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Erasure of Defects:: Vortex Unwinding by Domain Wall Sweeping - Softcover

 
9786203471816: Erasure of Defects:: Vortex Unwinding by Domain Wall Sweeping

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Topological defects–such as Domain Walls, cosmic strings, and magnetic monopoles–are expected to appear during a phase transition in the GUT of particle physics. Such monopoles would be the universe's dominant matter during the early universe. However, this is in tension with the fact that monopoles have not been observed. The former is known as the cosmological monopole problem. Different solutions to this problem are known today, with inflation being the most well-known. In this scenario, the universe inflates, dilutes the monopoles, and their density decreases to acceptable levels. Another solution was proposed by Dvali, Liu, and Vachaspati in 1997.The main idea is that Domain Walls, generated during the same phase transition, swept away the monopoles before decaying.In general, this solution proposes that defect interactions lead to a defect erasure mechanism. This mechanism has been investigated in a SU(5) grand unified model.

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  • PublisherLAP LAMBERT Academic Publishing
  • Publication date2021
  • ISBN 10 620347181X
  • ISBN 13 9786203471816
  • BindingPaperback
  • LanguageEnglish
  • Number of pages104

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Taschenbuch. Condition: Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -Topological defects-such as Domain Walls, cosmic strings, and magnetic monopoles-are expected to appear during a phase transition in the GUT of particle physics. Such monopoles would be the universe's dominant matter during the early universe. However, this is in tension with the fact that monopoles have not been observed. The former is known as the cosmological monopole problem. Different solutions to this problem are known today, with inflation being the most well-known. In this scenario, the universe inflates, dilutes the monopoles, and their density decreases to acceptable levels. Another solution was proposed by Dvali, Liu, and Vachaspati in 1997.The main idea is that Domain Walls, generated during the same phase transition, swept away the monopoles before decaying.In general, this solution proposes that defect interactions lead to a defect erasure mechanism. This mechanism has been investigated in a SU(5) grand unified model. 104 pp. Englisch. Seller Inventory # 9786203471816

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Taschenbuch. Condition: Neu. nach der Bestellung gedruckt Neuware - Printed after ordering - Topological defects-such as Domain Walls, cosmic strings, and magnetic monopoles-are expected to appear during a phase transition in the GUT of particle physics. Such monopoles would be the universe's dominant matter during the early universe. However, this is in tension with the fact that monopoles have not been observed. The former is known as the cosmological monopole problem. Different solutions to this problem are known today, with inflation being the most well-known. In this scenario, the universe inflates, dilutes the monopoles, and their density decreases to acceptable levels. Another solution was proposed by Dvali, Liu, and Vachaspati in 1997.The main idea is that Domain Walls, generated during the same phase transition, swept away the monopoles before decaying.In general, this solution proposes that defect interactions lead to a defect erasure mechanism. This mechanism has been investigated in a SU(5) grand unified model. Seller Inventory # 9786203471816

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Condition: New. Dieser Artikel ist ein Print on Demand Artikel und wird nach Ihrer Bestellung fuer Sie gedruckt. Autor/Autorin: Valbuena Bermudez Juan SebastianI am a Researcher Ph.D. Student at the ORIGINS Cluster, the Ludwig-Maximilians Universitaet Muenchen, and the Max Planck Institute for Physics since May 2020.I completed the Theoretical and Mathematical. Seller Inventory # 537080074

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Taschenbuch. Condition: Neu. Neuware -Topological defects¿such as Domain Walls, cosmic strings, and magnetic monopoles¿are expected to appear during a phase transition in the GUT of particle physics. Such monopoles would be the universe's dominant matter during the early universe. However, this is in tension with the fact that monopoles have not been observed. The former is known as the cosmological monopole problem. Different solutions to this problem are known today, with inflation being the most well-known. In this scenario, the universe inflates, dilutes the monopoles, and their density decreases to acceptable levels. Another solution was proposed by Dvali, Liu, and Vachaspati in 1997.The main idea is that Domain Walls, generated during the same phase transition, swept away the monopoles before decaying.In general, this solution proposes that defect interactions lead to a defect erasure mechanism. This mechanism has been investigated in a SU(5) grand unified model.Books on Demand GmbH, Überseering 33, 22297 Hamburg 104 pp. Englisch. Seller Inventory # 9786203471816

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