Mass and spin for classical strings in dS3
Abstract We demonstrate that all rigidly rotating strings with center of mass at the origin of the dS3 static patch satisfy the Higuchi bound. This extends the observation of Noumi et al. for the open GKP-like string to all solutions of the Larsen-Sanchez class. We argue that strings violating the b...
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Format: | Article |
Language: | English |
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SpringerOpen
2021-05-01
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Series: | Journal of High Energy Physics |
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Online Access: | https://doi.org/10.1007/JHEP05(2021)277 |
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author | Klaas Parmentier |
author_facet | Klaas Parmentier |
author_sort | Klaas Parmentier |
collection | DOAJ |
description | Abstract We demonstrate that all rigidly rotating strings with center of mass at the origin of the dS3 static patch satisfy the Higuchi bound. This extends the observation of Noumi et al. for the open GKP-like string to all solutions of the Larsen-Sanchez class. We argue that strings violating the bound end up expanding towards the horizon and provide a numerical example. Adding point masses to the open string only increases the mass/spin ratio. For segmented strings, we write the conserved quantities, invariant under Gubser’s algebraic evolution equation, in terms of discrete lightcone coordinates describing kink collisions. Randomly generated strings are found to have a tendency to escape through the horizon that is mostly determined by their energy. For rapidly rotating segmented strings with mass/spin < 1, the kink collisions eventually become causally disconnected. Finally we consider the scenario of cosmic strings captured by a black hole in dS and find that horizon friction can make the strings longer. |
first_indexed | 2024-12-18T11:58:22Z |
format | Article |
id | doaj.art-324c2321e0ce448da9b1207ba9a68b3e |
institution | Directory Open Access Journal |
issn | 1029-8479 |
language | English |
last_indexed | 2024-12-18T11:58:22Z |
publishDate | 2021-05-01 |
publisher | SpringerOpen |
record_format | Article |
series | Journal of High Energy Physics |
spelling | doaj.art-324c2321e0ce448da9b1207ba9a68b3e2022-12-21T21:09:00ZengSpringerOpenJournal of High Energy Physics1029-84792021-05-012021513010.1007/JHEP05(2021)277Mass and spin for classical strings in dS3Klaas Parmentier0Department of Physics, Columbia UniversityAbstract We demonstrate that all rigidly rotating strings with center of mass at the origin of the dS3 static patch satisfy the Higuchi bound. This extends the observation of Noumi et al. for the open GKP-like string to all solutions of the Larsen-Sanchez class. We argue that strings violating the bound end up expanding towards the horizon and provide a numerical example. Adding point masses to the open string only increases the mass/spin ratio. For segmented strings, we write the conserved quantities, invariant under Gubser’s algebraic evolution equation, in terms of discrete lightcone coordinates describing kink collisions. Randomly generated strings are found to have a tendency to escape through the horizon that is mostly determined by their energy. For rapidly rotating segmented strings with mass/spin < 1, the kink collisions eventually become causally disconnected. Finally we consider the scenario of cosmic strings captured by a black hole in dS and find that horizon friction can make the strings longer.https://doi.org/10.1007/JHEP05(2021)277Bosonic StringsLong stringsString theory and cosmic strings |
spellingShingle | Klaas Parmentier Mass and spin for classical strings in dS3 Journal of High Energy Physics Bosonic Strings Long strings String theory and cosmic strings |
title | Mass and spin for classical strings in dS3 |
title_full | Mass and spin for classical strings in dS3 |
title_fullStr | Mass and spin for classical strings in dS3 |
title_full_unstemmed | Mass and spin for classical strings in dS3 |
title_short | Mass and spin for classical strings in dS3 |
title_sort | mass and spin for classical strings in ds3 |
topic | Bosonic Strings Long strings String theory and cosmic strings |
url | https://doi.org/10.1007/JHEP05(2021)277 |
work_keys_str_mv | AT klaasparmentier massandspinforclassicalstringsinds3 |