Anisotropic strange quintessence stars in f ( R ) $f(R)$ gravity
نویسندگان
چکیده
منابع مشابه
Surface gravity of neutron stars and strange stars
The upper bound on the value of the surface gravity, gs, for neutron stars with equations of state respecting vsound ≤ c, is derived. This bound is inversely proportional to the maximum allowable mass Mmax, and it reads gs ≤ 1.411× 10 15 (Mmax/M⊙) −1 cm s. It implies an absolute upper bound 7.4× 10 cm s if one uses the 2σ lower bound on the neutron mass measured recently in 4U1700-37, 1.9M⊙. A ...
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ژورنال
عنوان ژورنال: Astrophysics and Space Science
سال: 2015
ISSN: 0004-640X,1572-946X
DOI: 10.1007/s10509-015-2426-0