N. Hubbard

activity

20152021

^{19}

Ne relevant to

^{18}

F(p,

α

)

^{15}

6 citations · 6 across the 2 of their papers we have counts for

collaborators

4 papers

nucl-ex2021

New experimental $^{23}$ Na( $α, p$ ) $^{26}$ Mg Reaction Rate for Massive Star and Type-Ia Supernova models

N. J. Hubbard, C. Aa. Diget, S. P. Fox +8

The $^{23}$ Na( $α, p$ ) $^{26}$ Mg reaction has been identified as having a significant impact on the nucleosynthesis of several nuclei between Ne and Ti in type-Ia supernovae, and of $…

nucl-ex2020★ 6 cited

Sub-threshold states in $^{19}$ Ne relevant to $^{18}$ F(p, $α$ ) $^{15}$ O

J. E. Riley, A. M. Laird, N. de Séréville +24

Classical novae result from thermonuclear explosions producing several $γ$ -ray emitters which are prime targets for satellites observing in the MeV range. The early 511 keV gamma-r…

nucl-ex2018

First Accurate Normalization of the $β$ -delayed $α$ Decay of $^{16}$ N and Implications for the $^{12}$ C $(α, γ)^{16}$ O Astrophysical Reaction Rate

O. S. Kirsebom, O. Tengblad, R. Lica +41

The $^{12} C (α, γ)^{16} O$ reaction plays a central role in astrophysics, but its cross section at energies relevant for astrophysical applications is only poorly cons…

nucl-ex2015

The 23Na(α,p) 26Mg reaction rate at astrophysically relevant energies

A. M. Howard, M. Munch, H. O. U. Fynbo +4

The production of 26 Al in massive stars is sensitive to the 23 Na(a,p) 26 Mg cross section. Recent experimental data suggest the currently recommended cross sections are underesti…

New experimental 23Na(α,p)26Mg Reaction Rate for Massive Star and Type-Ia Supernova models

Sub-threshold states in 19Ne relevant to 18F(p,α)15O

First Accurate Normalization of the β-delayed α Decay of 16N and Implications for the 12C(α,γ)16O Astrophysical Reaction Rate

The 23Na(α,p) 26Mg reaction rate at astrophysically relevant energies

New experimental $^{23}$ Na( $α, p$ ) $^{26}$ Mg Reaction Rate for Massive Star and Type-Ia Supernova models

Sub-threshold states in $^{19}$ Ne relevant to $^{18}$ F(p, $α$ ) $^{15}$ O

First Accurate Normalization of the $β$ -delayed $α$ Decay of $^{16}$ N and Implications for the $^{12}$ C $(α, γ)^{16}$ O Astrophysical Reaction Rate