NSR Query Results

Output year order : Descending
Format : Normal

NSR database version of April 24, 2024.

Search: Author = C.E.Fields

Found 3 matches.

Back to query form

2019FR05      Eur.Phys.J. A 55, 132 (2019)

Ch.L.Fryer, N.Lloyd-Ronning, R.Wollaeger, B.Wiggins, J.Miller, J.Dolence, B.Ryan, C.E.Fields

Understanding the engines and progenitors of gamma-ray bursts

doi: 10.1140/epja/i2019-12818-y
Citations: PlumX Metrics

2018FI01      Astrophys.J.Suppl.Ser. 234, 19 (2018)

C.E.Fields, F.X.Timmes, R.Farmer, I.Petermann, W.M.Wolf, S.M.Couch

The Impact of Nuclear Reaction Rate Uncertainties on the Evolution of Core-collapse Supernova Progenitors

NUCLEAR REACTIONS 14N(p, γ), 8Be(α, X)12C, 12C(12C, p), 12C(16O, p), 16O(16O, n), 16O(16O, p), 16O(16O, α), E<100 keV; calculated reaction rates and uncertainties; deduced variations induced by uncertainties in nuclear reaction rates grow with each passing phase of stellar evolution.

doi: 10.3847/1538-4365/aaa29b
Citations: PlumX Metrics

2017DE26      Rev.Mod.Phys. 89, 035007 (2017)

R.J.deBoer, J.Gorres, M.Wiescher, R.E.Azuma, A.Best, C.R.Brune, C.E.Fields, S.Jones, M.Pignatari, D.Sayre, K.Smith, F.X.Timmes, E.Uberseder

The 12C(α, γ)16O reaction and its implications for stellar helium burning

NUCLEAR REACTIONS 12C(α, γ)16O, E(cm)<6 MeV; analyzed available data; deduced σ, reaction rates and uncertainties.

doi: 10.1103/RevModPhys.89.035007
Citations: PlumX Metrics

Back to query form