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BIG BANG NUCLEOSYNTHESIS REVISITED VIA TROJAN HORSE METHOD MEASUREMENTS

R. G. PizzoneINFN—Laboratori Nazionali del Sud, Via Santa Sofia 62, I-95123 Catania, Italy; [email protected]R. SpartáDipartimento di Fisica e Astronomia, Università degli Studi di Catania, Via Santa Sofia 64, I-95123 Catania, ItalyC. A. BertulaniDepartment of Physics and Astronomy, Texas A&M University, Commerce, TX 75025, USAC. SpitaleriDipartimento di Fisica e Astronomia, Università degli Studi di Catania, Via Santa Sofia 64, I-95123 Catania, ItalyM. La CognataINFN—Laboratori Nazionali del Sud, Via Santa Sofia 62, I-95123 Catania, Italy; [email protected]J. LalmansinghDepartment of Physics and Astronomy, Texas A&M University, Commerce, TX 75025, USAL. LamiaDipartimento di Fisica e Astronomia, Università degli Studi di Catania, Via Santa Sofia 64, I-95123 Catania, ItalyA. MukhamedzhanovCyclotron Institute, Texas A&M University, College Station, TX 77843, USAA. TuminoINFN—Laboratori Nazionali del Sud, Via Santa Sofia 62, I-95123 Catania, Italy; [email protected]

2014en

ABI

Annotatsiya

Nuclear reaction rates are among the most important input for understanding the primordial nucleosynthesis and therefore for a quantitative description of the early Universe. An up-to-date compilation of direct cross sections of 2H(d,p)3H, 2H(d,n)3He, 7Li(p,alpha)4He and 3He(d,p)4He reactions is given. These are among the most uncertain cross sections used and input for Big Bang nucleosynthesis calculations. Their measurements through the Trojan Horse Method (THM) are also reviewed and compared with direct data. The reaction rates and the corresponding recommended errors in this work were used as input for primordial nucleosynthesis calculations to evaluate their impact on the 2H, 3,4He and 7Li primordial abundances, which are then compared with observations.

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DOI: 10.1088/0004-637x/786/2/112

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