Zobrazeno 1 - 10
of 308
pro vyhledávání: '"Mukhamedzhanov, A.M."'
Publikováno v:
In Physics Reports November 2012 520(3):135-174
Publikováno v:
EPJ Web of Conferences, Vol 184, p 01002 (2018)
We briefly describe the cosmological lithium problems followed by a summary of our recent theoretical work on the magnitude of the effects of electron screening, thepossible existence of dark matter parallel universes and the use of non-extensive (Ts
Externí odkaz:
https://doaj.org/article/aa1f8d94ac2f40af8ac40d056bf5dfbd
Autor:
Mrazek J., Burjan V., Kroha V., Mukhamedzhanov A.M., Tribble R., Spitaleri C., Siváček I., Glagolev V., Piskoř Š., Pizzone G.R., La Cognata M., D’Agata G., Tumino A., Lamia L., Sparta R., Rapisarda G., Romano S.
Publikováno v:
EPJ Web of Conferences, Vol 184, p 01014 (2018)
Asymptotic Normalization Coefficients method is one of the indirect methods used in nuclear astrophysics. The method allows to deduce a direct part of a radiative capture cross section from the measurement of a two body reaction under specific condit
Externí odkaz:
https://doaj.org/article/cf01985b06c5433b8ce741047faa2ebc
Publikováno v:
In Annals of Physics 2009 324(7):1516-1546
Autor:
Spitaleri, C., Typel, S., Bertulani, C.A., Mukhamedzhanov, A.M., Kajino, T., Lattuada, M., Cvetinovic, A., Messina, S., Guardo, G.L., Soić, Neven, Milin, Matko, Perrotta, S.S., Chengbo, Li, Čolovic, Petra, D’Agata, G., Dell’Aquila, Daniele, Fatuzzo, C.G., Gulino, M., Hou, S.Q., La Cognata, M., Lattuada, D., Nurkić, Deni, Popočovski, Romana, Skukan, Natko, Szilner, Suzana, Trippella, O., Uroić, Milivoj, Vukman, Nikola
For the first time in an application to nuclear astrophysics, a process induced by the unstable 5He = (4He-n) nucleus, the 3He+5He→2α reaction, has been studied through the Trojan Horse Method (THM). For that purpose, the quasi-free (QF) contribut
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=57a035e5b1ae::f2bdd4f9ec30f3a7684bb2670bcd2f0a
https://www.bib.irb.hr/1103717
https://www.bib.irb.hr/1103717
Autor:
Kiss, G.G., La Cognata, M., Spitaleri, C., Yarmukhamedov, R., 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., Trippella, O., Tumino, A., Anastasiou, M., Kuvin, S.A., Rijal, N., Schmidt, B., Igamov, S.B., Sakuta, S.B., Tursunmakhatov, K.I., Fülöp, Zs., Gyürky, Gy., Szücs, T., Halász, Z., Somorjai, E., Hons, Z., Mrázek, J., Tribble, R.E., Mukhamedzhanov, A.M.
Publikováno v:
In Physics Letters B 10 August 2020 807
Autor:
Kiss, G.G., La Cognata, M., Spitaleri, C., Yarmukhamedov, R., 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., Trippella, O., Tumino, A., Anastasiou, M., Kuvin, S.A., Rijal, N., Schmidt, B., Igamov, S.B., Sakuta, S.B., Tursunmakhatov, K.I., Fülöp, Zs., Gyürky, Gy., Szücs, T., Halász, Z., Somorjai, E., Hons, Z., Mrázek, J., Tribble, R.E., Mukhamedzhanov, A.M.
Publikováno v:
Physics Letters
The detection of the neutrinos produced in the p−p chain and in the CNO cycle can be used to test the Standard Solar Model. The $^{3}$He(α,γ)$^{7}$Be reaction is the first reaction of the 2nd and 3rd branch of the p−p chain, therefore, the unce
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______3000::89c51c14f8a4213dc34b9afe250d2642
http://repo.scoap3.org/api
http://repo.scoap3.org/api
Autor:
Mukhamedzhanov, A.M., Blokhintsev, L.D., Brown, S., Burjan, V., Cherubini, S., Goldberg, V.Z., Gulino, M., Irgaziev, B.F., Johnson, E., Kemper, K., Kroha, V., La Cognata, M., Lamia, L., Momotyuk, A., Pizzone, R.G., Roeder, B., Rogachev, G., Romano, S., Spitaleri, C., Tribble, R.E., Tumino, A.
Publikováno v:
In Nuclear Physics, Section A 2007 787(1):321-328
Autor:
La Cognata M., Spitaleri C., Trippella O., Kiss G.G., Rogachev G.V., Mukhamedzhanov A.M., Avila M., Guardo G.L., Koshchiy E., Kuchera A., Lamia L., Puglia S.M.R., Romano S., Santiago D., Spartà R.
Publikováno v:
EPJ Web of Conferences, Vol 86, p 00023 (2015)
The 13C(α, n)16O reaction is the neutron source for the main component of the s-process. It is is active inside the helium-burning shell of asymptotic giant branch stars, at temperatures ≲ 108 K. In this temperature region, corresponding to an ene
Externí odkaz:
https://doaj.org/article/0f294b620b42444398d5e1db3c4561d0
Publikováno v:
European Physical Journal A
European Physical Journal A, EDP Sciences, 2020, 56 (3), pp.87. ⟨10.1140/epja/s10050-020-00075-2⟩
European Physical Journal A, EDP Sciences, 2020, 56 (3), pp.87. ⟨10.1140/epja/s10050-020-00075-2⟩
Since the discovery of molecular resonances in $^{12}$C+$^{12}$C in the early sixties a great deal of research work has been undertaken to study $\alpha$-clustering and resonant effects of the fusion process at sub-Coulomb barrier energies. The modif
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8aa08f870b62af1755aabf09d44eef27
http://arxiv.org/abs/1909.06021
http://arxiv.org/abs/1909.06021