Bochner Flat Lorentzian Kähler Spacetime Manifold with (m,ρ)-quasi-Einstein Soliton
In this work, we characterize [Formula: see text]-quasi-Einstein solitons in Bochner flat Lorentzian Kähler spacetime manifolds. We have addressed various circumstances for [Formula: see text]-Einstein solitons to be steady, shrinking or expanding in terms of isotropic pressure, the cosmological constant, energy density and gravitational constant in different perfect fluids such as stiff matter, dust fluid, dark fluid and radiation fluid.
Authors
- Gyanvendra Pratap Singh (ORCID: https://orcid.org/0009-0000-2155-7180)
- Pawan Prajapati (ORCID: https://orcid.org/0000-0002-3678-0710)
- Santu Dey (ORCID: https://orcid.org/0000-0002-2601-3788)
- Young Jin Suh (ORCID: https://orcid.org/0000-0003-0319-0738)
Institutions
- Bidhan Chandra Krishi Viswavidyalaya (IN)
- Kyungpook National University (KR)
- Deen Dayal Upadhyaya Gorakhpur University (IN)
Publication Details
- Journal
- International Journal of Geometric Methods in Modern Physics
- Published
- 2025-10-31
- DOI
- https://doi.org/10.1142/s0219887826500635
- Primary Topic
- Geometric Analysis and Curvature Flows
- Type
- article
- Field-Weighted Citation Impact
- 0.00