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The formation and evolution of domain wallsDomain walls are sheet-like defects produced when the low energy vacuum has isolated degenerate minima. The researchers' computer code follows the evolution of a scalar field, whose dynamics are determined by its Lagrangian density. The topology of the scalar field determines the evolution of the domain walls. This approach treats both wall dynamics and reconnection. The researchers investigated not only potentials that produce single domain walls, but also potentials that produce a network of walls and strings. These networks arise in axion models where the U(1) Peccei-Quinn symmetry is broken into Z sub N discrete symmetries. If N equals 1, the walls are bounded by strings and the network quickly disappears. For N greater than 1, the network of walls and strings behaved qualitatively just as the wall network shown in the figures given here. This both confirms the researchers' pessimistic view that domain walls cannot play an important role in the formation of large scale structure and implies that axion models with multiple minimum can be cosmologically disastrous.
Document ID
19920003747
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Press, William H.
(Harvard-Smithsonian Center for Astrophysics Cambridge, MA., United States)
Ryden, Barbara S.
(Harvard-Smithsonian Center for Astrophysics Cambridge, MA., United States)
Spergel, David N.
(Princeton Univ. NJ., United States)
Date Acquired
August 15, 2013
Publication Date
January 1, 1991
Publication Information
Publication: NAS-NRC, High-Energy Astrophysics. American and Soviet Perspectives
Subject Category
Astrophysics
Accession Number
92N12965
Funding Number(s)
CONTRACT_GRANT: NSF PHY-86-04396
CONTRACT_GRANT: NSF PHY-82-17853
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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