K. Rehm

activity

20222026

^{22}

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

^{22}

Mg(

α

p

)

^{25}

Al reaction

12 citations · 13 across the 3 of their papers we have counts for

collaborators

4 papers

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-ex2025★ 1 cited

First experimental determination of the $^{40}$ Ar( $n, 2 n$ ) $^{39}$ Ar reaction cross section and $^{39}$ Ar production in Earth's atmosphere

S. Bhattacharya, M. Paul, R. N. Sahoo +28

The cosmogenic $^{39}$ Ar(t $_{1/2}$ = 268 years) isotope of argon is used for geophysical dating and tracing owing to its appropriate half-life and chemical inertness as a noble gas;…

nucl-ex2025

First measurement of 87Rb(α, xn) cross sections at weak r-process energies in supernova ν-driven ejecta to investigate elemental abundances in low-metallicity stars

C. Fougères, M. L. Avila, A. Psaltis +18

Observed abundances of Z ~ 40 elements in metal-poor stars vary from star to star, indicating that the rapid and slow neutron capture processes may not contribute alone to the synt…

nucl-ex2022★ 12 cited

Study of the $^{22}$ Mg waiting point relevant for x-ray burst nucleosynthesis via the $^{22}$ Mg( $α$ , $p$ ) $^{25}$ Al reaction

H. Jayatissa, M. L. Avila, K. E. Rehm +13

The $^{22}$ Mg( $α$ , $p$ ) $^{25}$ Al reaction rate has been identified as a major source of uncertainty for understanding the nucleosynthesis flow in Type-I x-ray bursts (XRBs). We repo…

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

First experimental determination of the 40Ar(n,2n)39Ar reaction cross section and 39Ar production in Earth's atmosphere

First measurement of 87Rb(α, xn) cross sections at weak r-process energies in supernova ν-driven ejecta to investigate elemental abundances in low-metallicity stars

Study of the 22Mg waiting point relevant for x-ray burst nucleosynthesis via the 22Mg(α,p)25Al reaction

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

First experimental determination of the $^{40}$ Ar( $n, 2 n$ ) $^{39}$ Ar reaction cross section and $^{39}$ Ar production in Earth's atmosphere

Study of the $^{22}$ Mg waiting point relevant for x-ray burst nucleosynthesis via the $^{22}$ Mg( $α$ , $p$ ) $^{25}$ Al reaction