Shape of higher-order images of equatorial emission rings around a Schwarzschild black hole: Analytical description with polar curves
نویسندگان
چکیده
Higher-order photon rings can be expected to detected in a more detailed image of the black hole found future observations. These are lensed images luminous matter surrounding and formed by photons that loop around it. In this paper we have succeeded derive an analytical expression for shape higher-order form is most convenient application: explicit equation curve polar coordinates. The formula describes apparent circular ring with given radius Schwarzschild as viewed distant observer arbitrary inclination. For derivation, strong deflection limit gravitational used. Our simple efficient alternative numerical calculation ray trajectories, main application studying $n=2$ $n=3$ rings.
منابع مشابه
The Dynamical Stability of Tori around a Schwarzschild Black Hole
Recently, geometrically thick disks around black holes have been studied by many authors. I) These models may exist in the inner region of accretion disks and explain the generation of high luminosity and colliminated jets in quasers and active galactic nuclei. In such tori, there is no reason for the rotation law to be Keplerian as pressure force plays a role in the equilibrium structure. Thes...
متن کاملEntropy of Schwarzschild black hole and string-black hole correspondence
The string-black hole correspondence is considered in the context of the correspondence principle proposed recently by Horowitz and Polchinski [7]. We demonstrate that the entropy of string states and the entropy of a Schwarzschild black hole can be matched including the subleading terms which depend on mass logarithmically. We argue the necessity to include the string interaction (with couplin...
متن کاملSchwarzschild black hole with global monopole charge
We derive the metric for a Schwarzschild black hole with global monopole charge by relaxing asymptotic flatness of the Schwarzschild field. We then study the effect of global monopole charge on particle orbits and the Hawking radiation. It turns out that existence, boundedness and stability of circular orbits scale up by (1 − 8πη2)−1, and the perihelion shift and the light bending by (1−8πη2)−3...
متن کاملEinstein rings as a tool for estimating distances and the mass of a Schwarzschild black hole
The bending of light due to the curvature of spacetime close to a black hole is so strong that light can even return to the point of emittance yielding an Einstein ring. Using the analytic solution of the geodesic equation in Schwarzschild spacetime and a distant star or a flash of light, we will be able to determine the mass of a black hole as well as the distance of the observer to this black...
متن کاملA Dual CFT for Schwarzschild Black Hole
We consider horizon as a boundary and study the symmetries of the Schwarzschild metric in the near-horizon region. Appropriate boundary conditions result the boundary killing vectors which obey a Virasoro algebra. The algebra of the corresponding charges has a central term with central charge c = 12 r3 H = 96M 3. If we identify this central charge as the central charge of the dual CFT (defined ...
متن کاملذخیره در منابع من
با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید
ژورنال
عنوان ژورنال: Physical review
سال: 2022
ISSN: ['0556-2813', '1538-4497', '1089-490X']
DOI: https://doi.org/10.1103/physrevd.106.064033