Springer Theses-A New Generation of Cosmic Superstring Simulations
Auteur:
Edition:
enBroché978303120231514 janvier 2024192 pages
Résumé
Topological defects are an expected consequence of phase transitions in the early Universe. Then these are used to obtain the most accurate to date calibrations of semi-analytical modelling and to show the impact of accuracy on observational consequences of strings.
Topological defects are an expected consequence of phase transitions in the early Universe. As such these objects, if detected, provide unequivocal evidence of physics beyond the Standard Model. This means they are prime targets for new observational facilities. However, our understanding of defects is heavily bottlenecked by computational limitations. In this book, the author explores the use of accelerator hardware to alleviate this problem, presenting the world’s first (multiple-)GPU defect simulations. Such simulations can evolve a network of line-like cosmic strings at an unprecedented resolution. Then these are used to obtain the most accurate to date calibrations of semi-analytical modelling and to show the impact of accuracy on observational consequences of strings. Lastly, a modified version of this application is used to study interconnected networks of strings in greater detail than ever before. This book benefits any student or researcher who wishes to learn aboutfield theory simulations in the early Universe and about supercomputing with multiple accelerators.
Topological defects are an expected consequence of phase transitions in the early Universe. As such these objects, if detected, provide unequivocal evidence of physics beyond the Standard Model. This means they are prime targets for new observational facilities. However, our understanding of defects is heavily bottlenecked by computational limitations. In this book, the author explores the use of accelerator hardware to alleviate this problem, presenting the world’s first (multiple-)GPU defect simulations. Such simulations can evolve a network of line-like cosmic strings at an unprecedented resolution. Then these are used to obtain the most accurate to date calibrations of semi-analytical modelling and to show the impact of accuracy on observational consequences of strings. Lastly, a modified version of this application is used to study interconnected networks of strings in greater detail than ever before. This book benefits any student or researcher who wishes to learn aboutfield theory simulations in the early Universe and about supercomputing with multiple accelerators.
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Contenu
Langue
en
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Broché
Date de sortie initiale
14 janvier 2024
Nombre de pages
192
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Avec illustrations
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Editeur principal
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Springer Nature Customer Service Center GmbH
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ProductSafety@springernature.com
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Hauteur de l'emballage
11 mm
Largeur d'emballage
155 mm
Largeur du produit
155 mm
Livre d‘étude
Non
Longueur d'emballage
235 mm
Longueur du produit
235 mm
Poids de l'emballage
391 g
Édition
24001
EAN
EAN
9783031202315
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Opérateur économique responsable dans l’UE
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