Study of the 6.05 MeV cascade transition in <mml:math altimg="si1.gif" overflow="scroll" xmlns:xocs="http://www.elsevier.com/xml/xocs/dtd" xmlns:xs="http://www.w3.org/2001/XMLSchema" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns="http://www.elsevier.com/xml/ja/dtd" xmlns:ja="http://www.elsevier.com/xml/ja/dtd" xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:tb="http://www.elsevier.com/xml/common/table/dtd" xmlns:sb="http://www.elsevier.com/xml/common/struct-bib/dtd" xmlns:ce="http://www.elsevier.com/xml/common/dtd" xmlns:xlink="http://www.w3.org/1999/xlink" xmlns:cals="http://www.elsevier.com/xml/common/cals/dtd"><mml:mmultiscripts><mml:mi mathvariant="normal">C</mml:mi><mml:mprescripts/><mml:none/><mml:mn>12</mml:mn></mml:mmultiscripts><mml:mo stretchy="false">(</mml:mo><mml:mi>α</mml:mi><mml:mo>,</mml:mo><mml:mi>γ</mml:mi><mml:mo stretchy="false">)</mml:mo><mml:mmultiscripts><mml:mi mathvariant="normal">O</mml:mi><mml:mprescripts/><mml:none/><mml:mn>16</mml:mn></mml:mmultiscripts></mml:math>-Reference-Cited by-同舟云学术

Study of the 6.05 MeV cascade transition in C12(α,γ)O16

Published:2011-09 Issue:5 Volume:703 Page:557-561
ISSN:0370-2693
Container-title:Physics Letters B
language:en
Short-container-title:Physics Letters B

Author:

Schürmann D.,Di Leva A.,Gialanella L.,Kunz R.,Strieder F.,De Cesare N.,De Cesare M.,DʼOnofrio A.,Fortak K.,Imbriani G.,Rogalla D.,Romano M.,Terrasi F.

Funder

DFG

INFN

Publisher

Elsevier BV

Subject

Nuclear and High Energy Physics

Reference42 articles.

1. The12C(α, γ)16O Reaction Rate and the Evolution of Stars in the Mass Range 0.8 ≤ M/M⊙ ≤ 25

2. Nucleosynthesis in Massive Stars with Improved Nuclear and Stellar Physics

3. Explosive Yields of Massive Stars fromZ= 0 toZ=Z⊙

4. On the Sensitivity of Massive Star Nucleosynthesis and Evolution to Solar Abundances and to Uncertainties in Helium‐Burning Reaction Rates

5. PRODUCTION OF26Al,44Ti, AND60Fe IN CORE-COLLAPSE SUPERNOVAE: SENSITIVITY TO THE RATES OF THE TRIPLE ALPHA AND12C(α, γ)16O REACTIONS

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