Paul McEwan

1 ta ish

University of Birmingham

1. Decay path measurements for the 2.429 MeV state in<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mmultiscripts><mml:mi mathvariant="normal">Be</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>9</mml:mn></mml:mrow></mml:mmultiscripts></mml:math>: Implications for the astrophysical<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>α</mml:mi><mml:mo>+</mml:mo><mml:mi>α</mml:mi><mml:mo>+</mml:mo><mml:mi>n</mml:mi></mml:mrow></mml:math>reaction

   P. Papka, T. A. D. Brown, Benjamin J. Fulton +15

   Maqola20072 iqtibos

   ABIABI:AkademIndex/2026.other.525590