Diffuse domain walls and intersecting flat directions

Physical Review D - Particles, Fields, Gravitation and Cosmology

Volumn 55, Issue 6, 1997, Pages 3820-3823

  Barr, S M ^a  

^a UNIVERSITY OF DELAWARE   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0642347086     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.55.3820     Document Type: Article

References (7)

1. For a review of cosmic strings, see A. Vilenkin, Phys. Rep.121, 263 (1985).
2. B. Bajc, A. Melfo, and G. Senjanović, Phys. Lett. B387, 796 (1996).
3. L. Hall, J. Lykken, and S. Weinberg, Phys. Rev. D27, 2359 (1983).
4. See, for instance, M. Dine and A. Nelson, Phys. Rev. D48, 1277 (1993);
5. M. Dine, A. Nelson, and Y. Shirman, 51, 1362 (1995).
6. Cosmological domain walls can be “inflated away.” For ways to avoid domain wall problems, see B. Rai and G. Senjanovic, Phys. Rev. D49, 2729 (1994);
7. G. Dvali and G. Senjanovic, Phys. Rev. Lett.74, 5178 (1995).