Discussing cosmic string configurations in a supersymmetric scenario without Lorentz invariance

DOI10.1088/1367-2630/12/5/053029zbMath1375.83056arXiv0807.4342OpenAlexW1976812489MaRDI QIDQ4594878

C. E. C. Lima, José A. Helayël-Neto, Cristine N. Ferreira

Publication date: 27 November 2017

Published in: New Journal of Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/0807.4342

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 (1)

Casimir energy and brane stability

Cites Work

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• Some Consequences of<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>TCP</mml:mi></mml:math>-Invariance
• Topology of cosmic domains and strings
• Parity-violating gravitational coupling of electromagnetic fields
• The Theory of Quantized Fields. I
• Cosmic string configuration in the supersymmetric CSKR theory

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