English
 
Help Privacy Policy Disclaimer
  Advanced SearchBrowse
  1. View item / 
  2. Item Summary

Item

ITEM ACTIONSEXPORT
Add to Basket
  Local TagsRelease HistoryDetailsSummary

Released
Journal Article

Revealing the strength of three-nucleon interactions with the Einstein Telescope

MPS-Authors
/persons/resource/persons192099

Dietrich,  Tim
Multi-messenger Astrophysics of Compact Binaries, AEI-Golm, MPI for Gravitational Physics, Max Planck Society;
Astrophysical and Cosmological Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society;

External Resource
No external resources are shared
Fulltext (restricted access)
There are currently no full texts shared for your IP range.
Fulltext (public)

2303.11201.pdf
(Preprint), 860KB

Supplementary Material (public)
There is no public supplementary material available
Citation

Rose, H., Kunert, N., Dietrich, T., Pang, P. T. H., Smith, R., Broeck, C. V. D., et al. (2023). Revealing the strength of three-nucleon interactions with the Einstein Telescope. Physical Review C, 108(2): 025811. doi:10.1103/PhysRevC.108.025811.


Cite as: https://hdl.handle.net/21.11116/0000-000C-F292-D
Abstract
Three-nucleon forces are crucial for the accurate description of nuclear
systems, including dense matter probed in neutron stars. We explore nuclear
Hamiltonians that reproduce two-nucleon scattering data and properties of light
nuclei, but differ in the three-nucleon interactions among neutrons. While no
significantly improved constraints can be obtained from current astrophysical
data, we show that observations of neutron star mergers by next-generation
detectors like the proposed Einstein Telescope could provide strong evidence to
distinguish between these Hamiltonians.