Results 11 to 20 of about 1,983,143 (282)

ANC experiments for nuclear astrophysics [PDF]

EPJ Web of Conferences, 2020
Among the indirect methods to determine nuclear cross-section present in literature, the so-called Asymptotic Normalization Coefficient (ANC) has proven to be useful in retrieving the direct part of a radiative capture cross-section in reactions of ...
D’Agata G., Burjan V., Mrázek J., Glagolev V., Kilic A. I., Kroha V., La Cognata M., Lamia L., Palmerini S., Piskoř Š., Pizzone R. G., Rapisarda G. G., Romano S., Siváĉek I., Spitaleri C., Spartá R., Tumino A.   +16 more
doaj   +6 more sources

Nuclear Astrophysics: CIPANP 2006 [PDF]

AIPConf.Proc.870:33-43,2006, 2006
I review progress that has been made in nuclear astrophysics over the past few years and summarize some of the questions that remain. Topics selected include solar neutrinos, supernovae (the explosion and associated nucleosynthesis), laboratory astrophysics, and neutron star structure.
arxiv   +4 more sources

Experimental nuclear astrophysics in Italy [PDF]

Rivista Del Nuovo Cimento, 2019
Nuclear astrophysics, the union of nuclear physics and astronomy, went through an impressive expansion during the last twenty years. This could be achieved thanks to milestone improvements in astronomical observations, cross section measurements ...
C. Broggini, O. Straniero, M. Taiuti, G. Angelis, G. Benzoni, G. Bruno, S. Bufalino, G. Cardella, N. Colonna, M. Contalbrigo, Giuseppe Cosentino, S. Cristallo, C. Curceanu, E. Filippo, R. Depalo, A. Leva, A. Feliciello, S. Gammino, A. Galatà, M. Cognata, R. Lea, S. Leoni, I. Lombardo, V. Manzari, D. Mascali, C. Massimi, A. Mengoni, D. Mengoni, D. Napoli, S. Palmerini, S. Piano, S. Pirrone, R. Pizzone, G. Politi, P. Prati, Gianfranco Prete, P. Russotto, G. Tagliente, G. Urciuoli   +38 more
semanticscholar   +7 more sources

Reactor neutrons in nuclear astrophysics [PDF]

EPJ Web of Conferences, 2017
The huge neutron fluxes offer the possibility to use research reactors to produce isotopes of interest, which can be investigated afterwards. An example is the half-lives of long-lived isotopes like 129I.
Reifarth René, Glorius Jan, Göbel Kathrin, Heftrich Tanja, Jentschel Michael, Jurado Beatriz, Käppeler Franz, Köster Ulli, Langer Christoph, Litvinov Yuri A., Weigand Mario   +10 more
doaj   +6 more sources

Nuclear astrophysics at FRANZ [PDF]

Journal of Physics: Conference Series, 2018
The neutron capture cross section of radioactive isotopes for neutron energies in the keV region will be measured by a time-of-flight (TOF) experiment. NAUTILUS will provide a unique facility realizing the TOF technique with an ultra-short flight path at
R. Reifarth, S. Dababneh, S. Fiebiger, J. Glorius, K. Göbel, M. Heil, P. Hillmann, T. Heftrich, C. Langer, O. Meusel, R. Plag, S. Schmidt, Z. Slavkovská, D. Veltum, M. Weigand, C. Wiesner, C. Wolf, A. Zadeh   +17 more
semanticscholar   +4 more sources

Transfer reactions for nuclear astrophysics [PDF]

EPJ Web of Conferences, 2018
Direct measurements of cross sections at stellar energies are very challenging - if at all possible. This is essentially due to the very low cross-sections of the reactions of interest (especially when it involves charged particles), and/or to the ...
Hammache Fairouz
doaj   +4 more sources

Frontiers in Nuclear Astrophysics [PDF]

Progress in Particle and Nuclear Physics, 2016
88 pages, 10 figures, 613 references, Progress in Particle and Nuclear Physics ...
C. Bertulani, T. Kajino
semanticscholar   +5 more sources

The Nuclear Astrophysics program at n_TOF (CERN) [PDF]

EPJ Web of Conferences, 2017
An important experimental program on Nuclear Astrophysics is being carried out at the n_TOF since several years, in order to address the still open issues in stellar and primordial nucleosynthesis.
Colonna N., Aberle O., Andrzejewski J., Audouin L., Bacak M., Balibrea J., Barbagallo M., Bečvář F., Berthoumieux E., Billowes J., Bosnar D., Brown A., Caamaño M., Calviño F., Calviani M., Cano-Ott D., Cardella R., Casanovas A., Cerutti F., Chen Y. H., Chiaveri E., Clai G., Cortés G., Cortés-Giraldo M. A., Cosentino, Cristallo S., Damone L. A., Diakaki M., Domingo-Pardo C., Dressler L. R., Dupont E., Durán I., Fernández-Domínguez B., Ferrari A., Ferreira P., Finocchiaro P., Furman V., Göbel K., García A. R., Gawlik A., Gilardoni S., Glodariu T., Gonçalves I. F., González E., Griesmayer E., Guerrero C., Gunsing F., Harada H., Heinitz S., Hernandez-Prieto A., Heyse J., Jenkins D. G., Jericha E., Käppeler F., Kadi Y., Kalamara A., Kavrigin P., Kimura A., Kivel N., Kokkoris M., Kroll J., Krtička M., Kurtulgil D., Langer C., Leal-Cidoncha E., Lederer C., Lerendegui-Marco J., Leeb H., Lo Meo S., Lonsdale S. J., Losito S., Macina D., Mallik A., Marganiec J., Martínez T., Masi A., Massimi C., Mastinu P., Mastromarco M., Maugeri E. A., Mazzone A., Mendoza E., Mengoni A., Mingrone F., Milazzo P. M., Mirea M., Musumarra A., Negret A., Nolte R., Oprea A., Patronis N., Pavlik A., Perkowski J., Piersanti L., Porras I., Praena J., Quesada J. M., Radeck D., Rauscher T., Reifarth R., Riego A., Robles M.S., Rubbia C., Ryan J. A., Sabaté-Gilarte M., Saxena A., Schillebeeckx P., Schumann D., Sedyshev P., Smith A. G., Sosnin N. V., Stamatopoulos A., Tagliente G., Tain J. L., Tarifeño-Saldivia A., Tassan-Got L., Tsinganis A., Valenta S., Vannini G., Variale V., Vaz P., Ventura A., Vlachoudis V., Vlastou R., Wallner A., Warren S., Weiss C., Woods P. J., Wright T., Žugec P.   +129 more
doaj   +10 more sources

A New Mass Model for Nuclear Astrophysics: Crossing 200 keV Accuracy [PDF]

Universe, 2021
By using a machine learning algorithm, we present an improved nuclear mass table with a root mean square deviation of less than 200 keV. The model is equipped with statistical error bars in order to compare with available experimental data.
M. Shelley, A. Pastore
semanticscholar   +1 more source

Transfer Reactions As a Tool in Nuclear Astrophysics [PDF]

Frontiers of Physics, 2021
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.
F. Hammache, N. de Séréville
semanticscholar   +1 more source