Difference of mirror charge radii $^{\mathrm{36}}$Ca-$^{\mathrm{36}}$S and $^{\mathrm{38}}$Ca-$^{\mathrm{38}}$Ar, and implications on the neutron equation of state

ORAL

Abstract

The charge radii of mirror nuclei $^{\mathrm{36}}$Ca-$^{\mathrm{36}}$S and $^{\mathrm{38}}$Ca-$^{\mathrm{38}}$Ar were used to deduce he first derivative $L$ of the symmetry energy in the nuclear equation of state (EOS) [1]. Here the linear correlation between the difference of mirror charger radii and $L$ were used [2] to set constraint on $L$. Implications on $L$ will be discussed in terms of correlation with the mean field calculations with Skyrme interactions, the covariant density functional theory (CODF) and the Multi-Reference In-Medium Similarity Renormalization Group (IMSRG) approach. [1] B. A. Brown et al., Phys. Rev. Res. 2, 022035 (R) (2020). [2] B. A. Brown, Phys. Rev. Lett. 119, 122502 (2017).

*This work was supported in part by the NSF, PHY-15-65546, PHY-18-11855 and PHY-19-13509; the U.S. DOE, NNSA, DE-NA0002924; the U.S. DOE, Office SC NP, DE-FG02-92ER40750 and DE-AC05-00OR22725 with UTBattelle LLC, DE-SC0017887; the NUCLEI2 SCiDAC4 collaboration DE-SC0018083; NSERC of Canada, SAPPJ-2017-00039; the DFG, German Research Foundation, 279384907-SFB 1245.

Authors

  • K. Minamisono

    • NSCL/Dept. of Physics and Astronomy,MSU
    • NSCL/Dep. Phys. Astron., MSU
  • B. A. Brown

    • NSCL/Dep. Phys. Astron., MSU
  • H. Hergert

    • NSCL/Dep. Phys. Astron., MSU
  • A. J. Miller

    • NSCL/Dep. Phys. Astron., MSU
  • R. C. Powel

    • NSCL/Dep. Phys. Astron., MSU
  • J. Watkins

    • NSCL/Dep. Phys. Astron., MSU
  • J. Peikarewicz

    • Dep. Phys., Florida State Univ.
  • D. Garand

    • NSCL, MSU
  • K. Koenig

    • NSCL, MSU
  • C. Sumithrarachchi

    • NSCL, MSU
  • R. Wirth

    • NSCL, MSU
  • A. Klose

    • Dep. Chem., Augustana Univ.
  • J. D. Lantis

    • NSCL/Dep. Chem., MSU
  • S. V. Pineda

    • NSCL/Dep. Chem., MSU
  • Y. Liu

    • Phys. Div., ORNL
  • B. Maass

    • Ins. Kernphyik, TUD
  • W. Noertershaeuser

    • Ins. Kernphyik, TUD
  • D. M. Rossi

    • Ins. Kernphyik, TUD
  • F. Sommer

    • Ins. Kernphyik, TUD
  • A. Teigelhoefer

    • TRIUMF