2012
DOI: 10.1007/s10714-012-1370-3
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Collapsing shear-free perfect fluid spheres with heat flow

Abstract: A global view is given upon the study of collapsing shear-free perfect fluid spheres with heat flow. We apply a compact formalism, which simplifies the isotropy condition and the condition for conformal flatness. This formalism also presents the simplest possible version of the main junction condition, demonstrated explicitly for conformally flat and geodesic solutions. It gives the right functions to disentangle this condition into well known differential equations like those of Abel, Riccati, Bernoulli and t… Show more

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Cited by 69 publications
(50 citation statements)
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References 57 publications
(152 reference statements)
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“…Our class of solution comprises a particular well behaved solution previously derived by one of us [44]. In continuation of our previous work [45] we present here a new class of solutions of Einstein-Maxwell field equations with well behaved neutral counterpart in isotropic coordinates by motivation of Das et al [46], Ivanov [47], and Murad and Pant [48]. Such solutions are expected to provide simplified but easy to mathematically analyzed compact stellar models of bare strange quark star, a star with nonzero ultra-high surface density.…”
Section: Introductionmentioning
confidence: 78%
“…Our class of solution comprises a particular well behaved solution previously derived by one of us [44]. In continuation of our previous work [45] we present here a new class of solutions of Einstein-Maxwell field equations with well behaved neutral counterpart in isotropic coordinates by motivation of Das et al [46], Ivanov [47], and Murad and Pant [48]. Such solutions are expected to provide simplified but easy to mathematically analyzed compact stellar models of bare strange quark star, a star with nonzero ultra-high surface density.…”
Section: Introductionmentioning
confidence: 78%
“…Nearly all spherically symmetric static solutions of the Einstein field equations were obtained using curvature coordi- (2005) presented a matrix method for generating relativistic solutions which describe compact objects in isotropic coordinates. Ivanov (2012), through his study of collapsing shear-free fluid spheres with heat flow was able to show a strong link between the solution-generating method for static, isotropic spheres and collapsing, radiating spheres. Lake (2003) has presented an algorithm which generates all static spherically symmetric perfect solutions by choosing a single monotone function (subject to boundary conditions).…”
Section: Introductionmentioning
confidence: 99%
“…In the present work we study the evolution of a conformally flat geometry, minimally coupled with a scalar field, along with the presence of a fluid. This specific case of spacetime metric is well-studied for radiating and/or shear-free stars [18][19][20][21][22][23][24][25] and is receiving increasing interest in the context of gravitational collapse quite recently [26][27][28]. We make the additional assumption that the evolution is self-similar in nature.…”
Section: Introductionmentioning
confidence: 99%