Why two is more attractive than one \(\ldots\) or Bianchi class-A models and Reissner-Nordström black holes in quantum \(N=2\) supergravity

DOI10.1016/S0920-5632(97)00392-7zbMath0976.83536arXivhep-th/9706138OpenAlexW2048349067WikidataQ57562521 ScholiaQ57562521MaRDI QIDQ5927259

Paulo Rodrigues Lima Vargas Moniz

Publication date: 8 March 2001

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

Full work available at URL: https://arxiv.org/abs/hep-th/9706138

zbMATH Keywords

Lorentz invariantMaxwell fieldsquantum supergravitysupersymmetry constraints

Mathematics Subject Classification ID

Black holes (83C57) Supergravity (83E50)

Related Items (1)

Supersymmetric quantum cosmology: a `Socratic' guide

Cites Work

• Unnamed Item
• Physical states in canonically quantized supergravity
• CANONICAL QUANTIZATION OF BIANCHI CLASS A MODELS IN N=2 SUPERGRAVITY
• SUPERSYMMETRIC QUANTUM COSMOLOGY SHAKEN, NOT STIRRED

This page was built for publication: Why two is more attractive than one \(\ldots\) or Bianchi class-A models and Reissner-Nordström black holes in quantum \(N=2\) supergravity