2012/03/31 by Jun Xu, Bao-An Li, Lie-Wen Chen +1
Physics and Astronomy · #Classical mechanics #Cosmology #Fifth force #Gravitation #High-Energy Particle Collisions Research #Lambda #Mathematical physics #Newtonian fluid #Newtonian potential #Nuclear physics research studies #Order (exchange) #Particle physics #Physics #Quantum mechanics #Quantum, superfluid, helium dynamics #Scale (ratio) #Yukawa potential #astro-ph.SR #nucl-ex #nucl-th
paper · pdf · doi:10.1088/0954-3899/40/3/035107
published as J. Phys. G: 40 (2013) 035107 · Additional discussions and references added; related Lab Talk is available via http://iopscience.iop.org/0954-3899/labtalk-article/52299
openalex publication_date 2013/02/07 · arxiv created 2013/02/11 · arxiv updated 2013/02/13 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
Effects of the non-Newtonian gravity on properties of finite nuclei are studied by consistently incorporating both the direct and exchange contribution of the Yukawa potential in the Hartree-Fock approach using a well-tested Skyrme force for the strong interaction. It is shown for the first time that the strength of the Yukawa term in the non-Newtonian gravity is limited to log(|α|)<1.75/[λ(\rm fm)]0.54 + 33.6 within the length scale of λ=1-10 fm in order for the calculated properties of finite nuclei not to be in conflict with accurate experimental data available.