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NSR database version of May 3, 2024.

Search: Author = Q.H.Peng

Found 5 matches.

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2017LI25      Chin.Phys.C 41, 095101 (2017)

J.-J.Liu, Q.-H.Peng, D.-M.Liu

Strongly screening electron capture for nuclides ^{52, 53, 59, 60}Fe by the Shell-Model Monte Carlo method in pre-supernovae

RADIOACTIVITY ^52,53,59,60Fe(EC); calculated strong screening rates in pre-supernovae using the Shell-Model Monte Carlo method, based on the nuclear random phase approximation and linear response theory model for electrons.

doi: 10.1088/1674-1137/41/9/095101
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2006WA15      Chin.Phys.Lett. 23, 1652 (2006)

P.Wang, Q.-H.Peng, S.-N.Zhang, X.-L.Luo

Fusion Reaction of ¹⁶O+¹⁴N and Its Implication for the Production of ²⁶Al in Explosive Oxygen Burning

NUCLEAR REACTIONS ¹⁶O(¹⁴N, np), (¹⁴N, pα), (¹⁴N, α), E=spectrum; analyzed reaction rates, branching ratios; deduced sensitivity to mixing mechanisms.

doi: 10.1088/0256-307X/23/6/082
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2004PE15      Nucl.Phys. A738, 515 (2004)

Q.-H.Peng

A New mechanism of Core Collapsed Supernova Explosion - The important role of Electron Capture process

doi: 10.1016/j.nuclphysa.2004.04.100
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2003JI04      Chin.Phys.Lett. 20, 647 (2003)

G.-F.Jiang, Q.-H.Peng, C.-K.Chou

Effects of Electron Screening on Electron Capture Rates in High Density Presupernova Core

RADIOACTIVITY ⁵⁵Co, ⁵⁶Ni(EC); calculated electron screening effects on capture rate in pre-supernova stellar environment.

doi: 10.1088/0256-307X/20/5/316
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1999LI29      Chin.Phys.Lett. 16, 619 (1999)

J.Li, B.Zhang, G.-Q.Wei, L.-P.Zhang, Q.-H.Peng

Abundances of the Neutron-Capture Elements in Metal-Poor Halo Star HD 126238

NUCLEAR STRUCTURE Z=30-83; analyzed stellar abundances; deduced model parameters, r-process and s-process contributions.

doi: 10.1088/0256-307X/16/8/027
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