Lowest l = 0proton resonance in 26Si and implications for nucleosynthesis of 26Al

Peplowski, P. N.; Baby, L. T.; Wiedenhöver, I.; Dekat, S. E.; Diffenderfer, E.; Gay, D. L.; Grubor-Urosevic, O.; Höflich, P.; Kaye, R. A.; Keeley, N.; Rojas, A.; Volya, A.

doi:10.1103/physrevc.79.032801

Title: Lowest l = 0proton resonance in ²⁶Si and implications for nucleosynthesis of ²⁶Al

Journal Article · Tue Mar 03 00:00:00 EST 2009 · Physical Review. C. Nuclear Physics

DOI:https://doi.org/10.1103/physrevc.79.032801· OSTI ID:1669895

Peplowski, P. N. ^[1]; Baby, L. T. ^[1]; Wiedenhöver, I. ^[1]; Dekat, S. E. ^[2]; Diffenderfer, E. ^[1]; Gay, D. L. ^[2]; Grubor-Urosevic, O. ^[3]; Höflich, P. ^[1]; Kaye, R. A. ^[4]; Keeley, N. ^[5]; Rojas, A. ^[1]; Volya, A. ^[1]

Florida State University, Tallahassee, FL (United States)
University of North Florida, Jacksonville, FL (United States)
Purdue University Calumet, Hammond, IN (United States)
Purdue University Calumet, Hammond, IN (United States); Ohio Wesleyan University, Delaware, OH (United States)
The Andrezj Sołtan Institute for Nuclear Studies, Warsaw (Poland)

Using a beam of the radioactive isotope ²⁵Al, produced with the new resolut facility, we measured the direct (d,n) proton-transfer reaction leading to low-lying proton-resonances in ²⁶Si. Here, we observed the lowest l = 0 proton resonance, identified with the 3⁺ state at 5.914 MeV excitation energy. This result eliminates the largest uncertainty about the astrophysical reaction rates involved in the nucleosynthesis of ²⁶Al.

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Research Organization:: Florida State Univ., Tallahassee, FL (United States)

Sponsoring Organization:: USDOE Office of Science (SC), Nuclear Physics (NP); National Science Foundation (NSF); Marie Curie Actions Grant

Grant/Contract Number:: FG02-02ER41220; FG02-92ER40750; MEIF-CT-2005-010158; PHY-04-56463; PHY-0216345; PHY-0216072

OSTI ID:: 1669895

Journal Information:: Physical Review. C. Nuclear Physics, Vol. 79, Issue 3; ISSN 0556-2813

Publisher:: American Physical Society (APS)Copyright Statement

Country of Publication:: United States

Language:: English

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Cited by: 31 works

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Classical-Nova Contribution to the Milky Way’s ${}^{26}{Al}$ Abundance: Exit Channel of the Key ${}^{25}{Al} (p, γ) {}^{26}{Si}$ Resonance Bennett, M. B.; Wrede, C.; Chipps, K. A. Physical Review Letters, Vol. 111, Issue 23 https://doi.org/10.1103/physrevlett.111.232503	journal	December 2013
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Resonances above the proton threshold in ${}^{26}{Si}$ Chipps, K. A. Physical Review C, Vol. 93, Issue 3 https://doi.org/10.1103/physrevc.93.035801	journal	March 2016
Thermonuclear ${}^{25}{Al} (p, γ) {}^{26}{Si}$ reaction rate in classical novae and Galactic ${}^{26}{Al}$ Wrede, C. Physical Review C, Vol. 79, Issue 3 https://doi.org/10.1103/physrevc.79.035803	journal	March 2009
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