Hostname: page-component-cd9895bd7-7cvxr Total loading time: 0 Render date: 2024-12-23T10:46:17.147Z Has data issue: false hasContentIssue false
  • English
  • Français

Constraining three-nucleon forces with multimessenger data

Published online by Cambridge University Press:  27 February 2023

Andrea Sabatucci Open the ORCID record for Andrea Sabatucci [Opens in a new window]
Andrea Sabatucci*
Affiliation:
Dipartimento di Fisica, “Sapienza” Università di Roma, Piazzale Aldo Moro 5, 00185, Roma, Italy email: [email protected] Sezione INFN Roma1, Roma 00185, Italy
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

A detailed description of the properties of dense matter in extreme conditions, as those within Neutron Star cores, is still an open problem, whose solution is hampered by both the lack of empirical data, and by the difficulties in developing a suitable theoretical framework for the microscopic nuclear dynamics in such regimes.

We report here the results of a study aimed at inferring the properties of the repulsive three-nucleon interaction, driving the stiffness of the equation of state at high densities, by performing bayesian inference on current and future astrophysical observations.

Keywords

stars: neutrongravitational wavesdense matterequation of state
Type
Contributed Paper
Information
Proceedings of the International Astronomical Union , Volume 16 , Symposium S363: Neutron Star Astrophysics at the Crossroads: Magnetars and the Multimessenger Revolution , June 2020 , pp. 195 - 198
Creative Commons
Creative Common License - CCCreative Common License - BY
This is an Open Access article, distributed under the terms of the Creative Commons Attribution licence (https://creativecommons.org/licenses/by/4.0/), which permits unrestricted re-use, distribution, and reproduction in any medium, provided the original work is properly cited.
Copyright
© The Author(s), 2023. Published by Cambridge University Press on behalf of International Astronomical Union

References

Maselli, A., Sabatucci, A., Benhar, O. 2021, Phys. Rev. C, 103, 065804 CrossRefGoogle Scholar
Abbott, B. (LIGO Scientific, Virgo) 2017, Phys. Rev. Lett., 119, 161101 CrossRefGoogle ScholarPubMed
Abbott, B. (LIGO Scientific, Virgo) 2019, Phys. Rev. X, 9, 011001Google Scholar
Riley, T. E., 2019, ApJ Lett., 887, L21 CrossRefGoogle Scholar
Akmal, A., Pandharipande, V. R., Revenhall, D. G. 1998, Phys. Rev. C, 58, 1804 CrossRefGoogle Scholar
Essick, R., Tews, I., Landry, P., Reddy, S., Holz, D. E. 2020, Phys. Rev. C, 102, 055803 CrossRefGoogle Scholar
Foreman-Mackey, D., Hogg, D. W., Lang, D., Goodman, J. 2013, PASP, 125, 306–312 CrossRefGoogle Scholar
Stephanov, M. A. 2006, PoS LAT2006, 024Google Scholar
Tonetto, L., Sabatucci, A., Benhar, O. 2021, Phys. Rev. D, 104, 083034 CrossRefGoogle Scholar