Numerical evidence for “multiscalar stars”

Physical Review D - Particles, Fields, Gravitation and Cosmology

Volumn 67, Issue 2, 2003, Pages

  Choptuik, Matthew W ^b  

^a ALBERT EINSTEIN INSTITUT   (Germany)

^b UNIVERSITY OF BRITISH COLUMBIA   (Canada)

Author keywords

[No Author keywords available]

Indexed keywords

ARTICLE; ASTRONOMY; DENSITY; MATHEMATICAL ANALYSIS; MOLECULAR STABILITY; OSCILLATION; PHASE TRANSITION;

EID: 0037438293     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.67.024010     Document Type: Article

References (23)

1. E. Seidel and W.M. Suen, Phys. Rev. Lett. 66, 1659 (1991).
2. L.A. Ureña-López, Class. Quantum Grav. 19, 2617 (2002).
3. D. Kaup, Phys. Rev. 172, 1331 (1968).
4. R. Ruffini and S. Bonnazzola, Phys. Rev. 187, 1767 (1969).
5. M. Colpi, S.L. Shapiro, and I. Wasserman, Phys. Rev. Lett. 57, 2485 (1986).
6. P. Jetzer, Phys. Rep. 220, 163 (1992).
7. E.W. Mielke and F.E. Schunck, gr-qc/9801063.
8. P. Bizoń and A. Wasserman, Commun. Math. Phys. 215, 357 (2000).
9. J.-W. Lee and I.-G. Koh, Phys. Rev. D 53, 2236 (1996).
10. F.S. Guzmán and T. Matos, Class. Quantum Grav. 17, L9 (2000).
11. M. Alcubierre, F.S. Guzmán, T. Matos, D. Núñez, L.A. Ureña-López, and P. Wiederhold, Class. Quantum Grav. 19, 5017 (2002).
12. T. Matos, F.S. Guzmán, and L.A. Ureña-López, Class. Quantum Grav. 17, 1707 (2000);
13. T. Matos and L.A. Ureña-López, Phys. Rev. D 63, 063506 (2001).
14. E.W. Mielke and F.E. Schunck, Nucl. Phys. B564, 185 (2000).
15. D.F. Torres, S. Capozziello, and G. Lambiase, Phys. Rev. D 62, 104012 (2000).
16. M.P. Dabrowski and F.E. Schunck, Astrophys. J. 535, 316 (2000).
17. G. Rosen, J. Math. Phys. 7, 2066 (1966);
18. J. Math. Phys.G. Rosen7, 2071 (1966);
19. see also P. Jetzer and D. Scialom, Phys. Lett. A 169, 12 (1992).
20. S. Coleman, Nucl. Phys. B262, 263 (1985).
21. T.D. Lee, Phys. Rev. D 35, 3637 (1987);
22. Phys. Rev. DR. Friedberg, T.D. Lee, and Y. Pang, 35, 3658 (1987).
23. S.H. Hawley and M.W. Choptuik, Phys. Rev. D 62, 104024 (2000).