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      General relativity as an effective field theory: The leading quantum corrections

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          Abstract

          I describe the treatment of gravity as a quantum effective field theory. This allows a natural separation of the (known) low energy quantum effects from the (unknown) high energy contributions. Within this framework, gravity is a well behaved quantum field theory at ordinary energies. In studying the class of quantum corrections at low energy, the dominant effects at large distance can be isolated, as these are due to the propagation of the massless particles (including gravitons) of the theory and are manifested in the nonlocal/nonanalytic contributions to vertex functions and propagators. These leading quantum corrections are parameter-free and represent necessary consequences of quantum gravity. The methodology is illustrated by a calculation of the leading quantum corrections to the gravitational interaction of two heavy masses.

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          On Field Theories with Non-Localized Action

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            Leading Quantum Correction to the Newtonian Potential

            I argue that the leading quantum corrections, in powers of the energy or inverse powers of the distance, may be computed in quantum gravity through knowledge of only the low energy structure of the theory. As an example, I calculate the leading quantum corrections to the Newtonian gravitational potential.
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              Author and article information

              Journal
              25 May 1994
              Article
              10.1103/PhysRevD.50.3874
              gr-qc/9405057
              a4391a1f-3140-453e-b8e0-ca848e0a5106
              History
              Custom metadata
              Phys.Rev.D50:3874-3888,1994
              34 pages, Latex, UMHEP-408
              gr-qc hep-ph hep-th

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