NEUMATT
NEUtron star MATter theory
The Equation of State of Nuclear Matter and
Neutron Star Structure
SELECTED PUBLICATIONS
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G. Taranto, G.F. Burgio, H.-J. Schulze,
Cassiopeia A and direct Urca cooling,
MNRAS 456, 1451 (2016).
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A. Drago, A. Lavagno, B. Metzger, G. Pagliara,
Quark deconfinement and the duration of short Gamma Ray Bursts,
Phys.Rev. D93 (2016) 103001.
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S. Carignano, A. Mammarella, M. Mannarelli,
Equation of state of imbalanced cold matter from chiral
perturbation theory,
Phys.Rev. D93 (2016) 051503.
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Dong, J. M.; Lombardo, U.; Zhang, H. F. et al.
Role of the nucleonic Fermi surface depletion in neutron star
cooling,
Astrophys. J. 817 (2016) 6.
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S. Seveso, P. M. Pizzochero, F. Grill and B. Haskell,
Mesoscopic pinning forces in neutron star crusts,
MNRAS 455 (2016) 3952.
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D. Logoteta, I. Vidana, I. Bombaci, A. Kievsky,
Comparative study of three-nucleon force models in nuclear matter,
Phys. Rev. C 91(2015) 064001.
Cassiopeia A and direct Urca cooling,
MNRAS 456, 1451 (2016).
Quark deconfinement and the duration of short Gamma Ray Bursts,
Phys.Rev. D93 (2016) 103001.
Equation of state of imbalanced cold matter from chiral perturbation theory,
Phys.Rev. D93 (2016) 051503.
Role of the nucleonic Fermi surface depletion in neutron star cooling,
Astrophys. J. 817 (2016) 6.
Mesoscopic pinning forces in neutron star crusts,
MNRAS 455 (2016) 3952.
Comparative study of three-nucleon force models in nuclear matter,
Phys. Rev. C 91(2015) 064001.