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researcher

X.-X. Bai

4 papers hereh-index 11458 citations54 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • middle author2

Across the 2 of 4 papers where every author was matched, so the position is known.

fields
  • nucl-ex4

identity via Semantic Scholar / OpenAlex

activity
20092014
most citedSpectroscopic factors for low-lying 16N levels and the astrophysical 15N(n,gamma)16N reaction rate

22 citations · 33 across the 2 of their papers we have counts for

collaborators

4 papers

nucl-ex2014★ 11 cited

Proton widths of the low-lying 16F states from the 15N(7Li, 6Li)16N reaction

Z. D. Wu, B. Guo, Z. H. Li +24

All the 16F levels are unbound by proton emission. To date the four low-lying 16F levels below 1 MeV have been experimentally identified with well established spin-parity values an…

nucl-ex2013★ 22 cited

Spectroscopic factors for low-lying 16N levels and the astrophysical 15N(n,gamma)16N reaction rate

B. Guo, Z. H. Li, Y. J. Li +23

Fluorine is a key element for nucleosynthetic studies since it is extremely sensitive to the physical conditions within stars. The astrophysical site to produce fluorine is suggest…

nucl-ex2012

Determination of astrophysical 12N(p,g)13O reaction rate from the 2H(12N, 13O)n reaction and its astrophysical implications

B. Guo, J. Su, Zhihong Li +20

The evolution of massive stars with very low-metallicities depends critically on the amount of CNO nuclides which they produce. The 12N(p,\,γ)13O reaction is an impor…

nucl-ex2009

The 13N(d,n)14O Reaction and the Astrophysical 13N(p,g)14O Reaction Rate

Z. H. Li, B. Guo, S. Q. Yan

13N(p,γ)14O is one of the key reactions in the hot CNO cycle which occurs at stellar temperatures around T9​ ≥ 0.1. Up to now, some uncertainties still exist for…

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