2010/08/31 by U. Camara dS, G. M. Sotkov · 18 citations
Mathematics · Physics and Astronomy · #Black Holes and Theoretical Physics #Cauchy stress tensor #Classical mechanics #Cosmology and Gravitation Theories #Domain (mathematical analysis) #Geometry #Gravitation #Massive gravity #Mathematical analysis #Mathematical physics #Mathematics #Noncommutative and Quantum Gravity Theories #Physics #Quantum mechanics #Renormalization group #Scalar (mathematics) #Spacetime #Superpotential #Supersymmetry #Tensor (intrinsic definition) #Theoretical physics #gr-qc #hep-th
paper · pdf · doi:10.1016/j.physletb.2010.09.042
published in Physics Letters B 694(1), 94-99 (Elsevier BV) · 12 pages,v2-misprints corrected,comments concerning BPS eqs. for NMG model in d>3 added in Sect.7
arxiv created 2010/09/13 · openalex publication_date 2010/09/22 · arxiv updated 2014/11/21 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
The properties of the asymptotic AdS3 space-times representing flat domain walls (DW's) solutions of the New Massive 3D Gravity with scalar matter are studied. Our analysis is based on Ist order BPS-like equations involving an appropriate superpotential. The Brown-York boundary stress-tensor is used for the calculation of DW's tensions as well as of the CFT2's central charges. The holographic renormalization group flows and the phase transitions in specific deformed CFT2 dual to 3D massive gravity model with quadratic superpotential are discussed.