Bayesian history matching is a statistical tool used to calibrate complex numerical models. Now, it has been applied to first-principles simulations of several nuclei, including 208Pb, whose properties are linked to the interior of neutron stars.
This is a preview of subscription content, access via your institution
Access options
Access Nature and 54 other Nature Portfolio journals
Get Nature+, our best-value online-access subscription
$29.99 / 30 days
cancel any time
Subscribe to this journal
Receive 12 print issues and online access
$209.00 per year
only $17.42 per issue
Buy this article
- Purchase on Springer Link
- Instant access to full article PDF
Prices may be subject to local taxes which are calculated during checkout
References
Arthuis, P., Barbieri, C., Vorabbi, M. & Finelli, P. Phys. Rev. Lett. 125, 182501 (2020).
Hu, B. et al. Nat. Phys. https://doi.org/10.1038/s41567-022-01715-8 (2022).
Miyagi, T., Stroberg, S. R., Navrátil, P., Hebeler, K. & Holt, J. D. Phys. Rev. C 105, 014302 (2022).
Epelbaum, E. & Meiβner, U.-G. Annu. Rev. Nucl. Part. Sci. 62, 159–185 (2012).
Vernon, I., Goldstein, M. & Bower, R. Stat. Sci. 29, 81–90 (2014).
Adhikari, D. et al. Phys. Rev. Lett. 126, 172502 (2021).
Author information
Authors and Affiliations
Corresponding author
Ethics declarations
Competing interests
The author declares no competing interests.
Rights and permissions
About this article
Cite this article
Rios, A. A historic match for nuclei and neutron stars. Nat. Phys. 18, 1137–1138 (2022). https://doi.org/10.1038/s41567-022-01782-x
Published:
Issue Date:
DOI: https://doi.org/10.1038/s41567-022-01782-x