Connections between the Shadow Radius and the Quasinormal Modes of Kerr-Sen Black Hole
نویسندگان
چکیده
The correspondence between the shadow radius and real part of quasinormal modes (QNMs) a Kerr–Sen black hole is studied. By using equation angular separation constant QNMs, expression QNMs related to established in eikonal limit. We found that, our formula can reduce previous result Kerr when Kerr-Sen parameter b sets zero.
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ژورنال
عنوان ژورنال: Universe
سال: 2022
ISSN: ['2218-1997']
DOI: https://doi.org/10.3390/universe8110604