Classical and general relativistic post-keplerian effects in binary pulsars hosting fast rotating main sequence stars

HIGHLIGHTS

• who: Lorenzo Iorio and collaborators from the Ministero dell'Istruzione, dell'Università e della Ricerca (MIU.R.)-Istruzione, Viale Unità di Italia, Bari, BA, Italy have published the Article: Classical and general relativistic post-Keplerian effects in binary pulsars hosting fast rotating main sequence stars, in the Journal: Eur. Phys. J. C (2019) 79:690 of /2019/
• what: For evolved models one should use polytropes with a higher polytropic index, as they are more centrally condensed, and typically n=3.43 matches the ESTER evolved models as far as J2 is concerned.

SUMMARY . . .

 

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