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Critical Gravity in Four Dimensions

H. Lü and C. N. Pope
Phys. Rev. Lett. 106, 181302 – Published 6 May 2011

Abstract

We study four-dimensional gravity theories that are rendered renormalizable by the inclusion of curvature-squared terms to the usual Einstein action with a cosmological constant. By choosing the parameters appropriately, the massive scalar mode can be eliminated and the massive spin-2 mode can become massless. This “critical” theory may be viewed as a four-dimensional analogue of chiral topologically massive gravity, or of critical “new massive gravity” with a cosmological constant, in three dimensions. We find that the on-shell energy for the remaining massless gravitons vanishes. There are also logarithmic spin-2 modes, which have positive energy. The mass and entropy of standard Schwarzschild-type black holes vanish. The critical theory might provide a consistent toy model for quantum gravity in four dimensions.

  • Received 14 January 2011

DOI:https://doi.org/10.1103/PhysRevLett.106.181302

© 2011 American Physical Society

Authors & Affiliations

H. Lü1,2 and C. N. Pope3,4

  • 1China Economics and Management Academy, Central University of Finance and Economics, Beijing 100081, China
  • 2Institute for Advanced Study, Shenzhen University, Nanhai Avenue 3688, Shenzhen 518060, China
  • 3George P. & Cynthia Woods Mitchell Institute for Fundamental Physics and Astronomy, Texas A&M University, College Station, Texas 77843, USA
  • 4DAMTP, Centre for Mathematical Sciences, Cambridge University, Wilberforce Road, Cambridge CB3 OWA, United Kingdom

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Issue

Vol. 106, Iss. 18 — 6 May 2011

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