JINA-CEE ION OPTICS SUMMER SCHOOL: JIOSS 2018

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group_secar2.0 [2018/09/11 16:12]
wagner 		group_secar2.0 [2018/09/11 16:13]
wagner
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 -by Alex, Nadeesha and Louis- -by Alex, Nadeesha and Louis-
  
-**DAY1**\\ +__**DAY1**\\ 
-**Getting started**\\+**Getting started**\\__
 Choosen example reaction: <sup>45</sup>V(p,γ)<sup>46</sup>Cr\\ Choosen example reaction: <sup>45</sup>V(p,γ)<sup>46</sup>Cr\\
 ⇒important for <sup>44</sup>Ti production rate in core collapse Supernova ([[https://www.sciencedirect.com/science/article/pii/S0375947403008704|Horoi et al. Nucl.Phys.A 718, (2003)]])\\ ⇒important for <sup>44</sup>Ti production rate in core collapse Supernova ([[https://www.sciencedirect.com/science/article/pii/S0375947403008704|Horoi et al. Nucl.Phys.A 718, (2003)]])\\
 Beam: <sup>45</sup>V<sup>13+</sup> of 135 MeV (1% enegry spread)\\ Beam: <sup>45</sup>V<sup>13+</sup> of 135 MeV (1% enegry spread)\\
 {{ :dipole.png?300 |}}\\ {{ :dipole.png?300 |}}\\
-*Understanding COSY Matrix output:*\\+**Understanding COSY Matrix output:**\\
 |1.0|0.0|0.0|0.0|-0.41| |1.0|0.0|0.0|0.0|-0.41|
 |2.2|1.0|0.0|0.0|-0.35|\\ |2.2|1.0|0.0|0.0|-0.35|\\
/srv/thewikis/JIOSS/data/pages/group_secar2.0.txt · Last modified: 2018/09/13 16:49 by plastun

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