Parametric representations of neutron-star equations of state with phase transitions
This paper explores the use of low-dimensional parametric representations of neutron-star equations of state that include discontinuities caused by phase transitions. The accuracies of optimal piecewise-analytic and spectral representations are evaluated for equations of state having first- or second-order phase transitions with a wide range of discontinuity sizes. These results suggest that the piecewise-analytic representations of these nonsmooth equations of state are convergent, while the spectral representations are not. Nevertheless, the lower-order ($2\ensuremath{\le}{N}_{\text{parms}}\ensuremath{\le}7$) spectral representations are found to be more accurate than the piecewise-analytic representations with the same number of parameters.
Authors
- Lee Lindblom (ORCID: https://orcid.org/0000-0002-3018-1098)
Institutions
- University of California San Diego (US)
Publication Details
- Journal
- Physical review. D/Physical review. D.
- Published
- 2024-08-09
- DOI
- https://doi.org/10.1103/physrevd.110.043018
- Citations
- 6
- Primary Topic
- Pulsars and Gravitational Waves Research
- Type
- article
- Field-Weighted Citation Impact
- 1.99
Funders
- National Science Foundation