r-processes. In the present study, the impact of nuclear ingredients, especially the nucl
Externí odkaz:
https://doaj.org/article/45a20b1ca88343a0b9f63b71eaf2e314
Autor:
Lattuada D., La Cognata M., Anzalone A., Balabanski D.L., Chesnevskaya S., Costa M., Crucillà V., Guardo G.L., Gulino M., Matei C., Pizzone R.G., Romano S., Spitaleri C., Tumino A., Xu Y
Publikováno v:
EPJ Web of Conferences, Vol 184, p 02008 (2018)
Present and future gamma-beam facilities represent a great opportunity to validate and evaluate the cross-sections of many photonuclear reactions at near-threshold energies, whose data mostly come from theoretical calculations. We developed a Monte C
Externí odkaz:
https://doaj.org/article/a00c2165dc2a402a806695f5838cbb32
Autor:
Cvetinović A., Spitaleri C., Spartá R., Rapisarda G.G., Puglia S.M.R., La Cognata M., Cherubini S., Guardo G.L., Gulino M., Lamia L., Pizzone R.G., Romano S., Sergi M.L., Tumino A.
Publikováno v:
EPJ Web of Conferences, Vol 184, p 02002 (2018)
The 10B(p,α0)7Be reaction has been studied by applying the Trojan Horse method to the 2H(10B,α0 7Be)n reaction. The bare-nucleus astrophysical S(E)-factor in absolute units was extracted in a wide energy range, from 2.2 MeV to 3 keV and normalized
Externí odkaz:
https://doaj.org/article/6c8a927621d749cda33612d4cf3db216
Autor:
Lamia L., Spitaleri C., Mazzocco M., Boiano A., Boiano C., Broggini C., Caciolli A., Depalo R., Di Pietro A., Figuera P., Galtarossa F., Guardo G.L., Gulino M., Hayakawa S., Kubono S., La Cognata M., La Commara M., La Rana G., Lattuada M., Menegazzo R., Pakou A., Parascandolo C., Piatti D., Pierroutsakou D., Pizzone R.G., Puglia S.M.R., Romano S., Rapisarda G.G., Sanchez-Benitez A.M., Sergi M.L., Sgouros O., Silva H., Soramel F., Soukeras V., Strano E., Torresi D., Trippella O., Tumino A., Yamaguchi H., Villante F.L., Zhang G.L.
Publikováno v:
EPJ Web of Conferences, Vol 165, p 01032 (2017)
The Trojan Horse Method (THM) has been applied extensively for the last 25 years to measure nuclear reaction cross sections of interest for astrophysics. Although it has been mainly applied for charged particle-induced reactions, recently it has been
Externí odkaz:
https://doaj.org/article/ee4eabb0b4ac472794d8338348dfad42
Autor:
Dell’Aquila D., Lombardo I., Verde G., Vigilante M., Acosta L., Agodi C., Cappuzzello F., Carbone D., Cavallaro M., Cherubini S., Cvetinovic A., D’Agata G., Francalanza L., Guardo G.L., Gulino M., Indelicato I., La Cognata M., Lamia L., Ordine A., Pizzone R.G., Puglia S.M.R., Rapisarda G.G., Romano S., Santagati G., Spartà R., Spadaccini G., Spitaleri C., Tumino A.
Publikováno v:
EPJ Web of Conferences, Vol 165, p 01020 (2017)
The Hoyle state in 12C(Ex = 7.654MeV) is characterized by a pronounced 3α cluster configuration. It is involved in the so-called 3α process in stars, that is responsible of 12C nucleosynthesis. We studied the decay path of the Hoyle state by using
Externí odkaz:
https://doaj.org/article/e6a9fef7aefc4f6f90333adffd2e8011
Autor:
Hayakawa S., Spitaleri C., Burtebayev N., Aimaganbetov A., Figuera P., Fisichella M., Guardo G.L., Igamov S., Indelicato I., Kiss G., Kliczewski S., La Cognata M., Lamia L., Lattuada M., Piasecki E., Rapisarda G.G., Romano S., Sakuta S.B., Siudak R., Trzcińska A., Tumino A., Urkinbayev A.
Publikováno v:
EPJ Web of Conferences, Vol 117, p 09013 (2016)
The 16O+16O fusion reaction is important in terms of the explosive oxygen burning process during late evolution stage of massive stars as well as understanding of the mechanism of low-energy heavy-ion fusion reactions. We aim to determine the excitat
Externí odkaz:
https://doaj.org/article/1a757bab8511453099402db0c829ceaf