Abstract
An equation of state (EoS) for symmetric nuclear matter is constructed using the density-dependent M3Y effective interaction and extended for isospin asymmetric nuclear matter. Theoretically obtained values of symmetric nuclear matter incompressibility, isobaric incompressibility, symmetry energy and its slope agree well with experimentally extracted values. Folded microscopic potentials using this effective interaction, whose density dependence is determined from nuclear matter calculations, provide excellent descriptions for proton, alpha and cluster radioactivities, elastic and inelastic scattering. The nuclear deformation parameters extracted from inelastic scattering of protons agree well with other available results. The high density behaviour of symmetric and asymmetric nuclear matter satisfies the constraints from the observed flow data of heavy-ion collisions. The neutron star properties studied using β-equilibrated neutron star matter obtained from this effective interaction reconcile with the recent observations of the massive compact stars.
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B A Li, L W Chen and C M Ko, Phys. Rep. 464, 113 (2008)
A W Steiner, M Prakash, J M Lattimer and P J Ellis, Phys. Rep. 411, 325 (2005)
P Danielewicz, R Lacey and W G Lynch, Science 298, 1592 (2002)
G Bertsch, J Borysowicz, H McManus and W G Love, Nucl. Phys. A 284, 399 (1977)
G R Satchler and W GLove, Phys. Rep. 55, 183 (1979)
E C Kemble, Phys. Rev. 48, 549 (1935)
D N Basu, P Roy Chowdhury and C Samanta, Nucl. Phys. A 811, 140 (2008)
Basu D N, Phys. Lett. B 566, 90 (2003)
P Roy Chowdhury, C Samanta and D N Basu, Phys. Rev. C 73, 014612 (2006); ibid, Phys. Rev. C 77, 044603 (2008); ibid, At. Data Nucl. Data Tables 94, 781 (2008)
Roy Chowdhury P, Basu D N and Samanta C, Phys. Rev. C 75, 047306 (2007)
Samanta C, Roy Chowdhury P and Basu D N, Nucl. Phys. A 789, 142 (2007)
Routray T R, Jagajjaya Nayak and Basu D N, Nucl. Phys. A 826, 223 (2009)
Gupta D and Basu D N, Nucl. Phys. A 748, 402 (2005)
Gupta D, Khan E and Blumenfeld Y, Nucl. Phys. A 773, 230 (2006)
Demorest P B, Pennucci T, Ransom S M, Roberts M S E and Hessels J W T, Nature 467, 1081 (2010)
Lane A M, Nucl. Phys. 35, 676 (1962)
Samanta C, Bandyopadhyay D and De J N, Phys. Lett. B 217, 381 (1989)
Roy Chowdhury P and Basu D N, Acta Phys. Pol. B 37, 1833 (2006)
Audi G, Wapstra A H and Thibault C, Nucl. Phys. A 729, 337 (2003)
Lunney D, Pearson J M and Thibault C, Rev. Mod. Phys. 75, 1021 (2003)
Royer G and Gautier C, Phys. Rev. C 73, 067302 (2006)
Lalazissis G A, Raman S and Ring P, At. Data Nucl. Data Tables 71, 1 (1999)
Vretenar D, Nikśić T and Ring P, Phys. Rev. C 68, 024310 (2003)
Sharma M M, Nucl. Phys. A 816, 65 (2009)
T Klähn et al, Phys. Rev. C 74, 035802 (2006)
Mukhopadhyay T and Basu D N, Nucl. Phys. A 789, 201 (2007)
Danielewicz P, Nucl. Phys. A 727, 233 (2003)
Pomorski K and Dudek J, Phys. Rev. C 67, 044316 (2003)
L Bennour et al, Phys. Rev. C 40, 2834 (1989)
Akmal A, Pandharipande V R, Ravenhall D G, Phys. Rev. C 58, 1804 (1998)
Centelles M, Roca-Maza X, Vinas X and Warda M, Phys. Rev. Lett. 102, 122502 (2009)
Lie-Wen Chen, Bao-Jun Cai, Che Ming Ko, Bao-An Li, Chun Shen and Jun Xu, Phys. Rev. C 80, 014322 (2009)
Piekarewicz J, Centelles M, Phys. Rev. C 79, 054311 (2009)
Hiroyuki Sagawa, Satoshi Yoshida, Guo-Mo Zeng, Jian-Zhong Gu and Xi-Zhen Zhang, Phys. Rev. C 76, 034327 (2007)
Warda M, Vin̈as X, Roca-Maza X and Centelles M, Phys. Rev. C 80, 024316 (2009)
P Roy Chowdhury, D N Basu and C Samanta, Phys. Rev. C 80, 011305(R) (2009) D N Basu, P Roy Chowdhury and C Samanta, Phys. Rev. C 80, 057304 (2009)
Zhigang Xiao, Bao-An Li, Lie-Wen Chen, Gao-Chan Yong and Ming Zhang, Phys. Rev. Lett. 102, 062502 (2009)
De-Hua Wen, Bao-An Li and Lie-Wen Chen, Phys. Rev. Lett. 103, 211102 (2009)
Bartel J, Quentin P, Brack M, Guet C and Hakansson H B, Nucl. Phys. A 386, 79 (1982)
Samanta C, Sakuragi Y, Ito M and Fujiwara M,J. Phys. G: Nucl. Part. Phys. 23, 1697 (1997)
P D Kunz, computer code DWUCK4, unpublished
S Raman et al, At. Data Nucl. Data Tables 78, 1 (2001)
J K Jewell et al, Phys. Lett. B 454, 191 (1999)
Mahadevan S, Prema P, Shastry C S and Gambhir Y K, Phys. Rev. C 74, 057601 (2006)
Poenaru D N, Greiner W, Ivascu M, Mazilu D and Plonski I H, Z. Phys. A 325, 435 (1986)
Sonzogni A A, Nucl. Data Sheets 95, 1 (2002)
Balasubramaniam M and Arunachalam N, Phys. Rev. C 71, 014603 (2005)
D K Srivastava, D N Basu and N K Ganguly, Phys. Lett. B 124, 6 (1983)
H Komatsu, Y Eriguchi and I Hachisu, Mon. Not. R. Astron. Soc. 237, 355 (1989)
R C Tolman, Phys. Rev. 55, 364 (1939) J R Oppenheimer and G M Volkoff, Phys. Rev. 55, 374 (1939)
Kurkela A, Romatschke P and Vuorinen A, Phys. Rev. D 81, 105021 (2010)
Heiselberg H, Pethick C J and Staubo E F, Phys. Rev. Lett. 70, 1355 (1993)
Stergioulas N and Friedman J L, Astrophys. J. 444, 306 (1995)
Feynman R P, Metropolis N and Teller E, Phys. Rev. 75, 1561 (1949)
Baym G, Pethick C J and Sutherland P, Astrophys. J. 170, 299 (1971)
Baym G, Bethe H A and Pethick C J, Nucl. Phys. A 175, 225 (1971)
Chowdhury P R, Bhattacharyya A and Basu D N, Phys. Rev. C 81, 062801(R) (2010)
Abhishek Mishra, Chowdhury P R, and Basu D N, Astropart. Phys. 36, 42 (2012)
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BASU, D.N. Effective interaction: From nuclear reactions to neutron stars. Pramana - J Phys 82, 809–822 (2014). https://doi.org/10.1007/s12043-014-0734-5
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DOI: https://doi.org/10.1007/s12043-014-0734-5