CONSTRAINING NEUTRON STAR MATTER WITH QUANTUM CHROMODYNAMICS

By A. Kurkela, E. Fraga, J. Schaffner-Bielich, A. Vuorinen. 2014

156 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/03785571c83c54c96733fa551fa0f59624003c72

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

1. I. Tews
2. S. Reddy
3. Stefano Gandolfi
4. J. Carlson
5. Hector O. Silva
6. Emanuele Berti
7. Justin Alsing
8. V. Cardoso

In Nuclear and High Energy Physics

1. I. Tews
2. S. Reddy
3. Stefano Gandolfi
4. J. Carlson
5. Hector O. Silva
6. Emanuele Berti
7. Justin Alsing
8. J. Lattimer

Citations in the corpus

• Evidence for a maximum mass cut-off in the neutron star mass distribution and constraints on the equation of state (2017, background): “Kurkela et al. (2014) found that cmaxs > 0.74 based on maximum mass considerations, although cautioned that their constraint may be overly restrictive.”
• Constraining the Speed of Sound inside Neutron Stars with Chiral Effective Field Theory Interactions and Observations (2018, methodology): “Kurkela et al. (2014), Fraga et al. (2016), and Annala et al. (2018) discussed the possibility of additionally constraining the EOS with information from pQCD at very high densities.”