Indirect study of the 3He(n, p)3H reaction at cosmological energies

C. Spampinato; R.G. Pizzone; R. Spart`a; M. Couder; W. Tan; V. Burian; K.Y. Chae; G. D’Agata; G.L. Guardo; M. La Cognata; L. Lamia; D. Lattuada; J. Mrazek; A. Oliva; S. Palmerini; P. Prajapati; G.G. Rapisarda; S. Romano; M.L. Sergi; C. Spitaleri; A. Tumino; M. Wiescher; S. Anguilar; D.W. Bardayan; D. Blankstein; L. Boccioli; L. Callahan; A. Clark; B. Frentz; M. Hall; A. Gula; S. Henderson; R. Kelmar; Q. Liu; J. Long; A. Majumdar; S. McGuinness; A. Nelson; P.D. O’Malley; C. Seymour; M. Skulski; J. Wilkinson

doi:10.1088/1742-6596/1668/1/012039

Journal of Physics: Conference Series

Paper • The following article is Open access

Indirect study of the ³He(n, p)³H reaction at cosmological energies

C. Spampinato^1,2,3,7, R.G. Pizzone¹, R. Spart`a^1,2, M. Couder⁴, W. Tan³, V. Burian⁶, K.Y. Chae⁹, G. D'Agata⁶, G.L. Guardo¹, M. La Cognata¹, L. Lamia^1,2, D. Lattuada⁸, J. Mrazek⁶, A. Oliva¹, S. Palmerini⁵, P. Prajapati¹, G.G. Rapisarda¹, S. Romano^1,2, M.L. Sergi¹, C. Spitaleri^1,2, A. Tumino^1,8, M. Wiescher⁴, S. Anguilar⁴, D.W. Bardayan⁴, D. Blankstein⁴, L. Boccioli^4,5, L. Callahan⁴, A. Clark⁴, B. Frentz⁴, M. Hall⁴, A. Gula⁴, S. Henderson⁴, R. Kelmar⁴, Q. Liu⁴, J. Long⁴, A. Majumdar⁴, S. McGuinness⁴, A. Nelson⁴, P.D. O'Malley⁴, C. Seymour⁴, M. Skulski⁴ and J. Wilkinson⁴

Published under licence by IOP Publishing Ltd
Journal of Physics: Conference Series, Volume 1668, Nuclear Physics in Astrophysics IX (NPA-IX), 15-20 September 2019, Frankfurt, Germany Citation C. Spampinato et al 2020 J. Phys.: Conf. Ser. 1668 012039 DOI 10.1088/1742-6596/1668/1/012039

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cspampinato@lns.infn.it

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¹ Laboratori Nazionali del Sud, INFN, Catania Italy

² Dipartimento di Fisica e Astronomia, Università di Catania, Italy

³ Centro Siciliano di Fisica Nucleare e Struttura della Materia, Catania Italy

⁴ Department of Physics, University of Notre Dame, USA

⁵ INFN and University of Perugia, Italy

⁶ Cyclotron Institute, Academy of Science of the Czech Rep., Rez, Czech Rep.

⁷ ELI-NP, Magurele, Romania

⁸ Kore University, Enna, Italy

⁹ SKKU Sungkyunkwan University, Korea

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Abstract

In the network of reactions present in the Big Bang nucleosynthesis, the ³He(n, p)³H reaction has an important role which impacts the final ⁷Li abundance. The Trojan Horse Method (THM) has been applied to the ³He(d, pt)H reaction in order to extract the astrophysical S(E)-factor of the ³He(n, p)³H reaction in the Gamow energy range. The experiment will be described in the present work together with the first preliminary results.

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