Fierz-Pauli theory reloaded: from a theory of a symmetric tensor field to linearized massive gravity
arXiv:2102.10813 · doi:10.1140/epjc/s10052-021-08962-8
Abstract
Modifying gravity at large distances by means of a massive graviton may explain the observed acceleration of the Universe without Dark Energy. The standard paradigm for Massive Gravity is the Fierz-Pauli theory, which, nonetheless, displays well known flaws in its massless limit. The most serious one is represented by the vDVZ discontinuity, which consists in a disagreement between the massless limit of the Fierz-Pauli theory and General Relativity. Our approach is based on a field theoretical treatment of Massive Gravity: General Relativity, in the weak field approximation, is treated as a gauge theory of a symmetric rank-2 tensor field. This leads us to propose an alternative theory of linearized Massive Gravity, describing five degrees of freedom of the graviton, with a good massless limit, without vDVZ discontinuity, and depending on one mass parameter only, in agreement with the Fierz-Pauli theory.
arXiv comment21 pages, no figures
References in corpus (21)
- Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
- Measurements of Omega and Lambda from 42 High-Redshift Supernovae
- Planck 2015 results. XIII. Cosmological parameters
- Cosmological Imprint of an Energy Component with General Equation of State
- Cosmology and the Fate of Dilatation Symmetry
- A Dynamical Solution to the Problem of a Small Cosmological Constant and Late-time Cosmic Acceleration
- Resummation of Massive Gravity
- Coupled Quintessence
- The String Dilaton and a Least Coupling Principle
- Generalization of the Fierz-Pauli Action
- Massive Gravity
- Theoretical Aspects of Massive Gravity
- Tests of General Relativity with the Binary Black Hole Signals from the LIGO-Virgo Catalog GWTC-1
- Resolving the Ghost Problem in non-Linear Massive Gravity
- A Map of the Universe
- On Non-Linear Actions for Massive Gravity
- Massive Cosmologies
- Infrared-modified gravities and massive gravitons
- Massive gravity and Fierz-Pauli theory
- A note on Harmonic Gauge(s) in Massive Gravity
- Constraints on interacting dynamical dark energy and a new test for CDM
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