O. Arnold

2 ta ish

Excellence Cluster 'Origin and Structure of the Universe'

1. Production of hydrogen isotopes and charged pions in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mi>p</mml:mi></mml:math> (3.5 GeV) <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mo>+</mml:mo><mml:mo> </mml:mo><mml:mmultiscripts><mml:mi>Nb</mml:mi><mml:mprescripts/><mml:none/><mml:mn>93</mml:mn></mml:mmultiscripts></mml:math> reactions

   R. Abou Yassine, O. Arnold, M. Becker +85

   MaqolaNuclear physics research studiesPhysical review. C20231 iqtibos

   ABIABI:AkademIndex/openalex/2023.article.001846

2. Inclusive <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mrow> <mml:msup> <mml:mi>e</mml:mi> <mml:mo>+</mml:mo> </mml:msup> <mml:msup> <mml:mi>e</mml:mi> <mml:mo>−</mml:mo> </mml:msup> </mml:mrow> </mml:math> production in collisions of pions with protons and nuclei in the second resonance region of baryons

   R. Abou Yassine, J. Adamczewski-Musch, O. Arnold +97

   MaqolaParticle physics theoretical and experimental studiesPhysical review. C20250 iqtibos

   ABIABI:AkademIndex/openalex/2025.article.000860