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Phys. Rev. C 80, 057304 (2009) [3 pages]

Isobaric incompressibility of isospin asymmetric nuclear matter

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D. N. Basu1,*, P. Roy Chowdhury2,†, and C. Samanta2,3,4,‡
1Variable Energy Cyclotron Centre, 1/AF Bidhan Nagar, Kolkata 700 064, India
2Saha Institute of Nuclear Physics, 1/AF Bidhan Nagar, Kolkata 700 064, India
3Physics Department, Virginia Commonwealth University, Richmond, Virginia 23284-2000, USA
4Physics Department, University of Richmond, Richmond, Virginia 23173, USA

Received 23 July 2009; revised 26 October 2009; published 18 November 2009

The isospin dependence of the saturation properties of asymmetric nuclear matter, particularly the incompressibility K(X)=K+KτX2+O(X4) at saturation density, is systematically studied using density-dependent M3Y interaction. Kτ characterizes the isospin dependence of the incompressibility at saturation density ρ0. The approximate expression KasyKsym-6L is often used for Kτ where L and Ksym represent the slope and curvature parameters of the symmetry energy at ρ0, respectively. It can be expressed accurately as Kτ=Ksym-6L-(Q0/K)L, where Q0 is the third-order-derivative parameter of symmetric nuclear matter at ρ0. The results of this addendum to [ Phys. Rev. C 80 011305 (2009)] indicate that the Q0 contribution to Kτ is not insignificant.

© 2009 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevC.80.057304
DOI:
10.1103/PhysRevC.80.057304
PACS:
21.65.Cd, 21.30.Fe, 21.10.Dr, 26.60.Kp