Constraining the Synthesis of the Lightest <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"> <mml:mi>p</mml:mi> </mml:math> Nucleus <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"> <mml:mrow> <mml:mm

We provide the first experimental cross section of the ^{73}As(p,γ)^{74}Se reaction to constrain one of the main destruction mechanisms of the p nucleus ^{74}Se in explosive stellar environments. The measurement was done using a radioactive ^{73}As beam at effective center-of-mass energies of 2.9 and 2.3 MeV/nucleon. Along with the total cross-section measurement, statistical properties of the ^{74}Se compound nucleus were extracted, constraining the reaction cross section in the upper Gamow window of the γ process. The impact of the experimentally constrained reaction rate on ^{74}Se production in Type II supernovae was investigated through Monte Carlo one-zone network simulations. The results indicate that the overproduction of ^{74}Se by Type II supernova models cannot be resolved by nuclear physics alone and point toward the need for a more detailed understanding of the astrophysical conditions of relevance for the γ process.

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Journal
Physical Review Letters
Published
2025-11-20
DOI
https://doi.org/10.1103/d7dr-h36j
Primary Topic
Nuclear physics research studies
Type
article
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Constraining the Synthesis of the Lightest <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"> <mml:mi>p</mml:mi> </mml:math> Nucleus <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"> <mml:mrow> <mml:mm

A. Tsantiri, A. Psaltis, G. Owens-Fryar, Ana Henriques et al.
Physical Review Letters
Nuclear physics research studies
article

Constraining the Synthesis of the Lightest <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"> <mml:mi>p</mml:mi> </mml:math> Nucleus <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"> <mml:mrow> <mml:mm

A. Tsantiri, A. Psaltis, G. Owens-Fryar, Ana Henriques, R. Jain, A. C. C. Villari, Samuel Nash, K. Bosmpotinis, A. A. Doetsch, H. Arora, C. Dembski, R. G. T. Zegers, H. Schatz, P. Tsintari, H. C. Berg, E. Good, F. Montes, Lorenzo Roberti, A. Richard, Pablo Giuliani, Lauren Balliet, C. S. Sumithrarachchi, M. Smith, T. Gaballah, R. S. Lubna, A. Spyrou, S. Lyons, A. Palmisano-Kyle, Belen Monteagudo Godoy, E. K. Ronning, S. N. Liddick, S. Uthayakumaar, Pavel A. Denissenkov, P. A. DeYoung, G. Balk, Jorge A. Pereira, R. Garg, M. K. Smith, J. M. Berkman, Ana Arribas Sebastián, C. Tinson, N. Dimitrakopoulos, N. Tubaro, E. Weissling, G. U. Ogudoro
article en

Abstract

We provide the first experimental cross section of the ^{73}As(p,γ)^{74}Se reaction to constrain one of the main destruction mechanisms of the p nucleus ^{74}Se in explosive stellar environments. The measurement was done using a radioactive ^{73}As beam at effective center-of-mass energies of 2.9 and 2.3 MeV/nucleon. Along with the total cross-section measurement, statistical properties of the ^{74}Se compound nucleus were extracted, constraining the reaction cross section in the upper Gamow window of the γ process. The impact of the experimentally constrained reaction rate on ^{74}Se production in Type II supernovae was investigated through Monte Carlo one-zone network simulations. The results indicate that the overproduction of ^{74}Se by Type II supernova models cannot be resolved by nuclear physics alone and point toward the need for a more detailed understanding of the astrophysical conditions of relevance for the γ process.

Physical Review LettersVol. 135(21)
University of Notre Dame (US), Pacific Northwest National Laboratory (US), Hope College (US), Central Michigan University (US), Duke University (US), University of Victoria (CA), Konkoly Observatory (HU), Triangle Universities Nuclear Laboratory (US), Caporal Assistance Network (US), Ohio University (US), Istituto Nazionale di Fisica Nucleare, Laboratori Nazionali del Sud (IT), Centralsjukhuset Kristianstad (SE), Facility for Rare Isotope Beams, University of Tennessee at Knoxville (US), Michigan State University (US), National Institute for Astrophysics (IT), Mississippi State University (US)
Openalex Percentile: Top 84%
Nuclear physics research studies
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