https://doi.org/10.1140/epjc/s10052-023-11325-0
Regular Article - Theoretical Physics
Optical properties of a non-commutative rotating black hole
Department of Mathematics, Lahore College for Women University, 54000, Lahore, Pakistan
Received:
20
November
2022
Accepted:
12
February
2023
Published online:
28
February
2023
This paper explores the shadow cast by a non-commutative rotating Hayward black hole. The apparent shape as well as the size of the shadow depends upon the spin, non-commutative parameter as well as the parameter g of the said black hole. The size of the shadow decreases with g as well as the non-commutative parameter. Also, the shape of the shadow deviates from a perfect circle for the high values of g and the spin. We then discuss the rate of energy emission. Moreover, we study the impact of plasma on the size, shape as well as the rate of energy emission. We found that the plasma reduces the size and deformation of the shadow.
© The Author(s) 2023
Open Access This article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons licence, and indicate if changes were made. The images or other third party material in this article are included in the article’s Creative Commons licence, unless indicated otherwise in a credit line to the material. If material is not included in the article’s Creative Commons licence and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. To view a copy of this licence, visit http://creativecommons.org/licenses/by/4.0/.
Funded by SCOAP3. SCOAP3 supports the goals of the International Year of Basic Sciences for Sustainable Development.