The cosmology of string theoretic axions

DOI10.1016/S0550-3213(97)00413-6zbMath0925.83092arXivhep-th/9608197OpenAlexW2103420732MaRDI QIDQ1371593

Tom Banks, Michael Dine

Publication date: 29 October 1997

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

Full work available at URL: https://arxiv.org/abs/hep-th/9608197

zbMATH Keywords

CP violationcompactification radiusbaryon number densitymassive string moduli

Mathematics Subject Classification ID

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

Related Items (16)

The landscape of QCD axion models ⋮ PROGRESS IN WEAKLY COUPLED STRING PHENOMENOLOGY ⋮ Strong CP and \(SUZ_{2}\) ⋮ String and M-theory cosmological solutions with Ramond forms ⋮ Stochastic axion dark matter in axion landscape ⋮ Axion kinetic misalignment and parametric resonance from inflation ⋮ Implications of protecting the QCD axion in the dual description ⋮ An \(M\) theory solution to the strong CP-problem, and constraints on the axiverse ⋮ POST-INFLATION INCREASE OF THE COSMOLOGICAL TENSOR-TO-SCALAR PERTURBATION RATIO ⋮ Towards a solution of the moduli problems of string cosmology ⋮ Are axidilaton stars massive compact halo objects? ⋮ Is there a stable hydrogen atom in higher dimensions? ⋮ Supersymmetry breakdown at a hidden wall ⋮ Grand unification at intermediate mass scales through extra dimensions ⋮ STRING COSMOLOGY ⋮ Impact of helical electromagnetic fields on the axion window

Cites Work

• Baryogenesis from flat directions of the supersymmetric standard model
• Heterotic and type I string dynamics from eleven dimensions

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