Publication Date:
2018-05-09
Description:
Author(s): R. Talwar, M. J. Bojazi, P. Mohr, K. Auranen, M. L. Avila, A. D. Ayangeakaa, J. Harker, C. R. Hoffman, C. L. Jiang, S. A. Kuvin, B. S. Meyer, K. E. Rehm, D. Santiago-Gonzalez, J. Sethi, C. Ugalde, and J. R. Winkelbauer In massive stars, the Ca 41 ( n , α ) Ar 38 and K 41 ( p , α ) Ar 38 reactions have been identified as the key reactions governing the abundance of Ca 41 , which is considered as a potential chronometer for solar system formation. So far, due to experimental limitations, the Ca 41 ( n , α ) Ar 38 reaction rate is solely base... [Phys. Rev. C 97, 055801] Published Tue May 08, 2018
Keywords:
Nuclear Astrophysics
Print ISSN:
0556-2813
Electronic ISSN:
1089-490X
Topics:
Physics
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