PhaseTracer2: from the effective potential to gravitational waves

Fuente: arXiv
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Auteurs principaux: Athron, Peter, Balazs, Csaba, Fowlie, Andrew, Morris, Lachlan, Searle, William, Xiao, Yang, Zhang, Yang
Format: Preprint
Publié: 2024
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author Athron, Peter
Balazs, Csaba
Fowlie, Andrew
Morris, Lachlan
Searle, William
Xiao, Yang
Zhang, Yang
author_facet Athron, Peter
Balazs, Csaba
Fowlie, Andrew
Morris, Lachlan
Searle, William
Xiao, Yang
Zhang, Yang
contents In recent years, the prospect of detecting gravitational waves sourced from a strongly first-order cosmological phase transition has emerged as one of the most exciting frontiers of gravitational wave astronomy. Cosmological phase transitions are an essential ingredient in the Standard Model of particle cosmology, and help explain the mechanism for creation of matter in the early Universe, provide insights into fundamental theories of physics, and shed light on the nature of dark matter. This underscores the significance of developing robust end-to-end tools for determining the resulting gravitational waves from these phase transitions. In this article we present PhaseTracer2, an improved version of the C++ software package PhaseTracer, designed for mapping cosmological phases and transitions in Standard Model extensions of multiple scalar fields. Building on the robust framework of its predecessor, PhaseTracer2 extends its capabilities by including new features crucial for a more comprehensive analysis of cosmological phase transitions. It can calculate more complex properties, such as the bounce action through the path deformation method or an interface with BubbleProfiler, thermodynamic parameters, and gravitational wave spectra. Its applicability has also been broadened via incorporating the dimensionally reduced effective potential for models obtained from DRalgo, as well as calculations in the MSbar and OS-like renormalisation schemes. This modular, flexible, and practical upgrade retains the speed and stability of the original PhaseTracer, while significantly expanding its utility.
format Preprint
id arxiv_https___arxiv_org_abs_2412_04881
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle PhaseTracer2: from the effective potential to gravitational waves
Athron, Peter
Balazs, Csaba
Fowlie, Andrew
Morris, Lachlan
Searle, William
Xiao, Yang
Zhang, Yang
Cosmology and Nongalactic Astrophysics
High Energy Physics - Phenomenology
In recent years, the prospect of detecting gravitational waves sourced from a strongly first-order cosmological phase transition has emerged as one of the most exciting frontiers of gravitational wave astronomy. Cosmological phase transitions are an essential ingredient in the Standard Model of particle cosmology, and help explain the mechanism for creation of matter in the early Universe, provide insights into fundamental theories of physics, and shed light on the nature of dark matter. This underscores the significance of developing robust end-to-end tools for determining the resulting gravitational waves from these phase transitions. In this article we present PhaseTracer2, an improved version of the C++ software package PhaseTracer, designed for mapping cosmological phases and transitions in Standard Model extensions of multiple scalar fields. Building on the robust framework of its predecessor, PhaseTracer2 extends its capabilities by including new features crucial for a more comprehensive analysis of cosmological phase transitions. It can calculate more complex properties, such as the bounce action through the path deformation method or an interface with BubbleProfiler, thermodynamic parameters, and gravitational wave spectra. Its applicability has also been broadened via incorporating the dimensionally reduced effective potential for models obtained from DRalgo, as well as calculations in the MSbar and OS-like renormalisation schemes. This modular, flexible, and practical upgrade retains the speed and stability of the original PhaseTracer, while significantly expanding its utility.
title PhaseTracer2: from the effective potential to gravitational waves
topic Cosmology and Nongalactic Astrophysics
High Energy Physics - Phenomenology
url https://arxiv.org/abs/2412.04881