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arxiv astro-ph/9801174 v2 pith:GZWFK3FM submitted 1998-01-18 astro-ph gr-qchep-th

Role of the scalar field in gravitational lensing

classification astro-ph gr-qchep-th
keywords lenslensingscalarchargegravitationalimageslargemass
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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A static and circularly symmetric lens characterized by mass and scalar charge parameters is constructed. For the small values of the scalar charge to the mass ratio, the gravitational lensing is qualitatively similar to the case of the Schwarzschild lens; however, for large values of this ratio the lensing characteristics are significantly different. The main features are the existence of two or nil Einstein ring(s) and a radial critical curve, formation of two or four images and possibility of detecting three images near the lens for sources located at relatively large angular positions. Such a novel lens may also be treated as a naked singularity lens.

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Cited by 3 Pith papers

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    Semiclassical one-loop analysis of solvable near-critical collapse solutions shows quantum corrections selecting a Boulware-like state and producing a growing mode that yields a finite mass gap and a transition to Typ...