Origin of r-process elements

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Theoretical calculation II (Wilson et al.

2006)

Wilson’s new simulation(2006)

M=20M progenitor mass

Improved EOS

Improved numerical method

Entropy~500k

timescale ~0.1sec

Nuclear Fireworks in Stars via the Breakout from the CNO Cycle

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ARIS 2014 - Joint Institute for Nuclear Astrophysics

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Theoretical calculation II (Wilson et al. 2006) Wilson’s new simulation(2006) M=20M progenitor mass Improved EOS Improved numerical method Entropy~500k timescale ~0.1sec

Page 1 and 2: Origin of r-process elements Kaori
Page 3 and 4: Network code Full dynamical netwo
Page 5: Theoretical calculation II (Wilson
Page 9 and 10: Theoretical calculation II (Wilson
Page 11 and 12: Heavy elements are formed at the la

Origin of r-process elements

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