Constraining neutron-star matter with microscopic and macroscopic collisions

Interpreting high-energy, astrophysical phenomena, such as supernova explosions or neutron-star collisions, requires a robust understanding of matter at supranuclear densities. However, our knowledge about dense matter explored in the cores of neutron stars remains limited. Fortunately, dense matter...

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Detalles Bibliográficos
Autores principales: Huth, Sabrina, Pang, Peter T. H., Tews, Ingo, Dietrich, Tim, Le Fèvre, Arnaud, Schwenk, Achim, Trautmann, Wolfgang, Agarwal, Kshitij, Bulla, Mattia, Coughlin, Michael W., Van Den Broeck, Chris
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Nature Publishing Group UK 2022
Materias:
Article
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC9177417/
https://www.ncbi.nlm.nih.gov/pubmed/35676430
http://dx.doi.org/10.1038/s41586-022-04750-w

Internet

https://www.ncbi.nlm.nih.gov/pmc/articles/PMC9177417/
https://www.ncbi.nlm.nih.gov/pubmed/35676430
http://dx.doi.org/10.1038/s41586-022-04750-w

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