Author

Peng, Qiu He

3 papers

Affiliationsfrom papers in this corpus

Unlisted, CN2021(1)

Collaboratorsmost frequent first

	Paper	Category
Dec 7, 2021#62111.01994	Directed flow of charged particles within idealized viscous hydrodynamics at energies available at the BNL Relativistic Heavy Ion Collider and at the CERN Large Hadron Collider Ze-Fang Jiang🇨🇳 · C. B. Yang🇨🇳 · Qi Peng🇨🇳	↳ hep-ph	PRC	20
Jul 13, 2017#11707.03504	Strongly screening electron capture rates of chromium isotopes in presupernova Jing-Jing Liu🇨🇳 · Qiu-He Peng🇨🇳 · Liang-Huan Hao · Xiao-Ping Kang · Dong-Mei Liu	nucl-th	Res.Astron.Astrophys.	19
Jan 23, 2017#11701.05771	Strongly screening on electron capture for Nuclides $^{52, 53, 59, 60}$ Fe by the Shell-Model Monte Carlo method in pre-supernova Jing-Jing Liu🇨🇳 · Qiu-He Peng🇨🇳 · Dong-Mei Liu	nucl-th	CPC	7

Directed flow of charged particles within idealized viscous hydrodynamics at energies available at the BNL Relativistic Heavy Ion Collider and at the CERN Large Hadron Collider
Ze-Fang Jiang🇨🇳 · C. B. Yang🇨🇳 · Qi Peng🇨🇳
Dec 7, 20212111.01994↳ hep-phPRC20 citations
Strongly screening electron capture rates of chromium isotopes in presupernova
Jing-Jing Liu🇨🇳 · Qiu-He Peng🇨🇳 · Liang-Huan Hao · Xiao-Ping Kang · Dong-Mei Liu
Jul 13, 20171707.03504nucl-thRes.Astron.Astrophys.19 citations
Strongly screening on electron capture for Nuclides $^{52, 53, 59, 60}$ Fe by the Shell-Model Monte Carlo method in pre-supernova
Jing-Jing Liu🇨🇳 · Qiu-He Peng🇨🇳 · Dong-Mei Liu
Jan 23, 20171701.05771nucl-thCPC7 citations

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Peng, Qiu He

Directed flow of charged particles within idealized viscous hydrodynamics at energies available at the BNL Relativistic Heavy Ion Collider and at the CERN Large Hadron Collider

Strongly screening electron capture rates of chromium isotopes in presupernova

Strongly screening on electron capture for Nuclides 52,53,59,60Fe by the Shell-Model Monte Carlo method in pre-supernova

Affiliations

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