Finite size effects on kaonic "pasta" structures

Physical Review C - Nuclear Physics

Volumn 73, Issue 3, 2006, Pages

  Maruyama, Toshiki ^a   Tatsumi, Toshitaka ^b   Voskresensky, Dmitri N ^c,d   Tanigawa, Tomonori ^a,e   Endo, Tomoki ^b   Chiba, Satoshi ^a  

^a JAPAN ATOMIC ENERGY AGENCY   (Japan)

^b KYOTO UNIVERSITY   (Japan)

^c NATIONAL RESEARCH NUCLEAR UNIVERSITY MEPHI   (Russian Federation)

^d GSI HELMHOLTZZENTRUM FÜR SCHWERIONENFORSCHUNG GMBH   (Germany)

^e JAPAN SOCIETY FOR THE PROMOTION OF SCIENCE   (Japan)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 33644939243     PISSN: 05562813     EISSN: 1089490X     Source Type: Journal    
DOI: 10.1103/PhysRevC.73.035802     Document Type: Article

References (87)

1. C. B. Das, S. das Gupta, W. G. Lynch, A. Z. Mekjian, and M. B. Tsang, Phys. Rep. PRPLCM 0370-1573 10.1016/j.physrep.2004.10.002 406, 1 (2005).
2. A. B. Migdal, E. E. Saperstein, M. A. Troitsky, and D. N. Voskresensky, Phys. Rep. 192, 179 (1990).
3. N. K. Glendenning, Phys. Rev. D PRVDAQ 0556-2821 10.1103/PhysRevD.46.1274 46, 1274 (1992);
4. N. K. Glendenning, Phys. Rep. PRPLCM 0370-1573 10.1016/S0370-1573(00) 00080-6 342, 393 (2001).
5. H. Heiselberg, C. J. Pethick, and E. F. Staubo, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.70.1355 70, 1355 (1993).
6. N. K. Glendenning and S. Pei, Phys. Rev. C PRVCAN 0556-2813 10.1103/PhysRevC.52.2250 52, 2250 (1995).
7. D. N. Voskresensky, M. Yasuhira, and T. Tatsumi, Phys. Lett. PYLBAJ 0370-2693 10.1016/S0370-2693(02)02186-X B541, 93 (2002);
8. T. Tatsumi and D. N. Voskresensky, nucl-th/0312114.
9. D. N. Voskresensky, M. Yasuhira, and T. Tatsumi, Nucl. Phys. NUPABL 0375-9474 10.1016/S0375-9474(03)01313-7 A723, 291 (2003).
10. T. Tatsumi, T. Maruyama, V. N. Voskresensky, T. Tanigawa, and S. Chiba, nucl-th/0502040.
11. T. Endo, T. Maruyama, S. Chiba, and T. Tatsumi, Nucl. Phys. NUPABL 0375-9474 10.1016/j.nuclphysa.2004.12.063 A749, 333 (2005).
12. M. Alford, K. Rajagopal, S. Reddy, and F. Wilczek, Phys. Rev. D PRVDAQ 0556-2821 10.1103/PhysRevD.64.074017 64, 074017 (2001).
13. P. F. Bedaque, Nucl. Phys. NUPABL 0375-9474 10.1016/S0375-9474(01)01234-9 A697, 569 (2002).
14. S. Reddy and G. Rupak, Phys. Rev. C PRVCAN 0556-2813 10.1103/PhysRevC.71. 025201 71, 025201 (2005).
15. P. F. Bedaque, H. Caldas, and G. Rupak, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.91.247002 91, 247002 (2003).
16. T. Tatsumi, E. Nakano, and K. Nawa, hep-ph/0506002.
17. D. N. Voskresensky, Phys. Lett. PYLBAJ 0370-2693 10.1016/S0370-2693(96) 01561-4 B392, 262 (1997).
18. E. E. Kolomeitsev and D. N. Voskresensky, Nucl. Phys. NUPABL 0375-9474 10.1016/j.nuclphysa.2005.05.154 A759, 373 (2005).
19. D. Kaplan and A. Nelson, Phys. Lett. PYLBAJ 0370-2693 10.1016/0370-2693(86)90331-X B175, 57 (1986).
20. G. E. Brown, C. H. Lee, M. Rho, and V. Thorsson, Nucl. Phys. NUPABL 0375-9474 10.1016/0375-9474(94)90335-2 A567, 937 (1994).
21. T. Muto, R. Tamagaki, and T. Tatsumi, Prog. Theor. Phys. Suppl. 112, 159 (1993).
22. T. Tatsumi, Prog. Theor. Phys. Suppl. 120, 111 (1995).
23. J. A. Pons, S. Reddy, P. J. Ellis, M. Prakash, and J. M. Lattimer, Phys. Rev. C PRVCAN 0556-2813 10.1103/PhysRevC.62.035803 62, 035803 (2000).
24. S. Reddy, G. F. Bertsch, and M. Prakash, Phys. Lett. PYLBAJ 0370-2693 10.1016/S0370-2693(00)00049-6 B475, 1 (2000).
25. N. K. Glendenning and J. Schaffner-Bielich, Phys. Rev. C PRVCAN 0556-2813 10.1103/PhysRevC.60.025803 60, 025803 (1999).
26. M. Christiansen and N. K. Glendenning, astro-ph/0008207.
27. M. B. Christiansen, N. K. Glendenning, and J. Schaffner-Bielich, Phys. Rev. C PRVCAN 0556-2813 10.1103/PhysRevC.62.025804 62, 025804 (2000).
28. T. Norsen and S. Reddy, Phys. Rev. C PRVCAN 0556-2813 10.1103/PhysRevC.63.065804 63, 065804 (2001).
29. T. Tatsumi and M. Yasuhira, Nucl. Phys. NUPABL 0375-9474 10.1016/S0375-9474(99)00170-0 A653, 133 (1999);
30. M. Yasuhira and T. Tatsumi, Nucl. Phys. NUPABL 0375-9474 10.1016/S0375-9474(01)00348-7 A690, 769 (2001).
31. E. E. Kolomeitsev, D. N. Voskresensky, and B. Kämpfer, Nucl. Phys. NUPABL 0375-9474 10.1016/0375-9474(95)00084-E A588, 889 (1995);
32. E. E. Kolomeitsev and D. N. Voskresensky, Phys. Rev. C PRVCAN 0556-2813 10.1103/PhysRevC.68.015803 68, 015803 (2003).
33. T. Muto, Prog. Theor. Phys. PTPKAV 0033-068X 10.1143/PTP.89.415 89, 415 (1993);
34. T. Muto, Nucl. Phys. NUPABL 0375-9474 10.1016/S0375-9474(01)01226-X A697, 225 (2002);
35. T. Muto, Nucl. Phys. NUPABL 0375-9474 10.1016/j.nuclphysa.2005.02.080 A754, 350 (2004).
36. C. H. Lee, Phys. Rep. PRPLCM 0370-1573 10.1016/0370-1573(96)00005-1 275, 197 (1996).
37. M. Prakash, I. Bombaci, M. Prakash, P. J. Ellis, J. M. Lattimer, and R. Knorren, Phys. Rep. PRPLCM 0370-1573 10.1016/S0370-1573(96)00023-3 280, 1 (1997).
38. G. E. Brown and H. A. Bethe, Astrophys. J. ASJOAB 0004-637X 10.1086/173844 423, 659 (1994).
39. G. E. Brown, K. Kubodera, D. Page, and P. Pizzochero, Phys. Rev. D PRVDAQ 0556-2821 10.1103/PhysRevD.37.2042 37, 2042 (1988).
40. T. Tatsumi, Prog. Theor. Phys. PTPKAV 0033-068X 10.1143/PTP.80.22 80, 22 (1988).
41. H. Fujii, T. Muto, T. Tatsumi, and R. Tamagaki, Nucl. Phys. NUPABL 0375-9474 10.1016/0375-9474(94)90719-6 A571, 758 (1994);
42. H. Fujii, T. Muto, T. Tatsumi, and R. Tamagaki, Phys. Rev. C PRVCAN 0556-2813 10.1103/PhysRevC.50.3140 50, 3140 (1994).
43. D. Page and E. Baron, Astrophys. J. ASJOAB 0004-637X 10.1086/185712 254, L17 (1990).
44. D. G. Ravenhall, C. J. Pethick, and J. R. Wilson, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.50.2066 50, 2066 (1983).
45. M. Hashimoto, H. Seki, and M. Yamada, Prog. Theor. Phys. PTPKAV 0033-068X 10.1143/PTP.71.320 71, 320 (1984).
46. R. D. Williams and S. E. Koonin, Nucl. Phys. NUPABL 0375-9474 10.1016/0375-9474(85)90191-5 A435, 844 (1985).
47. K. Oyamatsu, Nucl. Phys. NUPABL 0375-9474 10.1016/0375-9474(93)90020-X A561, 431 (1993).
48. C. P. Lorenz, D. G. Ravenhall, and C. J. Pethick, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.70.379 70, 379 (1993).
49. K. S. Cheng, C. C. Yao, and Z. G. Dai, Phys. Rev. C PRVCAN 0556-2813 10.1103/PhysRevC.55.2092 55, 2092 (1997).
50. T. Maruyama, K. Niita, K. Oyamatsu, T. Maruyama, S. Chiba, and A. Iwamoto, Phys. Rev. C PRVCAN 0556-2813 10.1103/PhysRevC.57.655 57, 655 (1998).
51. T. Kido, T. Maruyama, K. Niita, and S. Chiba, Nucl. Phys. NUPABL 0375-9474 10.1016/S0375-9474(99)00736-8 A663, 877 (2000).
52. G. Watanabe, K. Iida, and K. Sato, Nucl. Phys. NUPABL 0375-9474 10.1016/S0375-9474(00)00197-4 A676, 445 (2000);
53. G. Watanabe, K. Sato, K. Yasuoka, and T. Ebisuzaki, Phys. Rev. C PRVCAN 0556-2813 10.1103/PhysRevC.66.012801 66, 012801(R) (2002).
54. G. Watanabe and K. Iida, Phys. Rev. C PRVCAN 0556-2813 10.1103/PhysRevC.68.045801 68, 045801 (2003).
55. T. Maruyama, T. Tatsumi, D. N. Voskresensky, T. Tanigawa, S. Chiba, and T. Maruyama, nucl-th/0402002;
56. Proceedings of the International Symposium on the origin of Matter and Evolution of Galaxies, 2003, edited by, M. Terasawa,, (World Scientific, 2005), p. 417.
57. T. Maruyama, T. Tatsumi, D. N. Voskresensky, T. Tanigawa, and S. Chiba, Phys. Rev. C PRVCAN 0556-2813 10.1103/PhysRevC.72.015802 72, 015802 (2005).
58. T. Maruyama, T. Tatsumi, D. N. Voskresensky, T. Tanigawa, S. Chiba, and T. Maruyama, Prog. Theor. Phys. Suppl. 156, 145 (2004).
59. T. Maruyama, T. Tatsumi, V. N. Voskresensky, T. Tanigawa, and S. Chiba, Nucl. Phys. NUPABL 0375-9474 10.1016/j.nuclphysa.2004.12.031 A749, 186 (2005).
60. S. Kubis, Phys. Rev. C PRVCAN 0556-2813 10.1103/PhysRevC.70.065804 70, 065804 (2004).
61. S. Reddy (private communication).
62. R. G. Parr and W. Yang, Density-Functional Theory of Atoms and Molecules (Oxford University Press, Oxford, UK, 1989);
63. Density Functional Theory, edited by, E. K. U. Gross, and, R. M. Dreizler, (Plenum Press, New York, 1995).
64. E. Friedman, A. Gal, and C. J. Batty, Nucl. Phys. NUPABL 0375-9474 10.1016/0375-9474(94)90921-0 A579, 518 (1994);
65. C. J. Batty, E. Friedman, and A. Gal, Phys. Rep. PRPLCM 0370-1573 10.1016/S0370-1573(97)00011-2 287, 385 (1997).
66. E. Friedman, A. Gal, J. Mares, and A. Cieply, Phys. Rev. C PRVCAN 0556-2813 10.1103/PhysRevC.60.024314 60, 024314 (1999).
67. T. Waas, N. Kaiser, and W. Weise, Phys. Lett. PYLBAJ 0370-2693 10.1016/0370-2693(95)01289-3 B365, 12 (1996);
68. T. Waas, N. Kaiser, and W. Weise, Phys. Lett. PYLBAJ 0370-2693 10.1016/0370-2693(96)00472-8 B379, 34 (1996);
69. T. Waas and W. Weise, Nucl. Phys. NUPABL 0375-9474 10.1016/S0375-9474(97) 00487-9 A625, 287 (1997).
70. A. Ramos and E. Oset, Nucl. Phys. NUPABL 0375-9474 10.1016/S0375-9474(99) 00846-5 A671, 481 (2000).
71. J. Schaffner-Bielich, V. Koch, and M. Effenberger, Nucl. Phys. NUPABL 0375-9474 10.1016/S0375-9474(99)00690-9 A669, 153 (2000).
72. L. Tolós, A. Ramos, and A. Polls, Phys. Rev. C PRVCAN 0556-2813 10.1103/PhysRevC.65.054907 65, 054907 (2002).
73. J. A. Oller, E. Oset, and A. Ramos, Prog. Part. Nucl. Phys. PPNPDB 0146-6410 10.1016/S0146-6410(00)00104-6 45, 157 (2000).
74. D. N. Voskresensky and A. I. Chernoutsan, Sov. J. Nucl. Phys. 27, 742 (1978).
75. W. D. Myers and W. J. Swiatecki, Nucl. Phys. NUPABL 0375-9474 10.1016/0375-9474(95)00509-9 A601, 141 (1996).
76. Y. Akaishi and T. Yamazaki, Phys. Rev. C PRVCAN 0556-2813 10.1103/PhysRevC.65.044005 65, 044005 (2002);
77. T. Yamazaki and Y. Akaishi, Phys. Lett. PYLBAJ 0370-2693 10.1016/S0370-2693(02)01738-0 B535, 70 (2002).
78. A. Dote, H. Horiuchi, Y. Akaishi, and T. Yamazaki, Phys. Lett. PYLBAJ 0370-2693 10.1016/j.physletb.2004.03.046 B590, 51 (2004);
79. A. Dote, H. Horiuchi, Y. Akaishi, and T. Yamazaki, Phys. Rev. C PRVCAN 0556-2813 10.1103/PhysRevC.70.044313 70, 044313 (2004).
80. T. Kishimoto, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.83. 4701 83, 4701 (1999);
81. M. Iwasaki, Nucl. Instrum. Methods Phys. Res. NIMAER 0168-9002 10.1016/S0168-9002(01)00862-2 A473, 286 (2001).
82. T. Suzuki, Nucl. Phys. NUPABL 0375-9474 10.1016/j.nuclphysa.2005.02.087 A754, 375 (2005);
83. T. Suzuki,, Phys. Lett. PYLBAJ 0370-2693 10.1016/j.physletb.2004.07.046 B597, 263 (2004);
84. M. Agnello, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.94. 212303 94, 212303 (2005).
85. T. Maruyama, in progress.
86. Note that we consider a linearized KN Lagrangian for simplicity, which is not chiral symmetric.
87. Note that only the combination VCoul-μe-V0 matters because of the gauge invariance.