Mirror displacement energies and neutron skins

Physical Review C - Nuclear Physics

Volumn 66, Issue 5, 2002, Pages 513041-513045

  Duflo, J ^a   Zuker, A P ^a  

^a CENTRE DE CALCUL DE L INSTITUT NATIONAL DE PHYSIQUE NUCLEAIRE ET DE PHYSIQUE DES PARTICULES   (France)

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[No Author keywords available]

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EID: 0036876093     PISSN: 05562813     EISSN: 1089490X     Source Type: Journal    
DOI: 10.1103/PhysRevC.66.051304     Document Type: Article

References (28)

1. A. Trzcińka et al., Phys. Rev. Lett. 87, 082501 (2001).
2. A. Krasznahorkay et al., Phys. Rev. Lett. 82, 3216 (1999).
3. T. Suzuki et al., Phys. Rev. Lett. 75, 3241 (1995).
4. C.J. Pethick and D.G. Ravenhall, Nucl. Phys. A606, 173 (1996).
5. J. Dobaczewski, W. Nazarewicz, and T. Werner, Z. Phys. A 354, 27 (1996).
6. B.A. Brown and W.A. Richter, Phys. Rev. C 54, 673 (1996).
7. J.M. Gómez and J. Martorell, Nucl. Phys. A410, 475 (1983).
8. E. Chabanat, P. Bonche, P. Haensel, J. Meyer, and R. Schaeffer, Nucl. Phys. A627, 710 (1997).
9. B.A. Brown, Phys. Rev. Lett. 85, 5296 (2000).
10. J.A. Nolen and J.P. Schiffer, Annu. Rev. Nucl. Sci. 19, 471 (1969).
11. J. Jänecke, in Isospin in Nuclear Physics, edited by D. H. Wilkinson (North-Holland, Amsterdam, 1969), p. 471.
12. J. Duflo, Nucl. Phys. A576, 29 (1994).
13. G. Audi and A.H. Wapstra, Nucl. Phys. A595, 409 (1995).
14. B.A. Brown, W.A. Richter, and R. Lindsay, Phys. Lett. B 483, 49 (2000).
15. A. Bohr and B. Mottelson, Nuclear Structure, Vol. 1 (Benjamin, Reading, 1964).
16. R. Machleidt and H. Müther, Phys. Rev. C 63, 034005 (2001).
17. G. Colò, M.A. Nagarajan, P. Van Isacker, and A. Vitturi, Phys. Rev. C 52, R1175 (1995).
18. A.P. Zuker, Nucl. Phys. A576, 65 (1994).
19. J. Duflo and A.P. Zuker, Phys. Rev. C 52, R23 (1995).
20. M. Dufour and A.P. Zuker, Phys. Rev. C 54, 1641 (1996).
21. J. Duflo and A.P. Zuker, Phys. Rev. C 59, R2347 (1999).
22. B.K. Agrawal, T. Sil, S.K. Samaddar, J.N. Dee, and S. Shlomo, Phys. Rev. C 64, 024305 (2001).
23. A.P. Zuker, S. Lenzi, G. Martínez Pinedo, and A. Poves, Phys. Rev. Lett. 89, 142502 (2002).
24. <) for "the proton (neutron) excess mirror partner."
25. v = 300 keV to be an upper limit (private communication).
26. rvπ, as our calculations do indeed. (C) We compare with experimental results but make no use whatsoever of them.
27. in ([14], bottom Fig. 2c), crosses and squares should be interchanged. Then it only takes good eyes to check the agreement.
28. This description of the NSA is compact and accurate but nonstandard. In the late 1970's some experiments appeared to be consistent with vanishing neutron skin, and it was pointed out that under this assumption the NSA would disappear [S. Shlomo and E. Friedman, Phys. Rev. Lett. 39, 1180 (1977)]. After this proposal turned out to be unrealistic, little emphasis was put on the strong correlation between CDE and neutron skin, with few exceptions (such as [7]).