26Al production: The Allende meteorite (Chihuahua) stellar nucleosynthesis and solar models


Por: Araujo-Escalona, V., Andrade, E., Barrón-Palos, L., Canto, C., Favela, F., Huerta, A., De Lucio, O., Ortiz, M.E., Solís, C., Chávez, E.

Publicada: 1 ene 2015
Categoría: Physics and Astronomy (miscellaneous)

Resumen:
In 1969 a meteorite fell near the small town of Allende, state of Chihuahua in the north of Mexico. Its study yielded information that changed the current understanding of the solar model. In particular traces of 26Al were found. Abundances of that isotope had been seen in the universe and were related to regions of active heavy nucleosynthesis. Its presence on the solar system was unexpected. It is now understood that cosmic rays induce nuclear reactions on materials to produce 26Al, on Earth this is well known and it is the basis of many environmental studies, so it is not only the product of some high metalicity star collapse. Taking advantage of the recently reinforced laboratory infrastructure of the Instituto de Física, at UNAM in Mexico City, we proposed to measure the cross section for 26Al production via some of the most likely reactions, from the nuclear physics point of view (highest Q-values). In this paper the study of the 28Si(d,a)26 Al nuclear reaction is shown. A target is prepared by a mixture of silicon and aluminum powders. It is irradiated with a deuteron beam (â‰1 µA current) at the MV CN-Van de Graaff accelerator laboratory. The number of projectiles is deduced by Rutherford Backscattering Spectrometry (RBS). The produced 26Al nuclei are then counted at the Accelerator Mass Spectrometry Laboratory. © 2015 AIP Publishing LLC.

Filiaciones:
Araujo-Escalona, V.:
 InstitutO de Fisica, UNAM, Mexico

Andrade, E.:
 InstitutO de Fisica, UNAM, Mexico

Barrón-Palos, L.:
 InstitutO de Fisica, UNAM, Mexico

Canto, C.:
 InstitutO de Fisica, UNAM, Mexico

Favela, F.:
 InstitutO de Fisica, UNAM, Mexico

Huerta, A.:
 InstitutO de Fisica, UNAM, Mexico

De Lucio, O.:
 InstitutO de Fisica, UNAM, Mexico

Ortiz, M.E.:
 InstitutO de Fisica, UNAM, Mexico

Solís, C.:
 InstitutO de Fisica, UNAM, Mexico

Chávez, E.:
 InstitutO de Fisica, UNAM, Mexico
ISSN: 0094243X
Editorial
AMER INST PHYSICS, 2 HUNTINGTON QUADRANGLE, STE 1NO1, MELVILLE, NY 11747-4501 USA, Estados Unidos America
Tipo de documento: Conference Paper
Volumen: 1671 Número:
Páginas:
WOS Id: 000371691800015