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  • Ban, ShufangKTH,Fysik (author)

Nuclear symmetry energy in relativistic mean field theory

  • Article/chapterEnglish2006

Publisher, publication year, extent ...

  • Elsevier BV,2006
  • printrdacarrier

Numbers

  • LIBRIS-ID:oai:DiVA.org:kth-7391
  • https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-7391URI
  • https://doi.org/10.1016/j.physletb.2005.11.077DOI

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  • Language:English
  • Summary in:English

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  • Subject category:ref swepub-contenttype
  • Subject category:art swepub-publicationtype

Notes

  • QC 20100623
  • The physical origin of the nuclear symmetry energy is studied within the relativistic mean field (RMF) theory. Based on the nuclear binding energies calculated with and without mean isovector potential for several isobaric chains we confirm earlier Skyrme-Hartree-Fock result that the nuclear symmetry energy strength depends on the mean level spacing epsilon(A) and an effective mean isovector potential strength K(A). A detailed analysis of the isospin dependence of these two components contributing to the nuclear symmetry energy reveals a quadratic dependence due to the mean-isoscalar potential, similar to epsilon T-2, and, completely unexpectedly, the presence of a strong linear component similar to kappa T(T + 1 + epsilon/kappa) in the isovector potential. The latter generates a nuclear symmetry energy in RMF theory that is proportional to E-sym similar to T(T + 1) at variance to the non-relativistic calculation. The origin of the linear term in RMF theory needs to be further explored.

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  • Meng, J. (author)
  • Satula, W. (author)
  • Wyss, RamonKTH,Kärnfysik(Swepub:kth)u1ayc3r9 (author)
  • KTHFysik (creator_code:org_t)

Related titles

  • In:Physics Letters B: Elsevier BV633:2-3, s. 231-2360370-26931873-2445

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Ban, Shufang
Meng, J.
Satula, W.
Wyss, Ramon
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NATURAL SCIENCES
NATURAL SCIENCES
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and Subatomic Physic ...
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Physics Letters ...
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Royal Institute of Technology

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