Search Results - "Coc, A"

BAYESIAN ESTIMATION OF THERMONUCLEAR REACTION RATES by Iliadis, C., Anderson, K. S., Coc, A., Timmes, F. X., Starrfield, S.

“…ABSTRACT The problem of estimating non-resonant astrophysical S-factors and thermonuclear reaction rates, based on measured nuclear cross sections, is of major…”
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Charged-particle thermonuclear reaction rates: II. Tables and graphs of reaction rates and probability density functions by Iliadis, C., Longland, R., Champagne, A.E., Coc, A., Fitzgerald, R.

“…Numerical values of charged-particle thermonuclear reaction rates for nuclei in the A = 14 to 40 region are tabulated. The results are obtained using a method,…”
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Bayesian Estimation of Thermonuclear Reaction Rates for Deuterium+Deuterium Reactions by Gómez Iñesta, Á., Iliadis, C., Coc, A.

“…The study of d+d reactions is of major interest since their reaction rates affect the predicted abundances of D, 3He, and 7Li. In particular, recent…”
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Charged-particle thermonuclear reaction rates: III. Nuclear physics input by Iliadis, C., Longland, R., Champagne, A.E., Coc, A.

“…The nuclear physics input used to compute the Monte Carlo reaction rates and probability density functions that are tabulated in the second paper of this issue…”
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Charged-particle thermonuclear reaction rates: I. Monte Carlo method and statistical distributions by Longland, R., Iliadis, C., Champagne, A.E., Newton, J.R., Ugalde, C., Coc, A., Fitzgerald, R.

“…A method based on Monte Carlo techniques is presented for evaluating thermonuclear reaction rates. We begin by reviewing commonly applied procedures and point…”
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Charged-particle thermonuclear reaction rates: IV. Comparison to previous work by Iliadis, C., Longland, R., Champagne, A.E., Coc, A.

“…We compare our Monte Carlo reaction rates (see Paper II of this issue) to previous results that were obtained by using the classical method of computing…”
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A compilation of charged-particle induced thermonuclear reaction rates by Angulo, C., Arnould, M., Rayet, M., Descouvemont, P., Baye, D., Leclercq-Willain, C., Coc, A., Barhoumi, S., Aguer, P., Rolfs, C., Kunz, R., Hammer, J.W., Mayer, A., Paradellis, T., Kossionides, S., Chronidou, C., Spyrou, K., Degl'Innocenti, S., Fiorentini, G., Ricci, B., Zavatarelli, S., Providencia, C., Wolters, H., Soares, J., Grama, C., Rahighi, J., Shotter, A., Lamehi Rachti, M.

“…Low-energy cross section data for 86 charged-particle induced reactions involving light (1 ⩽ Z ⩽ 14), mostly stable, nuclei are compiled. The corresponding…”
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Compilation and R-matrix analysis of Big Bang nuclear reaction rates by Descouvemont, Pierre, Adahchour, Abderrahim, Angulo, Carmen, Coc, Alain, Vangioni-Flam, Elisabeth

“…We use the R-matrix theory to fit low-energy data on nuclear reactions involved in Big Bang nucleosynthesis. Special attention is paid to the rate…”
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Big bang nucleosynthesis constraints on scalar-tensor theories of gravity by Coc, Alain, Olive, Keith A., Uzan, Jean-Philippe, Vangioni, Elisabeth

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Search for superscreening effects in a superconductor by Ujić, P, de Oliveira Santos, F, Lewitowicz, M, Achouri, N L, Assié, M, Bastin, B, Borcea, C, Borcea, R, Buta, A, Coc, A, de France, G, Kamalou, O, Kiener, J, Lepailleur, A, Meot, V, Pautrat, A, Saint Laurent, M G, Sorlin, O, Stanoiu, M, Tatischeff, V

“…The decay of (19)O(β(-)) and (19)Ne(β(+)) implanted in niobium in its superconducting and metallic phases was measured using purified radioactive beams…”
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Synthesis of Intermediate-Mass Elements in Classical Novae: From Si to Ca by José, Jordi, Coc, Alain, Hernanz, Margarita

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Indirect techniques for astrophysical reaction rates determinations by Hammache, F., Oulebsir, N., Benamara, S., De Séréville, N., Coc, A., Laird, A., Stefan, I., Roussel, P.

“…Direct measurements of nuclear reactions of astrophysical interest can be challenging. Alternative experimental techniques such as transfer reactions and…”
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Explosive Hydrogen Burning of O 17 in Classical Novae by Fox, C., Iliadis, C., Champagne, A. E., Coc, A., José, J., Longland, R., Newton, J., Pollanen, J., Runkle, R.

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Hydrogen Burning of O 17 in Classical Novae by Chafa, A., Tatischeff, V., Aguer, P., Barhoumi, S., Coc, A., Garrido, F., Hernanz, M., José, J., Kiener, J., Lefebvre-Schuhl, A., Ouichaoui, S., de Séréville, N., Thibaud, J.-P.

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Studying astrophysical reactions with low-energy RI beams at CRIB by Yamaguchi, H., Kahl, D., Hayakawa, S., Sakaguchi, Y., Wakabayashi, Y., Hashimoto, T., Cherubini, S., Gulino, M., Spitaleri, C., Rapisarda, G.G., La Cognata, M., Lamia, L., Romano, S., Kubono, S., Iwasa, N., Teranishi, T., Kawabata, T., Kwon, Y.K., Binh, D.N., Khiem, L.H., Duy, N.N., Kato, S., Komatsubara, T., Coc, A., De Sereville, N., Hammache, F., Kiss, G., Bishop, S.

“…Studies on nuclear astrophysics, nuclear structure, and other interests have been performed using the radioactive-isotope (RI) beams at the low-energy RI beam…”
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Gamma-Ray Emission from Novae Related to Positron Annihilation: Constraints on its Observability Posed by New Experimental Nuclear Data by Hernanz, Margarita, José, Jordi, Coc, Alain, Gómez-Gomar, Jordi, Isern, Jordi

“…Classical novae emit gamma-ray radiation at 511 keV and below (with a cutoff at around 20-30 keV), related to positron annihilation and its Comptonization in…”
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Study of key resonances in the 30P(p,γ)31S reaction in classical novae by Meyer, A, de Séréville, N, Hammache, F, Adsley, P, Assié, M, Beaumel, D, Delafosse, C, Flavigny, F, Georgiadou, A, Gottardo, A, Grassi, L, Guillot, J, Barkach, T Id, MacCormick, M, Matea, I, Olivier, L, Perrot, L, Portail, C, Stefan, I, Parikh, A, Coc, A, Kiener, J, Tatischeff, V, Laird, A M, Fox, S P, Hubbard, N, Riley, J, De Oliveira, F, Bastin, B, Béroff, K, Sánchez Benítez, Á M, Alellara, A, Assunção, M, Guimaraes, V, Oulebsir, N, G D’Agata

“…Among reactions with strong impact on classical novae model predictions, 30P(p,γ)31S is one of the few remained that are worthy to be measured accurately,…”
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A Novel Approach to Measure the Cross Section of the 18O(p, α)15N Resonant Reaction in the 0-200 keV Energy Range by Cognata, M. La, Spitaleri, C, Mukhamedzhanov, A, Banu, A, Cherubini, S, Coc, A, Crucillà, V, Goldberg, V, Gulino, M, Irgaziev, B, Kiss, G. G, Lamia, L, Mrazek, J, Pizzone, R. G, Puglia, S. M. R, Rapisarda, G. G, Romano, S, Sergi, M. L, Tabacaru, G, Trache, L, Tribble, R. E, Trzaska, W, Tumino, A

“…The 18O(p, Delta *a)15N reaction is of primary importance to pin down the uncertainties, due to nuclear physics input, affecting present-day models of…”
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Big-Bang reaction rates within the R-matrix model by Descouvemont, P., Adahchour, A., Angulo, C., Coc, A., Vangioni-Flam, E.

“…We use the R-matrix theory to fit S-factor data on nuclear reactions involved in Big Bang nucleosynthesis. We derive the reaction rates with associated…”
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STANDARD BIG BANG NUCLEOSYNTHESIS UP TO CNO WITH AN IMPROVED EXTENDED NUCLEAR NETWORK by Coc, Alain, Goriely, Stéphane, Xu, Yi, Saimpert, Matthias, Vangioni, Elisabeth

“…Primordial or big bang nucleosynthesis (BBN) is one of the three strong pieces of evidence for the big bang model together with the expansion of the universe…”
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