Study of 3He(n,p)3H reaction at cosmological energies with trojan horse method

C. Spampinato; R.G. Pizzone; R. Spartà; M. Couder; W. Tan; V. Burian; K.Y. Chae; G. D’Agata; G.L. Guardo; I. Indelicato; M. La Cognata; L. Lamia; D. Lattuada; J. Mrazek; A. Oliva; S. Palmerini; P.M. Prajapati; G.G. Rapisarda; S. Romano; M.L. Sergi; C. Spitaleri; A. Tumino; M. Wiescher; S. Anguilar; D. Bardyan; 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. O’Malley; C. Seyymour; M. Skulski; J. Wilkinson

doi:10.1051/epjconf/202022702013

EPJ

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Proceedings

Open Access

EPJ Web of Conferences 227, 02013 (2020)
https://doi.org/10.1051/epjconf/202022702013

Study of ³He(n,p)³H reaction at cosmological energies with trojan horse method

C. Spampinato¹^,2^,3^*, R.G. Pizzone¹, R. Spartà¹^,2, M. Couder⁴, W. Tan³, V. Burian⁶, K.Y. Chae⁹, G. D’Agata⁶, G.L. Guardo¹, I. Indelicato¹, M. La Cognata¹, L. Lamia¹^,2, D. Lattuada⁸, J. Mrazek⁶, A. Oliva¹, S. Palmerini⁵, P.M. Prajapati¹, G.G. Rapisarda¹, S. Romano¹^,2, M.L. Sergi¹, C. Spitaleri¹^,2, A. Tumino¹^,8, M. Wiescher⁴, S. Anguilar⁴, D. Bardyan⁴, D. Blankstein⁴, L. Boccioli⁴^,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. O’Malley⁴, C. Seyymour⁴, M. Skulski⁴ and J. Wilkinson⁴

¹ Laboratori Nazionali del Sud, INFN, Catania Italy
² Dipartimento di Fisica e Astronomia, Universita di Catania, Italy
³ Centro Siciliano di Fisica Nucleare e Struttura della Materia, Catania Italy
⁴ Physics and Astronomy Department, Notre Dame University, 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

^* carlo_spa@msn.com

Published online: 14 January 2020

Abstract

In the network of reactions present in the Big Bang nucleosynthesis, the ³He(n, p)³H 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 in the Gamow energy range. The experiment will be described in the present work together with the first preliminary results.

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