HIGHLIGHTS
- who: F. M. da Silva from the , Departamento de Fu00edsica, Universidade Federal do Espu00edrito Santo, AvFernando Ferrari, Vitu00f3ria, ES CEP, Brazil have published the research work: Rapidly rotating neutron stars in gravity, in the Journal: Eur. Phys. J. C (2023) 83:295 of /2023/
- what: The organization of the paper has the following structure: The authors obtained sequences of solutions for four rotation regimes: non-rotating stars which are represented by dashed curves in the plots, stars rotating at 300 Hz represented by dash double-dot curves, stars rotating at 716 Hz shown in the . . .
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