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A new generation of cosmic superstri...

Correira, José Ricardo C. C. C.

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A new generation of cosmic superstring simulations

Record Type:	Electronic resources : Monograph/item
Title/Author:	A new generation of cosmic superstring simulations/ by José Ricardo C. C. C. Correira.
Author:	Correira, José Ricardo C. C. C.
Published:	Cham :Springer International Publishing : : 2023.,
Description:	xiv, 192 p. :ill. (chiefly color), digital ;24 cm.
Notes:	"Doctoral thesis accepted by Centro de Astrofísica da Universidade do Porto Rua das Estrelas s/n, Porto, Portugal."
[NT 15003449]:	A brief description of Cosmology -- Topological Defects -- Supercomputing with Graphics Processing Units -- Calibration of Extended VOS models -- Strings in U(1)_L x U(1)_L simulations -- A New Generation of String Simulations.
Contained By:	Springer Nature eBook
Subject:	Superstring theories - Computer simulation. -
Online resource:	https://doi.org/10.1007/978-3-031-20229-2
ISBN:	9783031202292

A new generation of cosmic superstring simulations
Correira, José Ricardo C. C. C.

A new generation of cosmic superstring simulations[electronic resource] /by José Ricardo C. C. C. Correira. - Cham :Springer International Publishing :2023. - xiv, 192 p. :ill. (chiefly color), digital ;24 cm. - Springer theses,2190-5061. - Springer theses..

"Doctoral thesis accepted by Centro de Astrofísica da Universidade do Porto Rua das Estrelas s/n, Porto, Portugal."

A brief description of Cosmology -- Topological Defects -- Supercomputing with Graphics Processing Units -- Calibration of Extended VOS models -- Strings in U(1)_L x U(1)_L simulations -- A New Generation of String Simulations.

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 about field theory simulations in the early Universe and about supercomputing with multiple accelerators.

ISBN: 9783031202292

Standard No.: 10.1007/978-3-031-20229-2doiSubjects--Topical Terms:

3629565
Superstring theories
--Computer simulation.

LC Class. No.: QC794.6.S85 / C67 2023

Dewey Class. No.: 539.7258

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500 $a "Doctoral thesis accepted by Centro de Astrofísica da Universidade do Porto Rua das Estrelas s/n, Porto, Portugal."
505 0 $a A brief description of Cosmology -- Topological Defects -- Supercomputing with Graphics Processing Units -- Calibration of Extended VOS models -- Strings in U(1)_L x U(1)_L simulations -- A New Generation of String Simulations.
520 $a 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 about field theory simulations in the early Universe and about supercomputing with multiple accelerators.
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