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Neutrino-Induced Nucleosynthesis ofA>64Nuclei: TheνpProcess

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Fröhlich, C., Martínez-Pinedo, G., Liebendörfer, M., Thielemann, F.-K., Bravo, E., Hix, W. R., Langanke, K., Zinner, N. T.·2006·Physical Review Letters

Abstract

We present a new nucleosynthesis process that we denote as the nu p process, which occurs in supernovae (and possibly gamma-ray bursts) when strong neutrino fluxes create proton-rich ejecta. In this process, antineutrino absorptions in the proton-rich environment produce neutrons that are immediately captured by neutron-deficient nuclei. This allows for the nucleosynthesis of nuclei with mass numbers A>64, , making this process a possible candidate to explain the origin of the solar abundances of (92,94)Mo and (96,98)Ru. This process also offers a natural explanation for the large abundance of Sr seen in a hyper-metal-poor star.

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Metadata

Authors
Fröhlich, C., Martínez-Pinedo, G., Liebendörfer, M., Thielemann, F.-K., Bravo, E., Hix, W. R., Langanke, K., & Zinner, N. T.
Venue
Physical Review Letters
Published
2006-04-10
Volume
96
Issue
14
Pages
142502-142502
ISSN
  • 0031-9007 (ISSN-L)
  • 1079-7114
OpenAlex
W1972276701
Cited by
602
References
0
FWCI
15.32
Type
journal article
Language
en
Open access
bronze

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CoChat. (2026). Citation check: Neutrino-Induced Nucleosynthesis ofA>64Nuclei: TheνpProcess. https://app.cochat.ai/papers/10.1103/physrevlett.96.142502
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Fröhlich, C., Martínez-Pinedo, G., Liebendörfer, M., Thielemann, F.-K., Bravo, E., Hix, W. R., Langanke, K., & Zinner, N. T. (2006). Neutrino-Induced Nucleosynthesis ofA>64Nuclei: TheνpProcess. Physical Review Letters. https://doi.org/10.1103/physrevlett.96.142502

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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).

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