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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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  • EditoreLAP LAMBERT Academic Publishing
  • Data di pubblicazione2021
  • ISBN 10 620347181X
  • ISBN 13 9786203471816
  • RilegaturaCopertina flessibile
  • LinguaInglese
  • Numero di pagine104
  • Contatto del produttorenon disponibile

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Juan Sebastian Valbuena Bermudez
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Condizione: 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. Codice articolo 537080074

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Juan Sebastian Valbuena Bermudez
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Taschenbuch. Condizione: 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. Codice articolo 9786203471816

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Juan Sebastian Valbuena Bermudez
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Taschenbuch. Condizione: 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. Codice articolo 9786203471816

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Taschenbuch. Condizione: 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. Codice articolo 9786203471816

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