Canuto et al. 1979
Canuto, V., B. Datta, and G. Kalman, 1979: Astrophysical determination of the scale parameter in QCD. Phys. Lett. B, 85, 467-470, doi:10.1016/0370-2693(79)91297-8.
We consider the phase transition to quark matter in a system of high density matter, taking into account the spin-2 interaction among nucleons. We find that the transition is possible only if the spin-2 coupling constant is ten times smaller than its value at low energies. From this we are able to determine the scale parameter of QCD.
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Canuto, V., Datta, B., and Kalman, G.: Astrophysical determination of the scale parameter in QCD, Phys. Lett. B, 85, 467-470, doi:10.1016/0370-2693(79)91297-8, 1979.
Canuto, V., B. Datta, and G. Kalman (1979), Astrophysical determination of the scale parameter in QCD, Phys. Lett. B, 85, 467-470, doi:10.1016/0370-2693(79)91297-8.
Canuto, V., B. Datta, and G. Kalman, 1979: Astrophysical determination of the scale parameter in QCD. Phys. Lett. B, 85, 467-470, doi:10.1016/0370-2693(79)91297-8.
Canuto, V., Datta, B., & Kalman, G. 1979, Phys. Lett. B, 85, 467, doi:10.1016/0370-2693(79)91297-8.
Canuto V, Datta B, Kalman G. Astrophysical determination of the scale parameter in QCD, Phys Lett B 1979;85:467-470. doi:10.1016/0370-2693(79)91297-8.
V. Canuto, B. Datta, G. Kalman, Phys. Lett. B 85, 467-470, doi:10.1016/0370-2693(79)91297-8 (1979).
