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STARLIB: a next-generation reaction-rate library for nuclear astrophysics

STARLIB: a next-generation reaction-rate library for nuclear astrophysics

http://www.wikidata.org/entity/Q57426412

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Coulomb dissociation ofN20,21 Exploring masses and CNO surface abundances of red giant stars Improved Direct Measurement of the 64.5 keV Resonance Strength in the ^{17}O(p,α)^{14}N Reaction at LUNA.Primordial nucleosynthesis Measurement of theErc.m.=138keV resonance in the23Na(p,γ)24Mg reaction and the abundance of sodium in AGB stars Correlated uncertainties in Monte Carlo reaction rate calculations New measurements of low-energy resonances in theNe22(p,γ)Na23reaction High-intensity-beam study ofO17(p,γ)F18and thermonuclear reaction rates forO17+p Nuclear astrophysics in the laboratory and in the universe Coulomb dissociation ofP27at 500 MeV/u Recent results in nuclear astrophysics

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STARLIB: a next-generation reaction-rate library for nuclear astrophysics

http://www.wikidata.org/entity/Q57426412

description

wetenschappelijk artikel

@nl

наукова стаття, опублікована в липні 2013

@uk

name

STARLIB: A NEXT-GENERATION REACTION-RATE LIBRARY FOR NUCLEAR ASTROPHYSICS

@nl

STARLIB: a next-generation reaction-rate library for nuclear astrophysics

@en

type

label

STARLIB: A NEXT-GENERATION REACTION-RATE LIBRARY FOR NUCLEAR ASTROPHYSICS

@nl

STARLIB: a next-generation reaction-rate library for nuclear astrophysics

@en

prefLabel

STARLIB: A NEXT-GENERATION REACTION-RATE LIBRARY FOR NUCLEAR ASTROPHYSICS

@nl

STARLIB: a next-generation reaction-rate library for nuclear astrophysics

@en

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The Astrophysical Journal Supplement series

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STARLIB: a next-generation reaction-rate library for nuclear astrophysics

@en

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A. E. Champange

http://www.w3.org/2001/XMLSchema#string

A. L. Sallaska

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C. Iliadis

http://www.w3.org/2001/XMLSchema#string

F. X. Timmes

http://www.w3.org/2001/XMLSchema#string

S. Goriely

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S. Starrfield

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18

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scholarly article

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10.1088/0067-0049/207/1/18

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1

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207

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2013-07-02T00:00:00Z

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1304.7811

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2013ApJS..207...18S

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