arXiv:2404.16079v1 Announce Type: new
Abstract: With the help of Newman-Janis method new spinning black hole (BH) solution for a non-local gravity model was obtained. We show how to account the quantum gravitational correction part in BH shadows modelling using spinning BH metrics with a model independent approach. It is confirmed that in the future to follow the increasing of the experimental accuracy and therefore to reproduce new results theoretically one could take into account different field correction terms instead of introducing of new fields and/or curvature expansions.
With the advancement of the Newman-Janis method, a new spinning black hole (BH) solution has been derived for a non-local gravity model. This solution allows for the modeling of black hole shadows, taking into account quantum gravitational corrections. A model-independent approach is used, which suggests that in the future, instead of introducing new fields and/or curvature expansions, different field correction terms can be considered to reproduce new results theoretically.
Roadmap for Readers
1. Introduction to Spinning Black Hole Solutions
Begin by explaining the importance of spinning black hole solutions in understanding gravity models and black hole shadows. Discuss the Newman-Janis method and its significance in obtaining a new spinning black hole solution for a non-local gravity model.
2. Quantum Gravitational Corrections in Black Hole Shadows
Explore the concept of quantum gravitational corrections in the modeling of black hole shadows. Explain how the spinning black hole metrics derived using the Newman-Janis method can be utilized to account for these corrections.
3. Model-Independent Approach
Introduce the concept of a model-independent approach to black hole shadow modeling. Explain how this approach allows for the consideration of different field correction terms instead of introducing new fields or curvature expansions.
4. Future Prospects and Challenges
- Discuss the potential challenges in incorporating different field correction terms into black hole shadow modeling.
- Highlight the opportunities for future research in improving the accuracy of experimental results and theoretical predictions.
- Explore the implications of using the spinning black hole solution for a non-local gravity model in other areas of gravitational research.
5. Conclusion
Summarize the key findings of the research and emphasize the potential of the new spinning black hole solution and the model-independent approach in advancing our understanding of black hole shadows and gravity models.