New Massive Gravity Domain Walls

Abstract

The properties of the asymptotic $Ad{S}_3$ 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 $I^{st}$ 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 $CF{T}_2$'s central charges. The holographic renormalization group flows and the phase transitions in specific deformed $CF{T}_2$ dual to 3D massive gravity model with quadratic superpotential are discussed.

arXiv comment12 pages,v2-misprints corrected,comments concerning BPS eqs. for NMG model in d>3 added in Sect.7

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Cited by in corpus (13)

• Comments on Holographic Entanglement Entropy and RG Flows
• Type D Solutions of 3D New Massive Gravity
• Gravitational solitons, hairy black holes and phase transitions in BHT massive gravity
• Conserved quantities and Virasoro algebra in New massive gravity
• Critical Higher Order Gravities in Higher Dimensions
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• New Massive Gravity Holography
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• Holographic RG Flows from Quasi-Topological Gravity
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