1) Cherubini C, Filippi S, A Loppini A, Moradi R, Ruffini R, Wang Y and Xue S (2018). Perfect relativistic magnetohydrodynamics around black holes in horizon penetrating coordinates. PHYSICAL REVIEW D, vol. 97, p. 064038-1-064038-8, ISSN: 2470-0010, doi: 10.1103/PhysRevD.97.064038

2) Cipolletta F, Cherubini C, Filippi S, Rueda J A, Ruffini R (2017). Equilibrium Configurations of Classical Polytropic Stars with a Multi-Parametric Differential Rotation Law: A Numerical Analysis. COMMUNICATIONS IN COMPUTATIONAL PHYSICS, vol. 22, p. 863-888, ISSN: 1991-7120, doi: doi: 10.4208/cicp.OA-2017-0007

3) Cipolletta F, Cherubini C, Filippi S, Rueda j A and Ruffini R (2017). Last stable orbit around rapidly rotating neutron stars . PHYSICAL REVIEW D, vol. 96, p. 024046-1-024046-10, ISSN: 2470-0010, doi: 10.1103/PhysRevD.96.024046

4) Cipolletta F, Cherubini C, Filippi S, Rueda J A, Ruffini R (2015). Fast rotating neutron stars with realistic nuclear matter equation of state. PHYSICAL REVIEW D, PARTICLES, FIELDS, GRAVITATION, AND COSMOLOGY, vol.92, p. 023007-1-023007-14, ISSN:1550-7998, doi:10.1103/PhysRevD.92. 023007

5) Cherubini C and Filippi S, (2016) The Hamiltonian Field Theory of the Von Mises Wave Equation: Analytical and Computational Issues, COMMUNICATIONS IN COMPUTATIONAL PHYSICS, Vol. 19, Issue 03, 758-769.