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Your search keyword '"Burjan, S. V."' showing total 12 results
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12 results on '"Burjan, S. V."'

2. O-17(p,alpha)N-14 reaction measurement at astrophysical energies

Author

Sergi, M. L., Spitaleri, C, Pizzone, R. G., Burjan, S. V., Cherubini, S, Coc, A, Gulino, M, Hammache, F, Hons, Z, Irgaziev, B, Kiss, G. G., Kroha, V, La Cognata, M, Lamia, L, Mukhamedzhanov, A, Puglia, S. M. R., Rapisarda, G. G., Romano, S, De Sereville, N, Somorjai, E, Tumino, A, CSNSM AN, Centre de Sciences Nucléaires et de Sciences de la Matière (CSNSM), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11)-Centre de Spectrométrie Nucléaire et de Spectrométrie de Masse (CSNSM), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), and Institut de Physique Nucléaire d'Orsay (IPNO)

Subjects
NUCLEOSYNTHESIS, O-18(P, O-17(P, supernovae, TROJAN HORSE METHOD, Direct reactions, Nucleosynthesis in novae, [PHYS.ASTR.SR]Physics [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR], other explosive environments, [PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], Nuclear Astrophysics, REACTION-RATES, ALPHA)N-14, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], CROSS-SECTION
Abstract

International audience; The O-17(p,alpha)N-14 reaction is of paramount importance for the nucleosynthesis in a number of stellar sites, including red giants (RG), asymptotic giant branch (AGB) stars, massive stars and classical novae. We report on the indirect study of the O-17(p,alpha)N-14 reaction via the Trojan Horse Method by applying the approach recently developed for extracting the resonance strength of narrow resonance in the ultra-low energy region.

Published
2013
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6. THM determination of the 65 keV resonance strength intervening in the 17O(p,α)14N reaction rate

Author

Sergi, M. L., primary, Spitaleri, C., additional, Burjan, S. V., additional, Cherubini, S., additional, Coc, A., additional, Gulino, M., additional, Hammache, F., additional, Hons, Z., additional, Irgaziev, B., additional, Kiss, G. G., additional, Kroha, V., additional, La Cognata, M., additional, Lamia, L., additional, Mukhamedzhanov, A., additional, Pizzone, R. G., additional, Puglia, S. M. R., additional, Rapisarda, G. G., additional, Romano, S., additional, de Séréville, N., additional, Somorjai, E., additional, and Tumino, A., additional

Published
2015
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7. 17O(p,α)14N reaction measurement at astrophysical energies

Author

Sergi, M. L., primary, Spitaleri, C., additional, Pizzone, R. G., additional, Burjan, S. V., additional, Cherubini, S., additional, Coc, A., additional, Gulino, M., additional, Hammache, F., additional, Hons, Z., additional, Irgaziev, B., additional, Kiss, G. G., additional, Kroha, V., additional, La Cognata, M., additional, Lamia, L., additional, Mukhamedzhanov, A., additional, Puglia, S. M. R., additional, Rapisarda, G. G., additional, Romano, S., additional, de Séréville, N., additional, Somorjai, E., additional, and Tumino, A., additional

Published
2014
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8. The 17O(p,α)14N reaction measurement via the Trojan horse method and its application to 17O nucleosynthesis

Author

Sergi, M. L., primary, Spitaleri, C., additional, Pizzone, R. G., additional, Burjan, S. V., additional, Cherubini, S., additional, Coc, A., additional, Gulino, M., additional, Hammache, F., additional, Hons, Z., additional, Irgaziev, B., additional, Kiss, G. G., additional, Kroha, V., additional, La Cognata, M., additional, Lamia, L., additional, Mukhamedzhanov, A., additional, Puglia, S. M. R., additional, Rapisarda, G. G., additional, Romano, S., additional, de Séréville, N., additional, Somorjai, E., additional, and Tumino, A., additional

Published
2014
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9. THM determination of the 65 keV resonance strength intervening in the 17O(p,α)14N reaction rate.

Author

Sergi, M. L., Spitaleri, C., Burjan, S. V., Cherubini, S., Coc, A., Gulino, M., Hammache, F., Hons, Z., Irgaziev, B., Kiss, G. G., Kroha, V., La Cognata, M., Lamia, L., Mukhamedzhanov, A., Pizzone, R. G., Puglia, S. M. R., Rapisarda, G. G., Romano, S., de Séréville, N., and Somorjai, E.

Subjects
CHEMICAL kinetics, OXYGEN isotopes, NITROGEN isotopes, NUCLEOSYNTHESIS, RED giants, SUPERGIANT stars
Abstract

The 17O(p,α)14N reaction is of paramount importance for the nucleosynthesis in a number of stellar sites, including red giants (RG), asymptotic giant branch (AGB) stars, massive stars and classical novae. We report on the indirect study of the 17O(p,α)14N reaction via the Trojan Horse Method by applying the approach recently developed for extracting the resonance strength of the narrow resonance at Ec.m.R = 65 keV (EX =5.673 MeV). The strength of the 65 keV resonance in the 17O(p,α)14N reaction, measured by means of the THM, has been used to renormalize the corresponding resonance strength in the 17O + p radiative capture channel. [ABSTRACT FROM AUTHOR]

Published
2015
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10. The 17O(p,α)14N reaction measurement via the Trojan Horse Method and its application to 17O nucleosynthesis.

Author

Sergi, M. L., Spitaleri, C., Pizzone, R. G., Burjan, S. V ., Cherubini, S., Coc, A., Gulino, M., Hammache, F., Hons, Z., Irgaziev, B., Kiss, G. G., Kroha, V., Cognata, M. La, Lamia, L., Mukhamedzhanov, A., Puglia, S. M. R., Rapisarda, G. G., Romano, S., de Séréville, N., and Somorjai, E.

Subjects
NUCLEOSYNTHESIS, OXYGEN, ASTROPHYSICS, GAMMA ray astronomy, UNCERTAINTY (Information theory), NITROGEN, CHEMICAL kinetics, NOVAE (Astronomy)
Abstract

The role of oxygen in astrophysics is related to different problems as novae nucleosynthesis and gamma-ray astronomy. In particular, owing to the still present uncertainties on its rate, the 17O(p,α)14N is one of the most important reaction to be studied in order to get more information about the fate of oxygen in different astrophysical scenarios. [ABSTRACT FROM AUTHOR]

Published
2014
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11. New high accuracy measurement of theO17(p,α)N14reaction rate at astrophysical temperatures

Author

Sergi, M. L., primary, Spitaleri, C., additional, La Cognata, M., additional, Coc, A., additional, Mukhamedzhanov, A., additional, Burjan, S. V., additional, Cherubini, S., additional, Crucillá, V., additional, Gulino, M., additional, Hammache, F., additional, Hons, Z., additional, Irgaziev, B., additional, Kiss, G. G., additional, Kroha, V., additional, Lamia, L., additional, Pizzone, R. G., additional, Puglia, S. M. R., additional, Rapisarda, G. G., additional, Romano, S., additional, de Séréville, N., additional, Somorjai, E., additional, Tudisco, S., additional, and Tumino, A., additional

Published
2010
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12. 17O(p,α)14N reaction measurement at astrophysical energies.

Author

Sergi, M. L., Spitaleri, C., Pizzone, R. G., Burjan, S. V., Cherubini, S., Coc, A., Gulino, M., Hammache, F., Hons, Z., Irgaziev, B., Kiss, G. G., Kroha, V., La Cognata, M., Lamia, L., Mukhamedzhanov, A., Puglia, S. M. R., Rapisarda, G. G., Romano, S., de Séréville, N., and Somorjai, E.

Subjects
NUCLEAR astrophysics research, NUCLEAR reactions, COLLISIONS (Nuclear physics), DIRECT reactions (Nuclear physics), NUCLEOSYNTHESIS, SUPERNOVAE, GALACTIC X-ray sources, GIANT stars
Abstract

The 17O(p,a)14N reaction is of paramount importance for the nucleosynthesis in a number of stellar sites, including red giants (RG), asymptotic giant branch (AGB) stars, massive stars and classical novae. We report on the indirect study of the 17O(p,a)14N reaction via the Trojan Horse Method by applying the approach recently developed for extracting the resonance strength of narrow resonance in the ultra-low energy region. [ABSTRACT FROM AUTHOR]

Published
2014
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