Energy constraints for static wormholes in f(ℛ,𝒯 ) gravity
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Publication:6127227
DOI10.1142/S0219887823502365OpenAlexW4385350519MaRDI QIDQ6127227
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Publication date: 10 April 2024
Published in: International Journal of Geometric Methods in Modern Physics (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1142/s0219887823502365
Relativistic cosmology (83F05) Black holes (83C57) String and superstring theories in gravitational theory (83E30) Supergravity (83E50) Dynamical systems in other branches of physics (quantum mechanics, general relativity, laser physics) (37N20) Dark matter and dark energy (83C56)
Cites Work
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- Cosmological reconstruction and stability in \(f(R,T)\) gravity
- Van der Waals quintessence
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- The role of energy conditions in \(f(R)\) cosmology
- Non-existence of Bianchi type-III bulk viscous string cosmological model in \(f(R,T)\) gravity
- Evolution of the universe in inverse and \(\ln f(R)\) gravity
- Bounding f(R) gravity by particle production rate
- Wormholes in spacetime and their use for interstellar travel: A tool for teaching general relativity
- Cosmological perfect-fluids in f(R) gravity
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