| Original Articles |
|
|
|
|
Hot Nuclear Matter Equation of State and Finite Temperature Kaon Condensation |
| LI Ang1, ZUO Wei2, Schulze H. J.3, Lombardo U.3 |
| 1Department of Physics and Institute of Theoretical Physics and Astrophysics, Xiamen University, Xiamen 3610052Institute of Modern Physics, Chinese Academy of Sciences, Lanzhou 7300003INFN-LNS, Via Santa Sofia 44, I-95123 Catania, and Department of Physics and Astrophysics, Catania University, Via Santa Sofia 64, I-95123, Italy |
|
| Cite this article: |
|
LI Ang, ZUO Wei, Schulze H. J. et al 2008 Chin. Phys. Lett. 25 4233-4236 |
|
|
|
|
Abstract We perform a systematic calculation of the equation of state of asymmetric nuclear matter at finite temperature within the framework of the Brueckner--Hartree--Fock approach with a microscopic three-body force. When applying it to the study of hot kaon condensed matter, we find that the thermal effect is more profound in comparison with normal matter, in particular around the threshold density. Also, the increase of temperature makes the equation of state slightly stiffer through suppression of kaon condensation.
|
| Keywords:
21.65.+f
26.60.+c
24.10.Cn
97.60.Jd
13.75.Cs
|
|
|
Received: 07 June 2008
Published: 27 November 2008
|
|
|
|
|
|
|
|
[1] Kaplan D B and Nelson A E 1986 Phys. Lett. B175 57
[2] Brown G E, Kubodera K, Rho M and Thorsson V 1992 Phys. Lett. B 291 355 Lee C H 1996 Phys. Rep. 275 255 Lee C H, Brown G E, Min D P, and Rho M 1995 Nucl.Phys. A 585 401
[3] Prakash M, Bombaci I, Prakash Manju, Ellis P J, Lattimer JM and Knorren R 1997 Phys. Rep. 280 1
[4] Thorsson V, Prakash M, and Lattimer J M 1994 Nucl. Phys. A 572 693 Thorsson V, Prakash M, and Lattimer J M 1994 Nucl.Phys. A 574 851 erratum
[5] Kubis S and Kutschera M 2003 Nucl. Phys. A 720 189
[6]Guo H, Zhou R, Liu Y X, Liu B and Li X G 2004 Chin.Phys. Lett. 21 817
[7] Politzer H D and Wise M B 1991 Phys. Lett. B 273 156
[8] Glendenning N K 1992 Phys. Rev. D 46 1274 Glendenning N K and Schaffner J 1998 Phys. Rev. Lett. 81 4564 Glendenning N K and Schaffner J 1999 Phys. Rev. C 60 025803
[9] Yasuhira M and Tatsumi T 2000 Nucl. Phys. A 663 881 Yasuhira M and Tatsumi T 2000 Nucl. Phys. A 670218 Muto T, Yasuhira M, Tatsumi T and Iwamoto N 2003 Phys. Rev. D 67 103002
[10] Pons J A, Miralles J A, Prakash M and Lattimer J M 2001 Astrophys. J. 553 382
[11] Ramos A, Bielich J S and Wambach J 2001 Lett. Notes.Phys. 578 175
[12] Carlson J, Heiselberg H and Pandharipande V R 2001 Phys. Rev. C 63 017603
[13] Norsen T and Reddy S 2001 Phys. Rev. C 63065804
[14] Ellis P J, Knorren R and Prakash M 1995 Phys. Lett.B 349 11
[15] Zuo W, Li A, Li Z H and Lombardo U 2004 Phys. Rev.C 70 055802
[16] Li A, Burgio G F, Lombardo U and Zuo W 2006 Phys.Rev. C 74 055801
[17] Schaffner J and Mishustin I N 1995 Phys. Rev. C 53 1416
[18] Nicotra O E, Baldo M, Burgio G F and Schulze H J 2006 Astron. Astrophys. 451 213
[19] Baldo M and Ferreira L S 1999 Phys. Rev. C 59682
[20] Bombaci I and Lombardo U 1991 Phys. Rev. C 441892
[21] Zuo W, Bombaci I and Lombardo U 1999 Phys. Rev. C 60 024605
[22] Wiringa R B, Stoke V G J and Schiavilla R 1995 Phys.Rev. C 51 38
[23] Grang\'{e P, Lejeune A, Martzolff M and Mathiot J F 1989 Phys. Rev. C 40 1040
[24] Zuo W, Lejeune A, Lombardo U and Mathiot J F 2002 Nucl. Phys. A 706 418
[25] Bombaci I and Lombardo U 1991 Phys. Rev. C 441892
[26] Baldo M, Burgio G F and Schulze H J 1998 Phys. Rev. C 58 3688 Baldo M, Burgio G F and Schulze H J 2000 Phys. Rev. C 61 055801
[27] Tatsumi T and Yasuhira M 1998 Phys. Lett. B 441 9
[28] Yasuhira M and Tatsumi T 2001 Nucl. Phys. A 690 769
[29] Lyubovitskij V E, Gutsche T, Faessler A and Drukarev E G 2001 Phys. Rev. D 63 054026 |
|
Viewed |
|
|
|
Full text
|
|
|
|
|
Abstract
|
|
|
|
|
