Role of $$f(R,T,R_{\mu \nu }T^{\mu \nu })$$ f ( R , T , R μ ν T μ ν ) model on the stability of cylindrical stellar model
Crossref DOI link: https://doi.org/10.1140/epjc/s10052-017-4923-5
Published Online: 2017-05-30
Published Print: 2017-06
Update policy: https://doi.org/10.1007/springer_crossmark_policy
Yousaf, Z.
Bhatti, M. Zaeem-ul-Haq
Farwa, Ume
License valid from 2017-05-30