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Su Houng Lee with Kie Sang Jeong 1. Few words on Nuclear Symmetry Energy

Nuclear Symmetry Energy from QCD sum rules. Su Houng Lee with Kie Sang Jeong 1. Few words on Nuclear Symmetry Energy 2. A QCD sum rule method 3. Preliminary results . Korea Rare Isotope Accelerator ( KoRIA ) Talk by B. Hong. Nuclear Symmetry Energy .

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Su Houng Lee with Kie Sang Jeong 1. Few words on Nuclear Symmetry Energy

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  1. Nuclear Symmetry Energy from QCD sum rules Su Houng Lee with Kie Sang Jeong 1. Few words on Nuclear Symmetry Energy 2. A QCD sum rule method 3. Preliminary results

  2. Korea Rare Isotope Accelerator (KoRIA) Talk by B. Hong

  3. Nuclear Symmetry Energy Shetty, Yennello, arXiv:1002.0313

  4. Nuclear Symmetry Energy Li, Chen, Ko, Phys. Rep. 464, 113 (08)

  5. 1. Few words on symmetry energy

  6. QCD Energy Momentum Tensor Energy Density in asymmetric nuclear matter • Linear density approximation

  7. Linear density approximation Ep Ep p n nucleons in the vacuum • Nucleons in a background potential Ep Ep p n nucleons in the asymmetric matter

  8. Nucleon in Relativistic mean fields: (Di Toro et al) Medium modification Average potential Symmetry Energy Hadrons in nuclear medium from QCD Nucleons in symmetric nuclear matter: Cohen, Griegel, Furnstahl (91)  consistent with a strong scalar attraction and vector repulsion Vector meson in medium: Hatsuda and Lee (92) : 4 quark condensate are important

  9. QCD sum rules for Nucleon • Small M2 • Large M2 M2

  10. QCD sum rules for Nucleon in symmetric nuclear matter • Cohen, Griegel, Furnstahl 92

  11. QCD sum rules for Nucleon asymmetric nuclear matter • K.S. Jeong, Lee 11

  12. some detail • Expectation values

  13. Results – Symmetry Energy

  14. Results – Uncertainty

  15. Results Important operator

  16. Operators in at finite density • Linear density approximation • Condensate at finite density

  17. Summary • An attempt to get some insight of Symmetry energy from QCD • Vector densities are important • Higher dimensional operators are important at higher density

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