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Journals / Turkish Journal of Physics / 2003 / Cilt: 27 - Sayı: 2

Semi-infinite polarized nuclear matter with a Seyler- Blanchard interaction

Hesham Mohamed Mohamed MANSOUR
Khaled Abd El Aziz RAMADAN
Pages
107–119
DOI
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AI Summary & Key Takeaways

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⚡ TL;DR(Too Long; Didn't Read)

PACS number(s): 21.65.+f, 21.30.Fe

📌 3 Key Takeaways

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Objective & Hypothesis:The surface and curvature properties of semi-infinite polarized nuclear matter (SPNM) are calculated using a modified form of the Seyler-Blanchard potential.
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Key Findings & Data:The level density parameter is extracted from the free energy using $T^2$-approximation.
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Conclusion & Impact:PACS number(s): 21.65.+f, 21.30.Fe
🔬Design:Research Article
📍Scope:Comprehensive Sample
⚙️Variables:Domain Parameters

Özet

The surface and curvature properties of semi-infinite polarized nuclear matter (SPNM) are calculated using a modified form of the Seyler-Blanchard potential. The level density parameter is extracted from the free energy using $T^2$-approximation. Good agreement is obtained between our calculations for the level density and other parameters which characterize the surface and curvature properties of SPNM and previous theoretical estimates. PACS number(s): 21.65.+f, 21.30.Fe

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MANSOUR, H. M. M., RAMADAN, K. A. E. A. (2003). Semi-infinite polarized nuclear matter with a Seyler- Blanchard interaction. Turkish Journal of Physics, Cilt: 27 - Sayı: 2, 107–119. https://ajindex.com/articles/378221

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References (20)

  1. G. Fuller, Astrophys. J. 252, (1982), 741
  2. M. Prakash, J. Wambach, and Z.Y. Ma, Phys. Lett. 128B, (1983), 141
  3. C.J. Pethick, D.G. Ravenhall, and J.M. Lattimer, Phys. Lett. 128B, (1983), 137
  4. A. Bohr, and B.R. Mottelson, in Nuclear Structure, Vols. I and II (Benjamin, Reading, MA, 1969 and 1975)
  5. M. Abd-Alla, S. Ramadan, and M.Y.M. Hassan, Phys. Rev. C 36, (1987), 1565
  6. H.M.M. Mansour, M. Hammad, and M.Y.M. Hassan, Phys. Rev. C 56, (1997), 1418
  7. R.G. Seyler, and C.H. Blanchard, Phys. Rev. 124, (1961), 227
  8. M.Y.M. Hassan, S.S. Montasser, and S. Ramadan, J. Phys. G 6, (1980), 1229
  9. H.A. Bethe, Annu. Rev. Nucl. Sci. 21, (1971), 93
  10. O. Bohigas et al., Phys. Lett. 64B, (1967), 381
  11. B. Behera, J. Phys. G 10, (1984), 1731
  12. H. Krivine, and J. Triener, Phys. Lett. 124B, (1983), 127
  13. X. Vinas, M. Pi, and M. Baranco, J. Phys. G 9, (1983), 1193
  14. J. Triener, and H. Krivine, Ann. Phys. (N.Y.) 170, (1986), 406
  15. K. Kolehmainen et al., Nucl. Phys. A 439, (1985), 535
  16. J. Triener et al., Nucl. Phys. A 452, (1986), 93
  17. W. Stocker, and J. Burzlaff, Nucl. Phys. A 202, 265 (1973)
  18. M. Brack, Phys. Rev. Lett. 53, (1984), 119; 54, (1985), 581
  19. S.A. Moszkowski, Phys. Rev. C 2, (1970), 402
  20. M. Farine and J.M. Pearson, Nucl. Phys. A 338, (1980), 86.