S. Hou

most citedImproved thermonuclear rate of

^{42}

Ti(

p

γ

)

^{43}

V and its astrophysical implication in rp-process

2 citations · 2 across the 1 of their papers we have counts for

collaborators

2 papers

astro-ph.SR2025★ 2 cited

Improved thermonuclear rate of $^{42}$ Ti( $p$ , $γ$ ) $^{43}$ V and its astrophysical implication in rp-process

S. Q. Hou, C. Iliadis, M. Pignatari +4

Accurate $^{42}$ Ti( $p$ , $γ$ ) $^{43}$ V reaction rates are crucial for understanding the nucleosynthesis path of the rapid capture process (rp-process) that occurs in X-ray bursts. We…

nucl-ex2018

Experimentally well-constrained masses of $^{27}$ P and $^{27}$ S: Implications for studies of explosive binary systems

L. J. Sun, X. X. Xu, S. Q. Hou +58

The mass of $^{27}$ P was predicted to impact the X-ray burst (XRB) model predictions of burst light curves and the composition of the burst ashes. To address the uncertainties and…

Improved thermonuclear rate of 42Ti(p,γ)43V and its astrophysical implication in rp-process

Experimentally well-constrained masses of 27P and 27S: Implications for studies of explosive binary systems

Improved thermonuclear rate of $^{42}$ Ti( $p$ , $γ$ ) $^{43}$ V and its astrophysical implication in rp-process

Experimentally well-constrained masses of $^{27}$ P and $^{27}$ S: Implications for studies of explosive binary systems