English

Laboratory Tests of Low Density Astrophysical Equations of State

Nuclear Experiment 2013-05-30 v2

Abstract

Clustering in low density nuclear matter has been investigated using the NIMROD multi-detector at Texas A&M University. Thermal coalescence modes were employed to extract densities, ρ\rho, and temperatures, TT, for evolving systems formed in collisions of 47 AA MeV 40^{40}Ar + 112^{112}Sn,124^{124}Sn and 64^{64}Zn + 112^{112}Sn, 124^{124}Sn. The yields of dd, tt, 3^{3}He, and 4^{4}He have been determined at ρ\rho = 0.002 to 0.032 nucleons/fm3^{3} and TT= 5 to 10 MeV. The experimentally derived equilibrium constants for α\alpha particle production are compared with those predicted by a number of astrophysical equations of state. The data provide important new constraints on the model calculations.

Keywords

Cite

@article{arxiv.1110.3345,
  title  = {Laboratory Tests of Low Density Astrophysical Equations of State},
  author = {L. Qin and K. Hagel and R. Wada and J. B. Natowitz and S. Shlomo and A. Bonasera and G. Roepke and S. Typel and Z. Chen and M. Huang and J. Wang and H. Zheng and S. Kowalski and M. Barbui and M. R. D. Rodrigues and K. Schmidt and D. Fabris and M. Lunardon and S. Moretto and G. Nebbia and S. Pesente and V. Rizzi and G. Viesti and M. Cinausero and G. Prete and T. Keutgen and Y. El Masri and Z. Majka},
  journal= {arXiv preprint arXiv:1110.3345},
  year   = {2013}
}

Comments

5 pages, 3 figures