The effect of dark matter on schwarzschild and kerr black holes: Considerations on the weak deflection angles and the kerr shadow

We consider the effect of a spherical dark matter distribution that surrounds a black hole of mass m. The dark matter is only characterized by its mass M, inner radius rs , and thickness ∆rs . A black hole surrounded by an astrophysical environment such as dark matter is called a dirty black hole. C...

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Bibliographic Details
Main Author: Pantig, Reggie C.
Format: text
Language:English
Published: Animo Repository 2020
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Online Access:https://animorepository.dlsu.edu.ph/etd_doctoral/1406
https://animorepository.dlsu.edu.ph/cgi/viewcontent.cgi?article=2447&context=etd_doctoral
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Institution: De La Salle University
Language: English

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