A class of cosmological matrix models

DOI10.1016/j.physletb.2005.08.099zbMath1247.83281arXivhep-th/0506260OpenAlexW2051815668WikidataQ125289609 ScholiaQ125289609MaRDI QIDQ451910

Miao Li

Publication date: 25 September 2012

Published in: Physics Letters. B (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/hep-th/0506260

zbMATH Keywords

cosmologymatrix modelslight-like singularity

Mathematics Subject Classification ID

Relativistic cosmology (83F05) String and superstring theories in gravitational theory (83E30) Supersymmetric field theories in quantum mechanics (81T60) String and superstring theories; other extended objects (e.g., branes) in quantum field theory (81T30)

Related Items (12)

Some new light-cone time dependent solutions in deformed pp-wave backgrounds ⋮ Supersymmetric intersecting branes on the waves ⋮ Quantum evolution across singularities: the case of geometrical resolutions ⋮ Quantum evolution across singularities ⋮ Non-supersymmetric string theory ⋮ Adiabaticity and emergence of classical space-time in time-dependent matrix theories ⋮ Null cosmological singularities and free strings. II. ⋮ Matrix model in a class of time dependent supersymmetric backgrounds ⋮ Matrix string description of cosmic singularities in a class of time-dependent solutions ⋮ D-brane solutions in a light-like linear dilaton background ⋮ Time-dependent supergravity solutions in null dilaton background ⋮ D3-BRANES AT ANGLE IN LINEAR DILATON pp-WAVE BACKGROUND

Cites Work

• D0 branes on \(T^n\) and matrix theory
• Why Is the Matrix Model Correct?

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