Built on

C. J. Isham, A. Salam and J. A. Strathdee, F-dominance of gravity
1971
Earlier work this paper cites.
D. G. Boulware, S. Deser, Can gravitation have a finite range?
1972
Earlier work this paper cites.
J. Kluson, Hamiltonian Formalism of Bimetric Gravity In Vierbein Formulation
Original
1974
Earlier work this paper cites.
S. Deser and P. van Nieuwenhuizen, Nonrenormalizability of the Quantized Dirac-Einstein System
1974
Earlier work this paper cites.
Y. .M. Zinoviev, All spin-2 cubic vertices with two derivatives
Original
1983
Earlier work this paper cites.
N. Boulanger, T. Damour, L. Gualtieri and M. Henneaux, Inconsistency of interacting, multigraviton theories
2001
Earlier work this paper cites.
T. Biswas, A. Mazumdar and W. Siegel, Bouncing universes in string-inspired gravity
2006
Earlier work this paper cites.
S. H. S. Alexander, Is cosmic parity violation responsible for the anomalies in the WMAP data?
2008
Earlier work this paper cites.
C. de Rham and G. Gabadadze, Generalization of the Fierz-Pauli Action
Original
2010
Earlier work this paper cites.
T. Biswas, T. Koivisto and A. Mazumdar, Towards a resolution of the cosmological singularity in non-local higher derivative theories of gravity
Original
2010
Earlier work this paper cites.
C. de Rham, G. Gabadadze and A. J. Tolley, Resummation of Massive Gravity
Original
2011
Earlier work this paper cites.
G. D’Amico, C. de Rham, S. Dubovsky, G. Gabadadze, D. Pirtskhalava and A. J. Tolley, Massive Cosmologies
Original
2011
Earlier work this paper cites.
T. S. Koivisto, On new variational principles as alternatives to the Palatini method
Original
2011
Earlier work this paper cites.
T. S. Koivisto and D. F. Mota, CMB statistics in noncommutative inflation
Original
2011
Earlier work this paper cites.
S. F. Hassan, R. A. Rosen and A. Schmidt-May, Ghost-free Massive Gravity with a General Reference Metric
Original
2012
Earlier work this paper cites.
S. F. Hassan and R. A. Rosen, Bimetric Gravity from Ghost-free Massive Gravity
Original
2012
Earlier work this paper cites.
M. S. Volkov, Cosmological solutions with massive gravitons in the bigravity theory
Original
2012
Earlier work this paper cites.

Similar

M. von Strauss, A. Schmidt-May, J. Enander, E. Mortsell and S. F. Hassan, Cosmological Solutions in Bimetric Gravity and their Observational Tests
Original
2012
Cited alongside, same era.
M. S. Volkov, Exact self-accelerating cosmologies in the ghost-free bigravity and massive gravity
Original
2012
Cited alongside, same era.
M. Berg, I. Buchberger, J. Enander, E. Mortsell and S. Sjors, Growth Histories in Bimetric Massive Gravity
Original
2012
Cited alongside, same era.
M. S. Volkov, Exact self-accelerating cosmologies in the ghost-free massive gravity – the detailed derivation
Original
2012
Cited alongside, same era.
S. ’i. Nojiri and S. D. Odintsov, Ghost-free F ⁡ ( R ) F(R) bigravity and accelerating cosmology

Then

F. Kuhnel, On Instability of Certain Bi-Metric and Massive-Gravity Theories
Original
2013
Closest in time.
Y. Akrami, T. S. Koivisto and M. Sandstad, Accelerated expansion from ghost-free bigravity: a statistical analysis with improved generality
Original
2013
Closest in time.
G. Tasinato, K. Koyama and G. Niz, Vector instabilities and self-acceleration in the decoupling limit of massive gravity
Original
2013
Closest in time.
S. Deser and A. Waldron, Acausality of Massive Gravity
Original
2013
Closest in time.
S. Deser, M. Sandora and A. Waldron, Nonlinear Partially Massless from Massive Gravity?
Original

Beyond the bibliography

alphaXiv searches the wider corpus for related work and actual follow-ups.

Open on alphaXiv

alphaXiv is searching for related work…

Reading the bibliography…

2013

The Cosmology of Interacting Spin-2 Fields

Tamanini, Nicola, Saridakis, Emmanuel N., Koivisto, Tomi S.

Understand

We investigate the cosmology of interacting spin-2 particles, formulating the multi-gravitational theory in terms of vierbeins and without imposing any Deser-van Nieuwenhuizen-like constraint.

The resulting multi-vierbein theory represents a wider class of gravitational theories if compared to the corresponding multi-metric models.
Moreover, as opposed to its metric counterpart which in general seems to contain ghosts, it has already been proved to be ghost-free.
We outline a discussion about the possible matter couplings and we focus on the study of cosmological scenarios in the case of three and four interacting vierbeins.