activity
20122019
most citedStatistical Methods for Thermonuclear Reaction Rates and Nucleosynthesis Simulations

49 citations · 154 across the 7 of their papers we have counts for

collaborators

7 papers

nucl-ex2019★ 8 cited

A study of Cl excited states via S()

Kiana Setoodehnia, John H. Kelley, Caleb Marshall +2

Presolar grains originating in oxygen-neon novae may be identified by their sulfur isotopic ratios compared with theoretical estimates. These ratios depend on reliable S($p,…

nucl-ex2018★ 4 cited

Excited states of Ca and their significance in nova nucleosynthesis

Kiana Setoodehnia, Caleb Marshall, Richard Longland +3

Background: Discrepancies exist between the observed abundances of argon and calcium in oxygen-neon nova ejecta and those predicted by nova models. An improved characterization of…

nucl-th2014★ 19 cited

Thermonuclear reaction rate of Ne(,)Na from Monte-Carlo calculations

P. Mohr, R. Longland, C. Iliadis

The Ne(,)Na reaction impacts the break-out from the hot CNO-cycles to the -process in type I X-ray bursts. We present a revised thermonuclear reaction rate,…

nucl-ex2014★ 49 cited

Statistical Methods for Thermonuclear Reaction Rates and Nucleosynthesis Simulations

Christian Iliadis, Richard Longland, Alain Coc +2

Rigorous statistical methods for estimating thermonuclear reaction rates and nucleosynthesis are becoming increasingly established in nuclear astrophysics. The main challenge being…

astro-ph.SR2012★ 39 cited

Is γ-ray emission from novae affected by interference effects in the 18F(p,α)15O reaction?

A. M. Laird, A. Parikh, A. St. J. Murphy +14

The 18F(p,α)15O reaction rate is crucial for constraining model predictions of the γ-ray observable radioisotope 18F produced in novae. The determination of this rate is challengin…

nucl-ex2012★ 11 cited

Nuclear structure of 30S and its implications for nucleosynthesis in classical novae

K. Setoodehnia, A. A. Chen, D. Kahl +29

The uncertainty in the 29P(p,gamma)30S reaction rate over the temperature range of 0.1 - 1.3 GK was previously determined to span ~4 orders of magnitude due to the uncertain locati…