Symmetry energy of dilute warm nuclear matter

Physical Review Letters

Volumn 104, Issue 20, 2010, Pages

  Natowitz, J B ^a   Ropke G ^b   Typel, S ^c,d   Blaschke, D ^e,f   Bonasera, A ^a,g   Hagel, K ^a   Klahn T ^e,h   Kowalski, S ^a   Qin, L ^a   Shlomo, S ^a   Wada, R ^a   Wolter, H H ⁱ  

^a TEXAS A AND M UNIVERSITY   (United States)

^b UNIVERSITY OF ROSTOCK   (Germany)

^c EXCELLENCE CLUSTER UNIVERSE   (Germany)

^d GSI HELMHOLTZZENTRUM FÜR SCHWERIONENFORSCHUNG GMBH   (Germany)

^e UNIVERSITY OF WROC AW   (Poland)

^f JOINT INSTITUTE FOR NUCLEAR RESEARCH   (Russian Federation)

^g INFN LABORATORI NAZIONALI DEL SUD   (Italy)

^h ARGONNE NATIONAL LABORATORY   (United States)

ⁱ UNIVERSITY OF MUNICH   (Germany)

Author keywords

[No Author keywords available]

Indexed keywords

ASTROPHYSICAL PHENOMENA; BOUND STATE; DENSITY LIMIT; EXOTIC NUCLEI; EXPERIMENTAL DATA; HEAVY-ION COLLISIONS; INTERNAL SYMMETRY; LOW TEMPERATURES; MEAN FIELD APPROACH; NUCLEAR MATTERS; QUASI-PARTICLE APPROACH; SATURATION DENSITY; STATISTICAL APPROACH; THEORETICAL CALCULATIONS;

HEAVY IONS; NUCLEAR ENERGY;

ION SOURCES;

EID: 77952473664     PISSN: 00319007     EISSN: 10797114     Source Type: Journal    
DOI: 10.1103/PhysRevLett.104.202501     Document Type: Article

References (29)

1. J.M. Lattimer and M. Prakash, Phys. Rep. PRPLCM 0370-1573 442, 109 (2007). 10.1016/j.physrep.2007.02.003
2. G. Watanabe, Phys. Rev. Lett. 103, 121101 (2009). PRLTAO 0031-9007 10.1103/PhysRevLett.103.121101
3. P. Danielewicz, Nucl. Phys. A727, 233 (2003). NUPABL 0375-9474 10.1016/j.nuclphysa.2003.08.001
4. B.A. Li, Phys. Rep. PRPLCM 0370-1573 464, 113 (2008). 10.1016/j.physrep.2008.04.005
5. C. Fuchs and H.H. Wolter, Eur. Phys. J. A 30, 5 (2006). EPJAFV 1434-6001 10.1140/epja/i2005-10313-x
6. T. Klähn, Phys. Rev. C 74, 035802 (2006). PRVCAN 0556-2813 10.1103/PhysRevC.74.035802
7. C.J. Horowitz and A. Schwenk, Nucl. Phys. A776, 55 (2006). NUPABL 0375-9474 10.1016/j.nuclphysa.2006.05.009
8. S. Typel, G. Röpke, T. Klähn, D. Blaschke, and H.H. Wolter, Phys. Rev. C 81, 015803 (2010). PRVCAN 0556-2813 10.1103/PhysRevC.81.015803
9. J.P. Bondorf, Phys. Rep. PRPLCM 0370-1573 257, 133 (1995). 10.1016/0370-1573(94)00097-M
10. M. Schmidt, G. Röpke, and H. Schulz, Ann. Phys. (N.Y.) 202, 57 (1990). APNYA6 0003-4916 10.1016/0003-4916(90)90340-T
11. G. Röpke, Nucl. Phys. A379, 536 (1982); NUPABL 0375-9474 10.1016/0375-9474(82)90013-6
12. G. Röpke Nucl. Phys. A424, 594 (1984). NUPABL 0375-9474 10.1016/0375-9474(84)90011-3
13. G. Röpke, Phys. Rev. C 79, 014002 (2009). PRVCAN 0556-2813 10.1103/PhysRevC.79.014002
14. S. Typel, Phys. Rev. C 71, 064301 (2005). PRVCAN 0556-2813 10.1103/PhysRevC.71.064301
15. H.R. Jaqaman, Phys. Rev. C 38, 1418 (1988). PRVCAN 0556-2813 10.1103/PhysRevC.38.1418
16. H. Takemoto, Phys. Rev. C 69, 035802 (2004). PRVCAN 0556-2813 10.1103/PhysRevC.69.035802
17. V. Baran, Phys. Rep. PRPLCM 0370-1573 410, 335 (2005). 10.1016/j.physrep.2004.12.004
18. M.B. Tsang, Phys. Rev. Lett. 102, 122701 (2009). PRLTAO 0031-9007 10.1103/PhysRevLett.102.122701
19. S. Wuenschel, Phys. Rev. C 79, 061602(R) (2009). PRVCAN 0556-2813 10.1103/PhysRevC.79.061602
20. C. Sfienti, Phys. Rev. Lett. 102, 152701 (2009). PRLTAO 0031-9007 10.1103/PhysRevLett.102.152701
21. S. Kowalski, Phys. Rev. C 75, 014601 (2007). PRVCAN 0556-2813 10.1103/PhysRevC.75.014601
22. S. Albergo, Nuovo Cimento Soc. Ital. Fis. NIFAAM 1124-1861 89A, 1 (1985). 10.1007/BF02773614
23. M.B. Tsang, Phys. Rev. Lett. 86, 5023 (2001). PRLTAO 0031-9007 10.1103/PhysRevLett.86.5023
24. L.W. Chen, Phys. Rev. Lett. 94, 032701 (2005); PRLTAO 0031-9007 10.1103/PhysRevLett.94.032701
25. L.W. Chen Phys. Rev. C 76, 054316 (2007). PRVCAN 0556-2813 10.1103/PhysRevC.76.054316
26. S. Shlomo, Phys. Rev. C 79, 034604 (2009). PRVCAN 0556-2813 10.1103/PhysRevC.79.034604
27. J.M. Lattimer, Nucl. Phys. A535, 331 (1991). NUPABL 0375-9474 10.1016/0375-9474(91)90452-C
28. H. Shen, Nucl. Phys. A637, 435 (1998). NUPABL 0375-9474 10.1016/S0375-9474(98)00236-X
29. S. Typel (to be published).