Slide 12 Lecture 10: Cosmochemistry: origin of nuclei, solar system, and earth What is the bulk composition of the solar system? Where/when/how did the atoms of the solar…

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Slide 1 the s-process Fe Co Ni Rb Ga Ge Zn Cu Se Br As Zr Y Sr Kr (n,  ) ()() ()() r-process p-process 63 Ni, t 1/2 =100 a 64 Cu, t 1/2 =12 h,…

Lecture 15 Explosive Nucleosynthesis and the r-Process As the shock wave passes through the star, matter is briefly heated to temperatures far above what it would have experienced…

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Nuclear Astrophysics II Lecture 5 Fri. June 1, 2012 Prof. Shawn Bishop, Office 2013, Ex. 12437 [email protected] http://www.nucastro.ph.tum.de/ * Where to from here?…

Lecture 15 Explosive Nucleosynthesis and the r-Process As the shock wave passes through the star, matter is briefly heated to temperatures far above what it would have experienced…

* Lecture 10: Cosmochemistry: origin of nuclei, solar system, and earth What is the bulk composition of the solar system? Where/when/how did the atoms of the solar system…

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Nuclear Astrophysics II Lecture 5 Fri. June 1, 2012 Prof. Shawn Bishop, Office 2013, Ex. 12437 [email protected] http://www.nucastro.ph.tum.de/ * Where to from here?…