Proton capture on 
<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mmultiscripts><mml:mi mathvariant="normal">S</mml:mi><mml:mprescripts/><mml:none/><mml:mn>34</mml:mn></mml:mmultiscripts></mml:math>
 in the astrophysical energy regime of O-Ne novae

Lovely, M.; Lennarz, A.; Connolly, D.; Williams, M.; Alcorta, M.; Chen, A. A.; Davids, B.; Esker, N. E.; Fry, C.; Gillespie, S. A.; Giri, R.; Greife, U.; Hussein, A.; Hutcheon, D. A.; Karpesky, J.; Kroll, L.; Liang, J. F.; O’Malley, P. D.; Paneru, S. N.; Psaltis, A.; Ruiz, C.; Shotter, A.C.

doi:10.1103/physrevc.103.055801

Cited by 4 publications

(3 citation statements)

References 36 publications

Supporting

Mentioning

Contrasting

Order By: Relevance

“…Broadly, these techniques fall into the two categories of direct and indirect measurements. Direct measurements of explosive hydrogen and helium burning reactions at or near the astrophysical energies where they occur have been performed with rare isotope beams using recoil separators (DRAGON) [106,107,404,405], active targets (MUSIC, AT-TPC, ANASEN, and others) [189,190,192,406], or gas targets (JENSA) [406][407][408][409].…”

Section: How Did We Get Here?mentioning

confidence: 99%

Horizons: nuclear astrophysics in the 2020s and beyond

Schatz

Reyes

Best

et al. 2022

J. Phys. G: Nucl. Part. Phys.

View full text Add to dashboard Cite

Nuclear astrophysics is a field at the intersection of nuclear physics and astrophysics, which seeks to understand the nuclear engines of astronomical objects and the origin of the chemical elements. This white paper summarizes progress and status of the field, the new open questions that have emerged, and the tremendous scientific opportunities that have opened up with major advances in capabilities across an ever growing number of disciplines and subfields that need to be integrated. We take a holistic view of the field discussing the unique challenges and opportunities in nuclear astrophysics in regards to science, diversity, education, and the interdisciplinarity and breadth of the field. Clearly nuclear astrophysics is a dynamic field with a bright future that is entering a new era of discovery opportunities.

show abstract

Section: How Did We Get Here?mentioning

confidence: 99%

Horizons: nuclear astrophysics in the 2020s and beyond

Schatz

Reyes

Best

et al. 2022

J. Phys. G: Nucl. Part. Phys.

View full text Add to dashboard Cite

show abstract

“…The data taken for resonances in the 22 Ne(α, γ) 26 Mg reaction in 2019 are expected to be published in 2021. Further, the results from stable beam measurements to investigate reactions such as 22 Ne(p, γ) 23 Na [191,192], 76 Se(α, γ) [193], 34 S(p, γ) [194] and 19 F(p, γ) [195] have recently been published.…”

Section: Recent Measurementsmentioning

confidence: 99%

The status and future of direct nuclear reaction measurements for stellar burning

Aliotta¹,

Buompane²,

Couder³

et al. 2021

J. Phys. G: Nucl. Part. Phys.

View full text Add to dashboard Cite

The study of stellar burning began just over 100 years ago. Nonetheless, we do not yet have a detailed picture of the nucleosynthesis within stars and how nucleosynthesis impacts stellar structure and the remnants of stellar evolution. Achieving this understanding will require precise direct measurements of the nuclear reactions involved. This report summarizes the status of direct measurements for stellar burning, focusing on developments of the last couple of decades, and offering a prospectus of near-future developments.

show abstract

“…The data taken for resonances in the 22 Ne(α,γ) 26 Mg reaction in 2019 are expected to be published in 2021. Further, the results from stable beam measurements to investigate reactions such as 22 Ne(p,γ) 23 Na [193,194], 76 Se(α,γ) [195], 34 S(p,γ) [196] and 19 F(p,γ) [197] have recently been published.…”

Section: Recent Measurementsmentioning

confidence: 99%

The Status and Future of Direct Nuclear Reaction Measurements for Stellar Burning

Aliotta,

Buompane,

Couder

et al. 2021

Preprint

Self Cite

View full text Add to dashboard Cite

show abstract

Proton capture on S34 in the astrophysical energy regime of O-Ne novae

Cited by 4 publications

References 36 publications

Horizons: nuclear astrophysics in the 2020s and beyond

Horizons: nuclear astrophysics in the 2020s and beyond

The status and future of direct nuclear reaction measurements for stellar burning

The Status and Future of Direct Nuclear Reaction Measurements for Stellar Burning

Contact Info

Product

Resources

About