Zobrazeno 1 - 10
of 164
pro vyhledávání: '"Tesileanu, O."'
Autor:
Gai, M., Schweitzer, D., Stern, S. R., Young, A. H., Smith, R., Cwiok, M., Bihalowicz, J. S., Czyrkowski, H., Dabrowski, R., Dominik, W., Fijalkowska, A., Janas, Z., Janiak, L., Korgul, A., Matulewicz, T., Mazzocchi, C., Pfuetzner, M., Zaremba, M., Balabanski, D., Gheorghe, I., Matei, C., Tesileanu, O., Zamfir, N. V., Ahmed, M. W., Henshaw, S. S., Howell, C. R., Mueller, J. M., Myers, L. S., Stave, S., Sun, C., Weller, H. R., Wu, Y. K., Breskin, A., Dangendorf, V., Tittelmeier, K., Freer, M.
Gamma-Beams at the HIgS facility in the USA and anticipated at the ELI-NP facility, now constructed in Romania, present unique new opportunities to advance research in nuclear astrophysics; not the least of which is resolving open questions in oxygen
Externí odkaz:
http://arxiv.org/abs/1812.09536
Autor:
Renstrøm, T., Utsunomiya, H., Nyhus, H. T., Larsen, A. C., Guttormsen, M., Tveten, G. M., Filipescu, D. M., Gheorghe, I., Goriely, S., Hilaire, S., Lui, Y. -W., Midtbø, J. E., Péru, S., Shima, T., Siem, S., Tesileanu, O.
Publikováno v:
Phys. Rev. C 98, 054310 (2018)
The photo-neutron cross sections of $^{162,163}\rm{Dy}$ have been measured for the first time in an energy region from the neutron threshold ($S_n$) up to $\approx$ $13$~MeV. The ($\gamma$,n) reaction was induced with quasi-monochromatic laser Compto
Externí odkaz:
http://arxiv.org/abs/1804.07654
Autor:
Renstrøm, T., Nyhus, H. -T., Utsumoniya, H., Schwengner, R., Goriely, S., Larsen, A. C., Filipescu, D. M., Gheorghe, I., Bernstein, L. A., Bleuel, D. L., Glodariu, T., Görgen, A., Guttormsen, M., Hagen, T. W., Kheswa, B. V., Lui, Y. -W ., Negi, D., Ruud, I. E., Shima, T., Siem, S., Takahisa, K., Tesileanu, O., Tornyi, T. G., Tveten, G. M., Wiedeking, M.
The $\gamma$-ray strength functions and level densities of $^{73,74}$Ge have been extracted up to the neutron separation energy S$_n$ from particle-$\gamma$ coincidence data using the Oslo method. Moreover, the $\gamma$-ray strength function of $^{74
Externí odkaz:
http://arxiv.org/abs/1510.05219
Autor:
Gai, M., Schweitzer, D., Stern, S.R., Young, A.H., Smith, R., Cwiok, M., Bihalowicz, J.S., Czyrkowski, H., Dabrowski, R., Dominik, W., Fijalkowska, A., Janas, Z., Janiak, L., Korgul, A., Matulewicz, T., Mazzocchi, C., Pfützner, M., Zaremba, M., Balabanski, D., Gheorghe, I., Matei, C., Tesileanu, O., Zamfir, N.V., Ahmed, M.W., Henshaw, S.S., Howell, C.R., Mueller, J.M., Myers, L.S., Stave, S., Sun, C., Weller, H.R., Wu, Y.K., Breskin, A., Dangendorf, V., Tittelmeier, K., Freer, M.
Publikováno v:
In Nuclear Inst. and Methods in Physics Research, A 21 February 2020 954
Akademický článek
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Akademický článek
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Autor:
Tesileanu, O., Matsakos, T., Massaglia, S., Trussoni, E., Mignone, A., Vlahakis, N., Tsinganos, K., Stute, M., Cayatte, V., Sauty, C., Stehle, C., Chieze, J. -P.
Astronomical observations, analytical solutions and numerical simulations have provided the building blocks to formulate the current theory of young stellar object jets. Although each approach has made great progress independently, it is only during
Externí odkaz:
http://arxiv.org/abs/1312.4334
Autor:
Csige, L., Filipescu, D. M., Glodariu, T., Gulyás, J., Günther, M. M., Habs, D., Karwowski, H. J., Krasznahorkay, A., Rich, G. C., Sin, M., Stroe, L., Tesileanu, O., Thirolf, P. G.
The photofission cross-section of 238U was measured at sub-barrier energies as a function of the gamma-ray energy using, for the first time, a monochromatic, high-brilliance, Compton-backscattered gamma-ray beam. The experiment was performed at the H
Externí odkaz:
http://arxiv.org/abs/1302.3425
Publikováno v:
A&A 507, 581-588 (2009)
The coupling between time-dependent, multidimensional MHD numerical codes and radiative line emission is of utmost importance in the studies of the interplay between dynamical and radiative processes in many astrophysical environments, with particula
Externí odkaz:
http://arxiv.org/abs/0910.1225
Publikováno v:
A&A 488, 429-440 (2008)
Time-dependent cooling processes are of paramount importance in the evolution of astrophysical gaseous nebulae and, in particular, when radiative shocks are present. The present work introduces a necessary set of tools that can be used to model radia
Externí odkaz:
http://arxiv.org/abs/0807.3657