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Evading the cosmological domain wall problem

Abstract:
Discrete symmetries are commonplace in field theoretical models but pose a severe problem for cosmology since they lead to the formation of domain walls during spontaneous symmetry breaking in the early universe. However if one of the vacuua is favoured over the others, either energetically, or because of initial conditions, it will eventually come to dominate the universe. Using numerical methods, we study the evolution of the domain wall network for a variety of field configurations in two and three dimensions and quantify the rate at which the walls disappear. Good agreement is found with a recent analytic estimate of the termination of the scaling regime of the wall network.
Publication status:
Published

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Publisher copy:
10.1103/PhysRevD.55.5129

Authors


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Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Theoretical Physics
Role:
Author


Journal:
Phys.Rev.D More from this journal
Volume:
55
Issue:
8
Pages:
5129-5135
Publication date:
1997-04-15
DOI:
EISSN:
1089-4918
ISSN:
0556-2821


Keywords:
Pubs id:
pubs:4225
UUID:
uuid:c35e11dd-8bfd-4383-8941-0b533a4c71a7
Local pid:
pubs:4225
Source identifiers:
4225
Deposit date:
2012-12-19

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