Proper time expansions and glasma dynamics
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arXiv
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| Main Authors: | , , , , |
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| Format: | Preprint |
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2025
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| _version_ | 1866913010919931904 |
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| author | Carrington, Margaret E Friesen, Bryce T. Pickering, Doug Sangster, Shane Soopramania, Kaene |
| author_facet | Carrington, Margaret E Friesen, Bryce T. Pickering, Doug Sangster, Shane Soopramania, Kaene |
| contents | The earliest phase of an ultrarelativistic heavy ion collision can be described as a highly populated system of gluons called glasma. The system's dynamics is governed by the classical Yang-Mills equation. Solutions can be found at early times using a proper time expansion. Since the expansion parameter is the time, this method is necessarily limited to the study of early time dynamics. In addition compute time and memory limitations restrict practical calculations to no more than eighth order in the expansion. The result is that the method produces reliable results only for very early times. In this paper we explore several different methods to increase the maximum time that can be reached. We find that, depending slightly on the quantity being calculated, the latest time for which reliable results are obtained can be extended approximately 1.5 times (from $\sim0.05$~fm/$c$ using previous methods to about $0.08$~fm/$c$). |
| format | Preprint |
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arxiv_https___arxiv_org_abs_2510_06390 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | Proper time expansions and glasma dynamics Carrington, Margaret E Friesen, Bryce T. Pickering, Doug Sangster, Shane Soopramania, Kaene Nuclear Theory The earliest phase of an ultrarelativistic heavy ion collision can be described as a highly populated system of gluons called glasma. The system's dynamics is governed by the classical Yang-Mills equation. Solutions can be found at early times using a proper time expansion. Since the expansion parameter is the time, this method is necessarily limited to the study of early time dynamics. In addition compute time and memory limitations restrict practical calculations to no more than eighth order in the expansion. The result is that the method produces reliable results only for very early times. In this paper we explore several different methods to increase the maximum time that can be reached. We find that, depending slightly on the quantity being calculated, the latest time for which reliable results are obtained can be extended approximately 1.5 times (from $\sim0.05$~fm/$c$ using previous methods to about $0.08$~fm/$c$). |
| title | Proper time expansions and glasma dynamics |
| topic | Nuclear Theory |
| url | https://arxiv.org/abs/2510.06390 |