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Phys. Rev. Lett. 103, 121101 (2009) [4 pages]

Formation of Nuclear “Pasta” in Supernovae

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Gentaro Watanabe1,2, Hidetaka Sonoda3,2, Toshiki Maruyama4, Katsuhiko Sato3,5, Kenji Yasuoka6, and Toshikazu Ebisuzaki2
1CNR INFM-BEC and Department of Physics, University of Trento, 38050 Povo, Italy
2RIKEN, 2-1 Hirosawa, Wako, Saitama 351-0198, Japan
3Department of Physics, University of Tokyo, Tokyo 113-0033, Japan
4ASRC, Japan Atomic Energy Agency, Tokai, Ibaraki 319-1195, Japan
5IPMU, University of Tokyo, Kashiwa, Chiba, 277-8568 Japan
6Department of Mechanical Engineering, Keio University, Yokohama, 223-8522, Japan

Received 3 April 2009; published 14 September 2009

See accompanying Physics Synopsis

In supernova cores, nuclear “pasta” phases such as a triangular lattice of rodlike nuclei and layered structure of slablike nuclei are considered to exist. However, it is still unclear whether or not they are actually formed in collapsing supernova cores. Using ab initio simulations called quantum molecular dynamics, here we solve this problem by demonstrating that a lattice of rodlike nuclei is formed from a bcc lattice by compression. We also find that, in the transition process, the system undergoes a zigzag configuration of elongated nuclei, which are formed by a fusion of two original spherical nuclei.

© 2009 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevLett.103.121101
DOI:
10.1103/PhysRevLett.103.121101
PACS:
26.50.+x, 02.70.Ns, 26.60.−c, 97.60.Bw