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pro vyhledávání: '"LAMIA, L."'
Autor:
Lamia, L. Lamia L.1,2,3 llamia@lns.infn.it
Publikováno v:
EPJ Web of Conferences. 6/7/2024, Vol. 297, p1-5. 5p.
Autor:
Carrasco-Rojas, D. P., Williams, M., Adsley, P., Lamia, L., Bastin, B., Faestermann, T., Fougeres, C., Hammache, F., Harrouz, D. S., Hertenberger, R., La Cognata, M., Meyer, A., Santos, F. de Oliveira, Palmerini, S., Pizzone, R. G., Romano, S., de Sereville, N., Tumino, A., Wirth, H. -F.
Background: Globular clusters show strong correlations between different elements, such as the well-known sodium-oxygen anticorrelation. One of the main sources of uncertainty in this anticorrelation is the $^{22}$Ne($p,\gamma$)$^{23}$Na reaction rat
Externí odkaz:
http://arxiv.org/abs/2302.12939
Autor:
Adsley, P, Williams, M, Harrouz, D S, Carrasco-Rojas, D P, de Séréville, N, Hammache, F, Longland, R, Bastin, B, Davids, B, Faestermann, T, Fougères, C, Greife, U, Hertenberger, R, Hutcheon, D, La Cognata, M, Laird, AM, Lamia, L, Lennarz, A, Meyer, A, Santos, F d'Oliveira, Palmerini, S, Psaltis, A, Pizzone, R G, Romano, S, Ruiz, C, Tumino, A, Wirth, H-F
Globular clusters contain multiple stellar populations, with some previous generation of stars polluting the current stars with heavier elements. Understanding the history of globular clusters is helpful in understanding how galaxies merged and evolv
Externí odkaz:
http://arxiv.org/abs/2212.03648
Autor:
Schatz, H., Reyes, A. D. Becerril, Best, A., Brown, E. F., Chatziioannou, K., Chipps, K. A., Deibel, C. M., Ezzeddine, R., Galloway, D. K., Hansen, C. J., Herwig, F., Ji, A. P., Lugaro, M., Meisel, Z., Norman, D., Read, J. S., Roberts, L. F., Spyrou, A., Tews, I., Timmes, F. X., Travaglio, C., Vassh, N., Abia, C., Adsley, P., Agarwal, S., Aliotta, M., Aoki, W., Arcones, A., Aryan, A., Bandyopadhyay, A., Banu, A., Bardayan, D. W., Barnes, J., Bauswein, A., Beers, T. C., Bishop, J., Boztepe, T., Côté, B., Caplan, M. E., Champagne, A. E., Clark, J. A., Couder, M., Couture, A., de Mink, S. E., Debnath, S., deBoer, R. J., Hartogh, J. den, Denissenkov, P., Dexheimer, V., Dillmann, I., Escher, J. E., Famiano, M. A., Farmer, R., Fisher, R., Fröhlich, C., Frebel, A., Fryer, C., Fuller, G., Ganguly, A. K., Ghosh, S., Gibson, B. K., Gorda, T., Gourgouliatos, K. N., Graber, V., Gupta, M., Haxton, W., Heger, A., Hix, W. R., Ho, W C. G., Holmbeck, E. M., Hood, A. A., Huth, S., Imbriani, G., Izzard, R. G., Jain, R., Jayatissa, H., Johnston, Z., Kajino, T., Kankainen, A., Kiss, G. G., Kwiatkowski, A., La Cognata, M., Laird, A. M., Lamia, L., Landry, P., Laplace, E., Launey, K. D., Leahy, D., Leckenby, G., Lennarz, A., Longfellow, B., Lovell, A. E., Lynch, W. G., Lyons, S. M., Maeda, K., Masha, E., Matei, C., Merc, J., Messer, B., Montes, F., Mukherjee, A., Mumpower, M., Neto, D., Nevins, B., Newton, W. G., Nguyen, L. Q., Nishikawa, K., Nishimura, N., Nunes, F. M., O'Connor, E., O'Shea, B. W., Ong, W-J., Pain, S. D., Pajkos, M. A., Pignatari, M., Pizzone, R. G., Placco, V. M., Plewa, T., Pritychenko, B., Psaltis, A., Puentes, D., Qian, Y-Z., Radice, D., Rapagnani, D., Rebeiro, B. M., Reifarth, R., Richard, A. L., Rijal, N., Roederer, I. U., Rojo, J. S., K, J. S, Saito, Y., Schwenk, A., Sergi, M. L., Sidhu, R. S., Simon, A., Sivarani, T., Skúladóttir, Á., Smith, M. S., Spiridon, A., Sprouse, T. M., Starrfield, S., Steiner, A. W., Strieder, F., Sultana, I., Surman, R., Szücs, T., Tawfik, A., Thielemann, F., Trache, L., Trappitsch, R., Tsang, M. B., Tumino, A., Upadhyayula, S., Martínez, J. O. Valle, Van der Swaelmen, M., Vázquez, C. Viscasillas, Watts, A., Wehmeyer, B., Wiescher, M., Wrede, C., Yoon, J., Zegers, R G. T., Zermane, M. A., Zingale, M.
Nuclear Astrophysics is a field at the intersection of nuclear physics and astrophysics, which seeks to understand the nuclear engines of astronomical objects and the origin of the chemical elements. This white paper summarizes progress and status of
Externí odkaz:
http://arxiv.org/abs/2205.07996
Autor:
Harrouz, D. S., de Séréville, N., Adsley, P., Hammache, F., Longland, R., Bastin, B., Faestermann, T., Hertenberger, R., La Cognata, M., Lamia, L., Meyer, A., Palmerini, S., Pizzone, R. G., Romano, S., Tumino, A., Wirth, H. -F.
[Background] Abundance anomalies in some globular clusters, such as the enhancement of potassium and the depletion of magnesium, can be explained in terms of an earlier generation of stars polluting the presently observed ones. It was shown that the
Externí odkaz:
http://arxiv.org/abs/2201.03411
Autor:
Negoita, F., Roth, M., Thirolf, P. G., Tudisco, S., Hannachi, F., Moustaizis, S., Pomerantz, I., Mckenna, P., Fuchs, J., Sphor, K., Acbas, G., Anzalone, A., Audebert, P., Balascuta, S., Cappuzzello, F., Cernaianu, M. O., Chen, S., Dancus, I., Freeman, R., Geissel, H., Ghenuche, P., Gizzi, L., Gobet, F., Gosselin, G., Gugiu, M., Higginson, D., D¶Humiêres, E., Ivan, C., Jaroszynski, D., Kar, S., Lamia, L., Leca, V., Neagu, L., Lanzalone, G., Meot, V., Mirfayzi, S. R., Mitu, I. O., Morel, P., Murphy, C., Petcu, C., Petrascu, H., Petrone, C., Raczka, P., Risca, M., Rotaru, F., Santos, J. J., Schumacher, D., Stutman, D., Tarisien, M., Tataru, M., Tatulea, B., Turcu, I. C. E., Versteegen, M., Ursescu, D., Gales, S., Zamfir, N. V.
High power lasers have proven being capable to produce high energy gamma rays, charged particles and neutrons to induce all kinds of nuclear reactions. At ELI, the studies with high power lasers will enter for the first time into new domains of power
Externí odkaz:
http://arxiv.org/abs/2201.01068
Autor:
Tognelli, E., Degl'Innocenti, S., Moroni, P. G. Prada, Lamia, L., Pizzone, R. G., Tumino, A., Spitaleri, C., Chiavassa, A.
Publikováno v:
published in Front. Astron. Space Sci., 13 May 2021, 8, 22
Theoretical prediction of surface stellar abundances of light elements -- lithium, beryllium, and boron -- represents one of the most interesting open problems in astrophysics. As well known, several measurements of 7-Li abundances in stellar atmosph
Externí odkaz:
http://arxiv.org/abs/2107.02518
Autor:
Nauruzbayev, D. K., Nurmukhanbetova, A. K., Goldberg, V. Z., La Cognata, M., Di Pietro, A., Figuera, P., Cherubini, S., Gulino, M., Lamia, L., Pizzone, R. G., Spart`a, R., Tumino, A., Serikov, A., Gazeeva, E. M.
The Thick Target Inverse Kinematic (TTIK) approach was used to measure excitation functions for the elastic 17O ({\alpha}, {\alpha}) scattering at the initial 17O beam energy of 54.4 MeV. We observed strong peaks corresponding to highly excited {\alp
Externí odkaz:
http://arxiv.org/abs/1910.08986
Akademický článek
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Autor:
Tumino, A., Spitaleri, C., La Cognata, M., Cherubini, S., Guardo, G. L., Gulino, M., Hayakawa, S., Indelicato, I., Lamia, L., Petrascu, H., Pizzone, R. G., Puglia, S. M. R., Rapisarda, G. G., Romano, S., Sergi, M. L., Spartá, R., Trache, L.
The goal of this reply is to draw attention of the readers that the major problems rose in the short Comment authored by A.M. Mukhamedzhanov, X. Tang and D.Y. Pang (arXiv:1806.05921) are totally groundless.
Comment: 4 pages, 2 figures
Comment: 4 pages, 2 figures
Externí odkaz:
http://arxiv.org/abs/1807.06148