The signature of string ball near surface horizon of cylindrical universe

DOI10.1007/S10509-012-1350-9zbMath1276.83064OpenAlexW2045085802MaRDI QIDQ383477

Mohammad Hasan, H. S. Yoon

Publication date: 4 December 2013

Published in: Astrophysics and Space Science (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/s10509-012-1350-9

zbMATH Keywords

universecylindrically symmetric modelstring ball

Mathematics Subject Classification ID

Relativistic cosmology (83F05) String and superstring theories; other extended objects (e.g., branes) in quantum field theory (81T30)

Related Items (2)

Time evolution of meson density during formation of expanding quark-antiquark system ⋮ The information loss for QCD matter in cylindrical black holes at LHC

Cites Work

• Closed string thermal torus from thermo field dynamics
• D-branes as coherent states in the open string channel
• Strings in horizons, dissipation and a possible interpretation of the Hagedorn temperature
• Cylindrically symmetric inhomogeneous universes with a cloud of strings
• Cylindrically symmetric inhomogeneous cosmological models with viscous fluid and varying \(\Lambda\)
• Some Magnetized Bulk Viscous String Cosmological Models in Cylindrically Symmetric Inhomogeneous Universe with Variable Λ-Term
• Quantum theory: concepts and methods

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