Zobrazeno 1 - 10
of 55
pro vyhledávání: '"Gyuri Gyürky"'
Autor:
Davide Trezzi, L. Di Paolo, I. Kochanek, V. Mossa, F. Ferraro, P. Colombetti, Carlo Bruno, K. Stöckel, Paolo Prati, Sandra Zavatarelli, F. R. Pantaleo, M. Junker, J. Balibrea-Correa, E. M. Fiore, A. Formicola, Gyuri Gyürky, F. Barile, G. Gervino, T. Chillery, G. F. Ciani, R. Depalo, A. Di Leva, Z. Elekes, M. P. Takács, R. Perrino, A. Best, Oscar Straniero, Marialuisa Aliotta, Filippo Terrasi, A. Guglielmetti, László Csedreki, A. Boeltzig, P. Corvisiero, C. Gustavino, F. Cavanna, Antonio Caciolli, Zs. Fülöp, Gianluca Imbriani, Carlo Broggini, M. Lugaro, E. Masha, Luigi Schiavulli, Daniel Bemmerer, Paola Marigo, D. Piatti, Roberto Menegazzo, Tamás Szücs, V. Paticchio, Thomas Davinson
Publikováno v:
The European Physical Journal A. 56
Direct measurements of reaction cross-sections at astrophysical energies often require the use of solid targets able to withstand high ion beam currents for extended periods of time. Thus, monitoring target thickness, isotopic composition, and target
Autor:
Gianluca Imbriani, Gianpiero Mangano, F. Ferraro, K. Stöckel, Thomas Davinson, F. R. Pantaleo, F. Cavanna, R. Menegazzo, E. M. Fiore, E. Masha, Luigi Schiavulli, A. Best, M. Junker, M. P. Takács, Oscar Straniero, I. Kochanek, Daniel Bemmerer, Gyuri Gyürky, A. Guglielmetti, László Csedreki, D. Piatti, Ofelia Pisanti, Marialuisa Aliotta, Tamás Szücs, G. Gervino, Michele Viviani, A. Di Leva, R. Perrino, Laura Elisa Marcucci, Carlo Broggini, Sandra Zavatarelli, Paola Marigo, Davide Trezzi, Maria Lugaro, G. F. Ciani, V. Paticchio, A. Formicola, A. Boeltzig, Alejandro Kievsky, Zs. Fülöp, C. Gustavino, Rosanna Depalo, C. G. Bruno, Z. Elekes, Paolo Prati, Antonio Caciolli, Francesco Barile, V. Mossa, P. Corvisiero, T. Chillery
Publikováno v:
Nature 587(2020), 210-213
Aliotta, M, Bruno, C G & Chillery, T & Davinson, T 2020, ' The baryon density of the Universe from an improved rate of deuterium burning ', Nature, vol. 587, pp. 210-213 . https://doi.org/10.1038/s41586-020-2878-4
Aliotta, M, Bruno, C G & Chillery, T & Davinson, T 2020, ' The baryon density of the Universe from an improved rate of deuterium burning ', Nature, vol. 587, pp. 210-213 . https://doi.org/10.1038/s41586-020-2878-4
Light elements were produced in the first few minutes of the Universe through a sequence of nuclear reactions known as Big Bang nucleosynthesis (BBN)1,2. Among the light elements produced during BBN1,2, deuterium is an excellent indicator of cosmolog
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::acc7c9771ebf8cadc24dc4679504e934
http://hdl.handle.net/11588/827426
http://hdl.handle.net/11588/827426
Autor:
H. Törnqvist, C. Brandau, B. Löher, T. Kisselbach, U. Spillmann, M. Steck, X. C. Chen, Tamás Szücs, Yu. A. Litvinov, L. Varga, R. Hensch, T. T. Nguyen, B. Thomas, Herbert A. Simon, C. Trageser, N. Klapper, O. Hinrichs, N. Petridis, M. Wang, B. Brückner, M. Groothuis, S. Yu. Torilov, Kathrin Göbel, T. Kausch, M. Volknandt, Thomas Davinson, Y. H. Zhang, Claudia Lederer-Woods, S. Fiebiger, Z. Slavkovská, T. Gaßner, Beatriz Jurado, A. Khodaparast, P. Hillmann, Christoph Langer, C. Kozhuharov, Lukas Bott, P. M. Hillenbrand, Mario Weigand, A. Taremi Zadeh, C. Wolf, R.J. Chen, Deniz Kurtulgil, U. Popp, Gyuri Gyürky, Jan Glorius, Sergey Litvinov, Xiaojuan Zhou, Thomas Stöhlker, P. Erbacher, Michael Lestinsky, Rene Reifarth, Gregory Lane, M. S. Sanjari, Matthew Reed, J. Stumm, Philip Woods, Matthias Heil, Y. M. Xing, R. Hess, A. Gumberidze, Saed Dababneh, Sergiy Trotsenko
Publikováno v:
Nucl.Instrum.Meth.A
Nucl.Instrum.Meth.A, 2020, 982, pp.164367. ⟨10.1016/j.nima.2020.164367⟩
Xing, Y M, Glorius, J, Varga, L, Bott, L, Bruckner, C B B, Chen, R J, Chen, X, Dababneh, S, Davinson, T, Erbacher, P, Fiebiger, S, Gassner, T, Gobel, K, Groothuis, M, Gumberidze, A, Gyurky, G, Heil, M, Hess, R, Hensch, R, Hillmann, P, Hillenbrand, P-M, Hinrichs, O, Jurado, B, Kausch, T, Khodaparast, A, Kisselbach, T, Klapper, N, Kozhuharov, C, Kurtulgil, D, Lane, G, Langer, C, Lederer-Woods, C, Lestinsky, M, Litvinov, S, Litvinov, Y A, Loher, B, Petridis, N, Popp, U, Reed, M, Reifarth, R, Sanjari, M S, Simon, H, Slavkovska, Z, Spillmann, U, Steck, M, Stohlker, T, Stumm, J, Szucs, T, Nguyen, T T, Zadeh, A T, Thomas, B, Torilov, S Y, Tornqvist, H, Trageser, C, Trotsenko, S, Volknandt, M, Wang, M, Weigand, M, Wolf, C, Woods, P J, Zhang, Y H & Zhou, X H 2020, ' Determination of luminosity for in-ring reactions : A new approach for the low-energy domain ', Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, vol. 982, 164367 . https://doi.org/10.1016/j.nima.2020.164367
Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
Nucl.Instrum.Meth.A, 2020, 982, pp.164367. ⟨10.1016/j.nima.2020.164367⟩
Xing, Y M, Glorius, J, Varga, L, Bott, L, Bruckner, C B B, Chen, R J, Chen, X, Dababneh, S, Davinson, T, Erbacher, P, Fiebiger, S, Gassner, T, Gobel, K, Groothuis, M, Gumberidze, A, Gyurky, G, Heil, M, Hess, R, Hensch, R, Hillmann, P, Hillenbrand, P-M, Hinrichs, O, Jurado, B, Kausch, T, Khodaparast, A, Kisselbach, T, Klapper, N, Kozhuharov, C, Kurtulgil, D, Lane, G, Langer, C, Lederer-Woods, C, Lestinsky, M, Litvinov, S, Litvinov, Y A, Loher, B, Petridis, N, Popp, U, Reed, M, Reifarth, R, Sanjari, M S, Simon, H, Slavkovska, Z, Spillmann, U, Steck, M, Stohlker, T, Stumm, J, Szucs, T, Nguyen, T T, Zadeh, A T, Thomas, B, Torilov, S Y, Tornqvist, H, Trageser, C, Trotsenko, S, Volknandt, M, Wang, M, Weigand, M, Wolf, C, Woods, P J, Zhang, Y H & Zhou, X H 2020, ' Determination of luminosity for in-ring reactions : A new approach for the low-energy domain ', Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, vol. 982, 164367 . https://doi.org/10.1016/j.nima.2020.164367
Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
Luminosity is a measure of the colliding frequency between beam and target and it is a crucial parameter for the measurement of absolute values, such as reaction cross sections. In this paper, we make use of experimental data from the ESR storage rin
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::706b64cf678d0e25f71239addfb8d579
https://hal.archives-ouvertes.fr/hal-02956014
https://hal.archives-ouvertes.fr/hal-02956014
Autor:
F. R. Pantaleo, E. M. Fiore, G. Zorzi, I. Kochanek, Rosanna Depalo, A. Boeltzig, Gianluca Imbriani, Carlo Broggini, Paolo Prati, Z. Elekes, T. Chillery, G. F. Ciani, A. Di Leva, V. Mossa, T. Davinson, E. Masha, P. Corvisiero, K. Stöckel, Luigi Schiavulli, M. Junker, R. Perrino, Carlo Bruno, Oscar Straniero, A. Best, Marialuisa Aliotta, C. Gustavino, Tamás Szücs, Sandra Zavatarelli, Gyuri Gyürky, Daniel Bemmerer, R. Menegazzo, V. Paticchio, A. Formicola, A. Guglielmetti, László Csedreki, F. Ferraro, G. Gervino, Zs. Fülöp, M. Lugaro, Paola Marigo, Laura Elisa Marcucci, F. Cavanna, Antonio Caciolli, Francesco Barile, Davide Trezzi, D. Piatti, M. P. Takács
Among the reactions involved in the production and destruction of deuterium during Big Bang Nucleosynthesis, the deuterium-burning D(p,$$\gamma $$)$$^3$$He reaction has the largest uncertainty and limits the precision of theoretical estimates of prim
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::973282e1d8d97c04d0a6d9d9bc182de5
http://hdl.handle.net/11577/3345483
http://hdl.handle.net/11577/3345483
Autor:
Claudia Lederer-Woods, O. Hinrichs, Deniz Kurtulgil, L. Varga, R. Hensch, Matthew Reed, N. Petridis, Rene Reifarth, U. Popp, U. Spillmann, M. S. Sanjari, P. Hillmann, Sergiy Trotsenko, B. Löher, Michael Lestinsky, X. C. Chen, M. Träger, T. Kisselbach, A. Khodaparast, Lukas Bott, G. J. Lane, Yu. A. Litvinov, P. M. Hillenbrand, M. Volknandt, Thomas Rauscher, Y. M. Xing, T. Gaßner, Christoph Langer, C. Kozhuharov, Thomas Stöhlker, B. Brückner, Mario Weigand, Kathrin Göbel, T. Davinson, Gyuri Gyürky, Jan Glorius, M. Groothuis, Helmut Weick, J. Stumm, S. Yu. Torilov, P. J. Woods, Sergey Litvinov, T. T. Nguyen, P. Erbacher, H. Törnqvist, A. Gumberidze, M. Steck, Klaus Blaum, C. Brandau, Tamás Szücs, Matthias Heil, Saed Dababneh, Beatriz Jurado, C. Trageser, Andrey Surzhykov, A. Taremi Zadeh, C. Wolf, R. Hess, S. Fiebiger, D. Savran, T. Kausch, B. Thomas, Herbert A. Simon, N. Klapper, F. Nolden, Z. Slavkovská
Publikováno v:
Physical Review Letters. 122
This project has received funding from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation programme (Grant Agreement No. 682841 “ASTRUm”). This work is supported by the Helmholtz International Ce
Autor:
A. Ornelas, Andreas Zilges, G. G. Kiss, E. Somorjai, Zsolt Fülöp, Thomas Rauscher, D. Galaviz, Gyuri Gyürky, Kerstin Sonnabend, P. Mohr, Z. Máté
Publikováno v:
Nuclear Physics A. 940:194-209
Alpha elastic scattering angular distributions of the 106 Cd(�,�) 106 Cd reaction were measured at three energies around the Coulomb barrier to provide a sensitive test for the � + nucleus optical potential parameter sets. Furthermore, the new
Publikováno v:
Physical Review C. 95
Background: $\ensuremath{\alpha}$-nucleus potentials play an essential role in the calculation of $\ensuremath{\alpha}$-induced reaction cross sections at low energies in the statistical model. Uncertainties of these calculations are related to ambig
Autor:
M. Junker, F. Ferraro, M. P. Takács, Gianluca Imbriani, Zsolt Fülöp, R. Menegazzo, Thomas Davinson, E. Samorjai, Sergio Cristallo, Paolo Prati, A. Di Leva, C. G. Bruno, Z. Elekes, D. K. Trezzi, Gyuri Gyürky, Oscar Straniero, F. R. Pantaleo, Marialuisa Aliotta, G. Gervino, F. Cavanna, Antonio Caciolli, Daniel Bemmerer, C. Gustavino, P. Corvisiero, V. Mossa, G. F. Ciani, Rosanna Depalo, A. Best, A. Formicola, A. Boeltzig, Luciano Piersanti, Carlo Broggini, A. Guglielmetti, D. Piatti, Tamás Szücs, Frank Strieder
Publikováno v:
Astronomy and Astrophysics 598(2017), A128
ArXiv Preprint-Server: https://arxiv.org/abs/1611.00632
ArXiv Preprint-Server: https://arxiv.org/abs/1611.00632
Context. Material processed by the CNO cycle in stellar interiors is enriched in 17O. When mixing processes from the stellar surface reach these layers, as occurs when stars become red giants and undergo the first dredge up, the abundance of 17O incr
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ebb375b426d5a2d7a3b0b36259d69403
http://hdl.handle.net/11577/3259442
http://hdl.handle.net/11577/3259442
Publikováno v:
Journal of Physics: Conference Series. 940:012052
Autor:
Antonio D'Onofrio, Michele Russo, Filippo Terrasi, Benedicta Normanna Limata, E. Somorjai, Gyuri Gyürky, Mario R. Romano, Nicola De Cesare, Lucio Gialanella, Detlef Rogalla, Cesare Rossi, C. Rolfs, Antonino Di Leva
Publikováno v:
Nuclear Instruments and Methods in Physics Research Section B: Beam Interactions with Materials and Atoms. 266:2117-2121
A pure 7 Be beam with an energy E = 1–8 MeV is available for nuclear and applied physics at the 3 MV Pelletron tandem accelerator CIRCE in Caserta. The beam is produced using an offline technique. Typical analyzed beam intensities are about 2 ppA,