Free Access

Fig. 1


Mass density ρ = ℰ /c2 vs. baryon density nb for NS matter for the set of EOS presented in Figs. 24. Dotted segments correspond to the central densities of NS models, which are unstable with respect to radial oscillations. Relation ρ = ρ(nb) deviates from linearity for nb> 0.3fm-3. Non-linearity grows with increasing nb and is EOS-dependent. For nb ≲ 0.2fm-3, the linear approximation ρnbmn (where mn is neutron mass) is valid. (Colour online.)

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.