W. Ong

activity

20222026

^{22}

Mg waiting point relevant for x-ray burst nucleosynthesis via the

^{22}

Mg(

α

p

)

^{25}

Al reaction

12 citations · 12 across the 6 of their papers we have counts for

collaborators

Showing 2026Show all

3 papers · 1 filter

nucl-ex2026

Implications for Type Ia Supernova Nucleosynthesis from an Experimentally Constrained $^{16}$ O $(p, α)^{13}$ N Reaction Rate

M. Alruwaili, C. Fougeres, A. M. Laird +13

The $^{16}$ O $(p, α)^{13}$ N reaction plays a key role in shaping the $α$ -particle abundance during explosive oxygen burning in Type Ia supernovae. By enhancing $α$ -production, this r…

nucl-ex2026

Detailed Study of the $^{59}$ Cu(p, $α)^{56}$ Ni Reaction and Constraints on Its Astrophysical Reaction Rate

E. Lopez-Saavedra, M. L. Avila, W. -J. Ong +20

The $^{59}$ Cu $(p, α)^{56}$ Ni reaction plays an important role in explosive astrophysical scenarios such as Type I X-ray bursts and the $ν p$ -process in neutrino-driven winds followin…

nucl-ex2026

Direct Measurement of the $^{59}$ Cu $(p, α)^{56}$ Ni Excitation Function to Constrain the Ni--Cu Cycle Strength and Its Impact on Explosive Nucleosynthesis

E. Lopez-Saavedra, M. L. Avila, W. -J. Ong +21

A new direct measurement of the 59Cu(p,a)56Ni excitation function from 2.43-5.88 MeV in the center-of-mass was performed in inverse kinematics using the high-efficiency MUSIC activ…

Implications for Type Ia Supernova Nucleosynthesis from an Experimentally Constrained 16O(p,α)13N Reaction Rate

Detailed Study of the 59Cu(p,α)56Ni Reaction and Constraints on Its Astrophysical Reaction Rate

Direct Measurement of the 59Cu(p,α)56Ni Excitation Function to Constrain the Ni--Cu Cycle Strength and Its Impact on Explosive Nucleosynthesis

Implications for Type Ia Supernova Nucleosynthesis from an Experimentally Constrained $^{16}$ O $(p, α)^{13}$ N Reaction Rate

Detailed Study of the $^{59}$ Cu(p, $α)^{56}$ Ni Reaction and Constraints on Its Astrophysical Reaction Rate

Direct Measurement of the $^{59}$ Cu $(p, α)^{56}$ Ni Excitation Function to Constrain the Ni--Cu Cycle Strength and Its Impact on Explosive Nucleosynthesis