English

Non-Newtonian gravity in finite nuclei

Nuclear Theory 2016-10-12 v1 Cosmology and Nongalactic Astrophysics Solar and Stellar Astrophysics

Abstract

In this talk, we report our recent study of constraining the non-Newtonian gravity at femtometer scale. We incorporate the Yukawa-type non-Newtonian gravitational potential consistently to the Skyrme functional form using the exact treatment for the direct contribution and density-matrix expansion method for the exchange contribution. The effects from the non-Newtonian potential on finite nuclei properties are then studied together with a well-tested Skyrme force. Assuming that the framework without non-Newtonian gravity can explain the binding energies and charge radii of medium to heavy nuclei within 2% error, we set an upper limit for the strength of the non-Newtonian gravitational potential at femtometer scale.

Keywords

Cite

@article{arxiv.1208.5036,
  title  = {Non-Newtonian gravity in finite nuclei},
  author = {Jun Xu and Bao-An Li and Lie-Wen Chen and Hao Zheng},
  journal= {arXiv preprint arXiv:1208.5036},
  year   = {2016}
}

Comments

Talk given at the 11th International Conference on Nucleus-Nucleus Collisions (NN2012), San Antonio, Texas, USA, May 27-June 1, 2012. To appear in the NN2012 Proceedings in Journal of Physics: Conference Series (JPCS)