Inter-brane potential and the decay of a non-BPS-D-brane to closed strings

DOI10.1016/j.physletb.2003.08.033zbMath1058.81672arXivhep-th/0307078OpenAlexW2094632559MaRDI QIDQ1409376

S.-H. Henry Tye, Saswat Sarangi

Publication date: 13 October 2003

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

Full work available at URL: https://arxiv.org/abs/hep-th/0307078

zbMATH Keywords

decay widthradiative correctionstachyonic modes

Mathematics Subject Classification ID

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

Related Items (7)

Pre-inflationary spacetime in string cosmology ⋮ Unitarity at infinity and topological holography ⋮ The \(D3\)-\(\bar{D}3\)-brane inflation model revisited ⋮ The Hagedorn temperature and open QCD-string tachyons in pure \(\mathcal N=1\) super-Yang-Mills ⋮ TACHYON DYNAMICS IN OPEN STRING THEORY ⋮ Instanton transition in thermal and moduli deformed de Sitter cosmology ⋮ D‐branes in Standard Model building, gravity and cosmology

Cites Work

• Cosmic string production towards the end of brane inflation
• String Theory
• Confinement on the brane.

This page was built for publication: Inter-brane potential and the decay of a non-BPS-D-brane to closed strings