Compact statis stars with polytropic equation of state in minimal dilatonic gravity

Understand

We present solution of the equations for relativistic static spherically symmetric stars (SSSS) in the model of minimal dilatonic gravity (MDG) using the polytropic equation of state.

• A polytropic equation of state, which has a good fitting with a more realistic one, is used.
• Results are obtained for all variables of a single neutron star in the model of MDG.
• The maximum mass about two solar masses is in accordance with the latest observations of pulsars.