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Inner crust equations of state for CompOSE

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Abstract

In this paper, we present some relativistic mean-field inner crust equations of state that have recently been uploaded in the CompOSE online repository. These equations of state fulfill experimental and microscopic constraints, and are also able to reproduce two solar-mass stars. We integrate the TOV equations to obtain the mass-radius relation, and we also calculate the tidal deformability, compactness, and effective tidal deformability to compare with the latest astrophysical data from NICER and LIGO and Virgo.

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Data Availibility Statement

This manuscript has associated data in a data repository. [Authors’ comment: The EoS tables for the inner crust are freely available in the online CompOSE repository: https://compose.obspm.fr/table/fam/5. Three of these tables are contained in the Appendix of this published article.]

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Acknowledgements

We thank C. Providência for carefully reading the manuscript. This work was partly supported by the FCT (Portugal) Projects No. UID/FIS/04564/2020 and POCI-01-0145-FEDER-029912, and by PHAROS COST Action CA16214. H.P. acknowledges the Grant CEECIND/03092/2017 (FCT, Portugal).

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  1. CFisUC, Department of Physics, University of Coimbra, 3004-516, Coimbra, Portugal

    Tuhin Malik & Helena Pais

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  1. Tuhin Malik
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Correspondence to Helena Pais.

Additional information

Communicated by Laura Tolos

Appendix

Appendix

See Table 3.

Table 3 The inner crust equation of state for the TM1e, DD2 and TW models
Full size table

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Malik, T., Pais, H. Inner crust equations of state for CompOSE. Eur. Phys. J. A 58, 154 (2022). https://doi.org/10.1140/epja/s10050-022-00799-3

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