3He(α,γ)7Be cross section measured using complementary techniques

Carmona-Gallardo M.; Rojas A.; Borge M.J.G.; Davids B.; Fulton B.R.; Hass M.; Nara Singh B.S.; Ruiz C.; Tengblad O.

doi:10.1051/epjconf/20146607003

EPJ Web of Conferences (Mar 2014)

3He(α,γ)7Be cross section measured using complementary techniques

Carmona-Gallardo M.,
Rojas A.,
Borge M.J.G.,
Davids B.,
Fulton B.R.,
Hass M.,
Nara Singh B.S.,
Ruiz C.,
Tengblad O.

Affiliations

Carmona-Gallardo M.: Instituto de Estructura de la Materia-CSIC
Rojas A.: TRIUMF
Borge M.J.G.: Instituto de Estructura de la Materia-CSIC
Davids B.: TRIUMF
Fulton B.R.: Department of Physics, University of York
Hass M.: Department of Particle Physics, Weizmann Institute of Science
Nara Singh B.S.: Department of Physics, University of York
Ruiz C.: TRIUMF
Tengblad O.: Instituto de Estructura de la Materia-CSIC

DOI: https://doi.org/10.1051/epjconf/20146607003
Journal volume & issue: Vol. 66
p. 07003

Abstract

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The astrophysical S-factor for the 3He(α,γ)7Be reaction plays an important role in the Solar Standard Model and in the Big Bang Nucleosynthesis scenario. The advances from two recent experiments performed using complementary techniques at center of mass (C.M.) energies between 1 and 3 MeV are discussed.

Published in EPJ Web of Conferences

ISSN: 2100-014X (Online)
Publisher: EDP Sciences
Country of publisher: France
LCC subjects: Science: Physics
Website: http://www.epj-conferences.org/

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